357 results on '"Connolly, N."'
Search Results
2. Ketone body β-hydroxybutyrate (BHB) preserves mitochondrial bioenergetics
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Llorente-Folch, I., Düssmann, H., Watters, O., Connolly, N. M. C., and Prehn, Jochen H. M.
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- 2023
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3. INTRODUCTION
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Connolly, N. D. B., primary
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- 2022
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4. Precision Measurement of The Most Distant Spectroscopically Confirmed Supernova Ia with the Hubble Space Telescope
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Rubin, D., Knop, R. A., Rykoff, E., Aldering, G., Amanullah, R., Barbary, K., Burns, M. S., Conley, A., Connolly, N., Deustua, S., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gibbons, R. A., Goldhaber, G., Goobar, A., Hsiao, E. Y., Huang, X., Kowalski, M., Lidman, C., Meyers, J., Nordin, J., Perlmutter, S., Saunders, C., Spadafora, A. L., Stanishev, V., Suzuki, N., and Wang, L.
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Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
We report the discovery of a redshift 1.71 supernova in the GOODS North field. The Hubble Space Telescope (HST) ACS spectrum has almost negligible contamination from the host or neighboring galaxies. Although the rest frame sampled range is too blue to include any Si ii line, a principal component analysis allows us to confirm it as a Type Ia supernova with 92% confidence. A recent serendipitous archival HST WFC3 grism spectrum contributed a key element of the confirmation by giving a host-galaxy redshift of 1.713 +/- 0.007. In addition to being the most distant SN Ia with spectroscopic confirmation, this is the most distant Ia with a precision color measurement. We present the ACS WFC and NICMOS 2 photometry and ACS and WFC3 spectroscopy. Our derived supernova distance is in agreement with the prediction of LambdaCDM., Comment: 13 pages, 6 figures, published in ApJ with updated analysis
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- 2012
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5. The Hubble Space Telescope Cluster Supernova Survey: VI. The Volumetric Type Ia Supernova Rate
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Barbary, K., Aldering, G., Amanullah, R., Brodwin, M., Connolly, N., Dawson, K. S., Doi, M., Eisenhardt, P., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gilbank, D. G., Gladders, M. D., Goldhaber, G., Goobar, A., Hattori, T., Hsiao, E., Huang, X., Ihara, Y., Kashikawa, N., Koester, B., Konishi, K., Kowalski, M., Lidman, C., Lubin, L., Meyers, J., Morokuma, T., Oda, T., Panagia, N., Perlmutter, S., Postman, M., Ripoche, P., Rosati, P., Rubin, D., Schlegel, D. J., Spadafora, A. L., Stanford, S. A., Strovink, M., Suzuki, N., Takanashi, N., Tokita, K., and Yasuda, N.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present a measurement of the volumetric Type Ia supernova (SN Ia) rate out to z ~ 1.6 from the Hubble Space Telescope Cluster Supernova Survey. In observations spanning 189 orbits with the Advanced Camera for Surveys we discovered 29 SNe, of which approximately 20 are SNe Ia. Twelve of these SNe Ia are located in the foregrounds and backgrounds of the clusters targeted in the survey. Using these new data, we derive the volumetric SN Ia rate in four broad redshift bins, finding results consistent with previous measurements at z > 1 and strengthening the case for a SN Ia rate that is equal to or greater than ~0.6 x 10^-4/yr/Mpc^3 at z ~ 1 and flattening out at higher redshift. We provide SN candidates and efficiency calculations in a form that makes it easy to rebin and combine these results with other measurements for increased statistics. Finally, we compare the assumptions about host-galaxy dust extinction used in different high-redshift rate measurements, finding that different assumptions may induce significant systematic differences between measurements., Comment: 11 pages, 7 figures. Submitted to the Astrophysical Journal. Revised version following referee comments. See the HST Cluster SN Survey website at http://supernova.lbl.gov/2009ClusterSurvey for control time simulations in a machine-readable table and a complete listing of transient candidates from the survey
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- 2011
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6. The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
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Suzuki, N., Rubin, D., Lidman, C., Aldering, G., Amanullah, R., Barbary, K., Barrientos, L. F., Botyanszki, J., Brodwin, M., Connolly, N., Dawson, K. S., Dey, A., Doi, M., Donahue, M., Deustua, S., Eisenhardt, P., Ellingson, E., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gilbank, D. G., Gladders, M. D., Goldhaber, G., Gonzalez, A. H., Goobar, A., Gude, A., Hattori, T., Hoekstra, H., Hsiao, E., Huang, X., Ihara, Y., Jee, M. J., Johnston, D., Kashikawa, N., Koester, B., Konishi, K., Kowalski, M., Linder, E. V., Lubin, L., Melbourne, J., Meyers, J., Morokuma, T., Munshi, F., Mullis, C., Oda, T., Panagia, N., Perlmutter, S., Postman, M., Pritchard, T., Rhodes, J., Ripoche, P., Rosati, P., Schlegel, D. J., Spadafora, A., Stanford, S. A., Stanishev, V., Stern, D., Strovink, M., Takanashi, N., Tokita, K., Wagner, M., Wang, L., Yasuda, N., and Yee, H. K. C.
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Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
We present ACS, NICMOS, and Keck AO-assisted photometry of 20 Type Ia supernovae SNe Ia from the HST Cluster Supernova Survey. The SNe Ia were discovered over the redshift interval 0.623 < z < 1.415. Fourteen of these SNe Ia pass our strict selection cuts and are used in combination with the world's sample of SNe Ia to derive the best current constraints on dark energy. Ten of our new SNe Ia are beyond redshift $z=1$, thereby nearly doubling the statistical weight of HST-discovered SNe Ia beyond this redshift. Our detailed analysis corrects for the recently identified correlation between SN Ia luminosity and host galaxy mass and corrects the NICMOS zeropoint at the count rates appropriate for very distant SNe Ia. Adding these supernovae improves the best combined constraint on the dark energy density \rho_{DE}(z) at redshifts 1.0 < z < 1.6 by 18% (including systematic errors). For a LambdaCDM universe, we find \Omega_\Lambda = 0.724 +0.015/-0.016 (68% CL including systematic errors). For a flat wCDM model, we measure a constant dark energy equation-of-state parameter w = -0.985 +0.071/-0.077 (68% CL). Curvature is constrained to ~0.7% in the owCDM model and to ~2% in a model in which dark energy is allowed to vary with parameters w_0 and w_a. Tightening further the constraints on the time evolution of dark energy will require several improvements, including high-quality multi-passband photometry of a sample of several dozen z>1 SNe Ia. We describe how such a sample could be efficiently obtained by targeting cluster fields with WFC3 on HST., Comment: 27 pages, 11 figures. Submitted to ApJ. This first posting includes updates in response to comments from the referee. See http://www.supernova.lbl.gov for other papers in the series pertaining to the HST Cluster SN Survey. The updated supernova Union2.1 compilation of 580 SNe is available at http://supernova.lbl.gov/Union
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- 2011
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7. The Hubble Space Telescope Cluster Supernova Survey: II. The Type Ia Supernova Rate in High-Redshift Galaxy Clusters
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Barbary, K., Aldering, G., Amanullah, R., Brodwin, M., Connolly, N., Dawson, K. S., Doi, M., Eisenhardt, P., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gilbank, D. G., Gladders, M. D., Goldhaber, G., Goobar, A., Hattori, T., Hsiao, E., Huang, X., Ihara, Y., Kashikawa, N., Koester, B., Konishi, K., Kowalski, M., Lidman, C., Lubin, L., Meyers, J., Morokuma, T., Oda, T., Panagia, N., Perlmutter, S., Postman, M., Ripoche, P., Rosati, P., Rubin, D., Schlegel, D. J., Spadafora, A. L., Stanford, S. A., Strovink, M., Suzuki, N., Takanashi, N., Tokita, K., and Yasuda, N.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.45 from the Hubble Space Telescope (HST) Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe. Finding 8 +/- 1 cluster SNe Ia, we determine a SN Ia rate of 0.50 +0.23-0.19 (stat) +0.10-0.09 (sys) SNuB (SNuB = 10^-12 SNe L_{sun,B}^-1 yr^-1). In units of stellar mass, this translates to 0.36 +0.16-0.13 (stat) +0.07-0.06 (sys) SNuM (SNuM = 10^-12 SNe M_sun^-1 yr^-1). This represents a factor of approximately 5 +/- 2 increase over measurements of the cluster rate at z < 0.2. We parameterize the late-time SN Ia delay time distribution with a power law (proportional to t^s). Under the assumption of a cluster formation redshift of z_f = 3, our rate measurement in combination with lower-redshift cluster SN Ia rates constrains s = -1.41 +0.47/-0.40, consistent with measurements of the delay time distribution in the field. This measurement is generally consistent with expectations for the "double degenerate" scenario and inconsistent with some models for the "single degenerate" scenario predicting a steeper delay time distribution at large delay times. We check for environmental dependence and the influence of younger stellar populations by calculating the rate specifically in cluster red-sequence galaxies and in morphologically early-type galaxies, finding results similar to the full cluster rate. Finally, the upper limit of one host-less cluster SN Ia detected in the survey implies that the fraction of stars in the intra-cluster medium is less than 0.47 (95% confidence), consistent with measurements at lower redshifts., Comment: 29 pages, 14 figures. Accepted for publication in ApJ on 16 February 2011. See the HST Cluster Supernova Survey website at http://supernova.lbl.gov/2009ClusterSurvey for a version with full-resolution images and a complete listing of transient candidates from the survey. This version fixes a typo in the metadata; the paper is unchanged from v2
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- 2010
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8. The extraordinary mid-infrared spectral properties of FeLoBAL Quasars
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Farrah, D., Urrutia, T., Lacy, M., Lebouteiller, V., Spoon, H. W. W., Bernard-Salas, J., Connolly, N., Afonso, J., Connolly, B., and Houck, J.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We present mid-infrared spectra of six FeLoBAL QSOs at 1
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- 2010
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9. Reducing Zero-point Systematics in Dark Energy Supernova Experiments
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Faccioli, L., Kim, A. G., Miquel, R., Bernstein, G., Bonissent, A., Brown, M., Carithers, W., Christiansen, J., Connolly, N., Deustua, S., Gerdes, D., Gladney, L., Kushner, G., Linder, E. V., McKee, S., Mostek, N., Shukla, H., Stebbins, A., Stoughton, C., and Tucker, D.
