A Large Catalog of Homogeneous Ultra-Violet/Optical GRB Afterglows: Temporal and Spectral Evolution
arXiv:1701.03713 · doi:10.3847/1538-4365/228/2/13
Abstract
We present the second Swift Ultra-Violet/Optical Telescope (UVOT) gamma-ray burst (GRB) afterglow catalog, greatly expanding on the first Swift UVOT GRB afterglow catalog. The second catalog is constructed from a database containing over 120,000 independent UVOT observations of 538 GRBs first detected by Swift, the High Energy Transient Explorer 2 (HETE2), the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL), the Interplanetary Network (IPN), Fermi, and Astro-rivelatore Gamma a Immagini Leggero (AGILE). The catalog covers GRBs discovered from 2005 Jan 17 to 2010 Dec 25. Using photometric information in three UV bands, three optical bands, and a `white' or open filter, the data are optimally co-added to maximize the number of detections and normalized to one band to provide a detailed light curve. The catalog provides positional, temporal, and photometric information for each burst, as well as Swift Burst Alert Telescope (BAT) and X-Ray Telescope (XRT) GRB parameters. Temporal slopes are provided for each UVOT filter. The temporal slope per filter of almost half the GRBs are fit with a single power-law, but one to three breaks are required in the remaining bursts. Morphological comparisons with the X-ray reveal that approximately 75% of the UVOT light curves are similar to one of the four morphologies identified by Evans et al. (2009). The remaining approximately 25% have a newly identified morphology. For many bursts, redshift and extinction corrected UV/optical spectral slopes are also provided at 2000, 20,000, and 200,000 seconds.
44 pages, 14 figures, to be published in Astrophysical Journal Supplemental
References in corpus (16)
- Gamma-Ray Bursts: Progress, Problems & Prospects
- The First Swift BAT Gamma-Ray Burst Catalog
- A statistical study of gamma-ray burst afterglows measured by the Swift Ultra-violet Optical Telescope
- The First Swift Ultra-Violet/Optical Telescope GRB Afterglow Catalog
- Correlations of Prompt and Afterglow Emission in Swift Long and Short Gamma Ray Bursts
- Accurate early positions for Swift GRBS: enhancing X-ray positions with UVOT astrometry
- GRB 060313: A New Paradigm for Short-Hard Bursts?
- Refined Astrometry and Positions for 179 Swift X-ray Afterglows
- GRB 090902B: afterglow observations and implications
- Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst
- The Two-Component Afterglow of Swift GRB 050802
- The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125
- The measurement errors in the Swift-UVOT and XMM-OM
- The exceptionally extended flaring activity in the X-ray afterglow of GRB 050730 observed with Swift and XMM-Newton
- The dark nature of GRB 130528A and its host galaxy
- Optimal Coaddition of Imaging Data for Rapidly Fading Gamma-Ray Burst Afterglows
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- Swift/UVOT: 18 Years of Long GRB Discoveries and Advances
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- A study of gamma-ray burst afterglows as they first come into view of the Swift Ultraviolet and Optical Telescope
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