Search results for "X-ray transient source"

showing 2 items of 2 documents

Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation

2023

Multi-messenger observations of the transient sky to detect cosmic explosions and counterparts of gravitational wave mergers critically rely on orbiting wide-FoV telescopes to cover the wide range of wavelengths where atmospheric absorption and emission limit the use of ground facilities. Thanks to continuing technological improvements, miniaturised space instruments operating as distributed-aperture constellations are offering new capabilities for the study of high energy transients to complement ageing existing satellites. In this paper we characterise the performance of the upcoming joint SpIRIT + HERMES-TP/SP nano-satellite constellation for the localisation of high-energy transients th…

Gamma ray transient sourceHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceX-ray transient sourceSpace telescopeTime domain astronomyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Discovery and Identification of MAXI J1621-501 as a Type I X-Ray Burster with a Super-orbital Period

2019

MAXI J1621-501 is the first Swift/XRT Deep Galactic Plane Survey transient that was followed up with a multitude of space missions (NuSTAR, Swift, Chandra, NICER, INTEGRAL, and MAXI) and ground-based observatories (Gemini, IRSF, and ATCA). The source was discovered with MAXI on 2017 October 19 as a new, unidentified transient. Further observations with NuSTAR revealed 2 Type I X-ray bursts, identifying MAXI J1621-501 as a Low Mass X-ray Binary (LMXB) with a neutron star primary. Overall, 24 Type I bursts were detected from the source during a 15 month period. At energies below 10 keV, the source spectrum was best fit with three components: an absorbed blackbody with kT = 2.3 keV, a cutoff p…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010504 meteorology & atmospheric sciencesX-ray bursterX-ray transient sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGalactic planeX-ray bursterLight curveOrbital period01 natural sciencesLow-mass X-ray binary starNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Science0103 physical sciencesRadiative transferEmission spectrumLow MassAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics0105 earth and related environmental sciencesAstrophysical Journal
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