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Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
We study the effect of filter zero-point uncertainties on future supernova dark energy missions. Fitting for calibration parameters using simultaneous analysis of all Type Ia supernova standard candles achieves a significant improvement over more traditional fit methods. This conclusion is robust under diverse experimental configurations (number of observed supernovae, maximum survey redshift, inclusion of additional systematics). This approach to supernova fitting considerably eases otherwise stringent mission calibration requirements. As an example we simulate a space-based mission based on the proposed JDEM satellite; however the method and conclusions are general and valid for any future supernova dark energy mission, ground or space-based., Comment: 30 pages,8 figures, 5 table, one reference added, submitted to Astroparticle Physics
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- 2010
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10. HST Discovery of a z = 3.9 Multiply Imaged Galaxy Behind the Complex Cluster Lens WARPS J1415.1+36 at z = 1.026
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Huang, X., Morokuma, T., Fakhouri, H. K., Aldering, G., Amanullah, R., Barbary, K., Brodwin, M., Connolly, N. V., Dawson, K. S., Doi, M., Faccioli, L., Fadeyev, V., Fruchter, A. S., Goldhaber, G., Gladders, M. D., Hennawi, J. F., Ihara, Y., Jee, M. J., Kowalski, M., Konishi, K., Lidman, C., Meyers, J., Moustakas, L. A., Perlmutter, S., Rubin, D., Schlegel, D. J., Spadafora, A. L., Suzuki, N., Takanashi, N., and Yasuda, N.
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Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We report the discovery of a multiply lensed Ly Alpha (Lya) emitter at z = 3.90 behind the massive galaxy cluster WARPS J1415.1+3612 at z = 1.026. Images taken by the Hubble Space Telescope(HST) using ACS reveal a complex lensing system that produces a prominent, highly magnified arc and a triplet of smaller arcs grouped tightly around a spectroscopically confirmed cluster member. Spectroscopic observations using FOCAS on Subaru confirm strong Lya emission in the source galaxy and provide redshifts for more than 21 cluster members, from which we obtain a velocity dispersion of 807+/-185 km/s. Assuming a singular isothermal sphere profile, the mass within the Einstein ring (7.13+/-0.38") corresponds to a central velocity dispersion of 686+15-19 km/s for the cluster, consistent with the value estimated from cluster member redshifts. Our mass profile estimate from combining strong lensing and dynamical analyses is in good agreement with both X-ray and weak lensing results., Comment: 5 pages, 2 figures, accepted by ApJL. See http://www.supernova.lbl.gov/ for additional information pertaining to the HST Cluster SN Survey. (This added URL is the only change in this version.)
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- 2009
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11. An Intensive HST Survey for z>1 Supernovae by Targeting Galaxy Clusters
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Dawson, K. S., Aldering, G., Amanullah, R., Barbary, K., Barrientos, L. F., Brodwin, M., Connolly, N., Dey, A., Doi, M., Donahue, M., Eisenhardt, P., Ellingson, E., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gilbank, D. G., Gladders, M. D., Goldhaber, G., Gonzalez, A. H., Goobar, A., Gude, A., Hattori, T., Hoekstra, H., Huang, X., Ihara, Y., Jannuzi, B. T., Johnston, D., Kashikawa, K., Koester, B., Konishi, K., Kowalski, M., Lidman, C., Linder, E. V., Lubin, L., Meyers, J., Morokuma, T., Munshi, F., Mullis, C., Oda, T., Panagia, N., Perlmutter, S., Postman, M., Pritchard, T., Rhodes, J., Rosati, P., Rubin, D., Schlegel, D. J., Spadafora, A., Stanford, S. A., Stanishev, V., Stern, D., Strovink, M., Suzuki, N., Takanashi, N., Tokita, K., Wagner, M., Wang, L., Yasuda, N., and Yee, H. K. C.
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Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST). By targeting massive galaxy clusters at 0.9
0.95, nine of which were in galaxy clusters. This strategy provides a SN sample that can be used to decouple the effects of host galaxy extinction and intrinsic color in high redshift SNe, thereby reducing one of the largest systematic uncertainties in SN cosmology., Comment: 15 pages, 8 figures, accepted by AJ, see http://www.supernova.lbl.gov for additional information pertaining to the HST Cluster SN Survey - Published
- 2009
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12. An Evolutionary Paradigm for Dusty Active Galaxies at Low Redshift
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Farrah, D., Connolly, B., Connolly, N., Spoon, H., Oliver, S., Prosper, H., Armus, L., Houck, J. R., Liddle, A. R., and Desai, V.
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Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
We apply methods from Bayesian inferencing and graph theory to a dataset of 102 mid-infrared spectra, and archival data from the optical to the millimeter, to construct an evolutionary paradigm for z<0.4 infrared-luminous galaxies (ULIRGs). We propose that the ULIRG lifecycle consists of three phases. The first phase lasts from the initial encounter until approximately coalescence. It is characterized by homogeneous mid-IR spectral shapes, and IR emission mainly from star formation, with a contribution from an AGN in some cases. At the end of this phase, a ULIRG enters one of two evolutionary paths depending on the dynamics of the merger, the available quantities of gas, and the masses of the black holes in the progenitors. On one branch, the contributions from the starburst and the AGN to the total IR luminosity decline and increase respectively. The IR spectral shapes are heterogeneous, likely due to feedback from AGN-driven winds. Some objects go through a brief QSO phase at the end. On the other branch, the decline of the starburst relative to the AGN is less pronounced, and few or no objects go through a QSO phase. We show that the 11.2 micron PAH feature is a remarkably good diagnostic of evolutionary phase, and identify six ULIRGs that may be archetypes of key stages in this lifecycle., Comment: ApJ accepted. Comments welcome. We suggest reading section 2 before looking at the figures. 26 pages, 21 figures, 1 table
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- 2009
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13. 30 Cardiovascular autonomic function assessed by heart rate recovery following active stand test in patients with severe aortic stenosis and response to aortic valve replacement
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Brandon, L, primary, Finucane, C, additional, Anne Kenny, R, additional, Connolly, N, additional, Maree, A, additional, Hensey, M, additional, O’Connor, S, additional, and Kerr, B, additional
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- 2023
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14. Discovery of an Unusual Optical Transient with the Hubble Space Telescope
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Barbary, K., Dawson, K. S., Tokita, K., Aldering, G., Amanullah, R., Connolly, N. V., Doi, M., Faccioli, L., Fadeyev, V., Fruchter, A. S., Goldhaber, G., Goobar, A., Gude, A., Huang, X., Ihara, Y., Konishi, K., Kowalski, M., Lidman, C., Meyers, J., Morokuma, T., Nugent, P., Perlmutter, S., Rubin, D., Schlegel, D., Spadafora, A. L., Suzuki, N., Swift, H. K., Takanashi, N., Thomas, R. C., and Yasuda, N.
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Astrophysics - Abstract
We present observations of SCP 06F6, an unusual optical transient discovered during the Hubble Space Telescope Cluster Supernova Survey. The transient brightened over a period of ~100 days, reached a peak magnitude of ~21.0 in both i_775 and z_850, and then declined over a similar timescale. There is no host galaxy or progenitor star detected at the location of the transient to a 3 sigma upper limit of i_775 = 26.4 and z_850 = 26.1, giving a corresponding lower limit on the flux increase of a factor of ~120. Multiple spectra show five broad absorption bands between 4100 AA and 6500 AA and a mostly featureless continuum longward of 6500 AA. The shape of the lightcurve is inconsistent with microlensing. The transient's spectrum, in addition to being inconsistent with all known supernova types, is not matched to any spectrum in the Sloan Digital Sky Survey (SDSS) database. We suggest that the transient may be one of a new class., Comment: 5 pages, 4 figures. Accepted for publication in ApJ. Data are available at http://supernova.lbl.gov/2006Transient/
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- 2008
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15. Looking Beyond Lambda with the Union Supernova Compilation
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Rubin, D., Linder, E. V., Kowalski, M., Aldering, G., Amanullah, R., Barbary, K., Connolly, N. V., Dawson, K. S., Faccioli, L., Fadeyev, V., Goldhaber, G., Goobar, A., Hook, I., Lidman, C., Meyers, J., Nobili, S., Nugent, P. E., Pain, R., Perlmutter, S., Ruiz-Lapuente, P., Spadafora, A. L., Strovink, M., Suzuki, N., and Swift, H.
