J/AJ/141/36 GRB 080607 multi-band light curves (Perley+, 2011) ================================================================================ Monster in the dark: the ultraluminous GRB 080607 and its dusty environment. Perley D.A., Morgan A.N., Updike A., Yuan F., Akerlof C.W., Miller A.A., Bloom J.S., Cenko S.B., Li W., Filippenko A.V., Prochaska J.X., Kann D.A., Tanvir N.R., Levan A.J., Butler N.R., Christian P., Hartmann D.H., Milne P., Rykoff E.S., Rujopakarn W., Wheeler J.C., Williams G.G. =2011AJ....141...36P ================================================================================ ADC_Keywords: Gamma rays ; Photometry, UBVRI ; Photometry, infrared Keywords: dust, extinction - gamma-ray burst: individual (080607) Abstract: We present early-time optical through infrared photometry of the bright Swift gamma-ray burst (GRB) 080607, starting only 6s following the initial trigger in the rest frame. Complemented by our previously published spectroscopy, this high-quality photometric data set allows us to solve for the extinction properties of the redshift 3.036 sightline, giving perhaps the most detailed information to date on the ultraviolet continuum absorption properties of any sightline outside our Local Group. Description: GRB 080607 triggered the Burst Alert Telescope on the Swift satellite at 06:07:27 on 2010 June 7 (UT dates are used throughout this paper; times are referenced to this trigger time, although it is important to note that there was significant emission before this trigger). Objects: ---------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------- 12 59 47.14 +15 55 09.6 GRB 080607 = GRB 080607 ---------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 69 146 Photometry of GRB 080607 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Tel Telescope name (1) 12- 17 F6.1 s tmid Exposure mid-time (2) 19- 23 A5 --- Filt Filter used (3) 25- 30 F6.1 s Exp ? Exposure time 32- 33 A2 --- l_mag [>=] Limit flag on mag 35- 40 F6.3 mag mag Observed & uncorrected magnitude in Filt 42- 46 F5.3 mag e_mag ? Uncertainty in mag 48 A1 --- n_mag [X] Indicates mag not used in modeling 50- 51 A2 --- l_Flux [<=] Limit flag on Flux 52- 60 F9.3 uJy Flux Observed flux density in Filt (4) 62- 69 F8.3 uJy e_Flux ? Uncertainty in Flux -------------------------------------------------------------------------------- Note (1): Telescope names as follows: P60 = Palomar 60 inch telescope KAIT = Katzman Automatic Imaging Telescope (KAIT) at Lick Observatory ROTSE = Robotic Optical Transient Search Experiment at the McDonald Observatory, Texas UKIRT = United Kingdom Infrared Telescope PAIRITEL = Peters Automatic Infrared Imaging Telescope at Mt. Hopkins, AZ SuperLOTIS = Livermore Optical Transient Imaging System at teward Observatory Kitt Peak site near Tucson, AZ. Note (2): Measured from the Swift trigger (UT 06:07:27). Note (3): KAIT and ROTSE unfiltered measurements are calibrated to R. UKIRT K-band measurements are calibrated to Ks. Filters used: V, R, I, J, H, K, Ks, i, z and clear. Note (4): Corrected for Galactic extinction (E(B-V)=0.023mag). -------------------------------------------------------------------------------- History: From electronic version of the journal ================================================================================ (End) Greg Schwarz [AAS], Patricia Vannier [CDS] 24-Jul-2012