The Calibration of theSwiftUVOT Optical Observations: A Recipe for Photometry
The Ultraviolet/Optical Telescope (UVOT) on boardSwifthas the capability to provide critical insight into the physics of the early afterglows of gamma‐ray bursts (GRBs). But without precise calibration of the UVOT to standard photometric systems, it is impossible to leverage late‐time, ground‐based...
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Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 2006-01, Vol.118 (839), p.37-61 |
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Sprache: | eng ; jpn |
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Zusammenfassung: | The Ultraviolet/Optical Telescope (UVOT) on boardSwifthas the capability to provide critical insight into the physics of the early afterglows of gamma‐ray bursts (GRBs). But without precise calibration of the UVOT to standard photometric systems, it is impossible to leverage late‐time, ground‐based follow‐up data to the early‐time UVOT observations. In this paper, we present a calibration of theSwiftUVOT photometry to the standard JohnsonUBVsystem for the UVOTU,B, andVfilters, and a step‐by‐step photometry recipe for analyzing these data. We base our analysis on aperture photometry performed on the ground‐based and UVOT observations of the local standard stars in the fields of supernovae (SNe) 2005am and 2005cf and a number of Landolt standard stars. We find that the optimal photometry aperture radius for UVOT data is small (2
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\documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document |
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ISSN: | 0004-6280 1538-3873 |
DOI: | 10.1086/498356 |