Temperature determination via STJ optical spectroscopy

Simple item page
dc.creatorReynolds, A. P.
dc.creatorde Bruijne, J. H. J.
dc.creatorPerryman, M. A. C.
dc.creatorPeacock, A.
dc.creatorBridge, C. M.
dc.date2003-01-21
dc.date.accessioned2026-07-07T10:31:39Z
dc.date.available2026-07-07T10:31:39Z
dc.descriptionESA's Superconducting Tunnel Junction (STJ) optical photon-counting camera (S-Cam2) incorporates an array of pixels with intrinsic energy sensitivity. Using the spectral fitting technique common in X-ray astronomy, we fit black bodies to nine stellar spectra, ranging from cool flare stars to hot white dwarfs. The measured temperatures are consistent with literature values at the expected level of accuracy based on the predicted gain stability of the instrument. Having also demonstrated that systematic effects due to count rate are likely to be small, we then proceed to apply the temperature determination method to four cataclysmic variable (CV) binary systems. In three cases we measure the temperature of the accretion stream, while in the fourth we measure the temperature of the white dwarf. The results are discussed in the context of existing CV results. We conclude by outlining the prospects for future versions of S-Cam.
dc.description9 pages, 9 figures (11 files); uses aa.cls; accepted for publication in A&A
dc.identifierhttps://arxiv.org/abs/astro-ph/0301409
dc.identifierhttp://arxiv.org/abs/astro-ph/0301409
dc.identifierAstron.Astrophys.400:1209,2003
dc.identifierdoi:10.1051/0004-6361:20030042
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178485
dc.subjectAstrophysics
dc.titleTemperature determination via STJ optical spectroscopy
dc.typetext

Files

Collections

arXiv