178 results on '"Seifert, H"'
Search Results
2. Prospektive multizentrische Validierung des Stockholm-3-Tests (STHLM3) in einer mitteleuropäischen Kohorte
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Sigle, A, Elyan, A, Saba, K, Wetterauer, C, Engesser, C, Püschel, H, Attianese, S, Maurer, P, Deckart, A, Strebel, R, Gratzke, C, Seifert, H, Rentsch, C, Mortezavi, A, Sigle, A, Elyan, A, Saba, K, Wetterauer, C, Engesser, C, Püschel, H, Attianese, S, Maurer, P, Deckart, A, Strebel, R, Gratzke, C, Seifert, H, Rentsch, C, and Mortezavi, A
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- 2023
3. Multicenter, Prospective Validation of a Phenotypic Algorithm to Guide Carbapenemase Testing in Carbapenem-Resistant Pseudomonas aeruginosa Using the ERACE-PA Global Surveillance Program
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Gill, C.M. Aktaþ, E. Alfouzan, W. Bourassa, L. Brink, A. Burnham, C.-A.D. Canton, R. Carmeli, Y. Falcone, M. Kiffer, C. Marchese, A. Martinez, O. Pournaras, S. Satlin, M.J. Seifert, H. Thabit, A.K. Thomson, K.S. Villegas, M.V. Nicolau, D.P. and Gill, C.M. Aktaþ, E. Alfouzan, W. Bourassa, L. Brink, A. Burnham, C.-A.D. Canton, R. Carmeli, Y. Falcone, M. Kiffer, C. Marchese, A. Martinez, O. Pournaras, S. Satlin, M.J. Seifert, H. Thabit, A.K. Thomson, K.S. Villegas, M.V. Nicolau, D.P.
- Abstract
Background: Carbapenemase-producing, carbapenem-resistant Pseudomonas aeruginosa (CP-CRPA) is a global challenge. However, detection efforts can be laborious because numerous mechanisms produce carbapenem resistance. A minimum inhibitory concentration-based algorithm (imipenem- or meropenem-resistant plus ceftazidime-nonsusceptible plus cefepime-nonsusceptible) was proposed to identify the isolates most likely to harbor a carbapenemase; however, prospective validation in geographies displaying genotypic diversity and varied carbapenemase prevalence is warranted. Methods: CRPA isolates were collected during the Enhancing Rational Antimicrobials for P. aeruginosa (ERACE-PA) global surveillance program from 17 sites in 12 countries. Isolates underwent susceptibility testing following local standards to ceftazidime, cefepime, and ceftolozane/tazobactam. Isolates underwent initial phenotypic carbapenemase screening followed by molecular testing if positive. The primary algorithm criteria were applied, and results were compared with phenotypic carbapenemase results to assess the performance of the algorithm. A secondary criterion, the algorithm criterion or imipenem- or meropenem-resistant plus ceftolozane/tazobactam-nonsusceptible, was assessed. Results: A total of 807 CRPA were assessed, and 464 isolates met the algorithm criteria described above. Overall, testing was reduced by 43% compared with testing all CRPA. Carbapenemase-positive isolates missed by the algorithm were largely driven by Guiana extended spectrum (GES). Addition of the criterion of imipenem- or meropenem-resistant plus ceftolozane/tazobactam-nonsusceptible decreased the number of CP-CRPA missed by the algorithm (21 vs 40 isolates, respectively), reducing number of isolates tested by 39%. Conclusions: Application of the initial algorithm (imipenem- or meropenem-resistant plus ceftazidime-nonsusceptible plus cefepime-nonsusceptible) performed well in a global cohort, with 33% phenotypically carbapenema
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- 2022
4. Elevated MICs of susceptible antipseudomonal cephalosporins in non-carbapenemase-producing, carbapenem-resistant pseudomonas aeruginosa: Implications for dose optimization
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Gill, C.M. Aktaş, E. Alfouzan, W. Bourassa, L. Brink, A. Burnham, C.-A.D. Canton, R. Carmeli, Y. Falcone, M. Kiffer, C. Marchese, A. Martinez, O. Pournaras, S. Seifert, H. Thabit, A.K. Villegas, M.V. Westblade, L.F. Nicolau, D.P. Wille, J. Rezende, T.T.F. Cekin, Z. Malkocoglu, G. Gijón, D. Tarakmeh, L.A. Chu, C.Y. Opperman, C.J. Tootla, H.D. Moodley, C. Coetzee, J. Vourli, S. Dimopoulos, G. Attallah, D.M. Tiseo, G. Leonildi, A. Giordano, C. Barnini, S. Menichetti, F. Di Pilato, V. Codda, G. Vena, A. Giacobbe, D.R. Satlin, M. Cardona, A. Curtis, L. Fang, F. Thomson, G. Thomson, K. the ERACE-PA Global Study Group and Gill, C.M. Aktaş, E. Alfouzan, W. Bourassa, L. Brink, A. Burnham, C.-A.D. Canton, R. Carmeli, Y. Falcone, M. Kiffer, C. Marchese, A. Martinez, O. Pournaras, S. Seifert, H. Thabit, A.K. Villegas, M.V. Westblade, L.F. Nicolau, D.P. Wille, J. Rezende, T.T.F. Cekin, Z. Malkocoglu, G. Gijón, D. Tarakmeh, L.A. Chu, C.Y. Opperman, C.J. Tootla, H.D. Moodley, C. Coetzee, J. Vourli, S. Dimopoulos, G. Attallah, D.M. Tiseo, G. Leonildi, A. Giordano, C. Barnini, S. Menichetti, F. Di Pilato, V. Codda, G. Vena, A. Giacobbe, D.R. Satlin, M. Cardona, A. Curtis, L. Fang, F. Thomson, G. Thomson, K. the ERACE-PA Global Study Group
- Abstract
The present study evaluated the in vitro potency of ceftazidime and cefepime among carbapenem-resistant Pseudomonas aeruginosa isolates collected as part of a global surveillance program and assessed the pharmacodynamic implications using previously published population pharmacokinetics. When susceptible, MICs resulted at the high end of distribution for both ceftazidime and cefepime, thus 6 g/day was required to achieve optimal pharmacodynamic profiles. These findings should be considered in the clinic and for the application of CLSI susceptibility breakpoints. © 2021 American Society for Microbiology.
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- 2021
5. Early identification and optimal management of carbapenem-resistant Gram-negative infection
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Bedos, J.P. Daikos, G. Dodgson, A.R. Pan, A. Petrosillo, N. Seifert, H. Vila, J. Ferrer, R. Wilson, P. and Bedos, J.P. Daikos, G. Dodgson, A.R. Pan, A. Petrosillo, N. Seifert, H. Vila, J. Ferrer, R. Wilson, P.
- Abstract
Background: Carbapenem resistance in Gram-negative bacteria is associated with severe infections in the hospital setting. No uniform screening policy or agreed set of criteria exists within the EU to inform treatment decisions for infections caused by carbapenem-resistant Gram-negative bacteria. Aim: To develop a range of consensus statements to survey experts in carbapenem resistance, to identify potential similarities and differences across the EU and across specialties. Methods: The survey contained 43 statements, covering six key topics relating to carbapenem-resistant organisms: microbiological screening; diagnosis; infection control implementation; antibiotic stewardship; use of resources; and influencing policy. Findings: In total, 136 survey responses were received (66% infectious disease specialists, 18% microbiologists, 11% intensive care specialists, 4% other/unknown) from France, Germany, Greece, Italy, Spain, and the UK. High, or very high, levels of agreement were seen for all 43 consensus statements, indicating good alignment concerning early identification and optimal management of infection due to carbapenem-resistant organisms. Conclusion: We offer the following recommendations: (1) screening is required when a patient may have been exposed to the healthcare system in countries/hospitals where carbapenem-resistant organisms are endemic; (2) rapid diagnostic tools should be available in every institution; (3) all institutions should have a specific policy for the control of carbapenem-resistant organisms, which is routinely audited; (4) clear strategies are required to define both appropriate and inappropriate use of carbapenems; (5) priority funding should be allocated to the management of infections due to carbapenem-resistant organisms; and (6) international co-operation is required to reduce country-to-country transmission of carbapenem-resistant organisms. © 2020 The Authors
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- 2021
6. Energetic ions in the Venusian system: Insights from the first Solar Orbiter flyby
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Allen, R.C., Cernuda, I., Pacheco, D., Berger, L., Xu, Z.G., Forstner, J.L. Freiherr von, Rodríguez-Pacheco, J., Wimmer-Schweingruber, R.F., Ho, G.C., Mason, G.M., Vines, S.K., Khotyaintsev, Y., Horbury, T., Maksimovic, M., Hadid, L.Z., Volwerk, M., Dimmock, A.P., Sorriso-Valvo, L., Stergiopoulou, K., Andrews, G.B., Angelini, V., Bale, S. D., Boden, S., Böttcher, S.I., Chust, T., Eldrum, S., Espada, P.P., Lara, F. Espinosa, Evans, V., Gómez-Herrero, R., Hayes, J.R., Hellín, A.M., Kollhoff, A., Krasnoselskikh, V., Kretzschmar, M., Kühl, P., Kulkarni, S.R., Lees, W.J., Lorfèvre, E., Martin, C., O’Brien, H., Plettemeier, D., Polo, O.R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C.E., Seifert, H., Souček, J., Steller, M., Štverák, Š., Terasa, J.C., Trávníček, P., Tyagi, K., Vaivads, A., Vecchio, A., Yedla, M., Allen, R.C., Cernuda, I., Pacheco, D., Berger, L., Xu, Z.G., Forstner, J.L. Freiherr von, Rodríguez-Pacheco, J., Wimmer-Schweingruber, R.F., Ho, G.C., Mason, G.M., Vines, S.K., Khotyaintsev, Y., Horbury, T., Maksimovic, M., Hadid, L.Z., Volwerk, M., Dimmock, A.P., Sorriso-Valvo, L., Stergiopoulou, K., Andrews, G.B., Angelini, V., Bale, S. D., Boden, S., Böttcher, S.I., Chust, T., Eldrum, S., Espada, P.P., Lara, F. Espinosa, Evans, V., Gómez-Herrero, R., Hayes, J.R., Hellín, A.M., Kollhoff, A., Krasnoselskikh, V., Kretzschmar, M., Kühl, P., Kulkarni, S.R., Lees, W.J., Lorfèvre, E., Martin, C., O’Brien, H., Plettemeier, D., Polo, O.R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C.E., Seifert, H., Souček, J., Steller, M., Štverák, Š., Terasa, J.C., Trávníček, P., Tyagi, K., Vaivads, A., Vecchio, A., and Yedla, M.
- Abstract
Contains fulltext : 242950.pdf (Publisher’s version ) (Open Access)
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- 2021
7. The Long Period of 3He-rich Solar Energetic Particles Measured by Solar Orbiter on 2020 November 17-23
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Bucik, R., Mason, G. M., Gomez-Herrero, R., Lario, D., Balmaceda, L., Nitta, N. V., Krupar, V., Dresing, N., Ho, G. C., Allen, R. C., Carcaboso, F., Rodriguez-Pacheco, J., Schuller, F., Warmuth, A., Wimmer-Schweingruber, R. F., von Forstner, J. L. Freiherr, Andrews, G. B., Berger, L., Cernuda, I., Lara, F. Espinosa, Lees, W. J., Martin, C., Pacheco, D., Prieto, M., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Tyagi, K., Maksimovic, M., Vecchio, A., Kollhoff, A., Kuhl, P., Xu, Z. G., Eldrum, S., Bucik, R., Mason, G. M., Gomez-Herrero, R., Lario, D., Balmaceda, L., Nitta, N. V., Krupar, V., Dresing, N., Ho, G. C., Allen, R. C., Carcaboso, F., Rodriguez-Pacheco, J., Schuller, F., Warmuth, A., Wimmer-Schweingruber, R. F., von Forstner, J. L. Freiherr, Andrews, G. B., Berger, L., Cernuda, I., Lara, F. Espinosa, Lees, W. J., Martin, C., Pacheco, D., Prieto, M., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Tyagi, K., Maksimovic, M., Vecchio, A., Kollhoff, A., Kuhl, P., Xu, Z. G., and Eldrum, S.
