Sylvain Chaty
Affiliations: | 1998 | Université Paris-Sud 11, Orsay, Bures-sur-Yvette, Île-de-France, France |
Website:
http://www.aim.univ-paris7.fr/CHATY/chaty/Bienvenue.htmlGoogle:
"Sylvain Chaty"Mean distance: (not calculated yet)
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Publications
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| Fortin F, Chaty S, Sander A. (2020) Optical and Infrared Study of the Obscured B[e] Supergiant High-mass X-Ray Binary IGR J16318-4848 The Astrophysical Journal. 894: 86 |
| Chaty S, Fortin F, López-Oramas A. (2020) Broad-band spectral energy distribution of the X-ray transient Swift J1745−26 from outburst to quiescence Astronomy and Astrophysics. 637 |
| Kretschmar P, Fürst F, Sidoli L, et al. (2019) Advances in Understanding High-Mass X-ray Binaries with INTEGRALand Future Directions New Astronomy Reviews. 86: 101546 |
| García F, Fogantini FA, Chaty S, et al. (2018) Spectral evolution of the supergiant HMXB IGR J16320-4751 along its orbit using XMM-Newton Astronomy and Astrophysics. 618 |
| Servillat M, Coleiro A, Chaty S, et al. (2014) Herschel observations of dust around the high-mass X-ray binary GX 301-2 The Astrophysical Journal. 797: 114 |
| Ackermann M, Ajello M, Allafort A, et al. (2013) Detection of the characteristic pion-decay signature in supernova remnants. Science (New York, N.Y.). 339: 807-11 |
| Chaty S, Coleiro A, Servillat M, et al. (2013) Herschel observations of INTEGRAL supergiant High Mass X-ray Binaries Interpretation. 176: 92 |
| Fermi LAT Collaboration, Ackermann M, Ajello M, et al. (2012) Periodic emission from the gamma-ray binary 1FGL J1018.6-5856. Science (New York, N.Y.). 335: 189-93 |
| Tomsick JA, Bodaghee A, Rodriguez J, et al. (2012) Is IGR J11014-6103 a Pulsar with the Highest Known Kick Velocity? The Astrophysical Journal. 750 |
| Lowell AW, Tomsick JA, Heinke CO, et al. (2012) XMM-Newton finds that SAX J1750.8-2900 may harbor the hottest, most luminous known neutron star Astrophysical Journal. 749 |