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Astrophysics - Abstract
The recent robust and homogeneous analysis of the world's supernova distance-redshift data, together with cosmic microwave background and baryon acoustic oscillation data, provides a powerful tool for constraining cosmological models. Here we examine particular classes of scalar field, modified gravity, and phenomenological models to assess whether they are consistent with observations even when their behavior deviates from the cosmological constant Lambda. Some models have tension with the data, while others survive only by approaching the cosmological constant, and a couple are statistically favored over LCDM. Dark energy described by two equation of state parameters has considerable phase space to avoid Lambda and next generation data will be required to constrain such physics., Comment: 32 pages, 19 figures
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- 2008
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16. Improved Cosmological Constraints from New, Old and Combined Supernova Datasets
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Kowalski, M., Rubin, D., Aldering, G., Agostinho, R. J., Amadon, A., Amanullah, R., Balland, C., Barbary, K., Blanc, G., Challis, P. J., Conley, A., Connolly, N. V., Covarrubias, R., Dawson, K. S., Deustua, S. E., Ellis, R., Fabbro, S., Fadeyev, V., Fan, X., Farris, B., Folatelli, G., Frye, B. L., Garavini, G., Gates, E. L., Germany, L., Goldhaber, G., Goldman, B., Goobar, A., Groom, D. E., Haissinski, J., Hardin, D., Hook, I., Kent, S., Kim, A. G., Knop, R. A., Lidman, C., Linder, E. V., Mendez, J., Meyers, J., Miller, G. J., Moniez, M., Mourao, A. M., Newberg, H., Nobili, S., Nugent, P. E., Pain, R., Perdereau, O., Perlmutter, S., Phillips, M. M., Prasad, V., Quimby, R., Regnault, N., Rich, J., Rubenstein, E. P., Ruiz-Lapuente, P., Santos, F. D., Schaefer, B. E., Schommer, R. A., Smith, R. C., Soderberg, A. M., Spadafora, A. L., Strolger, L. -G., Strovink, M., Suntzeff, N. B., Suzuki, N., Thomas, R. C., Walton, N. A., Wang, L., Wood-Vasey, W. M., and Yun, J. L.
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Astrophysics - Abstract
We present a new compilation of Type Ia supernovae (SNe Ia), a new dataset of low-redshift nearby-Hubble-flow SNe and new analysis procedures to work with these heterogeneous compilations. This ``Union'' compilation of 414 SN Ia, which reduces to 307 SNe after selection cuts, includes the recent large samples of SNe Ia from the Supernova Legacy Survey and ESSENCE Survey, the older datasets, as well as the recently extended dataset of distant supernovae observed with HST. A single, consistent and blind analysis procedure is used for all the various SN Ia subsamples, and a new procedure is implemented that consistently weights the heterogeneous data sets and rejects outliers. We present the latest results from this Union compilation and discuss the cosmological constraints from this new compilation and its combination with other cosmological measurements (CMB and BAO). The constraint we obtain from supernovae on the dark energy density is $\Omega_\Lambda= 0.713^{+0.027}_{-0.029} (stat)}^{+0.036}_{-0.039} (sys)}$, for a flat, LCDM Universe. Assuming a constant equation of state parameter, $w$, the combined constraints from SNe, BAO and CMB give $w=-0.969^{+0.059}_{-0.063}(stat)^{+0.063}_{-0.066} (sys)$. While our results are consistent with a cosmological constant, we obtain only relatively weak constraints on a $w$ that varies with redshift. In particular, the current SN data do not yet significantly constrain $w$ at $z>1$. With the addition of our new nearby Hubble-flow SNe Ia, these resulting cosmological constraints are currently the tightest available., Comment: 49 pages, 17 figures; accepted for publication in Astrophysical Journal. For data tables, code for cosmological analysis and full-resolution figures, see http://supernova.lbl.gov/Union
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- 2008
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17. My Social Media Philosophy in (Roughly) One Thousand Words
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CONNOLLY, N. D. B., primary
- Published
- 2020
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18. A Black Power Method
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Connolly, N. D. B., primary
- Published
- 2019
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19. THE HUBBLE SPACE TELESCOPE**Based in part on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc., under the NASA contract NAS 5-26555. The observations are associated with program GO-10496. CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS
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Barbary, K, Aldering, G, Amanullah, R, Brodwin, M, Connolly, N, Dawson, KS, Doi, M, Eisenhardt, P, Faccioli, L, Fadeyev, V, Fakhouri, HK, Fruchter, AS, Gilbank, DG, Gladders, MD, Goldhaber, G, Goobar, A, Hattori, T, Hsiao, E, Huang, X, Ihara, Y, Kashikawa, N, Koester, B, Konishi, K, Kowalski, M, Lidman, C, Lubin, L, Meyers, J, Morokuma, T, Oda, T, Panagia, N, Perlmutter, S, Postman, M, Ripoche, P, Rosati, P, Rubin, D, Schlegel, DJ, Spadafora, AL, Stanford, SA, Strovink, M, Suzuki, N, Takanashi, N, Tokita, K, and Yasuda, and N
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Space Sciences ,Physical Sciences ,cosmology: observations ,supernovae: general ,white dwarfs ,astro-ph.CO ,Astronomical and Space Sciences ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Physical Chemistry (incl. Structural) ,Astronomy & Astrophysics ,Astronomical sciences ,Particle and high energy physics ,Space sciences - Abstract
We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.46 from the Hubble Space Telescope Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe. Finding 8 1 cluster SNeIa, we determine an SN Ia rate of 0.50+0.23-0.19 (stat) +0.10-0.09 (sys) h 270 SNuB (SNuB ≡ 10-12 SNe L -1, Byr-1). In units of stellar mass, this translates to 0.36+0.16-0.13 (stat) +0.07-0.06 (sys) h 270 SNuM (SNuM ≡ 10 -12 SNe M -1⊙yr-1). This represents a factor of 5 2 increase over measurements of the cluster rate at z < 0.2. We parameterize the late-time SN Ia delay time distribution (DTD) with a power law: Ψ(t)ts . Under the approximation of a single-burst cluster formation redshift of zf = 3, our rate measurement in combination with lower-redshift cluster SN Ia rates constrains s = -1.41 +0.47-0.40, consistent with measurements of the DTD in the field. This measurement is generally consistent with expectations for the "double degenerate" scenario and inconsistent with some models for the "single degenerate" scenario predicting a steeper DTD at large delay times. We check for environmental dependence and the influence of younger stellar populations by calculating the rate specifically in cluster red-sequence galaxies and in morphologically early-type galaxies, finding results similar to the full cluster rate. Finally, the upper limit of one hostless cluster SN Ia detected in the survey implies that the fraction of stars in the intra-cluster medium is less than 0.47 (95% confidence), consistent with measurements at lower redshifts. © 2012. The American Astronomical Society. All rights reserved..
- Published
- 2012
20. THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS
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Barbary, K, Aldering, G, Amanullah, R, Brodwin, M, Connolly, N, Dawson, KS, Doi, M, Eisenhardt, P, Faccioli, L, Fadeyev, V, Fakhouri, HK, Fruchter, AS, Gilbank, DG, Gladders, MD, Goldhaber, G, Goobar, A, Hattori, T, Hsiao, E, Huang, X, Ihara, Y, Kashikawa, N, Koester, B, Konishi, K, Kowalski, M, Lidman, C, Lubin, L, Meyers, J, Morokuma, T, Oda, T, Panagia, N, Perlmutter, S, Postman, M, Ripoche, P, Rosati, P, Rubin, D, Schlegel, DJ, Spadafora, AL, Stanford, SA, Strovink, M, Suzuki, N, Takanashi, N, Tokita, K, Yasuda, N, and Project, Supernova Cosmology
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cosmology: observations ,supernovae: general ,white dwarfs ,astro-ph.CO ,Astronomy & Astrophysics ,Astronomical and Space Sciences ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Physical Chemistry ,Atomic ,Molecular ,Nuclear ,Particle and Plasma Physics ,Physical Chemistry (incl. Structural) - Abstract
We report a measurement of the Type Ia supernova (SN Ia) rate in galaxyclusters at 0.9 < z < 1.45 from the Hubble Space Telescope (HST) ClusterSupernova Survey. This is the first cluster SN Ia rate measurement withdetected z > 0.9 SNe. Finding 8 +/- 1 cluster SNe Ia, we determine a SN Ia rateof 0.50 +0.23-0.19 (stat) +0.10-0.09 (sys) SNuB (SNuB = 10^-12 SNe L_{sun,B}^-1yr^-1). In units of stellar mass, this translates to 0.36 +0.16-0.13 (stat)+0.07-0.06 (sys) SNuM (SNuM = 10^-12 SNe M_sun^-1 yr^-1). This represents afactor of approximately 5 +/- 2 increase over measurements of the cluster rateat z < 0.2. We parameterize the late-time SN Ia delay time distribution with apower law (proportional to t^s). Under the assumption of a cluster formationredshift of z_f = 3, our rate measurement in combination with lower-redshiftcluster SN Ia rates constrains s = -1.41 +0.47/-0.40, consistent withmeasurements of the delay time distribution in the field. This measurement isgenerally consistent with expectations for the "double degenerate" scenario andinconsistent with some models for the "single degenerate" scenario predicting asteeper delay time distribution at large delay times. We check forenvironmental dependence and the influence of younger stellar populations bycalculating the rate specifically in cluster red-sequence galaxies and inmorphologically early-type galaxies, finding results similar to the fullcluster rate. Finally, the upper limit of one host-less cluster SN Ia detectedin the survey implies that the fraction of stars in the intra-cluster medium isless than 0.47 (95% confidence), consistent with measurements at lowerredshifts.