- Abstract
We report observations of a relatively long period of 3He-rich solar energetic particles (SEPs) measured by Solar Orbiter. The period consists of several well-resolved ion injections. The high-resolution STEREO-A imaging observations reveal that the injections coincide with EUV jets/brightenings near the east limb, not far from the nominal magnetic connection of Solar Orbiter. The jets originated in two adjacent, large, and complex active regions as observed by the Solar Dynamics Observatory when the regions rotated to the Earth's view. It appears that the sustained ion injections were related to the complex configuration of the sunspot group and the long period of 3He-rich SEPs to the longitudinal extent covered by the group during the analyzed time period., Comment: accepted for publication in A&A, Letters to the Editor
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- 2021
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8. First year of energetic particle measurements in the inner heliosphere with Solar Orbiter's Energetic Particle Detector
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Wimmer-Schweingruber, R. F., Janitzek, N., Pacheco, D., Cernuda, I., Lara, F. Espinosa, Gómez-Herrero, R., Mason, G. M., Allen, R. C., Xu, Z. G., Carcaboso, F., Kollhoff, A., Kühl, P., von Forstner, J. L. Freiherr, Berger, L., Rodriguez-Pacheco, J., Ho, G. C., Andrews, G. B., Angelini, V., Aran, A., Boden, S., Böttcher, S. I., Carrasco, A., Dresing, N., Eldrum, S., Elftmann, R., Evans, V., Gevin, O., Hayes, J., Heber, B., Horbury, T. S., Kulkarni, S. R., Lario, D., Lees, W. J., Limousin, O., Malandraki, O., Martín, C., O'Brien, H., Mateo, M. Prieto, Ravanbakhsh, A., Polo, O. Rodriguez, Prieto, S. Sánchez, Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Vainio, R., Walsh, A., Yedla, M. K., Wimmer-Schweingruber, R. F., Janitzek, N., Pacheco, D., Cernuda, I., Lara, F. Espinosa, Gómez-Herrero, R., Mason, G. M., Allen, R. C., Xu, Z. G., Carcaboso, F., Kollhoff, A., Kühl, P., von Forstner, J. L. Freiherr, Berger, L., Rodriguez-Pacheco, J., Ho, G. C., Andrews, G. B., Angelini, V., Aran, A., Boden, S., Böttcher, S. I., Carrasco, A., Dresing, N., Eldrum, S., Elftmann, R., Evans, V., Gevin, O., Hayes, J., Heber, B., Horbury, T. S., Kulkarni, S. R., Lario, D., Lees, W. J., Limousin, O., Malandraki, O., Martín, C., O'Brien, H., Mateo, M. Prieto, Ravanbakhsh, A., Polo, O. Rodriguez, Prieto, S. Sánchez, Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Vainio, R., Walsh, A., and Yedla, M. K.
- Abstract
Solar Orbiter strives to unveil how the Sun controls and shapes the heliosphere and fills it with energetic particle radiation. To this end, its Energetic Particle Detector (EPD) has now been in operation, providing excellent data, for just over a year. EPD measures suprathermal and energetic particles in the energy range from a few keV up to (near-) relativistic energies (few MeV for electrons and about 500 MeV/nuc for ions). We present an overview of the initial results from the first year of operations and we provide a first assessment of issues and limitations. During this first year of operations of the Solar Orbiter mission, EPD has recorded several particle events at distances between 0.5 and 1 au from the Sun. We present dynamic and time-averaged energy spectra for ions that were measured with a combination of all four EPD sensors, namely: the SupraThermal Electron and Proton sensor (STEP), the Electron Proton Telescope (EPT), the Suprathermal Ion Spectrograph (SIS), and the High-Energy Telescope (HET) as well as the associated energy spectra for electrons measured with STEP and EPT. We illustrate the capabilities of the EPD suite using the 10-11 December 2020 solar particle event. This event showed an enrichment of heavy ions as well as $^3$He, for which we also present dynamic spectra measured with SIS. The high anisotropy of electrons at the onset of the event and its temporal evolution is also shown using data from these sensors. We discuss the ongoing in-flight calibration and a few open instrumental issues using data from the 21 July and the 10-11 December 2020 events and give guidelines and examples for the usage of the EPD data. We explain how spacecraft operations may affect EPD data and we present a list of such time periods in the appendix. A list of the most significant particle enhancements as observed by EPT during this first year is also provided.
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- 2021
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9. Early identification and optimal management of carbapenem-resistant Gram-negative infection
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Bedos, J. P., Daikos, G., Dodgson, A. R., Pan, A., Petrosillo, N., Seifert, H., Vila, J., Ferrer, R., Wilson, P., Bedos, J. P., Daikos, G., Dodgson, A. R., Pan, A., Petrosillo, N., Seifert, H., Vila, J., Ferrer, R., and Wilson, P.
- Abstract
Background: Carbapenem resistance in Gram-negative bacteria is associated with severe infections in the hospital setting. No uniform screening policy or agreed set of criteria exists within the EU to inform treatment decisions for infections caused by carbapenemAim: To develop a range of consensus statements to survey experts in carbapenem resistance, to identify potential similarities and differences across the EU and across specialties. Methods: The survey contained 43 statements, covering six key topics relating to carbapenem-resistant organisms: microbiological screening; diagnosis; infection control implementation; antibiotic stewardship; use of resources; and influencing policy. Findings: In total, 136 survey responses were received (66% infectious disease specialists, 18% microbiologists, 11% intensive care specialists, 4% other/unknown) from France, Germany, Greece, Italy, Spain, and the UK. High, or very high, levels of agreement were seen for all 43 consensus statements, indicating good alignment concerning early identification and optimal management of infection due to carbapenem-resistant organisms. Conclusion: We offer the following recommendations: (1) screening is required when a patient may have been exposed to the healthcare system in countries/hospitals where carbapenem-resistant organisms are endemic; (2) rapid diagnostic tools should be available in every institution; (3) all institutions should have a specific policy for the control of carbapenem-resistant organisms, which is routinely audited; (4) clear strategies are required to define both appropriate and inappropriate use of carbapenems; (5) priority funding should be allocated to the management of infections due to carbapenem-resistant organisms; and (6) international co-operation is required to reduce country-to-country transmission of carbapenem-resistant organisms. (c) 2020 The Authors. Published by Elsevier Ltd on behalf of The Healthcare Infection Society. This is an open access articl
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- 2021
10. Vertebral osteomyelitis in patients with Staphylococcus aureus bloodstream infection: Evaluation of risk factors for treatment failure
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Jung, N., Ernst, A., Joost, I, Yagdiran, A., Peyerl-Hoffmann, G., Grau, S., Breuninger, M., Hellmich, M., Kubosch, D. C., Klingler, J. H., Seifert, H., Kern, W., V, Kaasch, A. J., Rieg, S., Jung, N., Ernst, A., Joost, I, Yagdiran, A., Peyerl-Hoffmann, G., Grau, S., Breuninger, M., Hellmich, M., Kubosch, D. C., Klingler, J. H., Seifert, H., Kern, W., V, Kaasch, A. J., and Rieg, S.
- Abstract
Objectives: Staphylococcus aureus is the most common cause of pyogenic vertebral osteomyelitis (VO). Studies indicate that S. aureus VO results in poor outcome. We aimed to investigate risk factors for treatment failure in patients with Staphylococcus aureus bloodstream infection (SAB) and VO. Methods: We conducted a post hoc-analysis of data from a German bi-center prospective SAB cohort (2006-2014). Patients were followed-up for one year. Primary outcome was treatment failure defined as relapse and/or death within one year. Results: A total of 1069 patients with SAB were analyzed, with 92 VO patients. In addition to antibiotic treatment, surgery was performed in 60/92 patients. Treatment failed in 44/92 patients (death, n = 42; relapse, n = 2). Multivariable analysis revealed higher age (HR 1.04 [per year], 95%CI 1.01-1.07), Charlson comorbidity index (HR 1.20, 95%CI 1.06-1.36), presence of neurologic deficits (HR 2.53, 95%CI 1.15-5.53) and local abscess formation (HR 3.35, 95%CI 1.39-8.04) as independent risk factors for treatment failure. In contrast, surgery seemed to be associated with a favourable outcome (HR 0.45 (95%CI 0.20-0.997)). Conclusion: SAB patients with VO exhibit a high treatment failure rate. Red flags are older age, comorbidities, neurologic deficits and local abscess formation. Whether these patients benefit from intensified treatment (e.g. radical surgery, prolongation of antibiotics) should be investigated further. (C) 2021 The British Infection Association. Published by Elsevier Ltd. All rights reserved.
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- 2021
11. Outbreak of Pseudomonas aeruginosa infections after CT-guided spinal injections
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Paul, G., Meissner, A., Neuneier, J., Neuschmelting, V, Grau, S., Yagdiran, A., Scheyerer, M. J., Malin, J. J., Suarez, I, Lehmann, C., Exner, M., Wiesmuller, G. A., Higgins, P. G., Seifert, H., Fatkenheuer, G., Zweigner, J., Jung, N., Paul, G., Meissner, A., Neuneier, J., Neuschmelting, V, Grau, S., Yagdiran, A., Scheyerer, M. J., Malin, J. J., Suarez, I, Lehmann, C., Exner, M., Wiesmuller, G. A., Higgins, P. G., Seifert, H., Fatkenheuer, G., Zweigner, J., and Jung, N.
- Abstract
Background: Meningitis and spinal infections with Gram-negative bacteria after local injections for treatment of chronic back pain are rare. This study investigated an outbreak of Pseudomonas aeruginosa infections following computed tomography (CT)-guided spinal injections (SI). Methods: A case was defined as a spinal infection or meningitis with P. aeruginosa after SI between 10th January and 1st March 2019 in the same outpatient clinic. Patients without microbiological evidence of P. aeruginosa but with a favourable response to antimicrobial therapy active against P. aeruginosa were defined as probable cases. Findings: Twenty-eight of 297 patients receiving CT-guided SI during the study period developed meningitis or spinal infections. Medical records were available for 19 patients. In 15 patients, there was microbiological evidence of P. aeruginosa, and four patients were defined as probable cases. Two of 19 patients developed meningitis, while the remaining 17 patients developed spinal infections. The median time from SI to hospital admission was 8 days (interquartile range 2-23 days). Patients mainly presented with back pain (N=18; 95%), and rarely developed fever (N=3; 16%). Most patients required surgery (N=16; 84%). Seven patients (37%) relapsed and one patient died. Although the source of infection was not identified microbiologically, documented failures in asepsis when performing SI probably contributed to these infections. Conclusions: SI is generally considered safe, but non-adherence to asepsis can lead to deleterious effects. Spinal infections caused by P. aeruginosa are difficult to treat and have a high relapse rate. (C) 2021 The Healthcare Infection Society. Published by Elsevier Ltd. All rights reserved.
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- 2021
12. Comparison of the Acinetobacter baumannii Reference Strains ATCC 17978 and ATCC 19606 in Antimicrobial Resistance Mediated by the AdeABC Efflux Pump
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Lucassen, K., Gerson, S., Xanthopoulou, K., Wille, J., Wille, T., Seifert, H., Higgins, P. G., Lucassen, K., Gerson, S., Xanthopoulou, K., Wille, J., Wille, T., Seifert, H., and Higgins, P. G.
- Abstract
The Acinetobacter baumannii RND efflux pump AdeABC is regulated by the 2-component regulator AdeRS. In this study, we compared the regulation and expression of AdeABC of the reference strains ATCC 17978 and ATCC 19606. A clearly stronger efflux activity was demonstrated for ATCC 19606. An amino acid substitution at residue 172 of adeS was identified as a potential cause for differential expression of the pump. Therefore, we recommend caution with exclusively using single reference strains for research.
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- 2021
13. Energetic ions in the Venusian system : Insights from the first Solar Orbiter flyby
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Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., Yedla, M., Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., and Yedla, M.
- Abstract
The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the system and provide a characterization of galactic cosmic rays near the planet. Bursty suprathermal ion enhancements (up to similar to 10 keV) were observed as far as similar to 50R(V) downtail. These enhancements are likely related to a combination of acceleration mechanisms in regions of strong turbulence, current sheet crossings, and boundary layer crossings, with a possible instance of ion heating due to ion cyclotron waves within the Venusian tail. Upstream of the planet, suprathermal ions are observed that might be related to pick-up acceleration of photoionized exospheric populations as far as 5R(V) upstream in the solar wind as has been observed before by missions such as Pioneer Venus Orbiter and Venus Express. Near the closest approach of Solar Orbiter, the Galactic cosmic ray (GCR) count rate was observed to decrease by approximately 5 percent, which is consistent with the amount of sky obscured by the planet, suggesting a negligible abundance of GCR albedo particles at over 2 R-V. Along with modulation of the GCR population very close to Venus, the Solar Orbiter observations show that the Venusian system, even far from the planet, can be an effective accelerator of ions up to similar to 30 keV. This paper is part of a series of the first papers from the Solar Orbiter Venus flyby.
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- 2021
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14. Evidence for local particle acceleration in the first recurrent galactic cosmic ray depression observed by Solar Orbiter : The ion event on 19 June 2020
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Aran, A., Pacheco, D., Laurenza, M., Wijsen, N., Lario, D., Benella, S., Richardson, I. G., Samara, E., von Forstner, J. L. Freiherr, Sanahuja, B., Rodriguez, L., Balmaceda, L., Lara, F. Espinosa, Gomez-Herrero, R., Steinvall, Konrad, Vecchio, A., Krupar, V, Poedts, S., Allen, R. C., Andrews, G. B., Angelini, V, Berger, L., Berghmans, D., Boden, S., Bottcher, S. , I, Carcaboso, F., Cernuda, I, De Marco, R., Eldrum, S., Evans, V, Fedorov, A., Hayes, J., Ho, G. C., Horbury, T. S., Janitzek, N. P., Khotyaintsev, Yuri V., Kollhoff, A., Kuehl, P., Kulkarni, S. R., Lees, W. J., Louarn, P., Magdalenic, J., Maksimovic, M., Malandraki, O., Martinez, A., Mason, G. M., Martin, C., O'Brien, H., Owen, C., Parra, P., Prieto Mateo, M., Ravanbakhsh, A., Rodriguez-Pacheco, J., Rodriguez Polo, O., Sanchez Prieto, S., Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Verbeeck, C., Wimmer-Schweingruber, R. F., Xu, Z. G., Yedla, M. K., Zhukov, A. N., Aran, A., Pacheco, D., Laurenza, M., Wijsen, N., Lario, D., Benella, S., Richardson, I. G., Samara, E., von Forstner, J. L. Freiherr, Sanahuja, B., Rodriguez, L., Balmaceda, L., Lara, F. Espinosa, Gomez-Herrero, R., Steinvall, Konrad, Vecchio, A., Krupar, V, Poedts, S., Allen, R. C., Andrews, G. B., Angelini, V, Berger, L., Berghmans, D., Boden, S., Bottcher, S. , I, Carcaboso, F., Cernuda, I, De Marco, R., Eldrum, S., Evans, V, Fedorov, A., Hayes, J., Ho, G. C., Horbury, T. S., Janitzek, N. P., Khotyaintsev, Yuri V., Kollhoff, A., Kuehl, P., Kulkarni, S. R., Lees, W. J., Louarn, P., Magdalenic, J., Maksimovic, M., Malandraki, O., Martinez, A., Mason, G. M., Martin, C., O'Brien, H., Owen, C., Parra, P., Prieto Mateo, M., Ravanbakhsh, A., Rodriguez-Pacheco, J., Rodriguez Polo, O., Sanchez Prieto, S., Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Verbeeck, C., Wimmer-Schweingruber, R. F., Xu, Z. G., Yedla, M. K., and Zhukov, A. N.
