35 results on '"M J Middleton"'
Search Results
2. NuSTAR reveals the hidden nature of SS433
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M J Middleton, D J Walton, W Alston, T Dauser, S Eikenberry, Y-F Jiang, A C Fabian, F Fuerst, M Brightman, H Marshall, M Parker, C Pinto, F A Harrison, M Bachetti, D Altamirano, A J Bird, G Perez, J Miller-Jones, P Charles, S Boggs, F Christensen, W Craig, K Forster, B Grefenstette, C Hailey, K Madsen, D Stern, and W Zhang
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- 2021
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3. A new transient ultraluminous X-ray source in NGC 7090
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D J Walton, M Heida, M Bachetti, F Fürst, M Brightman, H Earnshaw, P A Evans, A C Fabian, B W Grefenstette, F A Harrison, G L Israel, G B Lansbury, M J Middleton, S Pike, V Rana, T P Roberts, G A Rodriguez Castillo, R Salvaterra, X Song, and D Stern
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- 2020
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4. The unusual broad-band X-ray spectral variability of NGC 1313 X-1 seen with XMM–Newton, Chandra, and NuSTAR
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D J Walton, C Pinto, M Nowak, M Bachetti, R Sathyaprakash, E Kara, T P Roberts, R Soria, M Brightman, C R Canizares, H P Earnshaw, F Fürst, M Heida, M J Middleton, D Stern, L Tao, N Webb, W N Alston, D Barret, A C Fabian, F A Harrison, and P Kosec
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- 2020
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5. XMM–Newton campaign on ultraluminous X-ray source NGC 1313 X-1: wind versus state variability
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C Pinto, D J Walton, E Kara, M L Parker, R Soria, P Kosec, M J Middleton, W N Alston, A C Fabian, M Guainazzi, T P Roberts, F Fuerst, H P Earnshaw, R Sathyaprakash, and D Barret
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- 2020
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6. Long-term Pulse Period Evolution of the Ultra-luminous X-ray Pulsar NGC 7793 P13
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F. Fürst, D. J. Walton, M. Heida, M. Bachetti, C. Pinto, M. J. Middleton, M. Brightman, H. P. Earnshaw, D. Barret, A. C. Fabian, P. Kretschmar, K. Pottschmidt, A. Ptak, T. Roberts, D. Stern, N. Webb, and J. Wilms
- Subjects
Astronomy - Abstract
Ultra-luminous X-ray pulsars (ULXPs) provide a unique opportunity to study persistent super-Eddington accretion. Here we present the results of a long-term monitoring campaign of ULXP NGC 7793 P13, focusing on the pulse period evolution and the determination of the orbital ephemeris. Over our four year monitoring campaign with Swift, XMM-Newton, and NuSTAR, we measure a continuous spin-up with an average value of ̇P≈−3.8×10−11s s−1. We find that the strength of the spin-up is independent of the observed X-ray flux, indicating that despite a drop in observed flux in 2019, accretion onto the source has continued at largely similar rates. The source entered an apparent off-state in early 2020, which might have resulted in a change of the accretion geometry as no pulsations were found in observations in July/August 2020.We use the long-term monitoring to update the orbital ephemeris, as well as the periodicities seen in both the observed optical/UV and X-ray fluxes. We find that the optical/UV period is very stable over the years, with PUV=63.75+0.17−0.12d. The best-fit orbital period determined from our X-ray timing results is 64.86±0.19 d, almost a day longer than previously implied, and the X-ray flux period is65.21±0.15 d, slightly shorter than measured previously. The physical origin of these different flux periods is currently unknown. We study the hardness ratio of the XMM-Newton and NuSTAR data between 2013–2020 to search for indications of spectral changes. We find that the hardness ratios at high energies are very stable and not directly correlated with the observed flux. At lower energies we observe a small hardening with increased flux, which might indicate increased obscuration through outflows at higher luminosities. Comparing the changes in flux with the observed pulsed fraction, we find that the pulsed fraction is significantly higher at low fluxes. This seems to imply that the accretion geometry already changed before the source entered the deep off-state. We discuss possible scenarios to explain this behavior, which is likely driven by a precessing accretion disk.