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- 2012
21. Effect of low dissolved oxygen on survival, emergence, and drift of tropical stream macroinvertebrates
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Connolly, N. M., Crossland, M. R., and Pearson, R. G.
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- 2004
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22. Roundtable: Defining the Black 1980s
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Allen, Jafari, primary, Connolly, N. D. B., additional, Fletcher, Bill, additional, Hinton, Elizabeth, additional, and Taylor, Keeanga-Yamahtta, additional
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- 2023
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23. Experimental mechanistic investigation of the nanostructuring of tungsten with low energy helium plasmas
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Fiflis, P., Connolly, N., and Ruzic, D.N.
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- 2016
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24. A World More Concrete: Real Estate and the Remaking of Jim Crow South Florida
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Connolly, N. D. B., author and Connolly, N. D. B.
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- 2014
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25. Mapping inequality
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Connolly, N. D. B., primary, Winling, LaDale, additional, Nelson, Robert K., additional, and Marciano, Richard, additional
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- 2018
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26. 7. Black Appointees, Political Legitimacy, and the American Presidency
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Connolly, N. D. B., primary
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- 2017
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27. 27 Fish in a barrel or sitting ducks? Preventive cardiology in the diabetic clinic; can proformas improve our shot?
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Connolly, N, primary, Kelly, R, additional, Bergin, P, additional, and Gholami, S, additional
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- 2022
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28. Fictional Characters and Characterisations
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Connolly, N.
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General Medicine - Abstract
Realists about fictional characters posit a certain theoretical role and a candidate to fill this role. I will delineate the role realists take fictional characters like Emma Woodhouse to fill, and I will argue that it is better filled by what I will call ‘characterisations’. In explaining what I mean by ‘characterisations’, I will show that the existence of these entities is comparatively uncontroversial. Realists should acknowledge their existence, but doing so, I will argue, obviates the need to acknowledge the existence of Emma and other fictional individuals.
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- 2022
29. The TWEAK receptor Fn14 is a potential cell surface portal for targeted delivery of glioblastoma therapeutics
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Perez, J G, Tran, N L, Rosenblum, M G, Schneider, C S, Connolly, N P, Kim, A J, Woodworth, G F, and Winkles, J A
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- 2016
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30. Reducing zero-point systematics in dark energy supernova experiments
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Faccioli, L., Kim, A.G., Miquel, R., Bernstein, G., Bonissent, A., Brown, M., Carithers, W., Christiansen, J., Connolly, N., Deustua, S., Gerdes, D., Gladney, L., Kushner, G., Linder, E.V., McKee, S., Mostek, N., Shukla, H., Stebbins, A., Stoughton, C., and Tucker, D.
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- 2011
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31. Colored, Caribbean, and Condemned: Miami's Overtown District and the Cultural Expense of Progress, 1940-1970
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Connolly, N. D. B.
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- 2006
32. Nutrient enrichment of a heterotrophic stream alters leaf litter nutritional quality and shredder physiological condition via the microbial pathway
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Connolly, N. M. and Pearson, R. G.
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- 2013
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33. Knocking on the Door
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Connolly, N. D. B., primary
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- 2014
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34. The Magic City
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Connolly, N. D. B., primary
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- 2014
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35. Pan-America
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Connolly, N. D. B., primary
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- 2014
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36. Bargaining and Hoping
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Connolly, N. D. B., primary
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- 2014
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37. A Little Insurance
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Connolly, N. D. B., primary
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- 2014
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38. Bulldozing Jim Crow
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Connolly, N. D. B., primary
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- 2014
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39. Conclusion The Tragic City
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Connolly, N. D. B., primary
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- 2014
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40. Suburban Renewal
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Connolly, N. D. B., primary
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- 2014
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41. Introduction America’s Playground
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Connolly, N. D. B., primary
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- 2014
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42. Elective cancer surgery in COVID-19–Free surgical pathways during the SARS-cov-2 pandemic: An international, multicenter, comparative cohort study
