J/MNRAS/421/2692 Optical/near-IR observations of GRB 080310 (Littlejohns+, 2012)

The origin of the early-time optical emission of Swift GRB 080310. Littlejohns O.M., Willingale R., O'Brien P.T., Beardmore A.P., Covino S., Perley D.A., Tanvir N.R., Rol E., Yuan F., Akerlof C., D'Avanzo P., Bersier D.F., Castro-Tirado A.J., Christian P., Cobb B.E., Evans P.A., Filippenko A.V., Flewelling H., Fugazza D., Hoversten E.A., Kamble A.P., Kobayashi S., Li W., Morgan A.N., Mundell C.G., Page K., Palazzi E., Quimby R.M., Schulze S., Steele I.A., de Ugarte Postigo A. <Mon. Not. R. Astron. Soc., 421, 2692-2712 (2012)> =2012MNRAS.421.2692L 2012MNRAS.421.2692L
ADC_Keywords: Gamma rays ; Photometry Keywords: gamma-ray burst: individual: GRB 080310 Abstract: We present broad-band multiwavelength observations of GRB 080310 at redshift z=2.43. This burst was bright and long-lived, and unusual in having extensive optical and near-infrared (IR) follow-up during the prompt phase. Using these data we attempt to simultaneously model the gamma-ray, X-ray, optical and IR emission using a series of prompt pulses and an afterglow component. Description: On 2008 March 10 the Swift Burst Alert Telescope (BAT) triggered and located GRB 080310 (trigger number 305288) on board at 08:37:58 UT (Cummings et al., 2008GCN..7382....1C 2008GCN..7382....1C). Swift slewed immediately which enabled the narrow field instruments to begin observing the burst 89s after the trigger. The burst was detected by the XRT and UVOT (white filter), with the latter providing the best Swift position of RA=14:40:13.80 and DE=-00:10:29.8 (J2000) with a 1σ error radius of 0.6 arcsec. In addition to Swift observations, and those instruments already mentioned, GRB 080310 was also observed on the ground with numerous optical and near-infrared (NIR) facilities, including Rapid Eye Mount (REM), Very Large Telescope (VLT) and the Faulkes Telescope North (FTN). Objects: ---------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------- 14 40 13.89 -00 10 30.4 GRB 080310 = XRF 080310 ---------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tables.dat 99 504 All near infrared and optical observations (tables A1-A8 of the paper) -------------------------------------------------------------------------------- See also: J/ApJ/693/1484 : Early optical afterglow catalog (Cenko+, 2009) J/ApJ/720/1513 : The afterglows of Swift-era GRBs. I. (Kann+, 2010) Byte-by-byte Description of file: tables.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 A2 --- Tab Table number (1) 4- 9 I6 s Time Central time after trigger of each exposure 11- 15 I5 s Texp Exposure time 17- 29 A13 --- Filter Filter (2) 31- 44 A14 --- Inst Instrument 45- 51 F7.2 uJy Flux Exctinction corrected flux 53- 58 F6.2 uJy e_Flux rms uncertainty on Flux 60- 99 A40 --- Ext External sources -------------------------------------------------------------------------------- Note (1): Calibration band as follows: A1 = All near infrared observations which were calibrated to the K-band A2 = All near infrared observations which were calibrated to the H-band A3 = All near infrared observations which were calibrated to the J-band A4 = All optical observations which were calibrated to the I-band A5 = All optical observations which were calibrated to the R-band A6 = All optical observations which were calibrated to the V-band A7 = All optical observations which were calibrated to the b-band A8 = All optical observations which were calibrated to the u-band Note (2): The filters quoted are the original filters that observations were taken, before conversion to the standard filters used in the later analysis. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 05-Mar-2013
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