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- 2021
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7. Thermal stability of winds driven by radiation pressure in super-Eddington accretion discs
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C Pinto, M Mehdipour, D J Walton, M J Middleton, T P Roberts, A C Fabian, M Guainazzi, R Soria, P Kosec, and J-U Ness
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- 2019
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8. The discovery of weak coherent pulsations in the ultraluminous X-ray source NGC 1313 X-2
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R Sathyaprakash, T P Roberts, D J Walton, F Fuerst, M Bachetti, C Pinto, W N Alston, H P Earnshaw, A C Fabian, M J Middleton, and R Soria
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- 2019
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9. Puzzling blue dips in the black hole candidate Swift J1357.2 − 0933, from ULTRACAM, SALT, ATCA, Swift, and NuSTAR
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J A Paice, P Gandhi, P A Charles, V S Dhillon, T R Marsh, D A H Buckley, M M Kotze, A Beri, D Altamirano, M J Middleton, R M Plotkin, J C A Miller-Jones, D M Russell, J Tomsick, W Díaz-Merced, and R Misra
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- 2019
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10. Discovery of a radio transient in M81
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G E Anderson, J C A Miller-Jones, M J Middleton, R Soria, D A Swartz, R Urquhart, N Hurley-Walker, P J Hancock, R P Fender, P Gandhi, S Markoff, and T P Roberts
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- 2019
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11. The black hole X-ray transient Swift J1357.2–0933 as seen with Swift and NuSTAR during its 2017 outburst
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Aru Beri, B E Tetarenko, A Bahramian, Diego Altamirano, Poshak Gandhi, G R Sivakoff, N Degenaar, M J Middleton, R Wijnands, J V Hernándz Santisteban, and John A Paice
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- 2019
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12. A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies
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H P Earnshaw, T P Roberts, M J Middleton, D J Walton, and S Mateos
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- 2018
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13. The remarkable X-ray variability of IRAS 13224–3809 – I. The variability process
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W N Alston, A C Fabian, D J K Buisson, E Kara, M L Parker, A M Lohfink, P Uttley, D R Wilkins, C Pinto, B De Marco, E M Cackett, M J Middleton, D J Walton, C S Reynolds, J Jiang, L C Gallo, A Zogbhi, G Miniutti, M Dovciak, and A J Young
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- 2018
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14. The ultraluminous X-ray source M81 X-6: a weakly magnetised neutron star with a precessing accretion disc?
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R. Amato, A. Gúrpide, N. A. Webb, O. Godet, M. J. Middleton, and HEP, INSPIRE
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High Energy Astrophysical Phenomena (astro-ph.HE) ,Space and Planetary Science ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph] - Abstract
We investigate the nature of the ULX M81 X-6, which has been suggested to harbour a neutron star (NS), by studying its long-term X-ray spectral and temporal evolution, using the rich set of available archival data from XMM-Newton, Chandra, NuSTAR, and Swift/XRT. We tracked the evolution of the source on the hardness-intensity diagram and find that the source oscillates between two main states: one characterised by a hard and luminous spectrum and the other at low hardness and luminosity. The properties of the soft component remain constant between the two states, suggesting that changes in the mass-transfer rate are not driving the spectral transitions. Instead, the bi-modal behaviour of the source and the known super-orbital period would point to the precession of the accretion disc. Here, we tested two theoretical models: (1) Lense-Thirring precession, which can explain the super-orbital period if the NS has a magnetic field $B$ $\lesssim10^{10}$ G, supporting the idea of M81 X-6 as a weakly magnetised NS, and (2) precession due to the torque of the NS magnetic field, which leads to $B \gtrsim$ 10$^{11}$ G. However, the latter scenario, assuming M81 X-6 shares similar properties with other NS-ULXs, is disfavoured because it would require magnetic field strengths ($B>10^{15}$ G) much higher than those known for other pulsating ULXs. We further show that the contribution from the hard component attributed to the putative accretion column sits just below the typical values found in pulsating ULXs, which, together with the low value of the pulsed fraction ($\leq10$\%) found for one XMM-Newton/pn observation, could explain the source's lack of pulsations. The spectral properties and variability of M81 X-6 can be accounted for if the accretor is a NS with a low magnetic field. Under the hypothesis of Lense-Thirring precession, we predict a spin period of the NS of a few seconds., 14 pages, 10 figures. Accepted for publication on Astronomy & Astrophysics
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- 2023
15. The X-ray disc/wind degeneracy in AGN
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M L Parker, G A Matzeu, J H Matthews, M J Middleton, T Dauser, J Jiang, and A M Joyce
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High Energy Astrophysical Phenomena (astro-ph.HE) ,Space and Planetary Science ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics::Galaxy Astrophysics - Abstract
