Results 11 to 20 of about 34,501 (181)
A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b [PDF]
Nature, 2023 The dayside thermal emission spectrum and brightness temperature map of the ultra-hot Jupiter WASP-18b obtained from the NIRISS instrument on the JWST showed water emission features, an atmosphere consistent with solar metallicity, as well as a steep and L. Coulombe, B. Benneke, R. Challener, Anjali A. A. Piette, Lindsey S. Wiser, M. Mansfield, R. MacDonald, H. Beltz, A. Feinstein, M. Radica, A. Savel, L. D. Santos, J. Bean, V. Parmentier, I. Wong, E. Rauscher, T. Komacek, E. Kempton, Xianyu Tan, M. Hammond, N. Lewis, M. Line, Elspeth K. H. Lee, Hinna Shivkumar, I. Crossfield, M. Nixon, B. Rackham, H. Wakeford, L. Welbanks, Xi Zhang, N. Batalha, Z. Berta-Thompson, Q. Changeat, Jean-Michel D'esert, N. Espinoza, J. Goyal, J. Harrington, H. Knutson, L. Kreidberg, M. L'opez-Morales, Avi Shporer, D. Sing, K. Stevenson, K. Aggarwal, E. Ahrer, M. Alam, T. Bell, J. Blecic, C. Cáceres, A. Carter, S. Casewell, N. Crouzet, P. Cubillos, L. Decin, J. Fortney, N. Gibson, K. Heng, T. Henning, N. Iro, S. Kendrew, P. Lagage, J. Leconte, M. Lendl, J. Lothringer, L. Mancini, T. Mikal-Evans, K. Molaverdikhani, N. Nikolov, K. Ohno, E. Pallé, C. Piaulet, S. Redfield, P. Roy, Shang-min Tsai, O. Venot, P. A. N. D. O. Physics, Trottier Institute for Research on Exoplanets, U. Montr'eal, Montreal, Qc, Canada, D. O. Astronomy, U. Michigan, A. Arbor, Mi, Usa, Earth, Planets Laboratory, Carnegie Institution for Science, Washington, Dc, School of Earth, Space Exploration, Arizona State University, Tempe, Az, S. Observatory, U. Arizona, Tucson, Nhfp Sagan Fellow, Carl Sagan Institute, Cornell University, Ithaca, Ny, Astrophysics, U. Chicago, Chicago., Il, U. Maryland, College Park, Md, Center for Computational Astrophysics, Flatiron Institute, New York., Space Telescope Science Institute, Baltimore., Universit'e Cote d'Azur, Observatoire Cote d'Azur, Cnrs, Laboratoire Lagrange, France, Nasa Goddard Space Flight Center, Greenbelt, Nasa Postdoctoral Program Fellow, Tsung-Dao Lee Institute, S. University, Shanghai, P. R. China, S. O. Physics, Astronomy, Atmospheric, Oceanic, P. Physics, D. Physics, U. Oxford, Oxford, Uk, D. O. Mathematics, Statistics, Faculty of Environment, Science, Economy, U. Exeter, Exeter, Devon, Center for Space, Habitability, U. Bern, Bern, Switzerland., A. S. M. F. Astronomy, U. Amsterdam, Amsterdam, The Netherlands., U. Kansas, Lawrence, Ks, D. O. Earth, Planetary Sciences, M. I. O. Technology, Cambridge, Ma, Kavli Institute for Astrophysics, S. Research, 51 Pegasi b Fellow, U. Bristol, Bristol, University of California at Santa Cruz, Santa Cruz, Ca, U. California, Department of Astrophysical, U. C. A. Boulder, Co, E. Agency, U. London, United Kingdom., National Institute of Science Education, Research, Hbni, Odisha, India., Planetary Sciences Group, Florida Space Institute, U. Florida, Orlando, Florida, Division of Geological, C. I. O. Technology., Pasadena, M. F. Astronomy, Heidelberg, H Germany, Center for Computational Astrophysics, Harvard, Smithsonian, J. University, Johns Hopkins Apl, Laurel, Indian Institute of Technology, Indore, Center for Exoplanets, U. Warwick, Coventry, B. Institute, N. R. Center, Moffet Field, N. Y. U. A. Dhabi, Abu Dhabi, Uae, Center for Astro, Particle, Instituto Nacional de Astrof'isica, U. A. Bello, Santiago, Chile., N'ucleo Milenio de Formaci'on Planetaria, C. D. A. Y. T. Afines, Casilla 