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James C Glasbey, Dmitri Nepogodiev, Joana Ff Simoes, Omar Omar, Elizabeth Li, Mary L Venn, Mohammad Abou Chaar, Vita Capizzi, Daoud Chaudhry, Anant Desai, Jonathan G Edwards, Jonathan P Evans, Marco Fiore, Jose Flavio Videria, Samuel J Ford, Ian Ganyli, Ewen A Griffiths, Rohan R Gujjuri, Angelos G Kolias, Haytham Ma Kaafarani, Ana Minaya-Bravo, Siobhan C McKay, Helen M Mohan, Keith Roberts, Carlos San Miguel-Méndez, Peter Pockney, Richard Shaw, Neil J Smart, Grant D Stewart, Sudha Sundar, Raghavan Vidya, Aneel A Bhangu, James C Glasbey, Omar Omar, Aneel A Bhangu, Kwabena Siaw-Acheampong, Ruth A Benson, Edward Bywater, Daoud Chaudhry, Brett E Dawson, Jonathan P Evans, James C Glasbey, Rohan R Gujjuri, Emily Heritage, Conor S Jones, Sivesh K Kamarajah, Chetan Khatri, Rachel A Khaw, James M Keatley, Andrew Knight, Samuel Lawday, Elizabeth Li, Harvinder S Mann, Ella J Marson, Kenneth A McLean, Siobhan C McKay, Emily C Mills, Dmitri Nepogodiev, Gianluca Pellino, Maria Picciochi, Elliott H Taylor, Abhinav Tiwari, Joana Ff Simoes, Isobel M Trout, Mary L Venn, Richard Jw Wilkin, Aneel A Bhangu, James C Glasbey, Neil J Smart, Ana Minaya-Bravo, Jonathan P Evans, Gaetano Gallo, Susan Moug, Francesco Pata, Peter Pockney, Salomone Di Saverio, Abigail Vallance, Dale Vimalchandran, Ewen A Griffiths, Sivesh K Kamarajah, Richard Pt Evans, Philip Townend, Keith Roberts, Siobhan McKay, John Isaac, Sohei Satoi, John Edwards, Aman S Coonar, Adrian Marchbank, Edward J Caruana, Georgia R Layton, Akshay Patel, Alessandro Brunelli, Samuel Ford, Anant Desai, Alessandro Gronchi, Marco Fiore, Max Almond, Fabio Tirotta, Sinziana Dumitra, Angelos Kolias, Stephen J Price, Daniel M Fountain, Michael D Jenkinson, Peter Hutchinson, Hani J Marcus, Rory J Piper, Laura Lippa, Franco Servadei, Ignatius Esene, Christian Freyschlag, Iuri Neville, Gail Rosseau, Karl Schaller, Andreas K Demetriades, Faith Robertson, Alex Alamri, Richard Shaw, Andrew G Schache, Stuart C Winter, Michael Ho, Paul Nankivell, Juan Rey Biel, Martin Batstone, Ian Ganly, Raghavan Vidya, Alex Wilkins, Jagdeep K Singh, Dinesh Thekinkattil, Sudha Sundar, Christina Fotopoulou, Elaine Leung, Tabassum Khan, Luis Chiva, Jalid Sehouli, Anna Fagotti, Paul Cohen, Murat Gutelkin, Rahel Ghebre, Thomas Konney, Rene Pareja, Rob Bristow, Sean Dowdy, T S Shylasree, R Kottayasamy Seenivasagam, Joe Ng, Keiiji Fujiwara, Grant D Stewart, Benjamin Lamb, Krishna Narahari, Alan McNeill, Alexandra Colquhoun, John McGrath, Steve Bromage, Ravi Barod, Veeru Kasivisvanathan, Tobias Klatte, Joana Ff Simoes, Tom Ef Abbott, Sadi Abukhalaf, Michel Adamina, Adesoji O Ademuyiwa, Arnav Agarwal, Murat Akkulak, Ehab Alameer, Derek Alderson, Felix Alakaloko, Markus Albertsmeiers, Osaid Alser, Muhammad Alshaar, Sattar Alshryda, Alexis P Arnaud, Knut Magne Augestad, Faris Ayasra, José Azevedo, Brittany K Bankhead-Kendall, Emma Barlow, David Beard, Ruth A Benson, Ruth Blanco-Colino, Amanpreet Brar, Ana Minaya-Bravo, Kerry A Breen, Chris Bretherton, Igor Lima Buarque, Joshua Burke, Edward J Caruana, Mohammad Chaar, Sohini Chakrabortee, Peter Christensen, Daniel Cox, Moises Cukier, Miguel F Cunha, Giana H Davidson, Anant Desai, Salomone Di Saverio, Thomas M Drake, John G Edwards, Muhammed Elhadi, Sameh Emile, Shebani Farik, Marco Fiore, J Edward Fitzgerald, Samuel Ford, Tatiana Garmanova, Gaetano Gallo, Dhruv Ghosh, Gustavo Mendonça Ataíde Gomes, Gustavo Grecinos, Ewen A Griffiths, Madalegna GrÜndl, Constantine Halkias, Ewen M Harrison, Intisar Hisham, Peter J Hutchinson, Shelley Hwang, Arda Isik, Michael D Jenkinson, Pascal Jonker, Haytham Ma Kaafarani, Debby Keller, Angelos Kolias, Schelto Kruijff, Ismail Lawani, Hans Lederhuber, Sezai Leventoglu, Andrey Litvin, Andrew Loehrer, Markus W Löffler, Maria Aguilera Lorena, Maria Marta Modolo, Piotr Major, Janet Martin, Hassan N Mashbari, Dennis Mazingi, Symeon Metallidis, Ana Minaya-Bravo, Helen M Mohan, Rachel Moore, David Moszkowicz, Susan Moug, Joshua S Ng-Kamstra, Mayaba Maimbo, Ionut Negoi, Milagros Niquen, Faustin Ntirenganya, Maricarmen Olivos, Kacimi Oussama, Oumaima Outani, Marie Dione Parreno-Sacdalanm, Francesco Pata, Carlos Jose Perez Rivera, Thomas D Pinkney, Willemijn van der Plas, Peter Pockney, Ahmad Qureshi, Dejan Radenkovic, Antonio Ramos-De la Medina, Keith Roberts, April C Roslani, Martin Rutegård, Juan José Segura-Sampedro, Irène Santos, Sohei Satoi, Raza Sayyed, Andrew Schache, Andreas A Schnitzbauer, Justina O Seyi-Olajide, Neil Sharma, Richard Shaw, Sebastian Shu, Kjetil Soreide, Antonino Spinelli, Grant D Stewart, Malin Sund, Sudha Sundar, Stephen Tabiri, Philip Townend, Georgios Tsoulfas, Gabrielle H van Ramshorst, Raghavan Vidya, Dale Vimalachandran, Oliver J Warren, Duane Wedderburn, Naomi Wright, C Allemand, L Boccalatte, M Figari, M Lamm, J Larrañaga, C Marchitelli, F Noll, D Odetto, M Perrotta, J Saadi, L Zamora, C Alurralde, E L Caram, D Eskinazi, J P Mendoza, M Usandivaras, R Badra, A Esteban, J S García, P M García, J I Gerchunoff, S M Lucchini, M A NIgra, L Vargas, T Hovhannisyan, A Stepanyan, T Gould, R Gourlay, B Griffiths, S Gananadha, M McLaren, J Cecire, N Joshi, S Salindera, A Sutherland, J H Ahn, G Charlton, S Chen, N Gauri, R Hayhurst, S Jang, F Jia, C Mulligan, W Yang, G Ye, H Zhang, M Ballal, D Gibson, D Hayne, J Moss, T Richards, P Viswambaram, U G Vo, J Bennetts, T Bright, M Brooke-Smith, R Fong, B Gricks, Y H Lam, B S Ong, M Szpytma, D Watson, K Bagraith, S Caird, E Chan, C Dawson, D Ho, E Jeyarajan, S Jordan, A Lim, G J Nolan, A Oar, D Parker, H Puhalla, A Quennell, L Rutherford, P Townend, M Von Papen, M Wullschleger, A Blatt, D Cope, N Egoroff, M Fenton, J Gani, N Lott, P Pockney, N Shugg, M Elliott, D Phung, D Phan, D Townend, C Bong, J Gundara, A Frankel, S Bowman, G R Guerra, J Bolt, K Buddingh, N N Dudi-Venkata, S Jog, H M Kroon, T Sammour, R Smith, C Stranz, M Batstone, K Lah, W McGahan, D Mitchell, A Morton, A Pearce, M Roberts, G Sheahan, B Swinson, N Alam, S Banting, L Chong, P Choong, S Clatworthy, D Foley, A Fox, M W Hii, B Knowles, J Mack, M Read, A Rowcroft, S Ward, G Wright, M Lanner, I Königsrainer, M Bauer, C Freyschlag, M Kafka, F Messner, D Öfner, I Tsibulak, K Emmanuel, M Grechenig, R Gruber, M Harald, L Öhlberger, J Presl, A Wimmer, I Namazov, E Samadov, D Barker, R Boyce, S Corbin, A Doyle, A Eastmond, R Gill, A Haynes, S Millar, M O'Shea, G Padmore, N Paquette, E Phillips, S St John, K Walkes, N Flamey, P Pattyn, W Oosterlinck, J Van den Eynde, R Van den Eynde, A Gatti, C Nardi, R Oliva, R De Cicco, I Cecconello, P Gregorio, L Pontual Lima, U Ribeiro Junior, F Takeda, R M Terra, M Sokolov, B Kidane, S Srinathan, M Boutros, N Caminsky, G Ghitulescu, G Jamjoum, J Moon, J Pelletier, T Vanounou, S Wong, M Boutros, S Dumitra, A Kouyoumdjian, B Johnston, C Russell, M Boutros, S Demyttenaere, R Garfinkle, J Abou-Khalil, C Nessim, J Stevenson, F Heredia, A Almeciga, A Fletcher, A Merchan, L O Puentes, J Mendoza Quevedo, G Bacic, D Karlovic, D Krsul, M Zelic, I Luksic, M Mamic, B Bakmaz, I Coza, E Dijan, Z Katusic, J Mihanovic, I Rakvin, K Frantzeskou, N Gouvas, G Kokkinos, P Papatheodorou, I Pozotou, O Stavrinidou, A Yiallourou, L Martinek, M Skrovina, I Szubota, J Žatecký, V Javurkova, J Klat, T Avlund, P Christensen, J L Harbjerg, L H Iversen, D W Kjaer, Hø Kristensen, M Mekhael, A L Ebbehøj, P Krarup, N Schlesinger, H Smith, A Abdelsamed, A Y Azzam, H Salem, A Seleim, A Abdelmajeed, M Abdou, N E Abosamak, M Al Sayed, F Ashoush, R Atta, E Elazzazy, M Elhoseiny, M Elnemr, M S Elqasabi, M E Elsayed Hewalla, I Elsherbini, E Essam, M Eweda, I Ghallab, E Hassan, M Ibrahim, M Metwalli, M Mourad, M S Qatora, M Ragab, A Sabry, H Saifeldin, M Saleh Mesbah Mohamed Elkaffas, A Samih, A Samir Abdelaal, S Shehata, K Shenit, D Attia, N Kamal, N Osman, A M Abbas, Has Abd Elazeem, M M Abdelkarem, S Alaa, A K Ali, A Ayman, M G Azizeldine, H Elkhayat, S M Elghazaly, F A Monib, M A Nageh, M M Saad, M Salah, M Shahine, E A Yousof, A Youssef, A Eldaly, M ElFiky, A Nabil, G Amira, I Sallam, M Sherief, A Sherif, A Abdelrahman, H Aboulkassem, G Ghaly, R Hamdy, A Morsi, H Salem, G Sherif, H Abdeldayem, I Abdelkader Salama, M Balabel, Y Fayed, A E Sherif, D Bekele, J Kauppila, E Sarjanoja, O Helminen, H Huhta, J H Kauppila, C Beyrne, L Jouffret, L Lugans, L Marie-Macron, E Chouillard, B De Simone, J Bettoni, S Dakpé, B Devauchelle, N Lavagen, S Testelin, S Boucher, R Breheret, A Gueutier, A Kahn, J KÜn-Darbois, A Barrabe, Z Lakkis, A Louvrier, S Manfredelli, P Mathieu, A Chebaro, V Drubay, M El Amrani, C Eveno, K Lecolle, G Legault, L Martin, G Piessen, F