Relativistic Fe K emission lines from accretion disks and from disk winds encode key information about black holes, and their accretion and feedback mechanisms. We show that these two processes can in principle produce indistinguishable line profiles, such that they cannot be disentangled spectrally. We argue that it is likely that in many cases both processes contribute to the net line profile, and their relative contributions cannot be constrained purely by Fe K spectroscopy. In almost all studies of Fe K emission to date, a single process (either disk reflection or wind Compton scattering) is assumed to dominate the total line profile. We demonstrate that fitting a single process emission model (pure reflection or pure wind) to a hybrid line profile results in large systematic biases in the estimates of key parameters, such as mass outflow rate and spin. We discuss various strategies to mitigate this effect, such as including high energy data covering the Compton hump, and the implications for future X-ray missions., Comment: 22 pages, 17 figures, accepted for publication in MNRAS
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- 2022
16. Factors Affecting the Involvement of Day Centre Care Staff in the Delivery of Physiotherapy to Adults with Intellectual Disabilities: An Exploratory Study in One London Borough
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M J Middleton and Sheila Kitchen
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medicine.medical_specialty ,business.industry ,Professional development ,Attendance ,Exploratory research ,Staffing ,Day centre care ,Social Welfare ,Education ,Nursing ,Borough ,Agency (sociology) ,Developmental and Educational Psychology ,Physical therapy ,medicine ,business - Abstract
Background Physiotherapists for adults with intellectual disabilities often work in day centres, relying on care staff to support programmes. This study investigates factors affecting physiotherapy delivery in 4 day centres in one London borough. Materials and Method Semi-structured interviews were carried out with day centre care staff, managers and physiotherapists. Results Service users’ needs were reported not to be met at three of the four centres. Barriers included low staffing levels, high absences and use of agency staff. Relevant variables included level of physiotherapist attendance, management priorities for care staff time, care staff confidence and whether a consistent team support delivery. Discrepancies emerged between staff and physiotherapists’ views on training needs. Conclusions Physiotherapy delivered in day centres is an important part of a complex care package. It requires effective multiagency working to meet the known – and potentially unidentified – needs of individuals and to ensure that care staff are adequately supported.
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- 2008
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17. High-speed CCD readout camera system
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M. J. Middleton, P. J. Phillips, A. W.K. Archibald, and Graham W. Smith
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Pixel ,Computer science ,business.industry ,Dynamic range ,Frame rate ,Photodiode ,law.invention ,law ,Computer data storage ,Computer vision ,Charge-coupled device ,Nyquist frequency ,Artificial intelligence ,business ,Image resolution - Abstract
A high resolution fast readout camera system has been dCVCIOPeJdarOWKI a specialised full frame 512 512 pixel format CCD sensor in conjunction with EEV Ltd. An eqwvalentreadoutrate of 600 frames per second with a spatial resolution of24 line pairs pet mm at the Nyquist limit is achieved. A binning capability increases the readout rate by up to a ftorof four. The system dynamic range is in excess of 1000 : 1.System features include image analysis by computer with dedicatedsoftware, non volatile memory ,highresolution andrealtime displays, instantly reset able, single shot image capture capability and remote head operation. 2 . INTRODUCTIONConvential CCD architectore has not been able to hieve fast readout with attendant high spatial resolution and highdynamic range.Thereare variants of hieving fast rea&rnt using solid state image technology with constraints on both of these parameters such as the Fairchild 222 1 CCD and Reticon photo diode arrays.Foilowing an in house technical wogram
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- 1994
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18. Impacts of flood mitigation works on coastal wetlands in New South Wales
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M J Middleton and R L Pressey
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geography.geographical_feature_category ,Floodplain ,Ecology ,business.industry ,Flooding (psychology) ,Wetland ,Urban economics ,Geography ,Habitat ,Urban planning ,Agriculture ,Flood mitigation ,business ,Environmental planning - Abstract
Agricultural and urban development of the coastal floodplains of New South Wales has involved major changes in the extent of natural habitats and in the decline of the state’s coastal wetlands – the programme of structural flood mitigation works in all major river systems. The stated aims of these works are to reduce the frequency of flooding in low-lying control areas, to facilitate removal of floodwaters after floods and to control flooding which cannot be prevented (NSW Department of Public Works, 1973). In practice, the pursuit of these aims has led to the elimination of reduction in value of much freshwater and estuarine wetland. While the benefits of flood mitigation to agricultural and urban economics have been significant and well documented (eg/ Macleay River County Council et al., 1963; Executive Committee for Councils, 1968) assessment of the adverse effects, particularly environmental impacts, has been limited (McGregor, 1979; Middleton et al., in press). Of the recent studies which have considered environmental aspects of specific proposals, few have included a systematic analysis of major potential impacts. Fewer still have generated new background information on the areas concerned and the authors know of no study which has considered all flora and fauna potentially affected. Notably, this general lack of environmental research applies to the recent series of floodplain management studies on major river systems in coastal New South Wales, few of which analysed the specific impacts of existing or proposed works.