36-D, U. Leicester, Leicester, L. Observatory, U. Leiden, Leiden, I. Torino, Pino Torinese, Italy, S. R. Institute, Austrian Academy of Sciences, Graz, Austria, I. O. Astronomy, K. Leuven, Leuven, Belgium, Trinity College Dublin, Dublin., Ireland, Universitats-Sternwarte, Ludwig-Maximilians-Universitat Munchen, Munchen, A. C. F. B. E. Research, Inst. for Nucl. Research, G. Centre, Berlin, Universit'e Paris-Saclay, Universit'e de Paris Cit'e, Cea, Aim, Gif-sur-Yvette, L. Bordeaux, U. Bordeaux, Pessac, D'epartement d'Astronomie, U. Geneve, Sauverny, Utah Valley University, Orem, Ut, University of RomeTor Vergata, Romé, I. A. Observatory, Exzellenzcluster Origins, Garching, Instituto de Astrof'isica de Canarias, Tenerife, Spain., A. Department, Van Vleck Observatory, Wesleyan University, Middletown, Ct, Riverside, Universit'e de Paris Cit'e, Universit'e Paris Est Creteil, Lisa, París +276 moresemanticscholar +1 more sourceRadio observations of the Black Hole X-ray Binary EXO 1846−031 re-awakening from a 34-year slumber [PDF]
Monthly notices of the Royal Astronomical Society, 2022
We present radio [1.3 GHz MeerKAT, 4−8 GHz Karl G. Jansky Very Large Array (VLA) and 15.5 GHz Arcminute Microkelvin Imager Large Array (AMI-LA)] and X-ray (Swift and MAXI) data from the 2019 outburst of the candidate Black Hole X-ray Binary (BHXB) EXO ...D. R. Williams, S. Motta, R. Fender, J. Miller-Jones, J. Neilsen, J. Allison, J. Bright, I. Heywood, P. Jacob, L. Rhodes, E. Tremou, P. Woudt, J. Eijnden, F. Carotenuto, D. Green, D. Titterington, A. V. D. Horst, P. S. J. B. C. F. Astrophysics, S. O. Physics, Astronomy, The University of Manchester, D. Physics, U. Oxford, Istituto Nazionale di Astrofisica, Osservatorio astronomico di Brera, D. O. Astronomy, U. C. Town, I. C. F. R. A. R. -. C. University, V. University, First Light Fusion Ltd., Uk, Center for Interdisciplinary Exploration, Research in Astrophysics, N. University, Electronics, R. University, Max Planck Institut fur Radioastronomie, National Radio Astronomy Observatory, A. Group, C. Laboratory, The George Washington University, Physics, Statistics Institute of Sciences, Center for Astro, Particle, P. Physics, N. Y. U. A. Dhabi +46 moresemanticscholar +1 more sourceThe Co-Ordinated radio and infrared survey for high-mass star formation – V. The CORNISH-South survey and catalogue [PDF]
Monthly notices of the Royal Astronomical Society, 2023
We present the first high spatial resolution radio continuum survey of the southern Galactic plane. The CORNISH project has mapped the region defined by 295○ < l < 350○; |b| < 1○ at 5.5-GHz, with a resolution of 2.5″ (FWHM).T. Irabor, M. Hoare, M. Burton, W. Cotton, P. Diamond, S. Dougherty, S. Ellingsen, R. Fender, G. Fuller, S. Garrington, P. Goldsmith, J. Green, A. Gunn, J. Jackson, S. Kurtz, S. L. L. J. Marti, I. McDonald, S. Molinari, T. Moore, M. Mutale, T. Muxlow, T. O'Brien, R. Oudmaijer, R. Paladini, J. Pandian, J. Paredes, A. Richards, Á. Sánchez-Monge, R. Spencer, M. Thompson, G. Umana, J. Urquhart, M. Wieringa, A. Physics, Astronomy, U. Leeds, UK., J. B. C. F. Astrophysics, D. Physics, U. Manchester, the Hera Team 1National Radio Astronomy Observatory, Usa, I. O. Astronomy, Astrophysics, National Autonomous University of Mexico, M'exico., Jet Propulsion Laboratory California Institute fo Technology, Pasadena, D. Sciences, Indian Institute of Science, Technology, Trivandrum, India., Green Bank