//////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9718 SUBJECT: GRB 090727: Swift detection of a burst DATE: 09/07/27 22:59:22 GMT FROM: Scott Barthelmy at NASA/GSFC P. A. Evans (U Leicester), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), A. P. Beardmore (U Leicester), M. M. Chester (PSU), S. T. Holland (CRESST/USRA/GSFC), N. P. M. Kuin (MSSL), C. B. Markwardt (CRESST/GSFC/UMD), K. L. Page (U Leicester), A. Rowlinson (U Leicester), M. H. Siegel (PSU), M. A. Stark (PSU) and T. N. Ukwatta (GSFC/GWU) report on behalf of the Swift Team: At 22:42:18 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 090727 (trigger=358520). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 315.972, +64.916 which is RA(J2000) = 21h 03m 53s Dec(J2000) = +64d 54' 58" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows a single peak with a duration of about 25 sec. The peak count rate was ~1000 counts/sec (15-350 keV), at ~1 sec after the trigger. The XRT began observing the field at 22:43:46.0 UT, 87.9 seconds after the BAT trigger. Using promptly downlinked data we find an uncatalogued X-ray source located at RA, Dec 315.96139, 64.92438 which is equivalent to: RA(J2000) = 21h 03m 50.73s Dec(J2000) = +64d 55' 27.8" with an uncertainty of 4.0 arcseconds (radius, 90% containment). This location is 34 arcseconds from the BAT onboard position, within the BAT error circle. This position may be improved as more data are received; the latest position is available at http://www.swift.ac.uk/sper. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density consistent with the Galactic value of 2.48e+21 cm^-2 (Kalberla et al. 2005). UVOT took a finding chart exposure of nominal 150 seconds with the White filter starting 91 seconds after the BAT trigger. No credible afterglow candidate has been found in the initial data products. Data from the 2.7'x2.7' sub-image are not available at this time. The 8'x8' region for the list of sources generated on-board covers 100% of the XRT error circle. The list of sources is typically complete to about 18 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.54. Burst Advocate for this burst is P. A. Evans (pae9 AT star.le.ac.uk). Please contact the BA by email if you require additional information regarding Swift followup of this burst. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone (see Swift TOO web site for information: http://www.swift.psu.edu/too.html.) //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9719 SUBJECT: GRB 090727: Liverpool Telescope possible OT candidate DATE: 09/07/28 02:19:38 GMT FROM: James Smith at ARI,Liverpool John Moors U R.J. Smith, C.G. Mundell (Liverpool JMU) on behalf of a large collaboration report: The 2-m Liverpool Telescope robotically reacted to GRB 090727 (SWIFT trigger 358520, Evans et al, GCN Circ. 9718), starting observing at 22:44:59UTC. A source which is not visible in the digitized sky survey is detected in both SDSS r' and i' filters at position 21:03:50.6 +64:55:30 J2000. This lies within the XRT error circle reported by Evans et al, GCN Circ. 9718. The approximate magnitude, calibrated with respect to nearby USNOB stars is R=21.3 +/- 0.2 and I = 20.2 +/- 0.2. The target is slightly crowded by brighter stellar sources and analysis is ongoing to determine if the OT candidate is fading. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9721 SUBJECT: GRB 090727: Enhanced Swift-XRT position DATE: 09/07/28 09:53:03 GMT FROM: Phil Evans at U of Leicester M.R. Goad, J.P. Osborne, A.P. Beardmore and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team. Using 5314 s of XRT Photon Counting mode data and 7 UVOT images for GRB 090727, we find an astrometrically corrected X-ray position (using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue): RA, Dec = 315.96078, +64.92481 which is equivalent to: RA (J2000): 21h 03m 50.59s Dec (J2000): +64d 55' 29.3" with an uncertainty of 1.6 arcsec (radius, 90% confidence). This position may be improved as more data are received. The latest position can be viewed at http://www.swift.ac.uk/xrt_positions. Position enhancement is described by Goad et al. (2007, A&A, 476, 1401) and Evans et al. (2009, arXiv:0812.3662). This circular was automatically generated, and is an official product of the Swift-XRT team. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9722 SUBJECT: GRB 090727: Liverpool Telescope Afterglow Confirmation and Optical Flare DATE: 09/07/28 10:35:59 GMT FROM: Carole Mundell at ARI, JMU,Liverpool R.J. Smith, C.G. Mundell, I.A. Steele, A. Melandri, S. Kobayashi, C.J. Mottram, D.F. Bersier, Z. Cano (Liverpool JMU), A. Gomboc (Ljubljana), C. Guidorzi (INAF-OAB) report: "Further analysis of the optical light curves of the uncatalogued optical source, at RA(J2000)=21:03:50.6, Dec(J2000)= +64:55:30, reported by Smith & Mundell (GCN Circ. 9719) show significant variability and confirm this object as the optical afterglow of GRB 090727 (SWIFT trigger 358520, Evans et al, GCN Circ. 9718; Goad et al. GCN Circ. 9721). Within the first 100 mins, the optical light curve shows an early-time flare, peaking at r'=19.4 mag, followed by a plateau and break - features that are the same as suggested by the partially sampled XRT light curve. Observations are ongoing." //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9723 SUBJECT: GRB 090727: Swift-XRT refined analysis DATE: 09/07/28 11:30:11 GMT FROM: Phil Evans at U of Leicester P. A. Evans (U Leicester) reports on behalf of the Swift-XRT team: We have analysed 11 ks of XRT data for GRB 090727 (Evans et al. GCN Circ. 9718), from 91 s to 29.2 ks after the BAT trigger. The data comprise 40 s in Windowed Timing (WT) mode from T+260 s to T+300 s, with the remainder in Photon Counting (PC) mode. The enhanced XRT position for this burst was given by Goad et al. (GCN. Circ 9721). The XRT initially observed the GRB for only 210 s before slewing away, and the data in this interval are dominated by a flare, making it impossible to determine the underlying decay rate. Fitting only the data from the second snapshot onwards (beginning at T+3.9 ks) we find a power-law decay with an index of alpha=0.73 (+/-0.19). A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.60 (+0.20, -0.14). The best-fitting absorption column is consistent with the Galactic value of 2.5 x 10^21 cm^-2 (Kalberla et al. 2005). If the light curve continues to decay with a power-law decay index of 0.73, the count rate at T+24 hours will be 0.0043 count s^-1, corresponding to an observed (unabsorbed) 0.3-10 keV flux of 2.3 x 10^-13 (2.9 x 10^-13) erg cm^-2 s^-1. The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00358520. This circular is an official product of the Swift-XRT team. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9724 SUBJECT: GRB 090727: Swift-BAT refined analysis DATE: 09/07/28 12:00:35 GMT FROM: Scott Barthelmy at NASA/GSFC C. B. Markwardt (GSFC/UMD), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (GSFC/UMBC), P. A. Evans (U Leicester), E. E. Fenimore (LANL), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), D. M. Palmer (LANL), A. M. Parsons (GSFC), T. Sakamoto (GSFC/UMBC), G. Sato (ISAS), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC), T. N. Ukwatta (GWU) (i.e. the Swift-BAT team): Using the data set from T-240 to T+962 