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- 2009
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19. Structural flood mitigation works and estuarine management in New South Wales—Case study of the Macleay River
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R. J. Williams, M. A. Rimmer, and M. J. Middleton
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Government ,business.industry ,Environmental resource management ,Wildlife ,Legislation ,Geography ,Habitat ,Agriculture ,General Earth and Planetary Sciences ,Environmental Chemistry ,Flood mitigation ,business ,Recreation ,Amateur ,General Environmental Science - Abstract
In many estuaries of New South Wales (N.S.W.), agricultural, urban, and industrial activities have benefited at the expense of naturally occurring attributes such as commercial and amateur fisheries, wildlife habitats, recreational resources, and esthetic and cultural values. The successful future management of the estuarine environment is contingent on a number of factors, including a paucity of baseline data, a lack of predictive models, the difficulty of quantifying natural attributes, and a previous tendency to study the effects of each development proposal on an individual rather than on a cumulative basis. A positive step in estuarine management was recently taken by the N.S.W. government with the passage of legislation whereby environmental considerations are incorporated into planning and management procedures. However, shortcomings still exist in the overall management approach. This paper illustrates some of these shortcomings by examining the adverse environmental effects of structural...
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- 1986
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20. The Oriental Goby, Acanthogobius flavimanus (Temminck and Schlegel), an introduced fish in the coastal waters of New South Wales, Australia
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M. J. Middleton
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biology ,Ecology ,media_common.quotation_subject ,Goby ,Population explosion ,Aquatic Science ,biology.organism_classification ,Estuarine fish ,Competition (biology) ,Fishery ,Abundance (ecology) ,%22">Fish ,Acanthogobius flavimanus ,Bay ,Ecology, Evolution, Behavior and Systematics ,media_common - Abstract
Since 1971 over 100 specimens of the oriental goby, Acanthogobius flavimanus, have been collected from New South Wales’ waters. When this species, a native of Japan, was introduced to San Francisco Bay (U.S.A.) it underwent a population explosion, becoming a common member of estuarine fish communities in that area. The occurrence of both reproductively maturing females and juveniles in the harbours of the Sydney region (central New South Wales coast) suggests that the species may have bred successfully here. However, the relatively low numbers of A. flavimanus collected during the study indicate that as yet there has been no population explosion in New South Wales waters. A number of aspects of the biology and ecology of the species was examined in an attempt to identify features which may limit its distribution and abundance in the Sydney region. The inhibition of successful reproduction by the relatively warm-water temperatures in this area and the potential for competition with native fishes are proposed as possible explanations.
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- 1982
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21. Structural differences in the fish communities of Zostera capricorni and Posidonia australis seagrass meadows in Botany Bay, New South Wales
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Johann D. Bell, B. C. Pease, JJ Burchmore, DA Pollard, and M. J. Middleton
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Biomass (ecology) ,Posidonia ,biology ,Ecology ,Plant Science ,Aquatic Science ,biology.organism_classification ,Fishery ,Seagrass ,Abundance (ecology) ,Botany ,Species richness ,Posidonia australis ,Zostera ,Zostera capricorni - Abstract
The structure of fish communities inhabiting separate meadows of the seagrasses Zostera capricorni Aschers. and Posidonia australis Hook f. in Botany Bay, central New South Wales, was studied over a 2-year period using a number of community parameters. The heterogeneity, species richness and total abundance of fishes were not found to be significantly different between the two seagrass habitats, although more species and more individuals were associated with Zostera. The number of species, abundance of individuals and total biomass were all significantly greater in both habitats during summer, and total biomass was significantly greater in the Posidonia. Ordination of species abundance data separated samples from the two habitats. In general, larger species of the Gobiidae and Syngnathidae were diagnostic of Posidonia and smaller members of these families were unique to, or more abundant in, Zostera. Occurrence, abundance and biomass data were used to identify the 20 dominant members of the fish community in each habitat. About 50% of the dominant fish species associated with each seagrass habitat were of some economic importance. Such species were usually residents or transients and made up most of the biomass in each habitat. Adults of these dominant economically important species were most abundant in both seagrass habitats during summer. Juveniles of several economically important species were present in both Posidonia and Zostera meadows. However, marked differences in time of occurrence, size and feeding behaviour of these juveniles between the two habitats suggest that such species use Zostera and Posidonia meadows sequentially. Differences in the structure of the communities, and utilization of resources by juveniles of several economically important species, appear to be related to variations in the structural complexity of the canopies created by the two seagrasses.