Observatory, A. R. Institute, Liverpool John Moore's University, Twelve Quays House, Centre for Astrophysics Research, U. Hertfordshire, Cosmos Science Institute, U. Barcelona, Iccub, Mart'i i Franqu'es, 08193 Barcelona, Spain., Departament de F'isica, Univ. de Ja'en, C. Space, Australia., A. Observatory, Planetarium, College Hill, N. Ireland, U. Oxford, Keble Road, Oxford, School of Physical Sciences, College of Optical Sciences, Engineering, U. Tasmania, I. N. D. A. -. Iaps, Italy, Centre for Gravitational Astrophysics, Planetary Science, U. Kent, Canterbury, Inaf - Catania, Infrared Processing Center, C. I. O. Technology., P. Institut, U. Cologne, 77 ZulpicherStr., 50937 Koln, H Germany, The Alma headquarters, Santiago, Chile., Open University, Walton Hall, M. Keynes +99 moresemanticscholar +1 more sourceThe Green Bank Northern Celestial Cap Pulsar Survey. II. The Discovery and Timing of 10 Pulsars [PDF]
, 2018 We present timing solutions for 10 pulsars discovered in 350 MHz searches with the Green Bank Telescope. Nine of these were discovered in the Green Bank Northern Celestial Cap survey and one was discovered by students in the Pulsar Search Collaboratory ...A. Kawash, M. Mclaughlin, D. Kaplan, M. DeCesar, L. Levin, D. Lorimer, R. Lynch, K. Stovall, J. Swiggum, E. Fonseca, A. M. Archibald, S. Banaszak, C. Biwer, J. Boyles, B. Cui, L. Dartez, D. Day, S. Ernst, A. J. Ford, J. Flanigan, S. Heatherly, J. Hessels, J. Hinojosa, F. Jenet, C. Karako-Argaman, V. Kaspi, V. Kondratiev, S. Leake, G. Lunsford, J. Martinez, A. Mata, T. Matheny, A. McEwen, M. Mingyar, A. Orsini, S. Ransom, M. Roberts, M. Rohr, X. Siemens, R. Spiewak, I. Stairs, J. V. Leeuwen, A. Walker, B. L. W. C. F. G. Waves, Cosmology, West Virginia University, U. Wisconsin-Milwaukee, Lafayette College, The University of Manchester, Green Bank Observatory, National Radio Astronomy Observatory, M. University, Astron, U. Amsterdam, S. University, Western Kentucky University, University of Texas Rio Grande Valley, Morehead State University, A. Institute, M. F. Radioastronomie, Eureka Scientific, Inc., S. U. O. Technology, U. Columbia, Colorado State University +64 moresemanticscholar +1 more sourceImage plane detection of FRB121102 with the MeerKAT radio telescope [PDF]
, 2022 We present the analysis of radio interferometric 2-s images from a MeerKAT observation of the repeating fast radio burst FRB121102 on September 2019, during which 11 distinct pulses have been previously detected using high time and frequency resolution ...J. Andrianjafy, N. Heeralall-Issur, A. Deshpande, K. Golap, P. Woudt, M. Caleb, E. Barr, W. Chen, F. Jankowski, M. Kramer, B. Stappers, J. W. D. O. Physics, University of Mauritius, Mauritius, R. R. Institute, Bangalore, India., Inter-University Centre for Astronomy, Astrophysics, Pune, Indian Institute of Technology, Kanpur, National Radio Astronomy Observatory, Socorro, USA., D. O. Astronomy, U. C. Town, Rondebosch, S. Africa, Sydney Institute for Astronomy, S. O. Physics, The University of Sydney, Sydney, Australia., 3D ASTRO3DARCCentreofExcellenceforAll-skyAstrophysics, Canberra, Max Planck Institut fur Radioastronomie, Bonn, H Germany, J. B. C. F. Astrophysics, D. Physics, Astronomy, The University of Manchester, Manchester, Uk +44 moresemanticscholar +1 more sourceMurchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1 [PDF]
Astronomy & Astrophysics, 2019 Aims. In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9 + 3.1.
