Results 1 to 10 of about 11,679,254 (79)
Euclid preparation. XXIX. Forecasts for ten different higher-order weak lensing statistics [PDF]
Astronomy & Astrophysics, 2023 Recent cosmic shear studies have shown that higher-order statistics (HOS) developed by independent teams now outperform standard two-point estimators in terms of statistical precision thanks to their sensitivity to the non-Gaussian features of large ...Euclid Collaboration V. Ajani, M. Baldi, A. Barthelemy, A. Boyle, P. Burger, V. Cardone, S. Cheng, S. Codis, C. Giocoli, J. Harnois-D'eraps, S. Heydenreich, Vanshika Kansal, M. Kilbinger, L. Linke, C. Llinares, N. Martinet, C. Parroni, A. Peel, S. Pires, L. Porth, I. Tereno, C. Uhlemann, M. Vicinanza, S. Vinciguerra, N. Aghanim, N. Auricchio, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, F. Castander, M. Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, C. Conselice, L. Conversi, L. Corcione, F. Courbin, M. Cropper, A. D. Silva, H. Degaudenzi, A. D. Giorgio, J. Dinis, M. Douspis, F. Dubath, X. Dupac, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, S. Galeotta, B. Garilli, B. Gillis, A. Grazian, F. Grupp, H. Hoekstra, W. Holmes, A. Hornstrup, P. Hudelot, K. Jahnke, M. Jhabvala, M. Kummel, T. Kitching, M. Kunz, H. Kurki-Suonio, P. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, S. Mei, Y. Mellier, M. Meneghetti, Michele Moresco, L. Moscardini, S. Niemi, J. Nightingale, T. Nutma, C. Padilla, S. Paltani, K. Pedersen, V. Pettorino, G. Polenta, M. Poncet, L. Popa, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, T. Schrabback, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, L. Stanco, J. Starck, P. Tallada-Cresp'i, A. Taylor, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, G. Zamorani, J. Zoubian, S. Andreon, S. Bardelli, A. Boucaud, E. Bozzo, C. Colodro-Conde, D. Ferdinando, G. Fabbian, M. Farina, J. Graci'a-Carpio, E. Keihanen, V. Lindholm, D. Maino, N. Mauri, C. Neissner, M. Schirmer, V. Scottez, E. Zucca, Y. Akrami, C. Baccigalupi, A. Balaguera-Antol'inez, M. Ballardini, F. Bernardeau, A. Biviano, A. Blanchard, S. Borgani, A. Borlaff, C. Burigana, R. Cabanac, A. Cappi, C. Carvalho, S. Casas, G. Castignani, T. Castro, K. Chambers, A. Cooray, J. Coupon, H. Courtois, S. Davini, S. D. Torre, G. Lucia, G. Desprez, H. Dole, J. Escartín, S. Escoffier, I. Ferrero, F. Finelli, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, H. Hildebrandt, A. Munoz, B. Joachimi, J. Kajava, C. Kirkpatrick, L. Legrand, A. Loureiro, M. Magliocchetti, R. Maoli, S. Marcin, M. Martinelli, C. Martins, S. Matthew, L. Maurin, R. Metcalf, P. Monaco, G. Morgante, S. Nadathur, A. Nucita, V. Popa, D. Potter, A. Pourtsidou, M. Pontinen, P. Reimberg, A. S'anchez, Z. Sakr, A. Schneider, E. Sefusatti, M. Sereno, A. Shulevski, A. Mancini, J. Steinwagner, R. Teyssier, J. Valiviita, A. Veropalumbo, M. Viel, I. -. Paris-Saclay, Universit'e de Paris Cit'e, Cea, Cnrs, Astrophysique, Instrumentation et Mod'elisation Paris-Saclay, 91191 Gif-sur-Yvette, France, I. F. Physics, Astrophysics, D. Physics, E. Zurich, 27 Wolfgang-Pauli-Strasse, 8093 Zurich, Switzerland., D. Bologna, V. G. 932, 40129 Bologna, Italy, I. Bologna, V. G. 