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Photometric calibration of the Swift ultraviolet/optical telescope

dc.contributor.authorHunsberger, S.
dc.contributor.authorMarshall, F.
dc.contributor.authorMorgan, A.
dc.contributor.authorPandey, S. B.
dc.contributor.authorDE PASQUALE, Massımılıano
dc.contributor.authorSmith, P. J.
dc.contributor.authorStill, M.
dc.contributor.authorKennedy, T.
dc.contributor.authorPage, M. J.
dc.contributor.authorLandsman, W.
dc.contributor.authorHolland, S. T.
dc.contributor.authorRoming, P.
dc.contributor.authorKuin, N. P. M.
dc.contributor.authorBrown, P. J.
dc.contributor.authorGronwall, C.
dc.contributor.authorKoch, S.
dc.contributor.authorIvanushkina, M.
dc.contributor.authorImmler, S.
dc.contributor.authorHuckle, H.
dc.contributor.authorHancock, B.
dc.contributor.authorCucchiara, A.
dc.contributor.authorChester, M. M.
dc.contributor.authorCarter, M.
dc.contributor.authorBroos, P.
dc.contributor.authorBoyd, P.
dc.contributor.authorBlustin, A. J.
dc.contributor.authorVanden Berk, D.
dc.contributor.authorSchady, P.
dc.contributor.authorMason, K. O.
dc.contributor.authorPoole, T. S.
dc.contributor.authorBreeveld, A. A.
dc.date.accessioned2022-02-18T09:27:12Z
dc.date.available2022-02-18T09:27:12Z
dc.date.issued2008
dc.identifier.citationPoole T. S. , Breeveld A. A. , Page M. J. , Landsman W., Holland S. T. , Roming P., Kuin N. P. M. , Brown P. J. , Gronwall C., Hunsberger S., et al., "Photometric calibration of the Swift ultraviolet/optical telescope", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.383, sa.2, ss.627-645, 2008
dc.identifier.issn0035-8711
dc.identifier.othervv_1032021
dc.identifier.otherav_3d0d5b9c-e83d-4c08-b2cb-67b5ffb178a5
dc.identifier.urihttp://hdl.handle.net/20.500.12627/177244
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2007.12563.x
dc.description.abstractWe present the photometric calibration of the Swift Ultraviolet/Optical Telescope (UVOT) which includes: optimum photometric and background apertures, effective area curves, colour transformations, conversion factors for count rates to flux and the photometric zero-points (which are accurate to better than 4 per cent) for each of the seven UVOT broad-band filters. The calibration was performed with observations of standard stars and standard star fields that represent a wide range of spectral star types. The calibration results include the position-dependent uniformity, and instrument response over the 1600-8000 angstrom operational range. Because the UVOT is a photon-counting instrument, we also discuss the effect of coincidence loss on the calibration results. We provide practical guidelines for using the calibration in UVOT data analysis. The results presented here supersede previous calibration results.
dc.language.isoeng
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectAstronomy and Astrophysics
dc.subjectSpace and Planetary Science
dc.subjectGeneral Physics and Astronomy
dc.subjectPhysics and Astronomy (miscellaneous)
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectPhysical Sciences
dc.titlePhotometric calibration of the Swift ultraviolet/optical telescope
dc.typeMakale
dc.relation.journalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.contributor.departmentUniversity Of London , ,
dc.identifier.volume383
dc.identifier.issue2
dc.identifier.startpage627
dc.identifier.endpage645
dc.contributor.firstauthorID3375313


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