//////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3523 SUBJECT: GRB050607: prompt REM observations DATE: 05/06/07 10:19:12 GMT FROM: Stefano Covino at Brera Astronomical Observatory V. Testa, D. Fugazza, S. Covino, S. Campana, E. Molinari, F.M. Zerbi, G. Chincarini, M. Rodono', G. Tosti, L.A. Antonelli, P. Conconi, G. Cutispoto, L. Nicastro, E. Palazzi, F. Vitali, E. Meurs, P. Goldoni, on behalf of the REM/ROSS Team We imaged the field of GRB050607 with the robotic 60-cm REM telescope located at La Silla, Chile. Observations were performed in fully automated mode simultaneously in the near infrared and in the optical, starting approximately 47 seconds after the alert. REM is equipped with the REMIR near infrared camera (10x10 sq arcmin FoV, JHK filters) and the ROSS optical spectrograph/imager (10x10 sq arcmin FoV, VRI filters and AMICI prism). Observations were performed under good seeing conditions. A quick-look analysis does not reveal any new bright object in H band down to approximately the 15th magnitude. This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3524 SUBJECT: GRB050607: P60 Observations DATE: 05/06/07 10:39:41 GMT FROM: Derek Fox at CIT D.B. Fox and S.B. Cenko report on behalf of the Caltech-NRAO-Carnegie GRB collaboration: "We have observed the BAT localization region for GRB050607 with the Robotic P60 in a sequence of exposures beginning at 09:29 UT, approximately 18 minutes after the burst. Inspection of our initial R-band (epoch 09:29) and i-band (09:34 UT) images reveals no bright new sources to the limit of the USNO-B1.0 catalog, R < 19 mag." //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3525 SUBJECT: GRB050607: Swift Detection of a long GRB DATE: 05/06/07 12:07:33 GMT FROM: Alon Retter at PSU A. Retter, J. Racusin, J. Kennea, D. Burrows (PSU), D. Palmer (LANL), K. McGowan (MSSL), J. Cummings (NRC/GSFC), S. Barthelmy, N. Gehrels (GSFC) on behalf of the Swift Team report: At 09:11:23 UT the Swift-BAT triggered on GRB 050607 (trigger 132247). The BAT refined ground position is RA, Dec 300.167, +9.137 (J2000) {20h00m40s, +09d 08' 13"}. The burst had 3 peaks over 30 seconds, with a T90 of 26.5 seconds from T+0 to T+26.5 seconds. Its spectrum is well fit by a simple power law with an index of 1.93 +/- 0.14. The total fluence was (8.9 +/- 1.2) x 10^-7 erg/cm2 over 15-350 keV. The peak flux was 1.15+/-0.16 photons/cm2/s from T+1 to T+2 seconds. The burst was 27 degrees off the BAT boresight in the 87% coded field of view. Swift slewed to the position of the burst immediately, starting 17 seconds after the burst trigger. The XRT was pointed promptly at the burst at 09:13:02 UT (100 s after the BAT burst trigger). The XRT did not centroid on-board, but ground analysis revealed a bright X-ray source near the center of the field of view, with position RA(J2000) = 20h 00m 42.5s Dec(J2000) = +09d 08' 30'' We estimate an uncertainty of approximately 8 arcseconds radius (90% containment). This position is 40 arcseconds from the BAT position. Immediate data from UVOT will not be available due to the instrument being in an engineering mode. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3526 SUBJECT: GRB050607 optical limit by "Pi of the Sky" DATE: 05/06/07 12:21:26 GMT FROM: Grzegorz Wrochna at Soltan Inst.for Nuclear Studies M.Cwiok, K.Krupska, K.Kwiecinska, L.Mankiewicz, M.Molak, K.Nawrocki, L.W.Piotrowski, M.Sokolowski, J.Uzycki, G.Wrochna, on behalf of "Pi of the Sky" collaboration http://grb.fuw.edu.pl "Pi of the Sky" apparatus has moved to the Swift-BAT trigger 132247 and it has taken series of 10s exposures starting 60s after the GRB (40s after the alert). No new object has been found within the Swift-BAT error box. The limiting magnitude is 11.5m (unfiltered) for single exposures and 12.5m for the sum of 10 images. However, the GRB counterpart might be hidden in the glow of 10.2m star GSC 01071-00926 (BD +8 4298), which is within the error box. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3527 SUBJECT: Optical Afterglow of GRB 050607 DATE: 05/06/07 13:16:16 GMT FROM: James Rhoads at STScI James Rhoads reports on behalf of a larger collaboration: I observed the field of GRB 050607 with the 4m Mayall Telescope at Kitt Peak, starting on 2005 June 7 UT 09:20:46. Observations continued until morning twilight at 11:18 UT. We detect a faint, fading optical source located at 20:00:42.79 +09:08:31.5 (J2000), about 8 arcseconds from the XRT source. We calibrated astrometry to the nearby USNO star, located at 20:00:42.70 9:08:35.0. Our *relative* astrometry should be good to < 0.5". The approximate I band magnitude is 22.65 (statistical error is 0.1 mag, systematic error is 0.2-0.3 mags) in our first exposure, which was 150 seconds commencing 563 seconds after the burst. Further analysis of the multiwavelength data set is in progress. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3528 SUBJECT: GRB 050607 - XRT refined data analysis DATE: 05/06/07 16:56:15 GMT FROM: Claudio Pagani at PSU/Swift-XRT C.Pagani, D. Grupe, D. Burrows, J. Kennea, J. Racusin (PSU), and N Gehrels (GSFC), on behalf of the Swift XRT team report: We analyzed the XRT data of the first two orbits of GRB 050607 (Retter et al., GCN #3525). The observations started at 09:13:02 UT (100 s after the BAT burst trigger). Preliminary analysis of the data obtained in the first 4.2ks of observations gives the following refined coordinates for the X-ray afterglow: Ra-2000: 20h 00m 42.6s Dec-2000: 09d 08' 26.9" The centroiding error is 6" radius (90%containment). This position is about 5" from the optical afterglow position reported by Rhoads (GCN #3527) and 3" from the previously reported XRT position (Retter et al., GCN #3525). The X-ray spectrum can be fitted with a single powerlaw with an X-ray photon index=1.86+/-0.44. The fit is consistent with Galactic absorption (NH=1.41e21 cm-2). The lightcurve has a peak around 310sec after the burst trigger. The source had a unabsorbed flux of 1.6e-12 ergs/s/cm2 at approximately one hour after the burst and is decaying with a decay slope alpha=0.58+/-0.12. This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3529 SUBJECT: GRB050607,optical observation DATE: 05/06/07 17:10:09 GMT FROM: Shouta Maeno at U.of Miyazaki Y.Tokunaga,S.maeno,E.sonoda,M.Yamauchi (University of Miyazaki) "We have observed the field covering the error circle of GRB 050607 (GCN3525 ; Swift BAT Trigger time is 09:11:23 UT) with the unfiltered CCD camera on the 30-cm telescope at University of Miyazaki. The observation was started 14:54:24 UT on June.07. We have compared with the USNO A2.0 catalog. Preliminary analysis shows there is no new source brighter than 16.5 mag at the position reported by J.Rhoads et al.(GCN 3527)" //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3530 SUBJECT: GRB 050607: MDM Observations DATE: 05/06/07 17:51:25 GMT FROM: Jules Halpern at Columbia U. J. P. Halpern (Columbia), J. Kemp (Joint Astronomy Centre and Columbia), and N. Mirabal (U. Michigan), report on behalf of the MDM Observatory GRB follow-up team: We monitored the location of Swift GRB 050607 and its decaying X-ray afterglow (Retter et al., GCN #3525; Pagani et al., GCN #3528) in the R band with the MDM 2.4m telescope beginning 16 minutes after the trigger, and extending to 2 hours. Seeing was approximately 1.1". The afterglow candidate discovered by Rhoads (GCN #3527) is present in all of our images with 22.5 < R < 23, and appears to have faded. However, it is difficult for us to characterize its variability at this stage in the analysis as there may also be extended emission. If correct, this is the faintest optical afterglow detected at the equivalent time (Berger et