933, I. Bologna, 62 vialeBertiPichat, 40129 Bologna, University Observatory, F. O. Physics, Ludwig-Maximilians-Universitat, 1. Scheinerstr., 81679 Munich, H Germany, Aim, Universit'e Paris-Saclay, U. Paris, Argelander Institut fur Astronomie, U. Bonn, 71 AufdemHugel, 53121 Bonn, Infn Roma, P. A. Moro, 2. -. C. D. D. Fisica, E. Marconi, 00133 Roma, I. Roma, 33 viaFrascati, 00078 Monte Porzio Catone, J. Baltimore, MD 21218, Usa, S. O. Mathematics, Statistics, Physics, N. University, Herschel Building, Newcastle-upon-Tyne, NE1 7RU, Uk, Departament de F'isica, F. Ciencias, Universidade de Lisboa, C8 Edif'icio, C. Grande, P. Lisboa, Portugal, I. D. A. E. C. D. Espacco, Tapada da Ajuda, 1049-001 Lisboa, A. Universit'e, Cnes, Lam, Marseille, I. O. Physics, Laboratory of Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, D. Fisica, S. Roma, 2. PiazzaleAldoMoro, I. D. Spatiale, 91405, Orsay, I. Torino, 20 viaOsservatorio, 1. P. Torinese, U. Genova, 33 viaDodecaneso, 16146, Genova, I. R. Tre, 84 viadellaVascaNavale, 00146, Roma, Department of PhysicsE. Pancini, U. Federico, 6. ViaCinthia, 80126, Napoli, U. Porto, Caup, Rua das Estrelas, P. Porto, U. Torino, 1. ViaP.Giuria, 10125 Torino, I. Torino, Inaf-Iasf Milano, 12 ViaAlfonsoCorti, 20133 Milano, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, Campus Uab, 08193 Bellaterra, Spain., Port d'Informaci'o Cient'ifica, C. Sn, I. D. E. D. Catalunya, Carrer Gran Capit'a 2-4, 08193 Barcelona, Institute of Space Sciences, Carrer de Can Magrans, sn., 08193 Barcelona, I. -. Capodimonte, 16 viaMoiariello, 80131 Napoli, I. Naples, D. Bologna, Centre National d'Etudes Spatiales, Toulouse, Institut national de physique nucl'eaire et de physique des particules, 3. R. Michel-Ange, 16 75794ParisC'edex, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, J. B. C. F. Astrophysics, D. Physics, Astronomy, U. Manchester, Oxford Road, M13 9PL, Esacesa, Camino Bajo de Castillo, sn., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, European Space AgencyESRIN, 1. LargoGalileoGalilei, 00044 Frascati, Mullard Space Science Laboratory, U. London, H. Mary, Dorking, Surrey RH5 6NT, 1049-001 Lisboa, D. O. Astronomy, U. Geneva, 16 ch.d'Ecogia, I. D. A. E. P. Spaziali, V. Cavaliere, 100, 00133 Roma, U. Lyon, 1. UnivClaudeBernardLyon, CNRSIN2p3, I. Lyon, Umr 5822, 69622, Villeurbanne, Inaf Trieste, 11 ViaG.B.Tiepolo, 34127 Trieste, Inaf - Padova, 5. Viadell'Osservatorio, 35131 Padova, M. F. P. Physics, 1. Giessenbachstr., 85748 Garching, Universitatssternwarte Munchen, F. Physik, Ludwig-Maximilians-Universitat Munchen, 1. Scheinerstrasse, 8. Munchen, L. Observatory, Leiden University, 2. NielsBohrweg, 2333 CA Leiden, The Netherlands., Jet propulsion Laboratory, C. I. O. Technology., 4800 Oak Grove Drive, Pasadena, Ca, 91109, T. Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark., Cosmic Dawn Center, I. Paris, 98 bis boulevard Arago, 75014, París, M. Astronomie, 17 Konigstuhl, 69117 Heidelberg, Nasa Goddard Space Flight Center, Greenbelt, MD 20771, U. Geneve, D'epartement de Physique Th'eorique, Centre for Theoretical Physics, 24 quai Ernest-Ansermet, 4. CH-1211Geneve, 64 P.O.Box, 0. Helsinki, Finland., H. I. O. Physics, 2. GustafHallstrominkatu, U. Helsinki, Helsinki, Institute of Theoretical Astrophysics, U. Oslo, P. O. B. 1. Blindern, 0315 Oslo, Norway, Nova Optical IR Instrumentation Group at Astron, 4. OudeHoogeveensedijk, 7991PD, Dwingeloo, Institute for Computational Cosmology, D. University, South Road, DH1 3LE, Astroparticule et Cosmologie, 7. Paris, Umr 7095, Sorbonne Universit'e, 98 bis boulevard Arago, 7. Paris, European Space AgencyESTEC, 1. Keplerlaan, 2. Noordwijk, K. Institute, U. Groningen, PO Box 800, 9700 AV Groningen, U. Aarhus, Ny Munkegade 120, C. DK-8000Aarhus, S. Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Institute of Space Science, Bucharest, 077125, România, Dipartimento di Fisica e AstronomiaG.Galilei, U. Padova, 8. viaMarzolo, 35131 Padova, INFN-Padova, D. Astronomia, U. Bologna, V. G. 932, Fcfm, U. D. Chile, Blanco Encalada 2008, Santiago, Chile., Institut fur Teilchenphysik, U. Innsbruck, Technikerstr. 258, 6020 Innsbruck, Austria, Cppm, Institut de Ci'encies de l'Espai, sn Cerdanyola del Vall'es, Centro de Investigaciones Energ'eticas, Medioambientales y Tecnol'ogicas, 40 AvenidaComplutense, 28014 Madrid, Universidad Polit'ecnica de Cartagena +499 moresemanticscholar +1 more sourceEuclid preparation. XXIX. Water ice in spacecraft. I. The physics of ice formation and contamination [PDF]
Astronomy & Astrophysics, 2023 Molecular contamination is a well-known problem in space flight. Water is the most common contaminant and alters numerous properties of a cryogenic optical system. Too much ice means that Euclid's calibration requirements and science goals cannot be met. Euclid Collaboration M. Schirmer, K. Thurmer, B. Bras, M. Cropper, J. Martín-Fleitas, Y. Goueffon, R. Kohley, A. Mora, M. Portaluppi, G. Racca, A. Short, S. Szmolka, L. Venancio, M. Altmann, Z. Balog, U. Bastian, M. Biermann, D. Busonero, C. Fabricius, F. Grupp, C. Jordi, W. Loffler, A. S. Sell'es, N. Aghanim, A. Amara, L. Amendola, M. Baldi, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G. Candini, V. Capobianco, C. Carbone, J. Carretero, M. Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, C. Conselice, L. Conversi, Y. Copin, L. Corcione, F. Courbin, A. D. Silva, H. Degaudenzi, A. D. Giorgio, J. Dinis, F. Dubath, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, S. Haugan, H. Hoekstra, W. Holmes, F. Hormuth, A. Hornstrup, K. Jahnke, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, M. Kunz, H. Kurki-Suonio, S. Ligori, P. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, E. Medinaceli, S. Mei, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, Michele Moresco, L. Moscardini, E. Munari, R. Nakajima, S. Niemi, J. Nightingale, T. Nutma, C. Padilla, S. Paltani, F. Pasian, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Popa, F. Raison, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. Saglia, D. Sapone, B. Sartoris, P. Schneider, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, J. Skottfelt, L. Stanco, P. Tallada-Cresp'i, A. Taylor, I. Tereno, R. Toledo-Moreo, I. Tutusaus, E. Valentijn, L. Valenziano, T. Vassallo, Y. Wang, J. Weller, A. Zacchei, J. Zoubian, S. Andreon, S. Bardelli, P. Battaglia, E. Bozzo, C. Colodro-Conde, M. Farina, J. Graci'a-Carpio, E. Keihanen, V. Lindholm, D. Maino, N. Mauri, N. Morisset, V. Scottez, M. Tenti, E. Zucca, Y. Akrami, C. Baccigalupi, M. Ballardini, A. Biviano, A. Blanchard, A. Borlaff, C. Burigana, R. Cabanac, A. Cappi, C. Carvalho, S. Casas, G. Castignani, T. Castro, K. Chambers, A. Cooray, J. Coupon, H. Courtois, J. Cuby, S. Davini, G. Lucia, G. Desprez, S. Domizio, H. Dole, J. Escartín, S. Escoffier, I. Ferrero, L. Gabarra, K. Ganga, J. García-Bellido, K. George, F. Giacomini, G. Gozaliasl, H. Hildebrandt, J. Kajava, Vanshika Kansal, C. Kirkpatrick, L. Legrand, P. Liebing, A. Loureiro, G. Maggio, M. Magliocchetti, G. Mainetti, R. Maoli, S. Marcin, M. Martinelli, N. Martinet, C. Martins, S. Matthew, M. Maturi, L. Maurin, R. Metcalf, P. Monaco, G. Morgante, S. Nadathur, A. Nucita, L. Patrizii, J. Pollack, V. Popa, D. Potter, M. Pontinen, A. S'anchez, Z. Sakr, A. Schneider, M. Sereno, A. Shulevski, P. Simon, J. Steinwagner, R. Teyssier, J. V. M. F. Astronomie, 17 Konigstuhl, 69117 Heidelberg, Germany, Sandia National Laboratories, Livermore, CA 94550, Usa, European Space AgencyESTEC, 1. Keplerlaan, 2. Noordwijk, The Netherlands., Mullard Space Science Laboratory, U. London, H. Mary, Dorking, Surrey RH5 6NT, Uk, Aurora Technology B.V., 39 Zwarteweg, 2201 AA Noordwijk, Airbus Sas, Toulouse, France, Esacesa, Camino Bajo de Castillo, sn., Urb. Villafranca del Castillo, 28692 Villanueva de la Canada, Madrid, Spain., Aurora Technology for European Space Agency, Camino Bajo de Castillo, sn., Urb. Villafranca del Castillo, Villanueva de la Cañada, 28014 Madrid, A. Rechen-Institut, Zentrum fur Astronomie der Universitat Heidelberg, Monchhofstr. 12-14, 69117 Heidelberg, Syrte, O. Paris, Universit'e Psl, Cnrs, Sorbonne Universit'e, LnE, 6. Paris, I. Torino, 20 viaOsservatorio, 1. P. Torinese, Italy, Institut de Ci'encies del Cosmos, U. Barcelona, 1. Mart'iiFranques, 08193 Barcelona, I. D. E. D. Catalunya, Carrer Gran Capit'a 2-4, 08193 Barcelona, M. F. P. Physics, 1. Giessenbachstr., 85748 Garching, University Observatory, F. O. Physics, Ludwig-Maximilians-Universitat, 1. Scheinerstr., 81679 Munich, D. Astrof'isica, E. Barcelona, Universit'e Paris-Saclay, I. D. Spatiale, 91405, Orsay, Institute of Cosmology, Gravitation, U. Portsmouth, PO1 3FX, I. Physik, U. Heidelberg, 16 Philosophenweg, D. Bologna, V. G. 932, 40129 Bologna, I. Bologna, V. G. 933, I. Bologna, 62 vialeBertiPichat, 40129 Bologna, D. Fisica, U. Genova, 33 viaDodecaneso, 16146, Genova, I. Genova, Department of PhysicsE. Pancini, U. Federico, 6. ViaCinthia, 80126, Napoli, I. -. Capodimonte, 16 viaMoiariello, 80131 Napoli, I. D. A. E. C. D. Espacco, U. Porto, Caup, Rua das Estrelas, P. Porto, Portugal, U. Torino, 1. ViaP.Giuria, 10125 Torino, I. Torino, Inaf-Iasf Milano, 12 ViaAlfonsoCorti, 20133 Milano, Institut de F'isica d'Altes Energies, T. Z. F. O. Science, Technology, Campus Uab, 08193 Bellaterra, Port d'Informaci'o Cient'ifica, C. Sn, I. Roma, 33 viaFrascati, 00078 Monte Porzio Catone, I. Naples, C. Toulouse, 14 Avenue Edouard Belin, 9. 