- Abstract
Context. In mid-June 2020, the Solar Orbiter (SolO) mission reached its first perihelion at 0.51 au and started its cruise phase, with most of the in situ instruments operating continuously. Aims. We present the in situ particle measurements of the first proton event observed after the first perihelion obtained by the Energetic Particle Detector (EPD) suite on board SolO. The potential solar and interplanetary (IP) sources of these particles are investigated. Methods. Ion observations from similar to 20 keV to similar to 1 MeV are combined with available solar wind data from the Radio and Plasma Waves (RPW) instrument and magnetic field data from the magnetometer on board SolO to evaluate the energetic particle transport conditions and infer the possible acceleration mechanisms through which particles gain energy. We compare > 17-20 MeV ion count rate measurements for two solar rotations, along with the solar wind plasma data available from the Solar Wind Analyser (SWA) and RPW instruments, in order to infer the origin of the observed galactic cosmic ray (GCR) depressions. Results. The lack of an observed electron event and of velocity dispersion at various low-energy ion channels and the observed IP structure indicate a local IP source for the low-energy particles. From the analysis of the anisotropy of particle intensities, we conclude that the low-energy ions were most likely accelerated via a local second-order Fermi process. The observed GCR decrease on 19 June, together with the 51.8-1034.0 keV nuc(-1) ion enhancement, was due to a solar wind stream interaction region (SIR). The observation of a similar GCR decrease in the next solar rotation favours this interpretation and constitutes the first observation of a recurrent GCR decrease by SolO. The analysis of the recurrence times of this SIR suggests that it is the same SIR responsible for the He-4 events previously measured in April and May. Finally, we point out that an IP structure more complex than a co
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- 2021
- Full Text
- View/download PDF
15. The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29
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Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, Asvestari, E., Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, and Asvestari, E.
- Abstract
Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (≲1 AU) heliosphere. Relativistic electrons as well as protons with energies > 50 MeV were observed by Solar Orbiter (SolO), Parker Solar Probe, the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230° in longitude close to 1 AU. The particle onset delays observed at the different spacecraft are larger as the flare–footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO
- Published
- 2021
- Full Text
- View/download PDF
16. Energetic ions in the Venusian system : Insights from the first Solar Orbiter flyby
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Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., Yedla, M., Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., and Yedla, M.
- Abstract
The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the system and provide a characterization of galactic cosmic rays near the planet. Bursty suprathermal ion enhancements (up to similar to 10 keV) were observed as far as similar to 50R(V) downtail. These enhancements are likely related to a combination of acceleration mechanisms in regions of strong turbulence, current sheet crossings, and boundary layer crossings, with a possible instance of ion heating due to ion cyclotron waves within the Venusian tail. Upstream of the planet, suprathermal ions are observed that might be related to pick-up acceleration of photoionized exospheric populations as far as 5R(V) upstream in the solar wind as has been observed before by missions such as Pioneer Venus Orbiter and Venus Express. Near the closest approach of Solar Orbiter, the Galactic cosmic ray (GCR) count rate was observed to decrease by approximately 5 percent, which is consistent with the amount of sky obscured by the planet, suggesting a negligible abundance of GCR albedo particles at over 2 R-V. Along with modulation of the GCR population very close to Venus, the Solar Orbiter observations show that the Venusian system, even far from the planet, can be an effective accelerator of ions up to similar to 30 keV. This paper is part of a series of the first papers from the Solar Orbiter Venus flyby.
- Published
- 2021
- Full Text
- View/download PDF
17. The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29
- Author
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Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, Asvestari, E., Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, and Asvestari, E.
- Abstract
Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (≲1 AU) heliosphere. Relativistic electrons as well as protons with energies > 50 MeV were observed by Solar Orbiter (SolO), Parker Solar Probe, the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230° in longitude close to 1 AU. The particle onset delays observed at the different spacecraft are larger as the flare–footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO
- Published
- 2021
- Full Text
- View/download PDF
18. The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29
- Author
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Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, Asvestari, E., Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, and Asvestari, E.
- Abstract
Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (≲1 AU) heliosphere. Relativistic electrons as well as protons with energies > 50 MeV were observed by Solar Orbiter (SolO), Parker Solar Probe, the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230° in longitude close to 1 AU. The particle onset delays observed at the different spacecraft are larger as the flare–footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO
- Published
- 2021
- Full Text
- View/download PDF
19. Energetic ions in the Venusian system : Insights from the first Solar Orbiter flyby
- Author
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Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., Yedla, M., Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., and Yedla, M.
- Abstract
The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the system and provide a characterization of galactic cosmic rays near the planet. Bursty suprathermal ion enhancements (up to similar to 10 keV) were observed as far as similar to 50R(V) downtail. These enhancements are likely related to a combination of acceleration mechanisms in regions of strong turbulence, current sheet crossings, and boundary layer crossings, with a possible instance of ion heating due to ion cyclotron waves within the Venusian tail. Upstream of the planet, suprathermal ions are observed that might be related to pick-up acceleration of photoionized exospheric populations as far as 5R(V) upstream in the solar wind as has been observed before by missions such as Pioneer Venus Orbiter and Venus Express. Near the closest approach of Solar Orbiter, the Galactic cosmic ray (GCR) count rate was observed to decrease by approximately 5 percent, which is consistent with the amount of sky obscured by the planet, suggesting a negligible abundance of GCR albedo particles at over 2 R-V. Along with modulation of the GCR population very close to Venus, the Solar Orbiter observations show that the Venusian system, even far from the planet, can be an effective accelerator of ions up to similar to 30 keV. This paper is part of a series of the first papers from the Solar Orbiter Venus flyby.
- Published
- 2021
- Full Text
- View/download PDF
20. Energetic ions in the Venusian system: Insights from the first Solar Orbiter flyby
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Allen, R.C., Cernuda, I., Pacheco, D., Berger, L., Xu, Z.G., Forstner, J.L. Freiherr von, Rodríguez-Pacheco, J., Wimmer-Schweingruber, R.F., Ho, G.C., Mason, G.M., Vines, S.K., Khotyaintsev, Y., Horbury, T., Maksimovic, M., Hadid, L.Z., Volwerk, M., Dimmock, A.P., Sorriso-Valvo, L., Stergiopoulou, K., Andrews, G.B., Angelini, V., Bale, S. D., Boden, S., Böttcher, S.I., Chust, T., Eldrum, S., Espada, P.P., Lara, F. Espinosa, Evans, V., Gómez-Herrero, R., Hayes, J.R., Hellín, A.M., Kollhoff, A., Krasnoselskikh, V., Kretzschmar, M., Kühl, P., Kulkarni, S.R., Lees, W.J., Lorfèvre, E., Martin, C., O’Brien, H., Plettemeier, D., Polo, O.R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C.E., Seifert, H., Souček, J., Steller, M., Štverák, Š., Terasa, J.C., Trávníček, P., Tyagi, K., Vaivads, A., Vecchio, A., Yedla, M., Allen, R.C., Cernuda, I., Pacheco, D., Berger, L., Xu, Z.G., Forstner, J.L. Freiherr von, Rodríguez-Pacheco, J., Wimmer-Schweingruber, R.F., Ho, G.C., Mason, G.M., Vines, S.K., Khotyaintsev, Y., Horbury, T., Maksimovic, M., Hadid, L.Z., Volwerk, M., Dimmock, A.P., Sorriso-Valvo, L., Stergiopoulou, K., Andrews, G.B., Angelini, V., Bale, S. D., Boden, S., Böttcher, S.I., Chust, T., Eldrum, S., Espada, P.P., Lara, F. Espinosa, Evans, V., Gómez-Herrero, R., Hayes, J.R., Hellín, A.M., Kollhoff, A., Krasnoselskikh, V., Kretzschmar, M., Kühl, P., Kulkarni, S.R., Lees, W.J., Lorfèvre, E., Martin, C., O’Brien, H., Plettemeier, D., Polo, O.R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C.E., Seifert, H., Souček, J., Steller, M., Štverák, Š., Terasa, J.C., Trávníček, P., Tyagi, K., Vaivads, A., Vecchio, A., and Yedla, M.
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Contains fulltext : 242950.pdf (Publisher’s version ) (Open Access)
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- 2021
21. Energetic ions in the Venusian system: Insights from the first Solar Orbiter flyby
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Allen, R.C., Cernuda, I., Pacheco, D., Berger, L., Xu, Z.G., Forstner, J.L. Freiherr von, Rodríguez-Pacheco, J., Wimmer-Schweingruber, R.F., Ho, G.C., Mason, G.M., Vines, S.K., Khotyaintsev, Y., Horbury, T., Maksimovic, M., Hadid, L.Z., Volwerk, M., Dimmock, A.P., Sorriso-Valvo, L., Stergiopoulou, K., Andrews, G.B., Angelini, V., Bale, S. D., Boden, S., Böttcher, S.I., Chust, T., Eldrum, S., Espada, P.P., Lara, F. Espinosa, Evans, V., Gómez-Herrero, R., Hayes, J.R., Hellín, A.M., Kollhoff, A., Krasnoselskikh, V., Kretzschmar, M., Kühl, P., Kulkarni, S.R., Lees, W.J., Lorfèvre, E., Martin, C., O’Brien, H., Plettemeier, D., Polo, O.R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C.E., Seifert, H., Souček, J., Steller, M., Štverák, Š., Terasa, J.C., Trávníček, P., Tyagi, K., Vaivads, A., Vecchio, A., Yedla, M., Allen, R.C., Cernuda, I., Pacheco, D., Berger, L., Xu, Z.G., Forstner, J.L. Freiherr von, Rodríguez-Pacheco, J., Wimmer-Schweingruber, R.F., Ho, G.C., Mason, G.M., Vines, S.K., Khotyaintsev, Y., Horbury, T., Maksimovic, M., Hadid, L.Z., Volwerk, M., Dimmock, A.P., Sorriso-Valvo, L., Stergiopoulou, K., Andrews, G.B., Angelini, V., Bale, S. D., Boden, S., Böttcher, S.I., Chust, T., Eldrum, S., Espada, P.P., Lara, F. Espinosa, Evans, V., Gómez-Herrero, R., Hayes, J.R., Hellín, A.M., Kollhoff, A., Krasnoselskikh, V., Kretzschmar, M., Kühl, P., Kulkarni, S.R., Lees, W.J., Lorfèvre, E., Martin, C., O’Brien, H., Plettemeier, D., Polo, O.R., Prieto, M., Ravanbakhsh, A., Sánchez-Prieto, S., Schlemm, C.E., Seifert, H., Souček, J., Steller, M., Štverák, Š., Terasa, J.C., Trávníček, P., Tyagi, K., Vaivads, A., Vecchio, A., and Yedla, M.
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Contains fulltext : 242950.pdf (Publisher’s version ) (Open Access)
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- 2021
22. Energetic ions in the Venusian system : Insights from the first Solar Orbiter flyby
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Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., Yedla, M., Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., and Yedla, M.
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The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the system and provide a characterization of galactic cosmic rays near the planet. Bursty suprathermal ion enhancements (up to similar to 10 keV) were observed as far as similar to 50R(V) downtail. These enhancements are likely related to a combination of acceleration mechanisms in regions of strong turbulence, current sheet crossings, and boundary layer crossings, with a possible instance of ion heating due to ion cyclotron waves within the Venusian tail. Upstream of the planet, suprathermal ions are observed that might be related to pick-up acceleration of photoionized exospheric populations as far as 5R(V) upstream in the solar wind as has been observed before by missions such as Pioneer Venus Orbiter and Venus Express. Near the closest approach of Solar Orbiter, the Galactic cosmic ray (GCR) count rate was observed to decrease by approximately 5 percent, which is consistent with the amount of sky obscured by the planet, suggesting a negligible abundance of GCR albedo particles at over 2 R-V. Along with modulation of the GCR population very close to Venus, the Solar Orbiter observations show that the Venusian system, even far from the planet, can be an effective accelerator of ions up to similar to 30 keV. This paper is part of a series of the first papers from the Solar Orbiter Venus flyby.
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- 2021
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23. The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29
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Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, Asvestari, E., Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, and Asvestari, E.