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- 1984
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22. Nitrogen Content of Gastrointestinal Tracts of Rats During Absorptive Period
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E. Geiger, M. J. Middleton, and L. E. Human
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Absorption (pharmacology) ,chemistry.chemical_classification ,Gastrointestinal tract ,food.ingredient ,Nitrogen ,Starch ,food and beverages ,Biology ,General Biochemistry, Genetics and Molecular Biology ,Rats ,Amino acid ,Gastrointestinal Tract ,chemistry.chemical_compound ,fluids and secretions ,food ,chemistry ,Skimmed milk ,Animals ,Composition (visual arts) ,Food science ,Digestion ,Homeostasis - Abstract
Summary1) The basal level of endogenously supplied nitrogen in adult rats is about 5 mg after 1 1/2 hours, and this level is unaffected by protein depletion. On feeding skim milk powder, 22–27% of the ingested protein disappeared from the gastrointestinal tract within 3 hours. Under the conditions of these experiments the alleged homeostatic action of the gut in supplementing amino acids to deficient protein meals may be only negligible. 2) No significant differences have been observed in gastric emptying time, rate of absorption, or digestion between skim milk powders dried at low or high temperature.
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- 1958
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23. Is atropine always necessary before general anesthesia?
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M J, Middleton, J M, Zitzer, and K F, Urbach
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Adult ,Atropine ,Cyclopropanes ,Male ,Clinical Trials as Topic ,Adolescent ,Nitrous Oxide ,Arrhythmias, Cardiac ,Anesthesia, General ,Middle Aged ,Ethyl Ethers ,Humans ,Thiopental ,Halothane ,Preanesthetic Medication ,Aged - Published
- 1967
24. Effect of galactose ingestion on the urinary amino acid excretion in the rat
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M. J. Middleton, E. Geiger, and L. E. Human
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Catabolite Repression ,medicine.medical_specialty ,Weanling ,Excretion ,chemistry.chemical_compound ,Eating ,Physiology (medical) ,Internal medicine ,medicine ,Ingestion ,Animals ,Amino Acids ,chemistry.chemical_classification ,Renal Reabsorption ,Galactose ,Carbohydrate ,medicine.disease ,Antifibrinolytic Agents ,Amino acid ,Body Fluids ,Rats ,Endocrinology ,Glucose ,chemistry ,Biochemistry ,Aminoaciduria - Abstract
Groups of weanling rats were fed diets containing various levels of galactose or glucose or both. The excretion of amino acids was not affected by the type or quantity of ingested carbohydrate. It seems likely, therefore, that the aminoaciduria observed in galactosemic infants must be due to some cause other than the toxic effects of galactose itself or a competition for the renal reabsorption mechanism.
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- 1958
25. A Potential Cyclotron Resonant Scattering Feature in the Ultraluminous X-Ray Source Pulsar NGC 300 ULX1 Seen by NuSTAR and XMM-Newton.
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D. J. Walton, M. Bachetti, F. Fürst, D. Barret, M. Brightman, A. C. Fabian, B. W. Grefenstette, F. A. Harrison, M. Heida, J. Kennea, P. Kosec, R. M. Lau, K. K. Madsen, M. J. Middleton, C. Pinto, J. F. Steiner, and N. Webb
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- 2018
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26. Evidence for Pulsar-like Emission Components in the Broadband ULX Sample.