al., astro-ph/0502468), even taking into account the 0.4 magnitudes of R-band Galactic absorption in this direction. Images are posted at http://www.astro.columbia.edu/~jules/grb/050607/ //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3531 SUBJECT: GRB 050607: Optical decay and spectral slope DATE: 05/06/07 18:26:06 GMT FROM: James Rhoads at STScI James Rhoads reports on behalf of a larger collaboration: We have measured the flux of the GRB 050607 optical afterglow (Rhoads 2005, GCNC 3527) in our five I band images from t=640 to t=6330 seconds post-burst. A power law decay with slope -0.5 gives a marginally acceptable fit to the I band light curve. A better fit can be obtained by a two-part power law, with an initial steep decay (exponent near -1) up to t ~ 1700 seconds, followed by a flatter decay (exponent near -0.3) from 1700 to 6300 seconds. The overall optical decay slope is in good agreement with the X-ray slope reported by Pagani et al (GCNC 3528). We also obtained images of Landolt standard field SA 113. We found a zero point error in our earlier photometry (GCNC 3527). Our new zero point based on our standard star observations gives a brighter afterglow magnitude at t=640 seconds: I = 21.46 +- 0.1 (statistical) +- 0.3 (systematic) The remaining systematic error will go away with a more careful reduction. As a consistency check we find magnitude I=16.2 for the star USNO 0975-17511046 (our astrometric reference at 20:00:42.703 +9:08:34.98), which has USNO tabulated magnitude Rmag=16.6 and B-R=0.7. In addition to our I band data, we also monitored the burst in B band and took smaller amounts of data in R, z, and g. All data discussed here were obtained with the Mosaic 1 camera on the 4m Mayall Telescope of the Kitt Peak National Observatory. Observations started at 2005 June 7 UT 09:20:46, and continued until 11:18 UT. The transient is faint in the B filter. Our first B band epoch, of 150 seconds centered at t=1384 seconds, does not show the afterglow clearly. A formal aperture flux measurement at the transient location yields flux 0.7 +- 0.25 microJansky, or B ~ 24.4 +- 0.4. This gives an estimated spectral power law slope of f_nu ~ nu^-1.5 or steeper, where we have accounted for the Galactic reddening based on the Schlegel et al prediction (A_V = 0.6 mag, E(B-I) = 0.44 mag). The faint B image is thus suggestive of a Lyman break in the spectrum, though we cannot rule out a red power law with our present analysis. We detect the transient at R band, placing a rough redshift bound z<5, We do not detect it in our less sensitive z band images (suggesting that the power law slope is not extremely red). An I band finding chart and light curve are now available at http://www.stsci.edu/~rhoads/GRB050607/ . //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3535 SUBJECT: GRB 050607: PROMPT VRcIc Observations DATE: 05/06/08 00:25:17 GMT FROM: Melissa Nysewander at UNC,Chapel Hill M. Nysewander, D. Reichart, J. A. Crain, A. Foster, M. Bayliss report on behalf of the UNC team of the FUN GRB Collaboration: We observed the BAT localization of GRB 050607 (Retter et al., GCN 3525) with PROMPT beginning 13m 30s after the burst. We do not detect a source within the refined XRT localization (Pagani et al., GCN 3528) nor the source identified by Rhoads (GCN 3527). 3-sigma limiting magnitudes are based on 10 USNO-B1.0 stars for Rc and Ic observations and 10 NOMAD stars for V observations. Initial limiting magnitudes are poor due to a camera cooling error: Mean Time Integration Filter Limiting Telescope Since GRB Time Magnitude 14m 08s 1 x 77.5s Ic 17.5 PROMPT-5 17m 43s 2 x 77.5s V 18.4 PROMPT-5 21m 16m 1 x 77.5s Rc 19.7 PROMPT-5 24m 06s 1 x 77.5s Ic 19.2 PROMPT-5 26m 21s 2 x 77.5s V 19.5 PROMPT-5 29m 51s 3 x 76.25s Rc 20.5 PROMPT-5 36m 17s 4 x 76.25s Ic 20.2 PROMPT-5 41m 48s 3 x 76.25s V 19.4 PROMPT-5 47m 17s 2 x 76.25s Rc 20.3 PROMPT-5 51m 25s 1 x 76.25s Ic 19.4 PROMPT-5 Stacking all images yields 3-sigma limiting magnitudes of Ic > 20.5, Rc > 21.2, and V > 19.8. PROMPT is still being built and commissioned. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3534 SUBJECT: GRB 050607: RAPTOR-S Early Optical Limits DATE: 05/06/08 00:11:19 GMT FROM: James Wren at LANL J. Wren, W. T. Vestrand, P. Wozniak, R. White, S. Evans report on behalf of the RAPTOR team at Los Alamos National Laboratory: The RAPTOR-S telescope responded robotically to GRB 050607 (Swift trigger 132247, GCN #3525). The first exposure began at 09:11:49.97 UT, 27.17 seconds after the trigger time and during the third peak in the 15-350 keV light curve of the GRB. Observations continued through morning twilight which began approximately 90 minutes later. Vibrations due to high winds degraded the quality of several of the response images. We do not detect the optical counterpart reported by Rhoads (GCN #3527). We are able to place the following limits on the early optical afterglow based on calibration to the USNO-A2.0 R-band (times are seconds since trigger): mag | mid-exposure | start | end | exposure limit | time | time | time | duration --------------------------------------------------------------------- 15.6 | 32.17 | 27.17 | 37.17 | 10 17.8 | 42.79 | 47.79 | 57.79 | 10 18.5 | 108.66 | 47.79 | 220.46 | 70 (sum of 7 10s images) 18.0 | 248.94 | 233.94 | 263.94 | 30 18.9 | 390.27 | 233.94 | 627.29 | 180 (sum of 6 30s images) 18.2 | 741.18 | 711.18 | 771.18 | 60 19.2 | 1303.89 | 711.18 | 1615.55 | 360 (sum of 6 60s images) //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3533 SUBJECT: GRB050607: KAIT optical limits DATE: 05/06/07 23:16:04 GMT FROM: Weidong Li at UC Berkeley KAIT/LOSS W. Li, R. Chornock, S. Jha, and A. V. Filippenko, University of California, Berkeley, report: "The robotic 0.76-m Katzman Automatic Imaging Telescope (KAIT) at Lick Observatory observed GRB050607 detected with Swift (Retter et al., GCN 3525). A series of images was automatically obtained from 09:12:12 UT (49s after the burst) to 10:10:19 UT (3536s after the burst) The sequence includes a combination of images taken with the V and I filters, as well as some that are unfiltered. We did not detect the optical afterglow as reported by Rhoads (GCN 3527, 3531) and Halpern et al. (GCN 3530). Our first 15s unfiltered image started at 49s after the burst has a limiting magnitude of about 18.4 when compared to the USNO-B1.0 catalog, while a combined unfiltered image centered at 09:16:13 UT (290s after the burst) has a limiting mag of about 19.6. " This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3536 SUBJECT: GRB 050607 : Lulin R-band observation DATE: 05/06/08 09:39:12 GMT FROM: Kuiyun Huang at IANCU GRB 050607 : Lulin R-band observation C.W. Chen (NCU), K.Y. Huang, W.H. Ip (NCU), Y. Urata(RIKEN), Y. Qiu (BAO), Y.Q. Lou (THCA) on behalf of EAFON report: " We have imaged the entire error region of GRB 050607 (Retter et al. GCN 3525) by using 1.0-m telescope at Lulin Observatory, Taiwan. The R band observations started at 16.14 UT ( about 6.95 hours after the burst). No source was detected at the X-ray afterglow position ( Pagani et al. GCN 3528). The limiting magnitude of our R band co-added image ( 300sec x 8) is 21.1 by comparing with USNOB1.0 stars. This message may be cited." //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3537 SUBJECT: Swift/UVOT observations of GRB050607 DATE: 05/06/08 10:58:45 GMT FROM: Alexander Blustin at MSSL-UCL Ivanushkina, M., Retter, A. (PSU), McGowan, K., Blustin, A. (MSSL), Gehrels, N. (NASA/GSFC) on behalf of the Swift UVOT team The Swift Ultra-Violet/Optical Telescope (UVOT) began observations of GRB050607 on June 7, 2005 at 22:36:23 UT, ~12 hours and 25 minutes after the initial Swift BAT