31401ToulouseCedex, Institut national de physique nucl'eaire et de physique des particules, 3. R. Michel-Ange, 16 75794ParisC'edex, Institute for Astronomy, U. Edinburgh, R. Observatory, B. Hill, Edinburgh EH9 3HJ, J. B. C. F. Astrophysics, D. Physics, Astronomy, U. Manchester, Oxford Road, M13 9PL, European Space AgencyESRIN, 1. LargoGalileoGalilei, 00044 Frascati, Roma, U. Lyon, 1. UnivClaudeBernardLyon, CNRSIN2p3, I. Lyon, Umr 5822, 69622 Villeurbanne, I. O. Physics, Laboratory of Astrophysics, E. P. F. Lausanne, Observatoire de Sauverny, 1290 Versoix, Switzerland., Departament de F'isica, F. Ciencias, Universidade de Lisboa, C8 Edif'icio, C. Grande, P. Lisboa, 1049-001 Lisboa, D. O. Astronomy, U. Geneva, 16 ch.d'Ecogia, I. D. A. E. P. Spaziali, V. Cavaliere, 100, 00133 Roma, INFN-Padova, 8. viaMarzolo, 35131 Padova, Universit'e de Paris Cit'e, Cea, Astrophysique, Instrumentation et Mod'elisation Paris-Saclay, 91191 Gif-sur-Yvette, Inaf Trieste, 11 ViaG.B.Tiepolo, 34127 Trieste, A. Universit'e, Cppm, Marseille, Institute of Theoretical Astrophysics, U. Oslo, P. O. B. 1. Blindern, 0315 Oslo, Norway, L. Observatory, Leiden University, 2. NielsBohrweg, 2333 CA Leiden, Jet propulsion Laboratory, C. I. O. Technology., 4800 Oak Grove Drive, Pasadena, Ca, 91109, von Hoerner Sulger GmbH, 8. Schlossplatz, 68723 Schwetzingen, T. Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark., Cosmic Dawn Center, U. Geneve, D'epartement de Physique Th'eorique, Centre for Theoretical Physics, 24 quai Ernest-Ansermet, 4. CH-1211Geneve, 64 P.O.Box, 0. Helsinki, Finland., H. I. O. Physics, 2. GustafHallstrominkatu, U. Helsinki, Helsinki, Nova Optical IR Instrumentation Group at Astron, 4. OudeHoogeveensedijk, 7991PD, Dwingeloo, Argelander Institut fur Astronomie, U. Bonn, 71 AufdemHugel, 53121 Bonn, Institute for Computational Cosmology, D. University, South Road, DH1 3LE, Astroparticule et Cosmologie, 7. Paris, I. Paris, 98 bis boulevard Arago, 75014, París, Umr 7095, 98 bis boulevard Arago, 7. Paris, C. Saclay, Dfrirfu, S. d’Astrophysique, Bat. 709, K. Institute, U. Groningen, PO Box 800, 9700 AV Groningen, Aim, 91191, Gif-sur-Yvette, S. Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Institute of Space Science, Str. Atomistilor, nr. 409 Muagurele, Ilfov, 077125, România, D. Galilei', U. Padova, D. Astronomia, U. Bologna, V. G. 932, Universitatssternwarte Munchen, F. Physik, Ludwig-Maximilians-Universitat Munchen, 1. Scheinerstrasse, 8. Munchen, Fcfm, U. D. Chile, Blanco Encalada 2008, Santiago, Chile., Institut de Ci'encies de l'Espai, Carrer de Can Magrans +499 moresemanticscholar +1 more sourceEuclid preparation. XVIII. The NISP photometric system [PDF]
Astronomy & Astrophysics, 2022 Euclid will be the first space mission to survey most of the extragalactic sky in the 0.95-2.02 $\mu$m range, to a 5$\sigma$ point-source median depth of 24.4 AB mag. This unique photometric data set will find wide use beyond Euclid's core science.Euclid Collaboration