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Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (≲1 AU) heliosphere. Relativistic electrons as well as protons with energies > 50 MeV were observed by Solar Orbiter (SolO), Parker Solar Probe, the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230° in longitude close to 1 AU. The particle onset delays observed at the different spacecraft are larger as the flare–footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO
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- 2021
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24. Early identification and optimal management of carbapenem-resistant Gram-negative infection
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Bedos, J. P., Daikos, G., Dodgson, A. R., Pan, A., Petrosillo, N., Seifert, H., Vila, J., Ferrer, R., Wilson, P., Bedos, J. P., Daikos, G., Dodgson, A. R., Pan, A., Petrosillo, N., Seifert, H., Vila, J., Ferrer, R., and Wilson, P.
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Background: Carbapenem resistance in Gram-negative bacteria is associated with severe infections in the hospital setting. No uniform screening policy or agreed set of criteria exists within the EU to inform treatment decisions for infections caused by carbapenemAim: To develop a range of consensus statements to survey experts in carbapenem resistance, to identify potential similarities and differences across the EU and across specialties. Methods: The survey contained 43 statements, covering six key topics relating to carbapenem-resistant organisms: microbiological screening; diagnosis; infection control implementation; antibiotic stewardship; use of resources; and influencing policy. Findings: In total, 136 survey responses were received (66% infectious disease specialists, 18% microbiologists, 11% intensive care specialists, 4% other/unknown) from France, Germany, Greece, Italy, Spain, and the UK. High, or very high, levels of agreement were seen for all 43 consensus statements, indicating good alignment concerning early identification and optimal management of infection due to carbapenem-resistant organisms. Conclusion: We offer the following recommendations: (1) screening is required when a patient may have been exposed to the healthcare system in countries/hospitals where carbapenem-resistant organisms are endemic; (2) rapid diagnostic tools should be available in every institution; (3) all institutions should have a specific policy for the control of carbapenem-resistant organisms, which is routinely audited; (4) clear strategies are required to define both appropriate and inappropriate use of carbapenems; (5) priority funding should be allocated to the management of infections due to carbapenem-resistant organisms; and (6) international co-operation is required to reduce country-to-country transmission of carbapenem-resistant organisms. (c) 2020 The Authors. Published by Elsevier Ltd on behalf of The Healthcare Infection Society. This is an open access articl
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- 2021
25. Vertebral osteomyelitis in patients with Staphylococcus aureus bloodstream infection: Evaluation of risk factors for treatment failure
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Jung, N., Ernst, A., Joost, I, Yagdiran, A., Peyerl-Hoffmann, G., Grau, S., Breuninger, M., Hellmich, M., Kubosch, D. C., Klingler, J. H., Seifert, H., Kern, W., V, Kaasch, A. J., Rieg, S., Jung, N., Ernst, A., Joost, I, Yagdiran, A., Peyerl-Hoffmann, G., Grau, S., Breuninger, M., Hellmich, M., Kubosch, D. C., Klingler, J. H., Seifert, H., Kern, W., V, Kaasch, A. J., and Rieg, S.
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Objectives: Staphylococcus aureus is the most common cause of pyogenic vertebral osteomyelitis (VO). Studies indicate that S. aureus VO results in poor outcome. We aimed to investigate risk factors for treatment failure in patients with Staphylococcus aureus bloodstream infection (SAB) and VO. Methods: We conducted a post hoc-analysis of data from a German bi-center prospective SAB cohort (2006-2014). Patients were followed-up for one year. Primary outcome was treatment failure defined as relapse and/or death within one year. Results: A total of 1069 patients with SAB were analyzed, with 92 VO patients. In addition to antibiotic treatment, surgery was performed in 60/92 patients. Treatment failed in 44/92 patients (death, n = 42; relapse, n = 2). Multivariable analysis revealed higher age (HR 1.04 [per year], 95%CI 1.01-1.07), Charlson comorbidity index (HR 1.20, 95%CI 1.06-1.36), presence of neurologic deficits (HR 2.53, 95%CI 1.15-5.53) and local abscess formation (HR 3.35, 95%CI 1.39-8.04) as independent risk factors for treatment failure. In contrast, surgery seemed to be associated with a favourable outcome (HR 0.45 (95%CI 0.20-0.997)). Conclusion: SAB patients with VO exhibit a high treatment failure rate. Red flags are older age, comorbidities, neurologic deficits and local abscess formation. Whether these patients benefit from intensified treatment (e.g. radical surgery, prolongation of antibiotics) should be investigated further. (C) 2021 The British Infection Association. Published by Elsevier Ltd. All rights reserved.
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- 2021
26. Outbreak of Pseudomonas aeruginosa infections after CT-guided spinal injections
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Paul, G., Meissner, A., Neuneier, J., Neuschmelting, V, Grau, S., Yagdiran, A., Scheyerer, M. J., Malin, J. J., Suarez, I, Lehmann, C., Exner, M., Wiesmuller, G. A., Higgins, P. G., Seifert, H., Fatkenheuer, G., Zweigner, J., Jung, N., Paul, G., Meissner, A., Neuneier, J., Neuschmelting, V, Grau, S., Yagdiran, A., Scheyerer, M. J., Malin, J. J., Suarez, I, Lehmann, C., Exner, M., Wiesmuller, G. A., Higgins, P. G., Seifert, H., Fatkenheuer, G., Zweigner, J., and Jung, N.
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Background: Meningitis and spinal infections with Gram-negative bacteria after local injections for treatment of chronic back pain are rare. This study investigated an outbreak of Pseudomonas aeruginosa infections following computed tomography (CT)-guided spinal injections (SI). Methods: A case was defined as a spinal infection or meningitis with P. aeruginosa after SI between 10th January and 1st March 2019 in the same outpatient clinic. Patients without microbiological evidence of P. aeruginosa but with a favourable response to antimicrobial therapy active against P. aeruginosa were defined as probable cases. Findings: Twenty-eight of 297 patients receiving CT-guided SI during the study period developed meningitis or spinal infections. Medical records were available for 19 patients. In 15 patients, there was microbiological evidence of P. aeruginosa, and four patients were defined as probable cases. Two of 19 patients developed meningitis, while the remaining 17 patients developed spinal infections. The median time from SI to hospital admission was 8 days (interquartile range 2-23 days). Patients mainly presented with back pain (N=18; 95%), and rarely developed fever (N=3; 16%). Most patients required surgery (N=16; 84%). Seven patients (37%) relapsed and one patient died. Although the source of infection was not identified microbiologically, documented failures in asepsis when performing SI probably contributed to these infections. Conclusions: SI is generally considered safe, but non-adherence to asepsis can lead to deleterious effects. Spinal infections caused by P. aeruginosa are difficult to treat and have a high relapse rate. (C) 2021 The Healthcare Infection Society. Published by Elsevier Ltd. All rights reserved.
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- 2021
27. Comparison of the Acinetobacter baumannii Reference Strains ATCC 17978 and ATCC 19606 in Antimicrobial Resistance Mediated by the AdeABC Efflux Pump
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Lucassen, K., Gerson, S., Xanthopoulou, K., Wille, J., Wille, T., Seifert, H., Higgins, P. G., Lucassen, K., Gerson, S., Xanthopoulou, K., Wille, J., Wille, T., Seifert, H., and Higgins, P. G.
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The Acinetobacter baumannii RND efflux pump AdeABC is regulated by the 2-component regulator AdeRS. In this study, we compared the regulation and expression of AdeABC of the reference strains ATCC 17978 and ATCC 19606. A clearly stronger efflux activity was demonstrated for ATCC 19606. An amino acid substitution at residue 172 of adeS was identified as a potential cause for differential expression of the pump. Therefore, we recommend caution with exclusively using single reference strains for research.
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- 2021
28. The Long Period of 3He-rich Solar Energetic Particles Measured by Solar Orbiter on 2020 November 17-23
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Bucik, R., Mason, G. M., Gomez-Herrero, R., Lario, D., Balmaceda, L., Nitta, N. V., Krupar, V., Dresing, N., Ho, G. C., Allen, R. C., Carcaboso, F., Rodriguez-Pacheco, J., Schuller, F., Warmuth, A., Wimmer-Schweingruber, R. F., von Forstner, J. L. Freiherr, Andrews, G. B., Berger, L., Cernuda, I., Lara, F. Espinosa, Lees, W. J., Martin, C., Pacheco, D., Prieto, M., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Tyagi, K., Maksimovic, M., Vecchio, A., Kollhoff, A., Kuhl, P., Xu, Z. G., Eldrum, S., Bucik, R., Mason, G. M., Gomez-Herrero, R., Lario, D., Balmaceda, L., Nitta, N. V., Krupar, V., Dresing, N., Ho, G. C., Allen, R. C., Carcaboso, F., Rodriguez-Pacheco, J., Schuller, F., Warmuth, A., Wimmer-Schweingruber, R. F., von Forstner, J. L. Freiherr, Andrews, G. B., Berger, L., Cernuda, I., Lara, F. Espinosa, Lees, W. J., Martin, C., Pacheco, D., Prieto, M., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Tyagi, K., Maksimovic, M., Vecchio, A., Kollhoff, A., Kuhl, P., Xu, Z. G., and Eldrum, S.
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We report observations of a relatively long period of 3He-rich solar energetic particles (SEPs) measured by Solar Orbiter. The period consists of several well-resolved ion injections. The high-resolution STEREO-A imaging observations reveal that the injections coincide with EUV jets/brightenings near the east limb, not far from the nominal magnetic connection of Solar Orbiter. The jets originated in two adjacent, large, and complex active regions as observed by the Solar Dynamics Observatory when the regions rotated to the Earth's view. It appears that the sustained ion injections were related to the complex configuration of the sunspot group and the long period of 3He-rich SEPs to the longitudinal extent covered by the group during the analyzed time period., Comment: accepted for publication in A&A, Letters to the Editor
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29. First year of energetic particle measurements in the inner heliosphere with Solar Orbiter's Energetic Particle Detector
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Wimmer-Schweingruber, R. F., Janitzek, N., Pacheco, D., Cernuda, I., Lara, F. Espinosa, Gómez-Herrero, R., Mason, G. M., Allen, R. C., Xu, Z. G., Carcaboso, F., Kollhoff, A., Kühl, P., von Forstner, J. L. Freiherr, Berger, L., Rodriguez-Pacheco, J., Ho, G. C., Andrews, G. B., Angelini, V., Aran, A., Boden, S., Böttcher, S. I., Carrasco, A., Dresing, N., Eldrum, S., Elftmann, R., Evans, V., Gevin, O., Hayes, J., Heber, B., Horbury, T. S., Kulkarni, S. R., Lario, D., Lees, W. J., Limousin, O., Malandraki, O., Martín, C., O'Brien, H., Mateo, M. Prieto, Ravanbakhsh, A., Polo, O. Rodriguez, Prieto, S. Sánchez, Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Vainio, R., Walsh, A., Yedla, M. K., Wimmer-Schweingruber, R. F., Janitzek, N., Pacheco, D., Cernuda, I., Lara, F. Espinosa, Gómez-Herrero, R., Mason, G. M., Allen, R. C., Xu, Z. G., Carcaboso, F., Kollhoff, A., Kühl, P., von Forstner, J. L. Freiherr, Berger, L., Rodriguez-Pacheco, J., Ho, G. C., Andrews, G. B., Angelini, V., Aran, A., Boden, S., Böttcher, S. I., Carrasco, A., Dresing, N., Eldrum, S., Elftmann, R., Evans, V., Gevin, O., Hayes, J., Heber, B., Horbury, T. S., Kulkarni, S. R., Lario, D., Lees, W. J., Limousin, O., Malandraki, O., Martín, C., O'Brien, H., Mateo, M. Prieto, Ravanbakhsh, A., Polo, O. Rodriguez, Prieto, S. Sánchez, Schlemm, C. E., Seifert, H., Terasa, J. C., Tyagi, K., Vainio, R., Walsh, A., and Yedla, M. K.
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Solar Orbiter strives to unveil how the Sun controls and shapes the heliosphere and fills it with energetic particle radiation. To this end, its Energetic Particle Detector (EPD) has now been in operation, providing excellent data, for just over a year. EPD measures suprathermal and energetic particles in the energy range from a few keV up to (near-) relativistic energies (few MeV for electrons and about 500 MeV/nuc for ions). We present an overview of the initial results from the first year of operations and we provide a first assessment of issues and limitations. During this first year of operations of the Solar Orbiter mission, EPD has recorded several particle events at distances between 0.5 and 1 au from the Sun. We present dynamic and time-averaged energy spectra for ions that were measured with a combination of all four EPD sensors, namely: the SupraThermal Electron and Proton sensor (STEP), the Electron Proton Telescope (EPT), the Suprathermal Ion Spectrograph (SIS), and the High-Energy Telescope (HET) as well as the associated energy spectra for electrons measured with STEP and EPT. We illustrate the capabilities of the EPD suite using the 10-11 December 2020 solar particle event. This event showed an enrichment of heavy ions as well as $^3$He, for which we also present dynamic spectra measured with SIS. The high anisotropy of electrons at the onset of the event and its temporal evolution is also shown using data from these sensors. We discuss the ongoing in-flight calibration and a few open instrumental issues using data from the 21 July and the 10-11 December 2020 events and give guidelines and examples for the usage of the EPD data. We explain how spacecraft operations may affect EPD data and we present a list of such time periods in the appendix. A list of the most significant particle enhancements as observed by EPT during this first year is also provided.