R Pruvot, S Truant, P Zerbib, Q Ballouhey, B Barrat, J Laloze, H Salle, A Taibi, J Usseglio, D Bergeat, A Merdrignac, Roy B Le, L O Perotto, A Scalabre, A Aimé, A Ezanno, B Malgras, P Bouche, S Tzedakis, E Cotte, O Glehen, V Kepenekian, J Lifante, G Passot, A D'Urso, E Felli, D Mutter, P Pessaux, B Seeliger, J Bardet, R Berry, G Boddaert, S Bonnet, E Brian, C Denet, D Fuks, D Gossot, M Grigoroiu, A Laforest, Y Levy-Zauberman, C Louis-Sylvestre, A Moumen, G Pourcher, A Seguin-Givelet, E Tribillon, E Duchalais, F Espitalier, C Ferron, O Malard, U Bork, M Distler, J Fritzmann, J Kirchberg, C Praetorius, C Riediger, J Weitz, T Welsch, P Wimberger, K Beyer, C Kamphues, J Lauscher, F N Loch, C Schineis, M Albertsmeier, M Angele, A Kappenberger, H Niess, T Schiergens, J Werner, R Becker, J Jonescheit, I Pergolini, D Reim, C Boeker, I Hakami, J Mall, P Liokatis, W Smolka, K Nowak, T Reinhard, F Hölzle, A Modabber, P Winnand, M Knitschke, P Kauffmann, S Wolfer, J Kleeff, K Lorenz, C Michalski, U Ronellenfitsch, R Schneider, E Bertolani, A Königsrainer, M W Löffler, M Quante, C Steidle, L ÜberrÜck, C Yurttas, C S Betz, J Bewarder, A Böttcher, S Burg, C Busch, M Gosau, A Heuer, J Izbicki, T O Klatte, D Koenig, N Moeckelmann, C Nitschke, M Priemel, R Smeets, U Speth, S Thole, F G Uzunoglu, T Vollkommer, N Zeller, M J Battista, K Gillen, A Hasenburg, S Krajnak, V Linz, R Schwab, K Angelou, D Haidopoulos, A Rodolakis, P Antonakis, K Bramis, L Chardalias, I Contis, N Dafnios, D Dellaportas, G Fragulidis, A Gklavas, M Konstadoulakis, N Memos, I Papaconstantinou, A Polydorou, T Theodosopoulos, A Vezakis, M I Antonopoulou, D K Manatakis, N Tasis, N Arkadopoulos, N Danias, P Economopoulou, P Kokoropoulos, A Larentzakis, N Michalopoulos, J Selmani, T Sidiropoulos, V Tsaousis, P Vassiliu, K Bouchagier, S Klimopoulos, D Paspaliari, G Stylianidis, K Baxevanidou, K Bouliaris, P Chatzikomnitsa, M Efthimiou, A Giaglaras, C Kalfountzos, G Koukoulis, A M Ntziovara, K Petropoulos, K Soulikia, I Tsiamalou, K Zervas, S Zourntou, I Baloyiannis, A Diamantis, E Gkrinia, J Hajiioannou, C Korais, O Koukoura, K Perivoliotis, A Saratziotis, C Skoulakis, D Symeonidis, K Tepetes, G Tzovaras, D Zacharoulis, V Alexoudi, K Antoniades, I Astreidis, P Christidis, D Deligiannidis, T Grivas, O Ioannidis, I Kalaitsidou, L Loutzidou, A Mantevas, D Michailidou, K Paraskevopoulos, S Politis, A Stavroglou, D Tatsis, I Tilaveridis, K Vahtsevanos, G Venetis, I Karaitianos, T Tsirlis, A Charalabopoulos, T Liakakos, E Mpaili, D Schizas, E Spartalis, A Syllaios, C Zografos, C Anthoulakis, C Christou, V Papadopoulos, A Tooulias, D Tsolakidis, G Tsoulfas, D Zouzoulas, E Athanasakis, E Chrysos, J Tsiaoussis, S Xenaki, E Xynos, K Futaba, M F Ho, S F Hon, Twc Mak, Ssm Ng, C C Foo, B Banky, N Suszták, M Aremu, A Canas-Martinez, O Cullivan, C Murphy, P Owens, L Pickett, L Akmenkalne, J Byrne, M Corrigan, C Cullinane, A Daly, C Fleming, P Jordan, S Killeen, N Lynch, A McCarthy, H Mustafa, S O'Brien, P O'Leary, Was Syed, L Vernon, D Callanan, L Huang, A Ionescu, P Sheahan, I Balasubramanian, M Boland, K Conlon, D Evoy, N Fearon, T Gallagher, J Geraghty, H Heneghan, N Kennedy, D Maguire, D McCartan, E W McDermott, R S Prichard, D Winter, D Alazawi, C Barry, T Boyle, W Butt, E M Connolly, N Donlon, C Donohue, B A Fahey, R Farrell, C Fitzgerald, J Kinsella, J O Larkin, P Lennon, P J Maguire, P Mccormick, B J Mehigan, H Mohan, T Nugent, H O'Sullivan, N Ravi, J V Reynolds, A Rogers, P Shokuhi, J Smith, L A Smith, C Timon, Y Bashir, G Bass, T Connelly, B Creavin, H Earley, J A Elliott, A Gillis, D Kavanagh, P Neary, J O'riordan, I S Reynolds, D Rice, P Ridgway, M Umair, M Whelan, P Carroll, C Collins, K Corless, L Finnegan, A Fowler, A Hogan, M Kerin, A Lowery, P McAnena, K McKevitt, K Nizami, É Ryan, A Samy, J C Coffey, R Cunningham, M Devine, D Nally, C Peirce, S Tormey, N Hardy, P Neary, S O'Malley, M Ryan, S Macina, N M Mariani, E Opocher, A Pisani Ceretti, F Ferrari, F Odicino, E Sartori, C Cotsoglou, S Granieri, F Bianco, A Camillo, M Colledan, S Tornese, M F Zambelli, G Bissolotti, S Fusetti, F Lemma, M V Marino, A Mirabella, G Vaccarella, C Agostini, G Alemanno, I Bartolini, C Bergamini, A Bruscino, C Checcucci, R De Vincenti, A Di Bella, M Fambrini, L Fortuna, G Maltinti, P Muiesan, F Petraglia, P Prosperi, M N Ringressi, M Risaliti, F Sorbi, A Taddei, R Tucci, C Bassi, L Bortolasi, T Campagnaro, L Casetti, M De Pastena, A Esposito, M Fontana, A Guglielmi, L Landoni, G Malleo, G Marchegiani, S Nobile, S Paiella, C Pedrazzani, S Rattizzato, A Ruzzenente, R Salvia, G Turri, M Tuveri, P Bellora, G D'Aloisio, M Ferrari, E Francone, S Gentilli, H Nikaj, M Bianchini, M Chiarugi, F Coccolini, G Di Franco, N Furbetta, D Gianardi, S Guadagni, L Morelli, M Palmeri, D Tartaglia, G Anania, P Carcoforo, M Chiozza, A De Troia, M Koleva Radica, M Portinari, M G Sibilla, A Urbani, N Fabbri, C V Feo, S Gennari, S Parini, E Righini, L Ampollini, L Bellanti, M Bergonzani, G Bertoli, G Bocchialini, G D'Angelo, D Lanfranco, L Musini, T Poli, G P Santoro, A Varazzani, L Aguzzoli, G Borgonovo, C Castro Ruiz, S Coiro, G Falco, V D Mandato, V Mastrofilippo, M T Montella, V Annessi, M Zizzo, U Grossi, S Novello, M Romano, S Rossi, G Zanus, G Esposito, F Frongia, A Pisanu, M Podda, C Belluco, A Lauretta, G Montori, L Moras, M Olivieri, F Bussu, A G Carta, M L 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McNaught, R Alam, A Budacan, J Cahill, M Kalkat, S Karandikar, L Kenyon, D Naumann, A Patel, J Ayorinde, T Chase, T Cuming, A Ghanbari, L Humphreys, S Tayeh, A Aboelkassem Ibrahim, R Bichoo, H Cao, Akw Chai, J Choudhury, C Evans, H Fitzjohn, H Ikram, M Langstroth, M Loubani, A McMillan, S Nazir, Ssa Qadri, A Robinson, E Ross, T Sehgal, A Wilkins, J Dixon, J Dunning, K Freystaetter, M Jha, S Lester, A Madhavan, S V Thulasiraman, Y Viswanath, T Curl-Roper, C Delimpalta, Ccl Liao, V Velchuru, E Westwood, E Belcher, G Bond-Smith, S Chidambaram, F Di Chiara, K Fasanmade, L Fraser, H Fu, M Ganau, S Gore, J Graystone, D Jeyaretna, H Khatkar, M Lami, M Maher, S Mastoridis, R Mihai, R Piper, S Prabhu, Obf Risk, U Selbong, K Shah, R Smillie, H Soleymani Majd, S Sravanam, D Stavroulias, G D Tebala, M Vatish, C Verberne, K Wallwork, S Winter, M I Bhatti, H Boyd-Carson, E Elsey, E Gemmill, P Herrod, M Jibreel, E Lenzi, T Saafan, D Sapre, T Sian, N Watson, A Athanasiou, G Bourke, L Bradshaw, A Brunelli, J Burke, P Coe, F Costigan, H Elkadi, M Ho, J Johnstone, A Kanatas, V Kantola, A Kaufmann, A Laios, S Lam, E MacInnes, S Munot, C Nahm, M Otify, C Pompili, I Smith, G Theophilou, G Toogood, R Wade, D Ward, C West, S Annamalai, C Ashmore, A Boddy, T Hossain, A Kourdouli, A Gvaramadze, A Jibril, L Prusty, D Thekkinkattil, A Harky, M Shackcloth, A Askari, C Chan, N Cirocchi, S Kudchadkar, K Patel, J Sagar, S Shaw, R Talwar, M Abdalla, R Edmondson, O Ismail, D Jones, K Newton, N Stylianides, A Aderombi, U Andaleeb, O Bajomo, K Beatson, W Garrett, M Mehmood, V Ng, R Al-Habsi, G S Divya, B Keeler, B Al-Sarireh, R Egan, R Harries, A Henry, M Kittur, Z Li, K Parkins, F Soliman, N Spencer, D Thompson, C Burgess, C Gemmell, C Grieco, M Hollyman, L Hunt, J Morrison, S Ojha, N Ryan, F Abbadessa, S Barnard, C Chan, N Dawe, J Hammond, Ali F Mahmoud, I McPherson, C Mellor, J Moir, S Pandanaboyana, J Powell, B Rai, A Rogers, C Roy, A Sachdeva, C Saleh, S Tingle, T Williams, J Manickavasagam, C McDonald, N McGrath, N McSorley, K Ragupathy, L Ramsay, A Solth, O Kakisi, K Seebah, I Shaikh, L Sreedharan, M Youssef, J Shah, P Ameerally, N McLarty, S Mills, A Shenfine, K Sahnan, J Abu, E Addae-Boateng, D Bratt, L Brock, N Burnside, S Cadwell-Sneath, K Gajjar, C Gan, C Grundy, K