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D. J. Walton, F. Fürst, M. Heida, F. A. Harrison, D. Barret, D. Stern, M. Bachetti, M. Brightman, A. C. Fabian, and M. J. Middleton
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PULSARS ,NEUTRON stars ,X-ray binaries ,INTERSTELLAR medium ,STELLAR luminosity function - Abstract
We present broadband X-ray analyses of a sample of bright ultraluminous X-ray sources (ULX) with the goal of investigating the spectral similarity of this population to the known ULX pulsars, M82 X-2, NGC 7793 P13, and NGC 5907 ULX. We perform a phase-resolved analysis of the broadband XMM-Newton+NuSTAR data set of NGC 5907 ULX, finding that the pulsed emission from the accretion column in this source exhibits a similar spectral shape to that seen in both M82 X-2 and NGC 7793 P13, and that this is responsible for the excess emission observed at the highest energies when the spectra are fit with accretion disk models. We then demonstrate that similar “hard” excesses are seen in all ULXs in the broadband sample. Finally, for ULXs where the nature of the accretor is currently unknown, we test whether the hard excesses are all consistent with being produced by an accretion column similar to those present in M82 X-2, NGC 7793 P13, and NGC 5907 ULX. Based on the average shape of the pulsed emission, we find that in all cases a similar accretion column can successfully reproduce the observed data, consistent with the hypothesis that this ULX sample may be dominated by neutron star accretors. Compared to the known pulsar ULXs, our spectral fits for the remaining ULXs suggest that the non-pulsed emission from the accretion flow beyond the magnetosphere makes a stronger relative contribution than the component associated with the accretion column. If these sources do also contain neutron star accretors, this may help to explain the lack of detected pulsations. [ABSTRACT FROM AUTHOR]
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- 2018
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27. Structure of a fish community in a temperate tidal mangrove creek in Botany Bay, New South Wales
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M. J. Middleton, B. C. Pease, Johann D. Bell, JJ Burchmore, and DA Pollard
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geography ,geography.geographical_feature_category ,Ecology ,Temporary resident ,Marine habitats ,Species diversity ,Estuary ,Aquatic Science ,Biology ,Oceanography ,Fishery ,Habitat ,Botany ,Species evenness ,Mangrove ,Bay ,Ecology, Evolution, Behavior and Systematics - Abstract
The fish assemblage in the lower reaches of a temperate tidal mangrove creek entering Botany Bay near Sydney, New South Wales, was sampled using rotenone every second month between December 1977 and October 1980. Almost 17 000 fish (weight ~ 115 kg), belonging to 46 species and 24 families, were collected. Six species dominated the assemblage and another four were relatively common. Fourteen species, including four of the above, were economically important. These fishes made up 38% of individuals and 32% of biomass and were represented only by small juveniles. Nineteen species (41%) were temporary residents; these mainly comprised juveniles of large species that live elsewhere as adults. Fifteen species (33%), most of which only attain a small size (< 100 mm), were assumed to be permanent residents. The remaining 12 species (26%) occurred in only one sample and were, therefore, classified as rare. The diversity (HI) and evenness (J') of the fish community were low and showed little seasonality because a few species dominated the assemblage on an irregular basis. Numbers of species and of individuals varied seasonally and were significantly correlated. Peaks in these parameters lagged behind those in water temperature by 4 months and were largely the result of the relatively restricted recruitment periods of several abundant temporary resident species. The large numbers of juveniles and small species in the mangrove creek habitat were attributed to the availability of suitable shelter and food for such small fishes. Concerted use of the mangrove habitat by several abundant temporary resident species during the same general period each year appeared to be facilitated by the occupation of otherwise vacant feeding niches and some staggering of their peak recruitment periods. Exclusive use of this habitat by small juveniles of several species in Botany Bay confirms that mangrove habitats in temperate Australia, like some of those studied in tropical and subtropical regions, are important nursery areas for fishes inhabiting adjacent estuarine and inshore marine habitats as adults.
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- 1984
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28. Living on a Flare: Relativistic Reflection in V404 Cyg Observed by NuSTAR during Its Summer 2015 Outburst.