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- 2021
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30. Energetic ions in the Venusian system : Insights from the first Solar Orbiter flyby
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Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., Yedla, M., Allen, R. C., Cernuda, I, Pacheco, D., Berger, L., Xu, Z. G., von Forstner, J. L. Freiherr, Rodriguez-Pacheco, J., Wimmer-Schweingruber, R. F., Ho, G. C., Mason, G. M., Vines, S. K., Khotyaintsev, Yuri V., Horbury, T., Maksimovic, M., Hadid, L. Z., Volwerk, M., Dimmock, Andrew P., Sorriso-Valvo, Luca, Stergiopoulou, Katerina, Andrews, G. B., Angelini, V, Bale, S. D., Boden, S., Boettcher, S. , I, Chust, T., Eldrum, S., Espada, P. P., Lara, F. Espinosa, Evans, V, Gomez-Herrero, R., Hayes, J. R., Hellin, A. M., Kollhoff, A., Krasnoselskikh, V, Kretzschmar, M., Kuehl, P., Kulkarni, S. R., Lees, W. J., Lorfevre, E., Martin, C., O'Brien, H., Plettemeier, D., Polo, O. R., Prieto, M., Ravanbakhsh, A., Sanchez-Prieto, S., Schlemm, C. E., Seifert, H., Soucek, J., Steller, M., Stverak, S., Terasa, J. C., Travnicek, P., Tyagi, K., Vaivads, Andris, Vecchio, A., and Yedla, M.
- Abstract
The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the system and provide a characterization of galactic cosmic rays near the planet. Bursty suprathermal ion enhancements (up to similar to 10 keV) were observed as far as similar to 50R(V) downtail. These enhancements are likely related to a combination of acceleration mechanisms in regions of strong turbulence, current sheet crossings, and boundary layer crossings, with a possible instance of ion heating due to ion cyclotron waves within the Venusian tail. Upstream of the planet, suprathermal ions are observed that might be related to pick-up acceleration of photoionized exospheric populations as far as 5R(V) upstream in the solar wind as has been observed before by missions such as Pioneer Venus Orbiter and Venus Express. Near the closest approach of Solar Orbiter, the Galactic cosmic ray (GCR) count rate was observed to decrease by approximately 5 percent, which is consistent with the amount of sky obscured by the planet, suggesting a negligible abundance of GCR albedo particles at over 2 R-V. Along with modulation of the GCR population very close to Venus, the Solar Orbiter observations show that the Venusian system, even far from the planet, can be an effective accelerator of ions up to similar to 30 keV. This paper is part of a series of the first papers from the Solar Orbiter Venus flyby.
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- 2021
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31. The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29
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Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, Asvestari, E., Kollhoff, A., Kouloumvakos, A., Lario, D., Dresing, N., Gomez-Herrero, R., Rodriguez-Garcia, L., Malandraki, O. E., Richardson, I. G., Posner, A., Klein, K-L, Pacheco, D., Klassen, A., Heber, B., Cohen, C. M. S., Laitinen, T., Cernuda, I, Dalla, S., Lara, F. Espinosa, Vainio, R., Koeberle, M., Kuehl, R., Xu, Z. G., Berger, L., Eldrum, S., Bruedern, M., Laurenza, M., Kilpua, E. J., Aran, A., Rouillard, A. P., Bucik, R., Wijsen, N., Pomoell, J., Wimmer-Schweingruber, R. F., Martin, C., Boettcher, S. , I, von Forstner, J. L. Freiherr, Terasa, J-C, Boden, S., Kulkarni, S. R., Ravanbakhsh, A., Yedla, M., Janitzek, N., Rodriguez-Pacheco, J., Mateo, M. Prieto, Prieto, S. Sanchez, Espada, P. Parra, Polo, O. Rodriguez, Hellin, A. Martinez, Carcaboso, F., Mason, G. M., Ho, G. C., Allen, R. C., Andrews, G. Bruce, Schlemm, C. E., Seifert, H., Tyagi, K., Lees, W. J., Hayes, J., Bale, S. D., Krupar, V, Horbury, T. S., Angelini, V, Evans, V, O'Brien, H., Maksimovic, M., Khotyaintsev, Yuri V., Vecchio, A., Steinvall, Konrad, and Asvestari, E.
- Abstract
Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (≲1 AU) heliosphere. Relativistic electrons as well as protons with energies > 50 MeV were observed by Solar Orbiter (SolO), Parker Solar Probe, the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230° in longitude close to 1 AU. The particle onset delays observed at the different spacecraft are larger as the flare–footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO
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- 2021
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32. Microbiological diagnostics of bloodstream infections in Europe—an ESGBIES survey
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Idelevich, E.A. Seifert, H. Sundqvist, M. Scudeller, L. Amit, S. Balode, A. Bilozor, A. Drevinek, P. Kocak Tufan, Z. Koraqi, A. Lamy, B. Mareković, I. Miciuleviciene, J. Müller Premru, M. Pascual, A. Pournaras, S. Saegeman, V. Schønheyder, H.C. Schrenzel, J. Strateva, T. Tilley, R. Wiersinga, W.J. Zabicka, D. Carmeli, Y. Becker, K. ESCMID Study Group for Bloodstream Infections, Endocarditis Sepsis (ESGBIES) and Idelevich, E.A. Seifert, H. Sundqvist, M. Scudeller, L. Amit, S. Balode, A. Bilozor, A. Drevinek, P. Kocak Tufan, Z. Koraqi, A. Lamy, B. Mareković, I. Miciuleviciene, J. Müller Premru, M. Pascual, A. Pournaras, S. Saegeman, V. Schønheyder, H.C. Schrenzel, J. Strateva, T. Tilley, R. Wiersinga, W.J. Zabicka, D. Carmeli, Y. Becker, K. ESCMID Study Group for Bloodstream Infections, Endocarditis Sepsis (ESGBIES)
- Abstract
Objectives: High-quality diagnosis of bloodstream infections (BSI) is important for successful patient management. As knowledge on current practices of microbiological BSI diagnostics is limited, this project aimed to assess its current state in European microbiological laboratories. Methods: We performed an online questionnaire-based cross-sectional survey comprising 34 questions on practices of microbiological BSI diagnostics. The ESCMID Study Group for Bloodstream Infections, Endocarditis and Sepsis (ESGBIES) was the primary platform to engage national coordinators who recruited laboratories within their countries. Results: Responses were received from 209 laboratories in 25 European countries. Although 32.5% (68/209) of laboratories only used the classical processing of positive blood cultures (BC), two-thirds applied rapid technologies. Of laboratories that provided data, 42.2% (78/185) were able to start incubating BC in automated BC incubators around-the-clock, and only 13% (25/192) had established a 24-h service to start immediate processing of positive BC. Only 4.7% (9/190) of laboratories validated and transmitted the results of identification and antimicrobial susceptibility testing (AST) of BC pathogens to clinicians 24 h/day. Matrix-assisted laser desorption/ionization time-of-flight mass spectrometry from briefly incubated sub-cultures on solid media was the most commonly used approach to rapid pathogen identification from positive BC, and direct disc diffusion was the most common rapid AST method from positive BC. Conclusions: Laboratories have started to implement novel technologies for rapid identification and AST for positive BC. However, progress is severely compromised by limited operating hours such that current practice of BC diagnostics in Europe complies only partly with the requirements for optimal BSI management. © 2019 European Society of Clinical Microbiology and Infectious Diseases
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- 2019
33. Impact of single-room contact precautions on hospital-acquisition and transmission of multidrug-resistant Escherichia coli: a prospective multicentre cohort study in haematological and oncological wards
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Biehl, L. M., Higgins, P., Wille, T., Peter, K., Hamprecht, A., Peter, S., Doerfel, D., Vogel, W., Haefner, H., Lemmen, S., Panse, J., Rohde, H., Klupp, E. -M., Schafhausen, P., Imirzalioglu, C., Falgenhauer, L., Salmanton-Garcia, J., Stecher, M., Vehreschild, J. J., Seifert, H., Vehreschild, M. J. G. T., Biehl, L. M., Higgins, P., Wille, T., Peter, K., Hamprecht, A., Peter, S., Doerfel, D., Vogel, W., Haefner, H., Lemmen, S., Panse, J., Rohde, H., Klupp, E. -M., Schafhausen, P., Imirzalioglu, C., Falgenhauer, L., Salmanton-Garcia, J., Stecher, M., Vehreschild, J. J., Seifert, H., and Vehreschild, M. J. G. T.
- Abstract
Objectives: Colonization and infection with third-generation cephalosporin-resistant Escherichia coli (3GCR-EC) are frequent in haematological and oncological patients. In this high-risk setting, German guidelines recommend single-room contact precautions (SCP) for patients with 3GCR-EC that are non-susceptible to fluoroquinolones (F3GCR-EC). However, this recommendation is controversial, as evidence is limited. Methods: We performed a prospective, multicentre cohort study at four haematology and oncology departments assessing the impact of SCP on hospital-acquired colonization or bloodstream infection (BSI) with F3GCR-EC. Two sites performed SCP for F3GCR-EC patients including single rooms, gloves and gowns (SCP sites), and two did not (NCP sites). Active screening for 3GCR-EC was performed and isolates were characterized with molecular typing methods including whole genome sequencing and core genome multiple locus sequence typing to assess patient-to-patient transmission. Potential confounders were assessed by competing-risk regression analysis. Results: Within 12 months, 1386 patients at NCP sites and 1582 patients at SCP sites were included. Hospital-acquisition of F3GCR-EC was observed in 22/1386 (1.59%) and 16/1582 (1.01%) patients, respectively (p 0.191). There were 3/1386 (0.22%) patients with BSI caused by F3GCR-EC at NCP sites and 4/1582 (0.25%) at SCP sites (p 1.000). Patient-to-patient transmission occurred in three cases at NCP and SCP sites each (p 1.000). The number of patients needed to screen in order to prevent one patient-to-patient transmission of F3GCR-EC was determined to be 3729. Conclusions: Use of SCP had no significant impact on hospital-acquisition or patient-to-patient transmission of F3GCR-EC in this high-risk setting. (C) 2019 European Society of Clinical Microbiology and Infectious Diseases. Published by Elsevier Ltd. All rights reserved.
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- 2019
34. Microbiological diagnostics of bloodstream infections in Europe-an ESGBIES survey
- Author
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Idelevich, E. A., Seifert, H., Sundqvist, M., Scudeller, L., Amit, S., Balode, A., Bilozor, A., Drevinek, P., Tufan, Z. Kocak, Koraqi, A., Lamy, B., Marekovic, I., Miciuleviciene, J., Premru, M. Mueller, Pascual, A., Pournaras, S., Saegeman, V., Schonheyder, H. C., Schrenzel, J., Strateva, T., Tilley, R., Wiersinga, W. J., Zabicka, D., Carmeli, Y., Becker, K., Idelevich, E. A., Seifert, H., Sundqvist, M., Scudeller, L., Amit, S., Balode, A., Bilozor, A., Drevinek, P., Tufan, Z. Kocak, Koraqi, A., Lamy, B., Marekovic, I., Miciuleviciene, J., Premru, M. Mueller, Pascual, A., Pournaras, S., Saegeman, V., Schonheyder, H. C., Schrenzel, J., Strateva, T., Tilley, R., Wiersinga, W. J., Zabicka, D., Carmeli, Y., and Becker, K.
- Abstract
Objectives: High-quality diagnosis of bloodstream infections (BSI) is important for successful patient management. As knowledge on current practices of microbiological BSI diagnostics is limited, this project aimed to assess its current state in European microbiological laboratories. Methods: We performed an online questionnaire-based cross-sectional survey comprising 34 questions on practices of microbiological BSI diagnostics. The ESCMID Study Group for Bloodstream Infections, Endocarditis and Sepsis (ESGBIES) was the primary platform to engage national coordinators who recruited laboratories within their countries. Results: Responses were received from 209 laboratories in 25 European countries. Although 32.5% (68/209) of laboratories only used the classical processing of positive blood cultures (BC), two-thirds applied rapid technologies. Of laboratories that provided data, 42.2% (78/185) were able to start incubating BC in automated BC incubators around-the-clock, and only 13% (25/192) had established a 24-h service to start immediate processing of positive BC. Only 4.7% (9/190) of laboratories validated and transmitted the results of identification and antimicrobial susceptibility testing (AST) of BC pathogens to clinicians 24 h/day. Matrix-assisted laser desorption/ionization time-of-flight mass spectrometry from briefly incubated sub-cultures on solid media was the most commonly used approach to rapid pathogen identification from positive BC, and direct disc diffusion was the most common rapid AST method from positive BC. Conclusions: Laboratories have started to implement novel technologies for rapid identification and AST for positive BC. However, progress is severely compromised by limited operating hours such that current practice of BC diagnostics in Europe complies only partly with the requirements for optimal BSI management. (C) 2019 European Society of Clinical Microbiology and Infectious Diseases. Published by Elsevier Ltd. All rights reserved.
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- 2019
35. Impact of single-room contact precautions on hospital-acquisition and transmission of multidrug-resistant Escherichia coli: a prospective multicentre cohort study in haematological and oncological wards
- Author
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Biehl, L. M., Higgins, P., Wille, T., Peter, K., Hamprecht, A., Peter, S., Doerfel, D., Vogel, W., Haefner, H., Lemmen, S., Panse, J., Rohde, H., Klupp, E. -M., Schafhausen, P., Imirzalioglu, C., Falgenhauer, L., Salmanton-Garcia, J., Stecher, M., Vehreschild, J. J., Seifert, H., Vehreschild, M. J. G. T., Biehl, L. M., Higgins, P., Wille, T., Peter, K., Hamprecht, A., Peter, S., Doerfel, D., Vogel, W., Haefner, H., Lemmen, S., Panse, J., Rohde, H., Klupp, E. -M., Schafhausen, P., Imirzalioglu, C., Falgenhauer, L., Salmanton-Garcia, J., Stecher, M., Vehreschild, J. J., Seifert, H., and Vehreschild, M. J. G. T.