Hallam, K Hassell, M Hawari, A Joshi, H Khout, K Konstantinidi, Rxn Lee, D Nunns, R Schiemer, T Walton, H Weaver, L Whisker, K Williamson, J McVeigh, R Myatt, M A Williams, R Kaur, E Leung, S Sundar, M Michel, S Patil, S Ravindran, J Sarveswaran, L Scott, M Edmond, E King, M Almond, A Bhangu, O Breik, L D Cato, A Desai, S Ford, E Griffiths, M Idle, M Kamal, A Kisiel, R Kulkarni, Jkc Mak, T Martin, P Nankivell, A Parente, S Parmar, A M Pathanki, L Phelan, P Praveen, S Saeed, N Sharma, J Singh, F Tirotta, D Vijayan, A Geddes, J McCaul, J McMahon, A H Khan, F Khan, A Mansuri, S Mukherjee, M Patel, M Sarigul, S Singh, K L Tan, A Woodham, A Adiamah, H Brewer, A Chowdhury, J Evans, D Humes, J Jackman, A Koh, C 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J R Tan, A Thomas, P Whelan, A Anzak, A Banerjee, O Fuwa, F Hughes, J D Jayasinghe, C Knowles, H Kocher, I Leal Silva, F S Ledesma, A Minicozzi, L Navaratne, R Rahman, R Ramamoorthy, C Sohrabi, M Thaha, B Thakur, M Venn, V Yip, R Baumber, J Parry, S Evans, L Jeys, G Morris, M Parry, J Stevenson, N Ahmadi, G Aresu, Z M Barrett-Brown, A S Coonar, H Durio Yates, D Gearon, J Hogan, M King, A Peryt, I S Pradeep, C Smith, M Adishesh, R Atherton, K Baxter, M Brocklehurst, M Chaudhury, N Krishnamohan, J McAleer, G Owens, E Parkin, P Patkar, I Phang, A Aladeojebi, M Ali, B Barmayehvar, A Gaunt, M Gowda, E Halliday, M Kitchen, F Mansour, M Thomas, D Zakai, N Abbassi-Ghadi, H Assalaarachchi, A Currie, M Flavin, A Frampton, M Hague, C Hammer, J Hopper, J Horsnell, S Humphries, A Kamocka, T K Madhuri, S Preston, P Singh, J Stebbing, A Tailor, D Walker, F Aljanadi, M Jones, P Mhandu, C O'Donnell, R Turkington, Z Al-Ishaq, S Bhasin, A S Bodla, A Burahee, A Crichton, R Fossett, N Pigadas, S Pickford, E Rahman, D Snee, R Vidya, N Yassin, F Colombo, D Fountain, M T Hasan, K Karabatsou, R Laurente, O Pathmanaban, A Al-Mukhtar, S Brown, J Edwards, A Giblin, C Kelty, M Lee, G Lye, T Newman, A Sharkey, C Steele, N Sureshkumar Shah, E Whitehall, R Athwal, A Baker, L Jones, C Konstantinou, S Ramcharan, S Singh, J Vatish, R Wilkin, M Ethunandan, G K Sekhon, H Shields, R Singh, F Wensley, S Lawday, A Lyons, T Abbott, S Anwar, K Ghufoor, C Sohrabi, E Chung, R Hagger, A Hainsworth, A Karim, H Owen, A Ramwell, K Williams, C Baker, A Davies, J Gossage, M Kelly, W Knight, J Hall, G Harris, G James, C Kang, D J Lin, A D Rajgor, T Royle, R Scurrah, B Steel, L J Watson, D Choi, R Hutchison, A Jain, V Luoma, H Marcus, R May, A Menon, B Pramodana, L Webber, I A Aneke, P Asaad, B Brown, J Collis, S Duff, A Khan, F Moura, B Wadham, H Warburton, T Elmoslemany, M Jenkinson, C Millward, R Zakaria, S Mccluney, C Parmar, S Shah, J Allison, M S Babar, B Collard, S Goodrum, K Lau, A Patel, R Scott, E Thomas, H Whitmore, D Balasubramaniam, B Jayasankar, S Kapoor, A Ramachandran, A Elhamshary, Smb Imam, K Kapriniotis, V Kasivisvanathan, J Lindsay, S Rakhshani-Moghadam, N Beech, M Chand, L Green, N Kalavrezos, H Kiconco, R McEwen, C Schilling, D Sinha, J Pereca, J Singh, S Chopra, D Egbeare, R Thomas, T Combellack, Sef Jones, M Kornaszewska, M Mohammed, A Sharma, G Tahhan, V Valtzoglou, J Williams, P Eskander, K Gash, L Gourbault, M Hanna, T Maccabe, C Newton, J Olivier, S Rozwadowski, E Teh, D West, H Al-Omishy, M Baig, H Bates, G Di Taranto, K Dickson, N Dunne, C Gill, D Howe, D Jeevan, A Khajuria, K Martin-Ucar AMcEvoy, P Naredla, V Ng, S Robertson, M Sait, D R Sarma, S Shanbhag, T Shortland, S Simmonds, J Skillman, N Tewari, G Walton, M A Akhtar, A Brunt, J McIntyre, K Milne, M M Rashid, A Sgro, K E Stewart, A Turnbull, M Aguilar Gonzalez, S Talukder, C Boyle, D Fernando, K Gallagher, A Laird, D Tham, M Bath, P Patki, C Sohrabi, C Tanabalan, T Arif, C Magee, T Nambirajan, S Powell, R Vinayagam, I Flindall, A Hanson, V Mahendran, S Green, M Lim, L MacDonald, V Miu, L Onos, K Sheridan, R Young, F Alam, O Griffiths, C Houlden, R Jones, V S Kolli, A K Lala, S Leeson, R Peevor, Z Seymour, L Chen, E Henderson, A Loehrer, K Brown, D Fleming, A Haynes, C Heron, C Hill, H Kay, E Leede, K McElhinney, K Olson, E C Osterberg, C Riley, P Srikanth, M Thornhill, D Blazer, G DiLalla, E S Hwang, W Lee, M Lidsky, J Plichta, L Rosenberger, R Scheri, K Shah, K Turnage, J Visgauss, S Zani, J Farma, J Clark, D Kwon, E Etchill, H E Gabre-Kidan AJenny, A Kent, M Ladd, C Long, H Malapati, A Margalit, S Rapaport, J Rose, K Stevens, L Tsai, D Vervoort, P Yesantharao, A Dehal, D Klaristenfeld, K Huynh, L Brown, I Ganly, J Mullinax, N Gusani, J Hazelton, J Maines, J S Oh, A Ssentongo, P Ssentongo, M Azam, A Choudhry, W Marx, J Fleming, A Fuson, J Gigliotti, A Ovaitt, Y Ying, M K Abel, V Andaya, K Bigay, M A Boeck, L Chen, H Chern, C Corvera, I El-Sayed, A Glencer, P Ha, Bcs Hamilton, C Heaton, K Hirose, D M Jablons, K Kirkwood, L Z Kornblith, J R Kratz, R Lee, P N Miller, E Nakakura, B Nunez-Garcia, R O'Donnell, D Ozgediz, P Park, B Robinson, A Sarin, B Sheu, M Varma, K Wai, R Wustrack, M J Xu, D Beswick, J Goddard, J Manor, J Song, T Fullmer, C Gaskill, N Gross, K Kiong, C L Roland, S N Zafar, M Abdallah, A Abouassi, M Almasri, G Kulkarni, H Marwan, M Mehdi, S Aoun, V S Ban, H H Batjer, J Caruso, D Abbott, A Acher, T Aiken, J Barrett, E Foley, P Schwartz, S N Zafar, A Hawkins, A Maiga, J Laufer, S Scasso
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Aged, 80 and over ,Male ,Critical Care ,SARS-CoV-2 ,International Cooperation ,COVID-19 ,Middle Aged ,Cohort Studies ,Logistic Models ,Postoperative Complications ,Elective Surgical Procedures ,Neoplasms ,Outcome Assessment, Health Care ,Humans ,Female ,Epidemics ,Aged - Abstract
PURPOSE As cancer surgery restarts after the first COVID-19 wave, health care providers urgently require data to determine where elective surgery is best performed. This study aimed to determine whether COVID-19–free surgical pathways were associated with lower postoperative pulmonary complication rates compared with hospitals with no defined pathway. PATIENTS AND METHODS This international, multicenter cohort study included patients who underwent elective surgery for 10 solid cancer types without preoperative suspicion of SARS-CoV-2. Participating hospitals included patients from local emergence of SARS-CoV-2 until April 19, 2020. At the time of surgery, hospitals were defined as having a COVID-19–free surgical pathway (complete segregation of the operating theater, critical care, and inpatient ward areas) or no defined pathway (incomplete or no segregation, areas shared with patients with COVID-19). The primary outcome was 30-day postoperative pulmonary complications (pneumonia, acute respiratory distress syndrome, unexpected ventilation). RESULTS Of 9,171 patients from 447 hospitals in 55 countries, 2,481 were operated on in COVID-19–free surgical pathways. Patients who underwent surgery within COVID-19–free surgical pathways were younger with fewer comorbidities than those in hospitals with no defined pathway but with similar proportions of major surgery. After adjustment, pulmonary complication rates were lower with COVID-19–free surgical pathways (2.2% v 4.9%; adjusted odds ratio [aOR], 0.62; 95% CI, 0.44 to 0.86). This was consistent in sensitivity analyses for low-risk patients (American Society of Anesthesiologists grade 1/2), propensity score–matched models, and patients with negative SARS-CoV-2 preoperative tests. The postoperative SARS-CoV-2 infection rate was also lower in COVID-19–free surgical pathways (2.1% v 3.6%; aOR, 0.53; 95% CI, 0.36 to 0.76). CONCLUSION Within available resources, dedicated COVID-19–free surgical pathways should be established to provide safe elective cancer surgery during current and before future SARS-CoV-2 outbreaks.