M. Schirmer, K. Jahnke, G. Seidel, H. Aussel, C. Bodendorf, F. Grupp, F. Hormuth, S. Wachter, P. Appleton, R. Barbier, J. Brinchmann, J. M. Carrasco, F. Castander, J. Coupon, F. Paolis, A. Franco, K. Ganga, P. Hudelot, E. Jullo, A. Lançon, A. Nucita, S. Paltani, G. Smadja, L. Venancio, F. Strafella, M. Weiler, A. Amara, T. Auphan, N. Auricchio, A. Balestra, R. Bender, D. Bonino, E. Branchini, M. Brescia, V. Capobianco, C. Carbone, J. Carretero, R. Casas, M. Castellano, S. Cavuoti, A. Cimatti, R. Clédassou, G. Congedo, C. Conselice, L. Conversi, Y. Copin, L. Corcione, A. Costille, F. Courbin, A. D. Silva, H. Degaudenzi, M. Douspis, F. Dubath, X. Dupac, S. Dusini, A. Ealet, S. Farrens, S. Ferriol, P. Fosalba, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, L. Guzzo, S. Haugan, H. Hoekstra, W. Holmes, A. Hornstrup, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, R. Kohley, M. Kummel, M. Kunz, H. Kurki-Suonio, R. Laureijs, S. Ligori, P. Lilje, I. Lloro, T. Maciaszek, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, F. Marulli, R. Massey, S. Maurogordato, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, Michele Moresco, L. Moscardini, E. Munari, R. Nakajima, R. Nichol, S. Niemi, C. Padilla, F. Pasian, K. Pedersen, W. Percival, V. Pettorino, S. Pires, M. Poncet, L. Popa, L. Pozzetti, É. Prieto, F. Raison, J. Rhodes, H. Rix, M. Roncarelli, E. Rossetti, R. Saglia, B. Sartoris, R. Scaramella, P. Schneider, A. Secroun, S. Serrano, C. Sirignano, G. Sirri, L. Stanco, P. Tallada-Cresp'i, A. Taylor, H. Teplitz, I. Tereno, R. Toledo-Moreo, F. Torradeflot, M. Trifoglio, E. Valentijn, L. Valenziano, Y. Wang, J. 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Nature, 2014 The majority of ultraluminous X-ray sources are point sources that are spatially offset from the nuclei of nearby galaxies and whose X-ray luminosities exceed the theoretical maximum for spherical infall (the Eddington limit) onto stellar-mass black ...M. Bachetti, F. Harrison, D. Walton, B. Grefenstette, D. Chakrabarty, F. Furst, D. Barret, A. Beloborodov, S. Boggs, F. Christensen, W. Craig, A. Fabian, C. Hailey, A. Hornschemeier, V. Kaspi, S. Kulkarni, T. Maccarone, J. Miller, V. Rana, D. Stern, S. Tendulkar, J. Tomsick, N. Webb, W. W. Z. U. D. Toulouse, UPS-OMP, Irap, F. Toulouse, F. Cnrs, Institut de Recherche en Astrophysique et Plan'etologie, A. Roche, BP 44346, 4. 31028ToulouseCedex, F. Toulouse, F. M. F. Astrophysics, 1. E. C. Boulevard, C. I. O. Technology., Pasadena, California 91125, Usa Harvard-Smithsonian Center for Astrophysics, Space Research, M. I. O. Technology, Cambridge, MA 02139, U. P. Department, Columbia University. 538 W 120th Street, New York., NY 10027, Usa Space Sciences Laboratory, U. California, Berkeley, CA 94720, Usa Dtu Space, National Space Institute, T. Denmark, Elektrovej 327, DK-2800 Lyngby, D. L. L. N. Laboratory, Livermore, CA 94550, USA. Department of Astronomy, U. Cambridge, Madingley Road, Cambridge CB3 0HA, UK Columbia Astrophysics Laboratory, Columbia University, Usa Nasa Marshall Space Flight Center, Greenbelt, MD 20771, USA. Department of physics, M. University, Montreal, Quebec, H3A 2T8, Canada Department of Physics, Texas Tech University, Lubbock, TX 79409, USA. Department of Astronomy, U. Michigan, 500 Church Street, A. Arbor, MI 48109-1042, Usa Jet Propulsion Laboratory, CA 91109, Usa +84 moresemanticscholar +1 more source