- Abstract
Objectives: Colonization and infection with third-generation cephalosporin-resistant Escherichia coli (3GCR-EC) are frequent in haematological and oncological patients. In this high-risk setting, German guidelines recommend single-room contact precautions (SCP) for patients with 3GCR-EC that are non-susceptible to fluoroquinolones (F3GCR-EC). However, this recommendation is controversial, as evidence is limited. Methods: We performed a prospective, multicentre cohort study at four haematology and oncology departments assessing the impact of SCP on hospital-acquired colonization or bloodstream infection (BSI) with F3GCR-EC. Two sites performed SCP for F3GCR-EC patients including single rooms, gloves and gowns (SCP sites), and two did not (NCP sites). Active screening for 3GCR-EC was performed and isolates were characterized with molecular typing methods including whole genome sequencing and core genome multiple locus sequence typing to assess patient-to-patient transmission. Potential confounders were assessed by competing-risk regression analysis. Results: Within 12 months, 1386 patients at NCP sites and 1582 patients at SCP sites were included. Hospital-acquisition of F3GCR-EC was observed in 22/1386 (1.59%) and 16/1582 (1.01%) patients, respectively (p 0.191). There were 3/1386 (0.22%) patients with BSI caused by F3GCR-EC at NCP sites and 4/1582 (0.25%) at SCP sites (p 1.000). Patient-to-patient transmission occurred in three cases at NCP and SCP sites each (p 1.000). The number of patients needed to screen in order to prevent one patient-to-patient transmission of F3GCR-EC was determined to be 3729. Conclusions: Use of SCP had no significant impact on hospital-acquisition or patient-to-patient transmission of F3GCR-EC in this high-risk setting. (C) 2019 European Society of Clinical Microbiology and Infectious Diseases. Published by Elsevier Ltd. All rights reserved.
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- 2019
36. Microbiological diagnostics of bloodstream infections in Europe-an ESGBIES survey
- Author
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Idelevich, E. A., Seifert, H., Sundqvist, M., Scudeller, L., Amit, S., Balode, A., Bilozor, A., Drevinek, P., Tufan, Z. Kocak, Koraqi, A., Lamy, B., Marekovic, I., Miciuleviciene, J., Premru, M. Mueller, Pascual, A., Pournaras, S., Saegeman, V., Schonheyder, H. C., Schrenzel, J., Strateva, T., Tilley, R., Wiersinga, W. J., Zabicka, D., Carmeli, Y., Becker, K., Idelevich, E. A., Seifert, H., Sundqvist, M., Scudeller, L., Amit, S., Balode, A., Bilozor, A., Drevinek, P., Tufan, Z. Kocak, Koraqi, A., Lamy, B., Marekovic, I., Miciuleviciene, J., Premru, M. Mueller, Pascual, A., Pournaras, S., Saegeman, V., Schonheyder, H. C., Schrenzel, J., Strateva, T., Tilley, R., Wiersinga, W. J., Zabicka, D., Carmeli, Y., and Becker, K.
- Abstract
Objectives: High-quality diagnosis of bloodstream infections (BSI) is important for successful patient management. As knowledge on current practices of microbiological BSI diagnostics is limited, this project aimed to assess its current state in European microbiological laboratories. Methods: We performed an online questionnaire-based cross-sectional survey comprising 34 questions on practices of microbiological BSI diagnostics. The ESCMID Study Group for Bloodstream Infections, Endocarditis and Sepsis (ESGBIES) was the primary platform to engage national coordinators who recruited laboratories within their countries. Results: Responses were received from 209 laboratories in 25 European countries. Although 32.5% (68/209) of laboratories only used the classical processing of positive blood cultures (BC), two-thirds applied rapid technologies. Of laboratories that provided data, 42.2% (78/185) were able to start incubating BC in automated BC incubators around-the-clock, and only 13% (25/192) had established a 24-h service to start immediate processing of positive BC. Only 4.7% (9/190) of laboratories validated and transmitted the results of identification and antimicrobial susceptibility testing (AST) of BC pathogens to clinicians 24 h/day. Matrix-assisted laser desorption/ionization time-of-flight mass spectrometry from briefly incubated sub-cultures on solid media was the most commonly used approach to rapid pathogen identification from positive BC, and direct disc diffusion was the most common rapid AST method from positive BC. Conclusions: Laboratories have started to implement novel technologies for rapid identification and AST for positive BC. However, progress is severely compromised by limited operating hours such that current practice of BC diagnostics in Europe complies only partly with the requirements for optimal BSI management. (C) 2019 European Society of Clinical Microbiology and Infectious Diseases. Published by Elsevier Ltd. All rights reserved.
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- 2019
37. Gonorrhoea
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Unemo, Magnus, Seifert, H. Steven, Hook, Edward W., Hawkes, Sarah, Ndowa, Francis, Dillon, Jo-Anne R., Unemo, Magnus, Seifert, H. Steven, Hook, Edward W., Hawkes, Sarah, Ndowa, Francis, and Dillon, Jo-Anne R.
- Abstract
The bacterium Neisseria gonorrhoeae causes the sexually transmitted infection (STI) gonorrhoea, which has an estimated global annual incidence of 86.9 million adults. Gonorrhoea can present as urethritis in men, cervicitis or urethritis in women, and in extragenital sites (pharynx, rectum, conjunctiva and, rarely, systemically) in both sexes. Confirmation of diagnosis requires microscopy of Gram-stained samples, bacterial culture or nucleic acid amplification tests. As no gonococcal vaccine is available, prevention relies on promoting safe sexual behaviours and reducing STI-associated stigma, which hinders timely diagnosis and treatment thereby increasing transmission. Single-dose systemic therapy (usually injectable ceftriaxone plus oral azithromycin) is the recommended first-line treatment. However, a major public health concern globally is that N. gonorrhoeae is evolving high levels of antimicrobial resistance (AMR), which threatens the effectiveness of the available gonorrhoea treatments. Improved global surveillance of the emergence, evolution, fitness, and geographical and temporal spread of AMR in N. gonorrhoeae, and improved understanding of the pharmacokinetics and pharmacodynamics for current and future antimicrobials in the treatment of urogenital and extragenital gonorrhoea, are essential to inform treatment guidelines. Key priorities for gonorrhoea control include strengthening prevention, early diagnosis, and treatment of patients and their partners; decreasing stigma; expanding surveillance of AMR and treatment failures; and promoting responsible antimicrobial use and stewardship. To achieve these goals, the development of rapid and affordable point-of-care diagnostic tests that can simultaneously detect AMR, novel therapeutic antimicrobials and gonococcal vaccine(s) in particular is crucial.
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- 2019
- Full Text
- View/download PDF
38. Microbiological diagnostics of bloodstream infections in Europe-an ESGBIES survey
- Author
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Idelevich, E. A., Seifert, H., Sundqvist, Martin, Scudeller, L., Amit, S., Balode, A., Bilozor, A., Drevinek, P., Tufan, Z. Kocak, Koraqi, A., Lamy, B., Marekovic, I., Miciuleviciene, J., Premru, M. Mueller, Pascual, A., Pournaras, S., Saegeman, V., Schønheyder, H. C., Schrenzel, J., Strateva, T., Tilley, R., Wiersinga, W. J., Zabicka, D., Carmeli, Y., Becker, K., Idelevich, E. A., Seifert, H., Sundqvist, Martin, Scudeller, L., Amit, S., Balode, A., Bilozor, A., Drevinek, P., Tufan, Z. Kocak, Koraqi, A., Lamy, B., Marekovic, I., Miciuleviciene, J., Premru, M. Mueller, Pascual, A., Pournaras, S., Saegeman, V., Schønheyder, H. C., Schrenzel, J., Strateva, T., Tilley, R., Wiersinga, W. J., Zabicka, D., Carmeli, Y., and Becker, K.
- Abstract
Objectives: High-quality diagnosis of bloodstream infections (BSI) is important for successful patient management. As knowledge on current practices of microbiological BSI diagnostics is limited, this project aimed to assess its current state in European microbiological laboratories. Methods: We performed an online questionnaire-based cross-sectional survey comprising 34 questions on practices of microbiological BSI diagnostics. The ESCMID Study Group for Bloodstream Infections, Endocarditis and Sepsis (ESGBIES) was the primary platform to engage national coordinators who recruited laboratories within their countries. Results: Responses were received from 209 laboratories in 25 European countries. Although 32.5% (68/209) of laboratories only used the classical processing of positive blood cultures (BC), two-thirds applied rapid technologies. Of laboratories that provided data, 42.2% (78/185) were able to start incubating BC in automated BC incubators around-the-clock, and only 13% (25/192) had established a 24-h service to start immediate processing of positive BC. Only 4.7% (9/190) of laboratories validated and transmitted the results of identification and antimicrobial susceptibility testing (AST) of BC pathogens to clinicians 24 h/day. Matrix-assisted laser desorption/ionization time-of-flight mass spectrometry from briefly incubated sub-cultures on solid media was the most commonly used approach to rapid pathogen identification from positive BC, and direct disc diffusion was the most common rapid AST method from positive BC. Conclusions: Laboratories have started to implement novel technologies for rapid identification and AST for positive BC. However, progress is severely compromised by limited operating hours such that current practice of BC diagnostics in Europe complies only partly with the requirements for optimal BSI management.