trigger (Retter et al., GCN 3525) as an uploaded ToO. Immediate data from UVOT were not available due to the instrument being in an engineering mode. No optical counterpart is detected at the afterglow position (Rhoads, GCN 3527) in summed images from any filter down to the following 3-sigma upper limits: Filter 3-sig UL Exposure (s) T_mid (s) V 20.21 2036 51530 B 20.95 897 46942 U 20.18 771 42806 UVW1 20.95 900 41963 UVM2 21.33 1482 46727 UVW2 21.30 900 47844 Where T_mid is the mid-time of the summed exposure in seconds after the BAT trigger. The magnitudes are based on preliminary zero-points, measured in orbit, and will require refinement with further calibration. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3538 SUBJECT: GRB050607: refined analysis of prompt REM observations DATE: 05/06/08 12:42:48 GMT FROM: Vincenzo Testa at INAF/Astro. Obs. of Rome V. Testa, E. Palazzi, P. D'Avanzo, L.A. Antonelli, E. Molinari, D. Fugazza, S. Covino, S. Campana, F.M. Zerbi, G. Chincarini, M. Rodono', G. Tosti, P. Conconi, G. Cutispoto, L. Nicastro, F. Vitali, E. Meurs, P. Goldoni, on behalf of the REM/ROSS Team We refined the analysis of the field of GRB050607 observed with the REM telescope (GCN 3523) in fully automated mode simultaneously in the near infrared and in the optical. Two R-band 3s exposures and five H-band 10s exposures have been re-analyzed to search for new objects at the positions reported by Rhoads (GCN 3527) and Pagani et al. (GCN 3528). We confirm the non-detection reported in GCN 3523 and derived upper limits at 3 sigma level (see the table below). The UT differences between optical and IR acquisitions are due to different overheads and observing strategies adopted by the two instruments. Filter Instrument UT t_exp Time_from_burst Mag. Upper Limit -------------------------------------------------------------------------- R ROSS 09:14:49 6s 207s 17.1 H REMIR 09:14:34 50s 192s 16.0 Observations were performed under moderate seeing conditions, the La Silla DIMM giving an instantaneous value of 1.5 arcsec, and in photometric conditions. Magnitudes have been calibrated with a set of stars around the position of the optical detection (GCN 3527) extracted from the 2MASS catalog for the H filter and from the USNO B1.0 catalog for the R filter. This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3539 SUBJECT: GRB 050607: RTT150 optical observations DATE: 05/06/08 15:22:37 GMT FROM: Rodion Burenin at IKI, Moscow R. Zhuchkov, I. Bikmaev, N. Sakhibullin (KSU/AST), R. Burenin, M. Pavlinsky, R. Sunyaev (IKI), Z. Aslan, I. Khamitov (TUG), U. Kiziloglu (METU), A. Alpar (Sabanci Uni.) report: We observed the error box of GRB 050607 (Retter et al., GCN 3525) with Russian-Turkish 1.5-m telescope (RTT150, Bakyrlytepe, TUBITAK National Observatory, Turkey). We made a set of 600s exposures in R and I, starting at 21:00 UT, June 07, i.e. approximately 12 hours after the burst. Observations were made under poor weather conditions (with 1.7'' seeing and cirruses). We detect nothing at the position of the OT found by Rhoads et al. (GCN 3527, 3531). The upper limits are approximately I=22.6 and R=23.7. Comparing to earlier measurements (Rhoads et al., GCN 3531) we confirm that the source is fading. This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3540 SUBJECT: GRB 050607 optical decay DATE: 05/06/09 03:20:22 GMT FROM: James Rhoads at STScI James Rhoads reports on behalf of a larger collaboration: We observed the afterglow of GRB 050607 with the 4m Mayall Telescope of Kitt Peak National Observatory from UT 2005 June 8 10:33 to 11:05. We obtained three I band exposures with total integration time of 26 minutes. The GRB counterpart is weakly detected in the sum of the three images, with a statistical error around 0.2 to 0.25 magnitudes. Relative photometry with respect to a nearby field star shows