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Transient optical emission from the error box of the γ-ray burst of 28 February 1997The ASTRO-H X-ray astronomy satelliteDiscovery of an X-ray afterglow associated with the γ-ray burst of 28 February 1997The ASTRO-H X-ray ObservatoryThe ASTRO-H MissionHitomiConstraints on the 3.5 keV Line in the Perseus Galaxy ClusterThe ASTRO-H (Hitomi) x-ray astronomy satelliteBeppoSAXObservations of GRB 980425: Detection of the Prompt Event and Monitoring of the Error BoxBeppoSAX detection and follow-up of GRB 9804251H0419-577: A two-state Seyfert galaxy?INTEGRAL observations of the cosmic X-ray background in the 5–100 keV range via occultation by the EarthThe broad band spectrum and variability of NGC 4151 observed by BeppoSAXVariability of winds in X-ray binariesIs GX 13+1 a dipping source?Hard X-ray colours of neutron star and black hole low mass X-ray binaries with INTEGRALCompact sources as the origin of the soft γ-ray emission of the Milky WayThe XEUS focal plane instrumentsSpectrum-RG/eROSITA/Lobster astrophysical missionThe X-ray emission from Nova V382 Velorum - I. The hard component observed withBeppoSAX[CSC][ITAL]BeppoSAX[/ITAL][/CSC] and [ITAL]Chandra[/ITAL] Observations of SAX J0103.2−7209 = 2E 0101.5−7225: A New Persistent 345 Second X-Ray Pulsar in the Small Magellanic CloudXMM-Newtonobservations of the low-mass X-ray binary EXO 0748−676 in quiescence
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description
hulumtues
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researcher
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wetenschapper
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հետազոտող
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name
A. Parmar
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A. Parmar
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Arvind Parmar
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Arvind Parmar
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A. Parmar
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A. Parmar
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Arvind Parmar
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Arvind Parmar
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A. Parmar
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A. Parmar
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A. Parmar
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Arvind Parmar
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Arvind Parmar
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0000-0002-3307-6517