sec from recent telemetry downlinks, we report further analysis of BAT GRB 090727 (trigger #358520) (Evans, et al., GCN Circ. 9718). The BAT ground-calculated position is RA, Dec = 315.917, 64.937 deg, which is RA(J2000) = 21h 03m 40.0s Dec(J2000) = +64d 56' 12.7" with an uncertainty of 2.2 arcmin, (radius, sys+stat, 90% containment). The partial coding was 83%. The mask-weighted light curve shows an initial FRED-like peak starting at ~T-5 sec, peaking at ~T_zero, and ending at ~T+20 sec. The second, weaker, peak starts at ~T+130 to ~T+150 sec. The third peak starts at ~T+180 sec, peaks at ~T+270 sec, and ends at ~T+320 sec. This third peak corresponds to the flare mentioned in Circ 9723 (Evans). T90 (15-350 keV) is 302 +- 23 sec (estimated error including systematics). The time-averaged spectrum from T-1.3 to T+318.9 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.24 +- 0.24. The fluence in the 15-150 keV band is 1.4 +- 0.2 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+0.12 sec in the 15-150 keV band is 0.5 +- 0.1 ph/cm2/sec. All the quoted errors are at the 90% confidence level. The results of the batgrbproduct analysis are available at http://gcn.gsfc.nasa.gov/notices_s/358520/BA/ //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9728 SUBJECT: GRB 090727: I-band observations from 1.23m CAHA DATE: 09/07/28 17:56:59 GMT FROM: Javier Gorosabel at IAA-CSIC J. Gorosabel (IAA-CSIC, Spain), N. Huelamo (LAEFF-CAB/INTA-CSIC, Spain), M. Fernandez (IAA-CSIC, Spain), M. Jelinek (IAA-CSIC, Spain), P. Kubanek (IAA-CSIC, Spain), A. de Ugarte Postigo (OAB-INAF, Italy), A.J. Castro-Tirado (IAA-CSIC, Spain), R.J. Smith (JMU, Liverpool, UK), C.G. Mundell (JMU, Liverpool, UK), on behalf of a larger collaboration, report: "We carried out I-band observations of the GRB 090727 XRT optical afterglow (Smith et al. GCN Circ. 9719; GCN Circ. 9722) with the 1.23m Calar Alto telescope. The observations were carried out on July 27.9646-28.0063 UT (0.45-1.45 hours post GRB) with an exposure time of 3600s. Very preliminary photometry yields I ~ 19.4 (Vega system) for the afterglow, against USNO B1.0 star with I=18.72 placed at (RA_J2000, DEC_J2000) = (21:03:49.099, +64:55:58.23)." //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9731 SUBJECT: GRB 090727: Swift/UVOT Upper Limits DATE: 09/07/29 02:00:58 GMT FROM: Margaret Chester at PSU M.M. Chester (PSU) and P. A. Evans (U Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 090727 92 s after the BAT trigger (Evans et al., GCN Circ. 9718). We do not find any new source at the position of the XRT afterglow (Goad et al., GCN Circ. 9721). Preliminary 3-sigma upper limits for the white finding chart and the co-added images, using the UVOT photometric system (Poole et al. 2008, MNRAS, 383, 627), are: Filter T_start(s) T_stop(s) Exp(s) Mag white_FC 92 241 147 >20.6 white 92 5987 541 >21.5 v 4760 57429 3737 >21.1 b 4145 46543 1752 >21.3 u 3939 52323 4261 >21.8 w1 5171 51651 4625 >22.1 m2 4965 57845 4989 >22.3 w2 4556 56519 3825 >21.7 The values quoted above are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.54 in the direction of the burst (Schlegel et al. 1998). //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9733 SUBJECT: GRB 090727: optical observations DATE: 09/07/29 12:31:34 GMT FROM: Vladimir Sokolov at SAO RAS A. Moskvitin, A. Valeev, T. Fatkhullin, O. Sholukhova & S. Fabrika (SAO-RAS Niznijh Arkhyz, Russia), on behalf of a larger colaboration, report: We observed the GRB090727 optical afterglow (Smith et al. GCN Circ. 9719, GCN Circ. 9722; J. Gorosabel et al. GCN Circ 9728 ) with the SAO RAS 6-m telescope in Caucasus. The observations were