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D. J. Walton, K. Mooley, A. L. King, J. A. Tomsick, J. M. Miller, T. Dauser, J. A. García, M. Bachetti, M. Brightman, A. C. Fabian, K. Forster, F. Fürst, P. Gandhi, B. W. Grefenstette, F. A. Harrison, K. K. Madsen, D. L. Meier, M. J. Middleton, L. Natalucci, and F. Rahoui
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METEOR showers ,X-ray binaries ,LUMINOSITY ,BLACK holes ,ACCRETION disks - Abstract
We present first results from a series of NuSTAR observations of the black hole X-ray binary V404 Cyg obtained during its summer 2015 outburst, primarily focusing on observations during the height of this outburst activity. The NuSTAR data show extreme variability in both the flux and spectral properties of the source. This is partly driven by strong and variable line-of-sight absorption, similar to previous outbursts. The latter stages of this observation are dominated by strong flares, reaching luminosities close to Eddington. During these flares, the central source appears to be relatively unobscured and the data show clear evidence for a strong contribution from relativistic reflection, providing a means to probe the geometry of the innermost accretion flow. Based on the flare properties, analogies with other Galactic black hole binaries, and also the simultaneous onset of radio activity, we argue that this intense X-ray flaring is related to transient jet activity during which the ejected plasma is the primary source of illumination for the accretion disk. If this is the case, then our reflection modeling implies that these jets are launched in close proximity to the black hole (as close as a few gravitational radii), consistent with expectations for jet launching models that tap either the spin of the central black hole, or the very innermost accretion disk. Our analysis also allows us to place the first constraints on the black hole spin for this source, which we find to be (99% statistical uncertainty, based on an idealized lamp-post geometry). [ABSTRACT FROM AUTHOR]
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- 2017
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29. The Broadband Spectral Variability of Holmberg IX X-1.
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D. J. Walton, F. Fürst, F. A. Harrison, M. J. Middleton, A. C. Fabian, M. Bachetti, D. Barret, J. M. Miller, A. Ptak, V. Rana, D. Stern, and L. Tao
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GALACTIC X-ray sources ,BLACKBODY radiation ,ACCRETION (Astrophysics) ,DATA analysis ,ASTROPHYSICS - Abstract
We present results from four new broadband X-ray observations of the extreme ultraluminous X-ray source Holmberg IX X-1 ( erg s
−1 ), performed by Suzaku and NuSTAR in coordination. Combined with the archival data, we now have broadband observations of this remarkable source from six separate epochs. Two of these new observations probe lower fluxes than seen previously, allowing us to extend our knowledge of the broadband spectral variability exhibited. The spectra are well fit by two thermal blackbody components that dominate the emission below 10 keV, as well as a steep () power-law tail that dominates above ∼15 keV. Remarkably, while the 0.3–10.0 keV flux varies by a factor of ∼3 between all these epochs, the 15–40 keV flux varies by only ∼20%. Although the spectral variability is strongest in the ∼1–10 keV band, both of the thermal components are required to vary when all epochs are considered. We also revisit the search for iron absorption features by leveraging the high-energy NuSTAR data to improve our sensitivity to extreme velocity outflows in light of the ultra-fast outflow recently detected in NGC 1313 X-1. Iron absorption from a similar outflow along our line of sight can be ruled out in this case. We discuss these results in the context of super-Eddington accretion models that invoke a funnel-like geometry for the inner flow, and propose a scenario in which we have an almost face-on view of a funnel that expands to larger radii with increasing flux, resulting in an increasing degree of geometrical collimation for the emission from intermediate-temperature regions. [ABSTRACT FROM AUTHOR]- Published
- 2017
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30. DISCOVERY OF COHERENT PULSATIONS FROM THE ULTRALUMINOUS X-RAY SOURCE NGC 7793 P13.
- Author
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F. Fürst, D. J. Walton, F. A. Harrison, D. Stern, D. Barret, M. Brightman, A. C. Fabian, B. Grefenstette, K. K. Madsen, M. J. Middleton, J. M. Miller, K. Pottschmidt, A. Ptak, V. Rana, and N. Webb
- Published
- 2016
- Full Text
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31. A 78 DAY X-RAY PERIOD DETECTED FROM NGC 5907 ULX1 BY SWIFT.
- Author
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D. J. Walton, F. Fürst, M. Bachetti, D. Barret, M. Brightman, A. C. Fabian, N. Gehrels, F. A. Harrison, M. Heida, M. J. Middleton, V. Rana, T. P. Roberts, D. Stern, L. Tao, and N. Webb
- Published
- 2016
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32. AN IRON K COMPONENT TO THE ULTRAFAST OUTFLOW IN NGC 1313 X-1.