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- 2019
- Full Text
- View/download PDF
39. Minimally invasive and endoscopic versus open necrosectomy for necrotising pancreatitis: a pooled analysis of individual data for 1980 patients
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Brunschot, S. van, Hollemans, R.A., Bakker, O.J., Besselink, M.G.H., Baron, T.H., Beger, H.G., Boermeester, M.A., Bollen, T.L., Bruno, M.J., Carter, R., French, J.J., Coelho, D., Dahl, B., Dijkgraaf, M.G., Doctor, N., Fagenholz, P.J., Farkas, G., Castillo, C.F.D., Fockens, P., Freeman, M.L., Gardner, T.B., Goor, H. van, Gooszen, H.G., Hannink, G.J., Lochan, R., McKay, C.J., Neoptolemos, J.P., Olah, A., Parks, R.W., Peev, M.P., Raraty, M., Rau, B., Rosch, T., Rovers, M.M., Seifert, H., Siriwardena, A.K., Horvath, K.D., Santvoort, H.C. van, Brunschot, S. van, Hollemans, R.A., Bakker, O.J., Besselink, M.G.H., Baron, T.H., Beger, H.G., Boermeester, M.A., Bollen, T.L., Bruno, M.J., Carter, R., French, J.J., Coelho, D., Dahl, B., Dijkgraaf, M.G., Doctor, N., Fagenholz, P.J., Farkas, G., Castillo, C.F.D., Fockens, P., Freeman, M.L., Gardner, T.B., Goor, H. van, Gooszen, H.G., Hannink, G.J., Lochan, R., McKay, C.J., Neoptolemos, J.P., Olah, A., Parks, R.W., Peev, M.P., Raraty, M., Rau, B., Rosch, T., Rovers, M.M., Seifert, H., Siriwardena, A.K., Horvath, K.D., and Santvoort, H.C. van
- Abstract
Item does not contain fulltext, OBJECTIVE: Minimally invasive surgical necrosectomy and endoscopic necrosectomy, compared with open necrosectomy, might improve outcomes in necrotising pancreatitis, especially in critically ill patients. Evidence from large comparative studies is lacking. DESIGN: We combined original and newly collected data from 15 published and unpublished patient cohorts (51 hospitals; 8 countries) on pancreatic necrosectomy for necrotising pancreatitis. Death rates were compared in patients undergoing open necrosectomy versus minimally invasive surgical or endoscopic necrosectomy. To adjust for confounding and to study effect modification by clinical severity, we performed two types of analyses: logistic multivariable regression and propensity score matching with stratification according to predicted risk of death at baseline (low: <5%; intermediate: >/=5% to <15%; high: >/=15% to <35%; and very high: >/=35%). RESULTS: Among 1980 patients with necrotising pancreatitis, 1167 underwent open necrosectomy and 813 underwent minimally invasive surgical (n=467) or endoscopic (n=346) necrosectomy. There was a lower risk of death for minimally invasive surgical necrosectomy (OR, 0.53; 95% CI 0.34 to 0.84; p=0.006) and endoscopic necrosectomy (OR, 0.20; 95% CI 0.06 to 0.63; p=0.006). After propensity score matching with risk stratification, minimally invasive surgical necrosectomy remained associated with a lower risk of death than open necrosectomy in the very high-risk group (42/111 vs 59/111; risk ratio, 0.70; 95% CI 0.52 to 0.95; p=0.02). Endoscopic necrosectomy was associated with a lower risk of death than open necrosectomy in the high-risk group (3/40 vs 12/40; risk ratio, 0.27; 95% CI 0.08 to 0.88; p=0.03) and in the very high-risk group (12/57 vs 28/57; risk ratio, 0.43; 95% CI 0.24 to 0.77; p=0.005). CONCLUSION: In high-risk patients with necrotising pancreatitis, minimally invasive surgical and endoscopic necrosectomy are associated with reduced death rates compared with open
- Published
- 2018
40. Minimally invasive and endoscopic versus open necrosectomy for necrotising pancreatitis: A pooled analysis of individual data for 1980 patients
- Author
-
Brunschot, S. (Sandra) van, Hollemans, R.A. (Robbert A), Bakker, O.J. (Olaf ), Besselink, M.G. (Marc), Baron, T.H. (Todd H), Berger, M.Y. (Marjolein), Boermeester, M.A. (Marja), Bollen, T.L. (Thomas), Bruno, M.J. (Marco), Carter, R. (Ross), French, J.J. (Jeremy J), Coelho, D. (Djalma), Dahl, B. (Björn), Dijkgraaf, M.G.W. (Marcel), Doctor, N. (Nilesh), Fagenholz, P.J. (Peter J), Farkas, G. (Gyula), Castillo, C.F.D. (Carlos Fernandez Del), Fockens, P. (Paul), Freeman, M.L. (Martin L), Gardner, T.B. (Timothy B), Goor, H. (Harry) van, Gooszen, H.G. (Hein), Hannink, G. (Gerjon), Lochan, R. (Rajiv), McKay, C. (Colin), Neoptolemos, J.P. (John), Oláh, A. (Atilla), Parks, R.W. (Rowan W), Peev, M.P. (Miroslav P), Raraty, M. (Michael), Rau, B. (Bettina), Rösch, T. (Thomas), Rovers, M.M. (Maroeska), Seifert, H. (Hans), Siriwardena, A.K. (Ajith K), Horvath, K.D. (Karen), Santvoort, H.C. (Hjalmar) van, Brunschot, S. (Sandra) van, Hollemans, R.A. (Robbert A), Bakker, O.J. (Olaf ), Besselink, M.G. (Marc), Baron, T.H. (Todd H), Berger, M.Y. (Marjolein), Boermeester, M.A. (Marja), Bollen, T.L. (Thomas), Bruno, M.J. (Marco), Carter, R. (Ross), French, J.J. (Jeremy J), Coelho, D. (Djalma), Dahl, B. (Björn), Dijkgraaf, M.G.W. (Marcel), Doctor, N. (Nilesh), Fagenholz, P.J. (Peter J), Farkas, G. (Gyula), Castillo, C.F.D. (Carlos Fernandez Del), Fockens, P. (Paul), Freeman, M.L. (Martin L), Gardner, T.B. (Timothy B), Goor, H. (Harry) van, Gooszen, H.G. (Hein), Hannink, G. (Gerjon), Lochan, R. (Rajiv), McKay, C. (Colin), Neoptolemos, J.P. (John), Oláh, A. (Atilla), Parks, R.W. (Rowan W), Peev, M.P. (Miroslav P), Raraty, M. (Michael), Rau, B. (Bettina), Rösch, T. (Thomas), Rovers, M.M. (Maroeska), Seifert, H. (Hans), Siriwardena, A.K. (Ajith K), Horvath, K.D. (Karen), and Santvoort, H.C. (Hjalmar) van
- Abstract
Objective Minimally invasive surgical necrosectomy and endoscopic necrosectomy, compared with open necrosectomy, might improve outcomes in necrotising pancreatitis, especially in critically ill patients. Evidence from large comparative studies is lacking. Design We combined original and newly collected data from 15 published and unpublished patient cohorts (51 hospitals; 8 countries) on pancreatic necrosectomy for necrotising pancreatitis. Death rates were compared in patients undergoing open necrosectomy versus minimally invasive surgical or endoscopic necrosectomy. To adjust for confounding and to study effect modification by clinical severity, we performed two types of analyses: logistic multivariable regression and propensity score matching with stratification according to predicted risk of death at baseline (low: <5%; intermediate: ≥5% to <15%; high: ≥15% to <35%; and very high: ≥35%). Results Among 1980 patients with necrotising pancreatitis, 1167 underwent open necrosectomy and 813 underwent minimally invasive surgical (n=467) or endoscopic (n=346) necrosectomy. There was a lower risk of death for minimally invasive surgical necrosectomy (OR, 0.53; 95% CI 0.34 to 0.84; p=0.006) and endoscopic necrosectomy (OR, 0.20; 95% CI 0.06 to 0.63; p=0.006). After propensity score matching with risk stratification, minimally invasive surgical necrosectomy remained associated with a lower risk of death than open necrosectomy in the very high-risk group (42/111 vs 59/111; risk ratio, 0.70; 95% CI 0.52 to 0.95; p=0.02). Endoscopic necrosectomy was associated with a lower risk of death than open necrosectomy in the high-risk group (3/40 vs 12/40; risk ratio, 0.27; 95% CI 0.08 to 0.88; p=0.03) and in the very high-risk group (12/57 vs 28/57; risk ratio, 0.43; 95% CI 0.24 to 0.77; p=0.005). Conclusion In high-risk patients with necrotising pancreatitis, minimally invasive surgical and endoscopic necrosectomy are associated with reduced death rates compared with open necrosecto
- Published
- 2018
- Full Text
- View/download PDF
41. Epidemiology, Diagnosis and Treatment of Adult Patients with Nosocomial Pneumonia - Update 2017
- Author
-
Dalhoff, K., Abele-Horn, M., Andreas, S., Deja, M., Ewig, S., Gastmeier, P., Gatermann, S., Gerlach, H., Grabein, B., Heussel, C. P., Hoeffken, G., Kolditz, M., Kramme, E., Kuehl, H., Lange, C., Mayer, K., Nachtigall, I., Panning, M., Pletz, M., Rath, P-M., Rohde, G., Rosseau, S., Schaaf, B., Schreiter, D., Schuette, H., Seifert, H., Spies, C., Welte, T., Dalhoff, K., Abele-Horn, M., Andreas, S., Deja, M., Ewig, S., Gastmeier, P., Gatermann, S., Gerlach, H., Grabein, B., Heussel, C. P., Hoeffken, G., Kolditz, M., Kramme, E., Kuehl, H., Lange, C., Mayer, K., Nachtigall, I., Panning, M., Pletz, M., Rath, P-M., Rohde, G., Rosseau, S., Schaaf, B., Schreiter, D., Schuette, H., Seifert, H., Spies, C., and Welte, T.
- Abstract
Nosocomial pneumonia (HAP) is a frequent complication of hospital care. Most data are available on ventilator-associated pneumonia. However, infections on general wards are increasing. A central issue are infections with multidrug resistant (MDR) pathogens which are difficult to treat in the empirical setting potentially leading to inappropriate use of antimicrobial therapy. This guideline update was compiled by an interdisciplinary group on the basis of a systematic literature review. Recommendations are made according to GRADE giving guidance for the diagnosis and treatment of HAP on the basis of quality of evidence and benefit/risk ratio. This guideline has two parts. First an update on epidemiology, spectrum of pathogens and antimicrobials is provided. In the second part recommendations for the management of diagnosis and treatment are given. New recommendations with respect to imaging, diagnosis of nosocomial viral pneumonia and prolonged infusion of antibacterial drugs have been added. The statements to risk factors for infections with MDR pathogens and recommendations for monotherapy vs combination therapy have been actualised. The importance of structured deescalation concepts and limitation of treatment duration is emphasized.
- Published
- 2018
42. Evaluation of the Use of Rectal Swabs for Laboratory Diagnosis of Clostridium difficile Infection
- Author
-
Jazmati, N., Kirpal, E., Piepenbrock, E., Stelzer, Y., Vehreschild, M. J. G. T., Seifert, H., Jazmati, N., Kirpal, E., Piepenbrock, E., Stelzer, Y., Vehreschild, M. J. G. T., and Seifert, H.
- Abstract
For the diagnosis of Clostridium difficile infection (CDI), microbiological testing is almost always accomplished through the analysis of stool specimens. We evaluated the performances of rectal swabs with liquid transport medium (FS) and nylon flocked dry swabs for the detection of C. difficile. Additionally, the impact on the diagnostic yield of storing swabs at -80 degrees C for up to 3 months was evaluated. Sixty clinical stool samples positive for C. difficile by PCR were used for simulating rectal swabbing. FS and dry swabs were dipped into the stool and tested by PCR directly after swabbing at 1 and 3 months after storage at -80 degrees C. Stool and the liquid medium of FS were additionally tested by a combination of glutamate dehydrogenase antigen (GDH) testing and toxin A/B enzyme immunoassay (EIA), as well as by toxigenic culture (TC). Using dry swabs, the PCR-based detection rate of C. difficile was equal to the rate using stool samples (30/3. [100%]), whereas the detection rate in FS was significantly lower (25/30 [83.2%]; P = 0.019). The sensitivities of FS for detecting C. difficile by PCR, TC, GDH testing, and toxin A/B EIA were 83.3%, 85.7%, 88%, and 68.9%, respectively. Storage of swabs at -80 degrees C had no impact on the detection rate. FS cannot replace stool samples in the two-step laboratory diagnosis of CDI, as the sensitivities were too low, probably due to diluting effects of the fecal sample in the liquid medium. For simple PCR-based detection of C. difficile, dry swabs proved to be a suitable alternative to the use of stool samples.
- Published
- 2018
43. Minimally invasive and endoscopic versus open necrosectomy for necrotising pancreatitis: a pooled analysis of individual data for 1980 patients
- Author
-
Brunschot, S. van, Hollemans, R.A., Bakker, O.J., Besselink, M.G.H., Baron, T.H., Beger, H.G., Boermeester, M.A., Bollen, T.L., Bruno, M.J., Carter, R., French, J.J., Coelho, D., Dahl, B., Dijkgraaf, M.G., Doctor, N., Fagenholz, P.J., Farkas, G., Castillo, C.F.D., Fockens, P., Freeman, M.L., Gardner, T.B., Goor, H. van, Gooszen, H.G., Hannink, G.J., Lochan, R., McKay, C.J., Neoptolemos, J.P., Olah, A., Parks, R.W., Peev, M.P., Raraty, M., Rau, B., Rosch, T., Rovers, M.M., Seifert, H., Siriwardena, A.K., Horvath, K.D., Santvoort, H.C. van, Brunschot, S. van, Hollemans, R.A., Bakker, O.J., Besselink, M.G.H., Baron, T.H., Beger, H.G., Boermeester, M.A., Bollen, T.L., Bruno, M.J., Carter, R., French, J.J., Coelho, D., Dahl, B., Dijkgraaf, M.G., Doctor, N., Fagenholz, P.J., Farkas, G., Castillo, C.F.D., Fockens, P., Freeman, M.L., Gardner, T.B., Goor, H. van, Gooszen, H.G., Hannink, G.J., Lochan, R., McKay, C.J., Neoptolemos, J.P., Olah, A., Parks, R.W., Peev, M.P., Raraty, M., Rau, B., Rosch, T., Rovers, M.M., Seifert, H., Siriwardena, A.K., Horvath, K.D., and Santvoort, H.C. van
- Abstract
Item does not contain fulltext, OBJECTIVE: Minimally invasive surgical necrosectomy and endoscopic necrosectomy, compared with open necrosectomy, might improve outcomes in necrotising pancreatitis, especially in critically ill patients. Evidence from large comparative studies is lacking. DESIGN: We combined original and newly collected data from 15 published and unpublished patient cohorts (51 hospitals; 8 countries) on pancreatic necrosectomy for necrotising pancreatitis. Death rates were compared in patients undergoing open necrosectomy versus minimally invasive surgical or endoscopic necrosectomy. To adjust for confounding and to study effect modification by clinical severity, we performed two types of analyses: logistic multivariable regression and propensity score matching with stratification according to predicted risk of death at baseline (low: <5%; intermediate: >/=5% to <15%; high: >/=15% to <35%; and very high: >/=35%). RESULTS: Among 1980 patients with necrotising pancreatitis, 1167 underwent open necrosectomy and 813 underwent minimally invasive surgical (n=467) or endoscopic (n=346) necrosectomy. There was a lower risk of death for minimally invasive surgical necrosectomy (OR, 0.53; 95% CI 0.34 to 0.84; p=0.006) and endoscopic necrosectomy (OR, 0.20; 95% CI 0.06 to 0.63; p=0.006). After propensity score matching with risk stratification, minimally invasive surgical necrosectomy remained associated with a lower risk of death than open necrosectomy in the very high-risk group (42/111 vs 59/111; risk ratio, 0.70; 95% CI 0.52 to 0.95; p=0.02). Endoscopic necrosectomy was associated with a lower risk of death than open necrosectomy in the high-risk group (3/40 vs 12/40; risk ratio, 0.27; 95% CI 0.08 to 0.88; p=0.03) and in the very high-risk group (12/57 vs 28/57; risk ratio, 0.43; 95% CI 0.24 to 0.77; p=0.005). CONCLUSION: In high-risk patients with necrotising pancreatitis, minimally invasive surgical and endoscopic necrosectomy are associated with reduced death rates compared with open