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- 2021
43. Poster abstracts
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Ferrie, J., Shipley, M., Cappuccio, F., Brunner, E., Miller, M., Kumari, M., Marmot, M., Coenen, A., Castillo, J. L., Araya, F., Bustamante, G., Montecino, L., Torres, C., Oporto, S., Gronli, J., Fiske, E., Murison, R., Bjorvatn, B., Sorensen, E., Ursin, R., Portas, C. M., Rajaraman, S., Gribok, A., Wesensten, N., Balkin, T., Reifman, J., Dursunoglu, N., Ozkurt, S., Baser, S., Delen, O., Sarikaya, S., Sadler, P., Mitchell, P., Françon, D., Decobert, M., Herve, B., Richard, A., Griebel, G., Avenet, P., Scatton, B., Fur, G. L., Eckert, D., Jordan, A., Wellman, A., Smith, S., Malhotra, A., White, D., Bruck, D., Thomas, I., Kritikos, A., Oertel, W., Stiasny-Kolster, K., Garcia-Borreguero, D., Poewe, W., Hoegl, B., Kohnen, R., Schollmayer, E., Keffel, J., Trenkwalder, C., Valle, A., Roizenblatt, S., Fregni, F., Boggio, P., Tufik, S., Ward, K., Robertson, L., Palmer, L., Eastwood, P., Hillman, D., Lee, J., Mukherjee, S., de Padova, V., Barbato, G., Ficca, G., Zilli, I., Salzarulo, P., Veldi, M., Hion, T., Vasar, V., Kull, M., Nowak, L., Davis, J., Latzer, Y., Tzischinsky, O., Crowley, S., Carskadon, M., Anca-Herschkovitsch, M., Frey, D., Ortega, J., Wiseman, C., Farley, C., Wright, K., Campbell, A., Neill, A., Spiegel, K., Leproult, R., Tasali, E., Scherberg, N., van Cauter, E., Noradina, A. T., Karim, N. A., Norlinah, I., Raymond, A. A., Sahathevan, R., Hamidon, B., Werth, E., Poryazova, R., Khatami, R., Bassetti, C., Beran, R. 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F., Moisello, C., Bove, M., Busi, M., Pelosin, E., Tononi, G., Eguchi, N., Sakata, M., Urade, Y., Doe, N., Yoshihara, K., Abe, K., Manabe, Y., Iwatsuki, K., Hayashi, T., Shoji, M., Kamiya, T., Gooley, J., Brainard, G., Rajaratnam, S., Kronauer, R., Czeisler, C., Lockley, S., Phillips, A., Robinson, P., Burgess, H., Revell, V., Eastman, C., Bihari, S., Ramakrishnan, N., Camerino, D., Conway, P. M., Costa, G., Vandewalle, G., Albouy, G., Sterpenich, V., Darsaud, A., Rauchs, G., Berken, P.-Y, Balteau, E., Maquet, P., Tendero, J. A., Domenech, M. P., Isern, F. S., Martínez, C., Roure, N., Sancho, E. E., Moreno, C. R., Silva, M., Marqueze, E. C., Waage, S., Bobko, N., Chernyuk, V., Yavorskiy, Y., Saxvig, I., Sørensen, E., de Mello, M. T., Esteves, A., Teixeira, C., Bittencourt, L. R., Silva, R., Pires, M. 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Y. S., Cassaglia, P., Yu, V. Y. H., Walker, A. M., Kohler, M., Kennedy, D., Martin, J., van Den Heuvel, C., Lushington, K., Herron, K., Khurana, C., Sterr, A., Olivadoti, M., Toth, L., Opp, M., Dang-Vu, T., Degueldre, C., Gais, S., Dang-Vu, T. T., Desseilles, M., Philips, C., Chijavadze, E., Babilodze, M., Chkhartishvili, E., Nachkebia, N., Mchedlidze, O., Dzadzamia, S., Griffiths, R., Walker, A., Horovitz, S., Fukunaga, M., Carr, W., Picchioni, D., de Zwart, J., van Gelderen, P., Braun, A., Duyn, J., Hanlon, E. H., Faraguna, U., Vyazovskiy, V., Cirelli, C., Ocampo-Garcés, A., Ibáñez, F., López, S., Vivaldi, E., Torrealba, F., Romanowski, C. P. 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L., Nagai, R., do Rosário Dias De Oliveira Latorre, M., Marina, F., Paterson, J., Jackson, M., Johnston, P., Papafotiou, K., Croft, R., Dawson, S., Leenaars, C., Sandberg, H., Joosten, R., Dematteis, M., Feenstra, M., Wehrle, R., Rieger, M., Widmann, A., Dietl, T., Philipp, S., Wetter, T., Drummond, S., Czisch, M., Cairns, A., Lebourgeois, M., Harsh, J., Baulk, S., Vakulin, A., Catcheside, P., Antic, N., Mcevoy, D., Orff, H., Salamat, J., Meloy, M. 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- Published
- 2007
- Full Text
- View/download PDF
44. Making the Second Ghetto
- Author
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Hirsch, Arnold R., primary and Connolly, N. D. B., additional
- Published
- 2021
- Full Text
- View/download PDF
45. Jim Crow Liberalism
- Author
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Connolly, N. D. B., author
- Published
- 2014
- Full Text
- View/download PDF
46. Magnitude of the inflammatory response to cardiopulmonary bypass and its relation to adverse clinical outcomes
- Author
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Holmes IV, J. H., Connolly, N. C., Paull, D. L., Hill, M. E., Guyton, S. W., Ziegler, S. F., and Hall, R. A.
- Published
- 2002
- Full Text
- View/download PDF
47. Chapter 6. Sunbelt Civil Rights: Urban Renewal and the Follies of Desegregation in Greater Miami
- Author
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Connolly, N. D. B., primary
- Published
- 2011
- Full Text
- View/download PDF
48. Marine sar analysis and interpretation system — MARSAIS
- Author
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Johannessen, J. A., Garello, R., Chapron, B., Romeiser, R., Pavlakis, P., Robinson, I., Connolly, N., Nittis, K., Hamre, T., Ufermann, S., Alpers, W., Espedal, H., Furevik, B., Cummins, V., and Tarchi, D.
- Published
- 2001
- Full Text
- View/download PDF
49. White Sand, Black Beach: Civil Rights, Public Space, and Miami’s Virginia Key Bush Gregory W.
- Author
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Connolly, N. D. B.
- Published
- 2018
50. 55 Influenza vaccine uptake in a cardiology outpatient department setting; a missed cardiovascular disease prevention opportunity
- Author
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Connolly, N, primary
- Published
- 2020
- Full Text
- View/download PDF
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