- Author
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D. J. Walton, M. J. Middleton, C. Pinto, A. C. Fabian, M. Bachetti, D. Barret, M. Brightman, F. Fuerst, F. A. Harrison, J. M. Miller, and D. Stern
- Published
- 2016
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33. A VERY LARGE ARRAY SEARCH FOR INTERMEDIATE-MASS BLACK HOLES IN GLOBULAR CLUSTERS IN M81.
- Author
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J. M. Wrobel, J. C. A. Miller-Jones, and M. J. Middleton
- Published
- 2016
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34. A HARD X-RAY STUDY OF THE ULTRALUMINOUS X-RAY SOURCE NGC 5204 X-1 WITH NuSTAR AND XMM-NEWTON.
- Author
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E. S. Mukherjee, D. J. Walton, M. Bachetti, F. A. Harrison, D. Barret, E. Bellm, S. E. Boggs, F. E. Christensen, W. W. Craig, A. C. Fabian, F. Fuerst, B. W. Grefenstette, C. J. Hailey, K. K. Madsen, M. J. Middleton, J. M. Miller, V. Rana, D. Stern, and W. Zhang
- Subjects
SPIRAL galaxies ,X-ray astronomy ,ASTRONOMICAL spectroscopy ,LUMINOSITY ,BLACK holes ,ACCRETION (Astrophysics) ,ACCRETION disks - Abstract
We present the results from coordinated X-ray observations of the ultraluminous X-ray source NGC 5204 X-1 performed by the Nuclear Spectroscopic Telescope Array and XMM-Newton in early 2013. These observations provide the first detection of NGC 5204 X-1 above , extending the broadband coverage to . The observations were carried out in two epochs separated by approximately 10 days, and showed little spectral variation with an observed luminosity of erg s
−1 . The broadband spectrum robustly confirms the presence of a clear spectral downturn above seen in some previous observations. This cutoff is inconsistent with the standard low/hard state seen in Galactic black hole binaries, as would be expected from an intermediate-mass black hole accreting at significantly sub-Eddington rates given the observed luminosity. The continuum is apparently dominated by two optically thick thermal-like components, potentially accompanied by a faint high-energy tail. The broadband spectrum is likely associated with an accretion disk that differs from a standard Shakura & Sunyaev thin disk. [ABSTRACT FROM AUTHOR]- Published
- 2015
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35. NUSTAR, XMM-NEWTON, AND SUZAKU OBSERVATIONS OF THE ULTRALUMINOUS X-RAY SOURCE HOLMBERG II X-1.
- Author
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D. J. Walton, M. J. Middleton, V. Rana, J. M. Miller, F. A. Harrison, A. C. Fabian, M. Bachetti, D. Barret, S. E. Boggs, F. E. Christensen, W. W. Craig, F. Fuerst, B. W. Grefenstette, C. J. Hailey, K. K. Madsen, D. Stern, and W. Zhang
- Subjects
- *
RUTHERFORD backscattering spectrometry , *FERMI Gamma-ray Space Telescope (Spacecraft) , *GAMMA ray telescopes , *BLACK holes , *COMPACT objects (Astronomy) - Abstract
We present the first broadband 0.3–25.0 keV X-ray observations of the bright ultraluminous X-ray source (ULX) Holmberg II X-1, performed by NuSTAR, XMM-Newton, and Suzaku in 2013 September. The NuSTAR data provide the first observations of Holmberg II X-1 above 10 keV and reveal a very steep high-energy spectrum, similar to other ULXs observed by NuSTAR to date. These observations further demonstrate that ULXs exhibit spectral states that are not typically seen in Galactic black hole binaries. Comparison with other sources implies that Holmberg II X-1 accretes at a high fraction of its Eddington accretion rate and possibly exceeds it. The soft X-ray spectrum ( keV) appears to be dominated by two blackbody-like emission components, the hotter of which may be associated with an accretion disk. However, all simple disk models under-predict the NuSTAR data above ∼10 keV and require an additional emission component at the highest energies probed, implying the NuSTAR data does not fall away with a Wien spectrum. We investigate physical origins for such an additional high-energy emission component and favor a scenario in which the excess arises from Compton scattering in a hot corona of electrons with some properties similar to the very high state seen in Galactic binaries. The observed broadband 0.3–25.0 keV luminosity inferred from these epochs is erg s−1, typical for Holmberg II X-1, with the majority of this flux (∼90%) emitted below 10 keV. [ABSTRACT FROM AUTHOR]
- Published
- 2015
- Full Text
- View/download PDF
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