carried out in the R band with a total exposure of 158 sec. The weather was cloudy with a sufficient atmospheric extinction. We estimated the brightness of the object as R = 21.53 +/- 0.17 at the middle epoch of 23:21:12 27 July 2009 UT (2334 sec after the trigger). Calibration was done aganist 10 USNO B1.0 stars. This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9735 SUBJECT: GRB 090727: GRT Optical Observation DATE: 09/07/29 19:19:45 GMT FROM: Takanori Sakamoto at NASA/GSFC T. Sakamoto (UMBC/GSFC), D. Donato (ORAU/GSFC), N. Gehrels (GSFC), T. Okajima (JHU/GSFC), T.N. Ukwatta (GWU/GSFC), Y. Urata (NCU), C.A. Wallace (FGCU) We observed the field of GRB 090727 detected by Swift (trigger #358520; Evans et al., GCN Circ. 9718) with the 14-inch Goddard Robotic Telescope (GRT) located at the Goddard Geophysical and Astronomical Observatory (http://cddisa.gsfc.nasa.gov/ggao/). 77 set of 30 sec exposures (excluding the bad quality images) were taken in the R filter starting from July 28 01:57:45 (UT) about 3.2 hours after the trigger and stopped on July 28 02:40:50 (UT). We do not detect the optical afterglow (Smith et al., GCN Circ. 9719; Gorosabel et al., GCN Circ. 9728; Moskvitin et al., GCN Circ. 9733) both in the individual images and the combined image. The estimated three sigma upper limit of the combined image (total exposure of 2310 sec) is ~16.6 mag using the USNO-B1 catalog. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 9743 SUBJECT: IPN Triangulation and Konus-Wind observaions of GRB090727B DATE: 09/08/03 11:35:38 GMT FROM: Dmitry Frederiks at Ioffe Institute S. Golenetskii, R. Aptekar, D. Frederiks, E. Mazets, and V. Pal'shin, on behalf of the Konus-Wind team, K. Hurley and T. Cline, on behalf of the Mars Odyssey and Konus GRB teams, I. G. Mitrofanov, D. Golovin, M. L. Litvak, and A. B. Sanin, on behalf of the HEND-Odyssey GRB team, W. Boynton, C. Fellows, K. Harshman, H. Enos, and R. Starr, on behalf of the GRS-Odyssey GRB team, and J. Goldsten, on behalf of the MESSENGER NS GRB team, report: The long GRB 090727B triggered Konus-Wind at T0=84749.412 s UT (23:32:29.412). The burst had a smooth temporal structure with a duration of ~25 s. The Konus-Wind light curves are available at http://www.ioffe.ru/LEA/GRBs/GRB090727_T84749/ This GRB was observed by Odyssey (HEND and GRS) and MESSENGER (GRNS). Wind-Odyssey-MESSENGER triangulation, together with Konus-Wind ecliptic latitude constrains, lead to the following preliminary, 3 sigma error box, which area is 1.00 sq. deg. ----------------------------------------------- RA(2000), deg Dec(2000), deg ----------------------------------------------- Center: 343.358 (22h 53m 26s) -46.700 (-46d 42' 00") Corners: 343.427 (22h 53m 42s) -45.867 (-45d 52' 01") 342.516 (22h 50m 03s) -45.873 (-45d 52' 22") 343.285 (22h 53m 08s) -47.527 (-47d 31' 37") 344.214 (22h 56m 51s) -47.507 (-47d 30' 25") ----------------------------------------------- IPN triangulation map can be found at http://www.ioffe.ru/LEA/GRBs/GRB090727_T84749/GRB20090727_84749_IPN.png As observed by Konus-Wind, the burst had a fluence of (1.15 ± 0.15)x10-5 erg/cm2, and a 256-ms peak flux, measured from T0+14.336 s, of (8.5 ± 3.2)x10-7 erg/cm2/s (both in the 20 keV - 2 MeV energy range). The time-integrated spectrum of the burst (from T0 to T0+24.832 s) is well fit, in the 20 keV - 2 MeV range, by GRB (Band) model, for which: the low-energy photon index alpha = -0.18(-0.27,+0.34), the high energy photon index beta = -2.97( < -2.50), the peak energy Ep = 152(-16, +17) keV (chi2 = 54/57 dof). All the quoted values are preliminary. All the quoted errors are at the 90% confidence level. --