Methods.D. Oni'c, M. Filipovi'c, I. Bojivci'c, N. Hurley-Walker, B. Arbutina, T. Pannuti, C. Maitra, D. Urovsevi'c, F. Haberl, N. Maxted, G. Wong, G. Rowell, M. Bell, J. Callingham, K. Dwarakanath, B. For, P. Hancock, L. Hindson, M. Johnston-Hollitt, A. Kapi'nska, E. Lenc, B. McKinley, J. Morgan, A. Offringa, L. Porter, P. Procopio, L. Staveley-Smith, R. Wayth, C. Wu, Q. Z. D. O. Astronomy, Faculty of Mathematics, U. Belgrade, 16 Studentskitrg, 11000 Belgrade, Serbia, Western Sydney University, Locked Bag 1797, DC PenrithSouth, Nsw, Australia., International Centre for Radio Astronomy Research, Curtin University, Gpo Box U1987, Perth WA 6845, S. Center, D. O. Earth, S. Sciences, Morehead State University, 235 Martindale Drive, Morehead, KY 40351, Usa, M. F. Physik, Giessenbachstrasse, 85748 Garching, H Germany, S. O. Physics, The University of New South Wales, Sydney 2052, School of Physical Sciences, The University of Adelaide, Adelaide 5005, U. Sydney, 15 Broadway, Ultimo, Nsw 2007, N. F. F. R. Astronomy, 2. POBus, 7. Dwingeloo, The Netherlands., R. R. Institute, Bangalore 560080, India., M468, U. O. S. Australia, Crawley, WA 6009, Centre for Astrophysics Research, Astronomy, Mathematics, U. Hertfordshire, C. Lane, Hatfield AL10 9AB, UK., C. Astronomy, S. Science, Marsfield, Nsw 1710, Research School for Astronomy, Astrophysics, Australian National University, Canberra, Act 2611, The University of Melbourne, Parkville, Vic 3010, S. Observatory, 80 Nandan Rd., X. Qu, S. Shi, China, 200000, Isaac Newton Institute of Chile, Yugoslavia Branch +103 moresemanticscholar +1 more source21 new long-term variables in the GX 339-4 field: two years of MeerKAT monitoring [PDF]
, 2022 We present 21 new long-term variable radio sources found commensally in two years of weekly MeerKAT monitoring of the low-mass X-ray binary GX 339-4.L. Driessen, B. Stappers, E. Tremou, R. Fender, P. Woudt, Rachel Armstrong, S. Bloemen, P. Groot, I. Heywood, A. Horesh, A. V. D. Horst, E. Koerding, V. McBride, J. Miller-Jones, K. Mooley, A. Rowlinson, R. K. K. J. B. C. F. Astrophysics, D. Physics, Astronomy, The University of Manchester, Manchester, M13 9PL, UK., Lesia, O. Paris, Cnrs, P. university, Sarbonne Universite, U. Paris, Meudon, France., Inter-University Centre for Astronomy, D. O. Astronomy, U. C. Town, X3 PrivateBag, Rondebosch 7701, S. Africa, Astrophysics, U. Oxford, Denys Wilkinson Building, Keble Road, O. 3RH, South African astronomical Observatory, 2. F. Street, B. Park, Observatory, Cape Town 7925, Department of AstrophysicsIMAPP, R. University, P. B. 9010, 6500 GL Nijmegen, The Netherlands., South African astronomical Observatory, 9. POBox, Observatory 7935, Electronics, R. University, 9. POBox, Makhanda 6140, R. I. O. Physics, The Hebrew University of Jerusalem, Jerusalem 91904, Israel, The George Washington University, NW 72521stStreet, Washington, DC 20052, Usa, Physics, Statistics Institute of Sciences, Iau Office of Astronomy for Development, C. Town, 7935, I. C. F. R. A. R. -. C. University, Gpo Box U1987, Perth, WA 6845, Australia., National Radio Astronomy Observatory, Socorro, NM 87801, Caltech, 1200 E. California Blvd. MC 249-17, Pasadena, CA 91125, Anton Pannekoek Institute, U. Amsterdam, Postbus 94249, GE 1090, Amsterdam, N. F. F. R. Astronomy, 4. OudeHoogeveensedijk, PD 7991, Dwingeloo +93 moresemanticscholar +1 more sourceCardiopulmonary exercise testing (CPET) in the United Kingdom—a national survey of the structure, conduct, interpretation and funding
Perioperative Medicine, 2018 BackgroundCardiopulmonary exercise testing (CPET) is an exercise stress test with concomitant expired gas analysis that provides an objective, non-invasive measure of functional capacity under stress.T. Reeves, S. Bates, T. Sharp, K. Richardson, S. Bali, J. Plumb, H. Anderson, J. Prentis, M. Swart, D. Levett, On behalf of the PeriOperative Italian Society +10 moresemanticscholar +1 more source