- Published
- 2018
44. Minimally invasive and endoscopic versus open necrosectomy for necrotising pancreatitis: a pooled analysis of individual data for 1980 patients
- Author
-
Brunschot, S. van, Hollemans, R.A., Bakker, O.J., Besselink, M.G.H., Baron, T.H., Beger, H.G., Boermeester, M.A., Bollen, T.L., Bruno, M.J., Carter, R., French, J.J., Coelho, D., Dahl, B., Dijkgraaf, M.G., Doctor, N., Fagenholz, P.J., Farkas, G., Castillo, C.F.D., Fockens, P., Freeman, M.L., Gardner, T.B., Goor, H. van, Gooszen, H.G., Hannink, G.J., Lochan, R., McKay, C.J., Neoptolemos, J.P., Olah, A., Parks, R.W., Peev, M.P., Raraty, M., Rau, B., Rosch, T., Rovers, M.M., Seifert, H., Siriwardena, A.K., Horvath, K.D., Santvoort, H.C. van, Brunschot, S. van, Hollemans, R.A., Bakker, O.J., Besselink, M.G.H., Baron, T.H., Beger, H.G., Boermeester, M.A., Bollen, T.L., Bruno, M.J., Carter, R., French, J.J., Coelho, D., Dahl, B., Dijkgraaf, M.G., Doctor, N., Fagenholz, P.J., Farkas, G., Castillo, C.F.D., Fockens, P., Freeman, M.L., Gardner, T.B., Goor, H. van, Gooszen, H.G., Hannink, G.J., Lochan, R., McKay, C.J., Neoptolemos, J.P., Olah, A., Parks, R.W., Peev, M.P., Raraty, M., Rau, B., Rosch, T., Rovers, M.M., Seifert, H., Siriwardena, A.K., Horvath, K.D., and Santvoort, H.C. van
- Abstract
Item does not contain fulltext, OBJECTIVE: Minimally invasive surgical necrosectomy and endoscopic necrosectomy, compared with open necrosectomy, might improve outcomes in necrotising pancreatitis, especially in critically ill patients. Evidence from large comparative studies is lacking. DESIGN: We combined original and newly collected data from 15 published and unpublished patient cohorts (51 hospitals; 8 countries) on pancreatic necrosectomy for necrotising pancreatitis. Death rates were compared in patients undergoing open necrosectomy versus minimally invasive surgical or endoscopic necrosectomy. To adjust for confounding and to study effect modification by clinical severity, we performed two types of analyses: logistic multivariable regression and propensity score matching with stratification according to predicted risk of death at baseline (low: <5%; intermediate: >/=5% to <15%; high: >/=15% to <35%; and very high: >/=35%). RESULTS: Among 1980 patients with necrotising pancreatitis, 1167 underwent open necrosectomy and 813 underwent minimally invasive surgical (n=467) or endoscopic (n=346) necrosectomy. There was a lower risk of death for minimally invasive surgical necrosectomy (OR, 0.53; 95% CI 0.34 to 0.84; p=0.006) and endoscopic necrosectomy (OR, 0.20; 95% CI 0.06 to 0.63; p=0.006). After propensity score matching with risk stratification, minimally invasive surgical necrosectomy remained associated with a lower risk of death than open necrosectomy in the very high-risk group (42/111 vs 59/111; risk ratio, 0.70; 95% CI 0.52 to 0.95; p=0.02). Endoscopic necrosectomy was associated with a lower risk of death than open necrosectomy in the high-risk group (3/40 vs 12/40; risk ratio, 0.27; 95% CI 0.08 to 0.88; p=0.03) and in the very high-risk group (12/57 vs 28/57; risk ratio, 0.43; 95% CI 0.24 to 0.77; p=0.005). CONCLUSION: In high-risk patients with necrotising pancreatitis, minimally invasive surgical and endoscopic necrosectomy are associated with reduced death rates compared with open
- Published
- 2018
45. Epidemiology, Diagnosis and Treatment of Adult Patients with Nosocomial Pneumonia - Update 2017
- Author
-
Dalhoff, K., Abele-Horn, M., Andreas, S., Deja, M., Ewig, S., Gastmeier, P., Gatermann, S., Gerlach, H., Grabein, B., Heussel, C. P., Hoeffken, G., Kolditz, M., Kramme, E., Kuehl, H., Lange, C., Mayer, K., Nachtigall, I., Panning, M., Pletz, M., Rath, P-M., Rohde, G., Rosseau, S., Schaaf, B., Schreiter, D., Schuette, H., Seifert, H., Spies, C., Welte, T., Dalhoff, K., Abele-Horn, M., Andreas, S., Deja, M., Ewig, S., Gastmeier, P., Gatermann, S., Gerlach, H., Grabein, B., Heussel, C. P., Hoeffken, G., Kolditz, M., Kramme, E., Kuehl, H., Lange, C., Mayer, K., Nachtigall, I., Panning, M., Pletz, M., Rath, P-M., Rohde, G., Rosseau, S., Schaaf, B., Schreiter, D., Schuette, H., Seifert, H., Spies, C., and Welte, T.
- Abstract
Nosocomial pneumonia (HAP) is a frequent complication of hospital care. Most data are available on ventilator-associated pneumonia. However, infections on general wards are increasing. A central issue are infections with multidrug resistant (MDR) pathogens which are difficult to treat in the empirical setting potentially leading to inappropriate use of antimicrobial therapy. This guideline update was compiled by an interdisciplinary group on the basis of a systematic literature review. Recommendations are made according to GRADE giving guidance for the diagnosis and treatment of HAP on the basis of quality of evidence and benefit/risk ratio. This guideline has two parts. First an update on epidemiology, spectrum of pathogens and antimicrobials is provided. In the second part recommendations for the management of diagnosis and treatment are given. New recommendations with respect to imaging, diagnosis of nosocomial viral pneumonia and prolonged infusion of antibacterial drugs have been added. The statements to risk factors for infections with MDR pathogens and recommendations for monotherapy vs combination therapy have been actualised. The importance of structured deescalation concepts and limitation of treatment duration is emphasized.
- Published
- 2018
46. Evaluation of the Use of Rectal Swabs for Laboratory Diagnosis of Clostridium difficile Infection
- Author
-
Jazmati, N., Kirpal, E., Piepenbrock, E., Stelzer, Y., Vehreschild, M. J. G. T., Seifert, H., Jazmati, N., Kirpal, E., Piepenbrock, E., Stelzer, Y., Vehreschild, M. J. G. T., and Seifert, H.
- Abstract
For the diagnosis of Clostridium difficile infection (CDI), microbiological testing is almost always accomplished through the analysis of stool specimens. We evaluated the performances of rectal swabs with liquid transport medium (FS) and nylon flocked dry swabs for the detection of C. difficile. Additionally, the impact on the diagnostic yield of storing swabs at -80 degrees C for up to 3 months was evaluated. Sixty clinical stool samples positive for C. difficile by PCR were used for simulating rectal swabbing. FS and dry swabs were dipped into the stool and tested by PCR directly after swabbing at 1 and 3 months after storage at -80 degrees C. Stool and the liquid medium of FS were additionally tested by a combination of glutamate dehydrogenase antigen (GDH) testing and toxin A/B enzyme immunoassay (EIA), as well as by toxigenic culture (TC). Using dry swabs, the PCR-based detection rate of C. difficile was equal to the rate using stool samples (30/3. [100%]), whereas the detection rate in FS was significantly lower (25/30 [83.2%]; P = 0.019). The sensitivities of FS for detecting C. difficile by PCR, TC, GDH testing, and toxin A/B EIA were 83.3%, 85.7%, 88%, and 68.9%, respectively. Storage of swabs at -80 degrees C had no impact on the detection rate. FS cannot replace stool samples in the two-step laboratory diagnosis of CDI, as the sensitivities were too low, probably due to diluting effects of the fecal sample in the liquid medium. For simple PCR-based detection of C. difficile, dry swabs proved to be a suitable alternative to the use of stool samples.
- Published
- 2018
47. Minimally invasive and endoscopic versus open necrosectomy for necrotising pancreatitis: a pooled analysis of individual data for 1980 patients
- Author
-
van Brunschot, S, Hollemans, RA, Bakker, OJ, Besselink, MG, Baron, TH, Beger, HG, Boermeester, MA, Bollen, TL, Bruno, Marco, Carter, R, French, JJ, Coelho, D, Dahl, B, Dijkgraaf, MG, Doctor, N, Fagenholz, PJ, Farkas, G, del Castillo, CF, Fockens, P, Freeman, ML, Gardner, TB, van Goor, H, Gooszen, HG, Hannink, G, Lochan, R, McKay, CJ, Neoptolemos, JP, Olah, A, Parks, RW, Peev, MP, Raraty, M, Rau, B, Rosch, T, Rovers, M, Seifert, H, Siriwardena, AK, Horvath, KD, van Santvoort, HC, van Brunschot, S, Hollemans, RA, Bakker, OJ, Besselink, MG, Baron, TH, Beger, HG, Boermeester, MA, Bollen, TL, Bruno, Marco, Carter, R, French, JJ, Coelho, D, Dahl, B, Dijkgraaf, MG, Doctor, N, Fagenholz, PJ, Farkas, G, del Castillo, CF, Fockens, P, Freeman, ML, Gardner, TB, van Goor, H, Gooszen, HG, Hannink, G, Lochan, R, McKay, CJ, Neoptolemos, JP, Olah, A, Parks, RW, Peev, MP, Raraty, M, Rau, B, Rosch, T, Rovers, M, Seifert, H, Siriwardena, AK, Horvath, KD, and van Santvoort, HC
- Published
- 2018
48. Photoselektive Vaporisation der Prostata: Erfahrungen mit Prostataadenomen >80cm3
- Author
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Ruszat, R., Wyler, S., Seifert, H.-H, Reich, O., Forster, T., Stief, C., Sulser, T., Bachmann, A., Ruszat, R., Wyler, S., Seifert, H.-H, Reich, O., Forster, T., Stief, C., Sulser, T., and Bachmann, A.
- Abstract
Zusammenfassung: Hintergrund: Wir berichten über unsere Erfahrungen mit der photoselektiven Vaporisation der Prostata (PVP) bei Patienten mit symptomatischer benigner Prostatahyperplasie (BPH) und Prostataadenomen >80cm3. Patienten und Methode: 201Patienten mit BPH wurden in die Studie eingeschlossen; 51 (25,4%) Patienten hatten ein Prostatavolumen >80cm3 und 150 (74,6%) Patienten ein Volumen <80cm3 im transrektalen Ultraschall. Ergebnisse: Die mittlere Operationszeit bei Patienten mit großen Adenomen war akzeptabel (79min). Es wurden keine transfusionsbedürftigen Blutungen oder TUR-Syndrome beobachtet. Die maximale Harnflussrate verbesserte sich bei Patienten mit großen Adenomen um 135%, 136% und 132% nach 6, 12 und 24Monaten. Die Komplikationsrate war zwischen den beiden Gruppen vergleichbar. Schlussfolgerung: Die PVP ist durch eine hohe perioperative Sicherheit und signifikante Verbesserung der Miktionsverhältnisse gekennzeichnet. Für Patienten mit Prostatavolumina >80cm3 stellt die PVP eine durchführbare Therapieoption dar
- Published
- 2018
49. Die Greenlight-Laservaporisation der Prostata zur Therapie des benignen Prostatasyndroms: Entwicklung und Stellenwert
- Author
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Seifert, H.-H, Hermanns, T., Sulser, T., Seifert, H.-H, Hermanns, T., and Sulser, T.
- Abstract
Zusammenfassung: Die Greenlight-Laservaporisation hat in den letzten 10Jahren breiten Einsatz in der Therapie des benignen Prostatasyndroms (BPS) gefunden. Neben der Steigerung der Effektivität des Lasers durch eine Erhöhung der maximalen Leistung auf zunächst 80W und später 120W führten auch die guten Ergebnisse der klinischen Evaluationen zu einer zunehmenden Akzeptanz dieses Lasersystems. In der vorliegenden Arbeit werden wesentliche Ergebnisse der klinischen Evaluation der Technik aus den letzten Jahren dargelegt, an denen Schweizer Kliniken maßgeblich beteiligt waren. Hier sind v.a. die geringe peri- und postoperative Morbidität sowie die bisher guten kurz- und mittelfristigen funktionellen Ergebnisse zu nennen. Neben diesen Vorteilen, die v.a. in der nahezu blutungsfreien Durchführung des Eingriffs begründet liegen, werden jedoch ebenso die Nachteile und Limitationen der Laservaporisation beleuchtet, die möglicherweise auch spezifische klinische Nebenwirkungen zur Folge haben. Der zukünftige Stellenwert der Technik wird daher auch vor dem Hintergrund der noch ausstehenden Langzeitdaten weiter evaluiert werden müssen
- Published
- 2018
50. Right hemihepatectomy for bile duct injury following laparoscopic cholecystectomy
- Author
-
Heinrich, S., Seifert, H., Krähenbühl, L., Fellbaum, C., Lorenz, M., Heinrich, S., Seifert, H., Krähenbühl, L., Fellbaum, C., and Lorenz, M.
- Abstract
Laparoscopic cholecystectomy (LC) has become the treatment of choice for patients with symptomatic cholecystolithiasis. But with the introduction of this technique, the incidence of bile duct injuries has increased. We report the case of a 33-year-old man who was transferred from an affiliated hospital to our department for the treatment of a bile duct injury 2 weeks after LC. Prior to transfer, a laparotomy had been performed, with insertion of a T-tube and a Robinson drain on day 5 after LC. Endoscopic retrograde cholangiography (ERC) on admission day revealed an extensive defect of the right biliary system, which could not be treated endoscopically. An emergency laparotomy had to be performed at night for acute bleeding from the portal vein. Due to massive inflammation in the porta hepatis and intraparenchymal destruction of the right bile duct, liver resection was performed 2 days later, after the patient had stabilized in the intensive care unit (ICU). The patient had a prolonged postoperative course, but he finally recovered well from these operations. In conclusion, the management of bile duct injuries should include ultrasound to detect and drain fluid collections and ERC to classify the injury. Emergency laparotomy should never be performed without these examinations, since the majority of bile duct injuries can be treated endoscopically. Surgery for this serious complication should always be performed at specialized centers for hepatobiliary surgery
- Published
- 2018
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