that the transient has faded by 2.3 +- 0.2 magnitudes between t=640 seconds and t=92300 seconds post-trigger. Based on a power law fit to the night 1 data (Rhoads, GCNC 3531), with decay slope 0.5, we would expect a fading of 2.9 magnitudes over the same period. This suggests that host galaxy light may be contributing detectably to our most recent flux measurement. However, the statistical significance of this excess is low. A single power law fit to the combined night one and night two data has a time decay slope of 0.4 and nearly acceptable residuals. If we exclude the first point (t=640 seconds) from the fit, on the supposition that the physics dominating the afterglow changed around 1e3 seconds, the decay slope in our other UT 050607 data becomes 0.3 and the UT 050608 point lies precisely on this shallow, extrapolated decay. Additional data would help distinguish among these possibilities, and further monitoring is encouraged. //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3541 SUBJECT: GRB 050607: MDM Observation DATE: 05/06/09 16:44:29 GMT FROM: Jules Halpern at Columbia U. J. P. Halpern (Columbia), J. Kemp (Joint Astronomy Centre and Columbia), and N. Mirabal (U. Michigan), report on behalf of the MDM Observatory GRB follow-up team: We reobserved the afterglow of GRB 050607 in the R band with the MDM 2.4m telescope for 30 minutes starting on June 8 08:15 UT, 23 hr after the burst. Seeing was approximately 1.1", similar to the previous night. An upper limit of R > 24.0 for a point source is found at the position of the afterglow. The possible host galaxy (Rhoads, GCN #3540) would be difficult to quantify in our image due to the nearby bright star. See http://www.astro.columbia.edu/~jules/grb/050607/ //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3555 SUBJECT: GRB 050607, radio observations DATE: 05/06/28 22:26:45 GMT FROM: Dale A. Frail at NRAO P. B. Cameron, and A. M. Soderberg (Caltech) report on behalf of the Caltech-NRAO-Carnegie collaboration: "We observed the field of GRB 050607 (GCN 3525) with the Very Large Array at 8.5 GHz on June 8.21, 9.50 and 19.45 UT, and once at 4.9 GHz on June 9.50 UT. No radio source is detected at the position of the optical afterglow (GCN 3527) with 2-sigma limits of 50-80 microJy at 8.5 GHz and 90 microJy at 4.9 GHz." //////////////////////////////////////////////////////////////////////// TITLE: GCN GRB OBSERVATION REPORT NUMBER: 3855 SUBJECT: GRB050525, GRB050607, GRB050802 BVRcIc field photometry DATE: 05/08/22 15:26:26 GMT FROM: Arne A. Henden at AAVSO A. Henden (AAVSO/USNO) reports on behalf of the USNO GRB Team: We have acquired BVRcIc all-sky photometry for 23x23arcmin fields centered on the coordinates of recent GRB localizations with the USNOFS 1.0-m telescope on 1 or 2 photometric nights but with bright moonlight and variable seeing. Stars brighter than V=12.0 are saturated and should be used with care. We have placed the photometric data on our anonymous ftp site: ftp://ftp.nofs.navy.mil/pub/outgoing/aah/grb/grb050525.dat ftp://ftp.nofs.navy.mil/pub/outgoing/aah/grb/grb050607.dat ftp://ftp.nofs.navy.mil/pub/outgoing/aah/grb/grb050802.dat The astrometry in these files is based on linear plate solutions with respect to UCAC2 or USNO-A2.0. The external errors are usually 200mas or better. The estimated external photometric error is about 0.03mag. Some fields are relatively crowded, and the large apertures required to handle the variable seeing also blended some measurements, so choose comparison stars wisely. We have one additional night for GRB050525 that will be added when reductions are complete. As always, you should check the dates on the .dat file prior to final publication to get the latest photometry. There is a README file on the ftp directory to give you information about the procedures used to calibrate these fields.