GRB170827A

This page lists all entries on GRB170827A in GRBweb

Summary IPN Swift GCN 21718 GCN 21721 GCN 21722 GCN 21724 GCN 21728 GCN 21729 GCN 21730 GCN 21743 GCN 21807

Summary table
Variable Value Source
T0 5:12:28 UTC GCN_circulars,Swift Det
ra 276.1508° Swift
decl -40.2016° Swift
pos_error 6.34e-04° Swift
T90 94.0 s Swift
T90_start 5:12:28 UTC Swift
fluence 1.40e-06 erg/cm² Swift
T100 94.0 s
GBM_located False
mjd 57992.216990740744 GCN_circulars,Swift Det
IPN table
GRB_name GRB170827A
ra 276.1792°
decl -40.2167°
pos_error 5.00e-02°
Swift table
GRB_name GRB170827A
t_trigger 5:12:28 UTC
ra 276.1508°
decl -40.2016°
pos_error 6.34e-04°
T90 94.0 s
fluence 1.40e-06 erg/cm²
GCN 21718 table
GRB_name GRB170827A
GCN_number 21718
Detection_method Swift Det
t_trigger 5:12:28 UTC
ra 276.1800°
decl -40.2200°
Circular_text TITLE: GCN CIRCULAR NUMBER: 21718 SUBJECT: GRB 170827A: Swift detection of a burst DATE: 17/08/27 05:25:35 GMT FROM: David Palmer at LANL F. E. Marshall (NASA/GSFC), A. D'Ai (INAF-IASFPA), K. L. Page (U Leicester), D. M. Palmer (LANL) and M. H. Siegel (PSU) report on behalf of the Swift Team: At 05:12:28 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 170827A (trigger=769567). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 276.180, -40.220 which is RA(J2000) = 18h 24m 43s Dec(J2000) = -40d 13' 11" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). As is typical for an image trigger, the immediately-available BAT lightcurve shows no obvious variation. The XRT began observing the field at 05:14:32.5 UT, 124.1 seconds after the BAT trigger. XRT found a bright, uncatalogued X-ray source located at RA, Dec 276.1508, -40.2016 which is equivalent to: RA(J2000) = +18h 24m 36.19s Dec(J2000) = -40d 12' 05.8" with an uncertainty of 4.9 arcseconds (radius, 90% containment). This location is 104 arcseconds from the BAT onboard position, within the BAT error circle. No event data are yet available to determine the column density using X-ray spectroscopy. The initial flux in the 2.5 s image was 4.23e-09 erg cm^-2 s^-1 (0.2-10 keV). UVOT took a finding chart exposure of 150 seconds with the White filter starting 133 seconds after the BAT trigger. Only partial images are available and neither the 2.7'x2.7' sub-image nor the 8'x8' region for the list of sources generated on-board covers the XRT error circle. Analysis of any potential afterglow will have to await further data. Burst Advocate for this burst is F. E. Marshall (marshall AT milkyway.gsfc.nasa.gov). 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.)
GCN 21721 table
GRB_name GRB170827A
GCN_number 21721
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 21721 SUBJECT: GRB 170827A: REM optical/NIR observations DATE: 17/08/27 09:28:32 GMT FROM: Paolo D'Avanzo at INAF-OAB P. D'Avanzo, D. Fugazza, S. Covino (INAF/OAB) report on behalf of the REM team: We observed the field of the short GRB 170827A (Marshall et al., GCN 21718) with the 60-cm robotic telescope REM located at the La Silla Observatory (Chile). The observations started at 05:14:24 UT, 116 seconds after the burst, and were carried out simultaneously in the g, r, i, z and H bands. A preliminary photometry of the first co-added images indicates that no obvious afterglow candidate is detected within the Swift/XRT error circle (Marshall et al., GCN 21718) down to the following 3sigma limiting AB magnitudes: r > 19.5 at T-T0 = 720s H > 17.5 at T-T0 = 585s Magnitudes are in the AB system and have been calibrated with respect to the 2MASS (H-band) and APASS (r-band) catalogues.
GCN 21722 table
GRB_name GRB170827A
GCN_number 21722
