//////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11931 SUBJECT: GRB 110414A: Swift detection of a burst DATE: 11/04/14 08:00:18 GMT FROM: Rhaana Starling at U of Leicester R. L. C. Starling (U Leicester), A. P. Beardmore (U Leicester), V. D'Elia (ASDC), P. A. Evans (U Leicester), J. M. Gelbord (PSU), B. Gendre (ASDC), C. Guidorzi (U Ferrara), S. T. Holland (CRESST/USRA/GSFC), A. Melandri (INAF-OAB), K. L. Page (U Leicester), A. Rowlinson (U Leicester), M. Stamatikos (OSU/NASA/GSFC), G. Stratta (ASDC) and G. Tagliaferri (INAF-OAB) report on behalf of the Swift Team: At 07:42:14 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 110414A (trigger=451343). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 97.876, +24.361 which is RA(J2000) = 06h 31m 30s Dec(J2000) = +24d 21' 39" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed multiple-peaked structure with a duration of about 50 sec. The peak count rate was ~400 counts/sec (15-350 keV), at ~0 sec after the trigger. The XRT began observing the field at 07:44:36.8 UT, 142.3 seconds after the BAT trigger. Using promptly downlinked data we find a bright, uncatalogued X-ray source with an enhanced position: RA, Dec 97.8726, 24.3624 which is equivalent to: RA(J2000) = 06h 31m 29.42s Dec(J2000) = +24d 21' 44.7" with an uncertainty of 2.3 arcseconds (radius, 90% containment). This location is 12 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 3.05 x 10^21 cm^-2 (Kalberla et al. 2005). The initial flux in the 2.5 s image was 4.11e-09 erg cm^-2 s^-1 (0.2-10 keV). UVOT took a finding chart exposure of nominal 250 seconds with the U filter starting 308 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 18.0 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.33. Burst Advocate for this burst is R. L. C. Starling (rlcs1 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: 11932 SUBJECT: GRB 110414A : Faulkes Telescope North observations DATE: 11/04/14 12:57:35 GMT FROM: Andrea Melandri at Liverpool John Moores U A. Melandri (INAF-OAB), C. Guidorzi (U. Ferrara), C.G. Mundell (Liverpool JMU), A. Gomboc, J. Japelj and D. Kopac (U. Ljubljana) on behalf of a large collaboration report: The 2-m Faulkes Telescope North robotically followed up GRB110414A (SWIFT trigger 451343; Starling et al. GCN 11931) starting about 4 min after the GRB trigger time. Observations were performed automatically with BVRi filters. We do not detect any clear fading object inside the reported XRT position down to a limiting magnitude of R~20.0. We do detect a faint uncatalogued source, in one single SDSS-i exposure, inside the XRT error circle with coordinates: RA = 06:31:29.37 Dec = +24:21:45.9 (+/- 1 arcsec) This object is not detected in subsequent SDSS-i frames. Fading is yet to be confirmed. This message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11934 SUBJECT: GRB 110414A: Enhanced Swift-XRT position DATE: 11/04/14 20:36:53 GMT FROM: Phil Evans at U of Leicester J.P. Osborne, A.P. Beardmore, P.A. Evans and M.R. Goad (U. Leicester) report on behalf of the Swift-XRT team. Using 1551 s of XRT Photon Counting mode data and 2 UVOT images for GRB 110414A, 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 = 97.87261, +24.36241 which is equivalent to: RA (J2000): 06h 31m 29.43s Dec (J2000): +24d 21' 44.7" with an uncertainty of 1.5 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, MNRAS, 397, 1177). This circular was automatically generated, and is an official product of the Swift-XRT team. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11935 SUBJECT: GRB 110414A: Swift-XRT refined Analysis DATE: 11/04/14 22:46:27 GMT FROM: Rhaana Starling at U of Leicester R. L. C. Starling (U Leicester) reports on behalf of the Swift-XRT team: We have analysed 9.1 ks of XRT data for GRB 110414A (Starling et al. GCN Circ. 11931), from 131 s to 22.7 ks after the BAT trigger. The data comprise 18 s in Windowed Timing (WT) mode (the first 9 s were taken while Swift was slewing) with the remainder in Photon Counting (PC) mode. The enhanced XRT position for this burst was given by Osborne et al. (GCN. Circ 11934). The late-time light curve (from T0+5.1 ks) can be modelled with a power-law decay with a decay index of alpha=1.67 (+0.23, -0.22). A spectrum formed from the WT mode data can be fitted with an absorbed power-law with a photon spectral index of 2.72 (+/-0.15). The best-fitting absorption column is 5.0 (+/-0.5) x 10^21 cm^-2, in excess of the Galactic value of 3.0 x 10^21 cm^-2 (Kalberla et al. 2005). The PC mode spectrum has a photon index of 2.32 (+0.17, -0.16) and a best-fitting absorption column of 4.0 (+/-0.6) x 10^21 cm^-2. The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 4.0 x 10^-11 (8.4 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 4.0 (+/-0.6) x 10^21 cm^-2 Galactic foreground: 3.0 x 10^21 cm^-2 Excess significance: 11.7 sigma Photon index: 2.32 (+0.17, -0.16) The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00451343. This circular is an official product of the Swift-XRT team. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11936 SUBJECT: GRB 110414A: Swift/UVOT Upper limits DATE: 11/04/14 23:01:09 GMT FROM: Tyler Pritchard at PSU T.A. Pritchard (PSU) and R. L. C. Starling (U Leicester) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 110414A 151 s after the BAT trigger (Starling et al., GCN Circ. 11931). No optical afterglow consistent with the XRT position (Starling et al., GCN Circ. 11931) is detected in the initial UVOT exposures. Preliminary 3-sigma upper limits using the UVOT photometric system (Poole et al. 2008, MNRAS, 383, 627) for the initial exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white_FC 150 300 147 >20.6 u_FC 308 558 246 >19.4 white 150 1013 334 >21.3 v 639 831 39 >18.4 b 565 758 39 >18.9 u 308 733 265 >19.5 w1 689 709 19 >18.5 m2 664 856 39 >18.8 w2 615 807 39 >19.2 The values quoted above are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.33 in the direction of the burst (Schlegel et al. 1998). //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11937 SUBJECT: GRB 110414A: Swift-BAT Refined Analysis DATE: 11/04/14 23:49:34 GMT FROM: Michael Stamatikos at OSU/GSFC J. R. Cummings (GSFC/UMBC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), E. E. Fenimore (LANL), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (GSFC/UMBC), G. Sato (ISAS), M. Stamatikos (OSU/NASA/GSFC), R. L. C. Starling (U Leicester), J. Tueller (GSFC), T. N. Ukwatta (MSU) (i.e. the Swift-BAT team): Using the data set from T-239 to T+963 sec from the recent telemetry downlink, we report further analysis of BAT GRB 110414A (trigger #451343) (Starling, et al., GCN Circ. 11931). The BAT ground-calculated position is RA, Dec = 97.876, 24.349 deg which is RA(J2000) = 06h 31m 30.2s Dec(J2000) = +24d 20' 56.5" with an uncertainty of 1.6 arcmin, (radius, sys+stat, 90% containment). The partial coding was 30%. The mask-weighted lightcurve shows several overlapping peaks with the first starting at ~T-100 sec, the main peaks at T-33, T+0, T+10, T+25, and a small peak at ~T+120 sec, and ending at ~T+130 sec. T90 (15-350 keV) is 152.0 +- 73.2 sec (estimated error including systematics). The time-averaged spectrum from T-38.4 to T+135.6 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.70 +- 0.14. The fluence in the 15-150 keV band is 3.5 +- 0.3 x 10^-06 erg/cm2. The 1-sec peak photon flux measured from T+8.62 sec in the 15-150 keV band is 1.1 +- 0.3 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/451343/BA/ //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11938 SUBJECT: GRB110414A: MITSuME Okayama Optical upper limits DATE: 11/04/15 02:12:07 GMT FROM: Daisuke Kuroda at OAO/NAOJ D. Kuroda, K. Yanagisawa, Y. Shimizu, H. Toda (OAO, NAOJ), S. Nagayama (NAOJ), M. Yoshida (Hiroshima), K. Ohta (Kyoto) and N. Kawai(Tokyo Tech) report on behalf of the MITSuME collaboration: We observed the field of GRB 110414A (Starling et al., GCN 11931) with the optical three color (g', Rc and Ic) CCD camera attached to the MITSuME 50cm telescope of Okayama Astrophysical Observatory. The observation started on 2011-04-14 10:35:42 UT (~2.9 h after the burst). We did not find any new point source within the Enhanced XRT circle (Osborne et al., GCN 11934) in all the three bands. Three sigma upper limits of the OT are listed below. We used GSC2.3 catalog for flux calibration. T0+[day] MID-UT T-EXP[sec] g' Rc Ic ------------------------------------------------------ 0.16212 11:35:41 6180.0 >19.3 >19.2 >18.4 ------------------------------------------------------ T0+ : Elapsed time after the burst [day] T-EXP: Total Exposure time [sec] //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11939 SUBJECT: GRB 110414A: GROND upper limits DATE: 11/04/15 20:24:50 GMT FROM: Alexander Kann at TLS Tautenburg D. A. Kann (TLS Tautenburg), J. Elliott, and J. Greiner (both MPE Garching) report on behalf of the GROND team: We observed the field of GRB 110414A (Swift trigger 451343; Starling et al., GCN 11931) simultaneously in g'r'i'z'JHK with GROND (Greiner et al. 2008, PASP 120, 405) mounted at the 2.2 m MPI/ESO telescope at La Silla Observatory (Chile). Observations started at 23:17 UT on April 14, 15.58 hours after the GRB trigger, and continued until 00:38 UT. They were obtained under challenging conditions, partially in astronomical twilight, with seeing of 1".5, average airmass of 2.1, bright moonlight and passing cirrus. From exposures of 1379 s in g'r'i'z' and 1440 s in JHK, no source is detected within the UVOT-enhanced XRT error circle reported by Osborne et al. (GCN 11934) or at the position of the possible i' detection (Melandri et al., GCN 11932) down to the following 3 sigma upper limits (all in AB): g' > 23.0, r' > 23.3, i' > 22.9, z' > 22.9, J > 20.1, H > 19.7 and, K > 17.3 If the i' detection of Melandri et al. (GCN 11932) is confirmed, our observations show the source has faded and is thus likely the afterglow of GRB 110414A. The given limits are derived based on calibrating the images against GROND zeropoints and 2MASS field stars and are not corrected for the Galactic foreground extinction corresponding to a reddening of E_(B-V) = 0.331 in the direction of the burst (Schlegel et al. 1998). //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 11940 SUBJECT: GRB110414A: MITSuME Ishigakijima Optical upper limits DATE: 11/04/15 22:48:58 GMT FROM: Daisuke Kuroda at OAO/NAOJ D. Kuroda (OAO, NAOJ), H. Hanayama, T. Miyaji, J. Watanabe (IAO, NAOJ), K. Yanagisawa (OAO, NAOJ), S.Nagayama (NAOJ), M. Yoshida (Hiroshima), K. Ohta (Kyoto) and N. Kawai(Tokyo Tech) report on behalf of the MITSuME collaboration: We observed the field of GRB 110414A (Starling et al., GCN 11931) with the optical three color (g', Rc and Ic) CCD camera attached to the Murikabushi 1m telescope of Ishigakijima Astronomical Observatory. The observation started on 10:57:59 UT (~3.3 h after the burst). We did not find any new point source within the Enhanced XRT circle (Osborne et al., GCN 11934) in all the three bands. Three sigma upper limits of the OT are listed below. We used GSC2.3 catalog for flux calibration. T0+[day] MID-UT T-EXP[sec] g' Rc Ic ------------------------------------------------------ 0.17783 11:58:19 6180.0 >19.7 >19.8 >19.1 ------------------------------------------------------ T0+ : Elapsed time after the burst [day] T-EXP: Total Exposure time [sec]