Detection_method Swift-UVOT Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 21722 SUBJECT: GRB 170827A: Swift/UVOT Upper Limits DATE: 17/08/27 15:15:10 GMT FROM: Frank Marshall at GSFC F. E. Marshall (NASA/GSFC) reports on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 170827A 134 s after the BAT trigger (Marshall et al., GCN Circ. 21718). No optical afterglow consistent with the XRT position (Marshall et al. GCN Circ. 21718) is detected in the initial UVOT exposures. Preliminary 3-sigma upper limits using the UVOT photometric system (Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the first finding chart (FC) exposure and a subsequent short exposure are: Filter T_start(s) T_stop(s) Exp(s) Mag white_FC 134 284 147 >19.8 u 292 298 6 >17.8 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.11 in the direction of the burst (Schlegel et al. 1998).
GCN 21724 table
GRB_name GRB170827A
GCN_number 21724
Detection_method Swift-BAT Det
ra 276.1890°
decl -40.2020°
Circular_text TITLE: GCN CIRCULAR NUMBER: 21724 SUBJECT: GRB 170827A, Swift-BAT refined analysis DATE: 17/08/27 16:58:00 GMT FROM: Amy Lien at GSFC T. N. Ukwatta (LANL), S. D. Barthelmy (GSFC), J. R. Cummings (CPI), H. A. Krimm (NSF/USRA), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), F. E. Marshall (NASA/GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU), M. Stamatikos (OSU), (i.e. the Swift-BAT team): Using the data set from T-239 to T+509 sec from the recent telemetry downlink, we report further analysis of BAT GRB 170827A (trigger #769567) (Marshall et al. GCN Circ. 21718). The BAT ground-calculated position is RA, Dec = 276.189, -40.202 deg which is RA(J2000) = 18h 24m 45.3s Dec(J2000) = -40d 12' 07.9" with an uncertainty of 1.9 arcmin, (radius, sys+stat, 90% containment). The partial coding was 98%. The mask-weighted light curve shows a weak pulse that starts at ~T+20 s and ends at ~T+140 s. T90 (15-350 keV) is 94.0 +- 12.5 sec (estimated error including systematics). The time-averaged spectrum from T+19.1 to T+138.9 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.29 +- 0.18. The fluence in the 15-150 keV band is 1.4 +- 0.1 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+67.13 sec in the 15-150 keV band is 0.4 +- 0.2 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/769567/BA/
GCN 21728 table
GRB_name GRB170827A
GCN_number 21728
Detection_method Other
ra 276.1506°
decl -40.2017°
Circular_text TITLE: GCN CIRCULAR NUMBER: 21728 SUBJECT: GRB 170827A: ePESSTO NTT afterglow candidate DATE: 17/08/28 02:33:35 GMT FROM: Paolo D'Avanzo at INAF-OAB J. Lyman (Univ. of Warwick), D. Homan (Univ of Edinburgh), P. D'Avanzo (INAF-OAB), Patricia Schady (MPE Garching), K. E. Heintz (DARK/NBI), E. Palazzi (INAF-IASFBo), L. Galbany (Univ. de Chile), J. Anderson (ESO), C. Inserra (Southampton), E. Kankare (QUB), K. Maguire (QUB), S. Smartt (QUB), K. W. Smith (QUB), O. Yaron (Weizmann), D. Young (QUB), I. Manulis (Weizmann) report: We observed the field of GRB 170827A (Marshall et al., GCN 21718) under the extended Public ESO Spectroscopic Survey for Transient Objects (ePESSTO; see Smartt et al. 2015, A&A, 579, 40 http://www.pessto.org ). The observations were performed on the ESO New Technology Telescope at La Silla with the SofI and EFOSC2 instrument in imaging mode starting from 2017-08-28 at 00:47:05 UT (i.e. 19.58 hours from the burst). Observations were carried out with the Z, J, R and I filters. Within the XRT error circle (Marshall et al., GCN 21718) we detect an object at the following coordinates: RA(J2000), Dec(J2000) = 18:24:36.14, -40:12:06.3 (+/- 0.5"). The object has a magnitude R~21.5 (based on preliminary photometry calibrated against the USNOB1 catalogue) at T-T0 = 20.08 hours. We cannot make any statement about variability at this time.We also notice the presence of a fainter object about 2.4" West.
GCN 21729 table
GRB_name GRB170827A
GCN_number 21729
Detection_method Swift-XRT Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 21729 SUBJECT: GROND observations of GRB170827A DATE: 17/08/28 09:40:33 GMT FROM: Patricia Schady at MPE/Swift P. Schady (MPE Garching) reports I observed the field of GRB 170827A (Swift trigger 769567; Marshall et al., GCN #21718) simultaneously in g'r'i'z'JHK with GROND (Greiner et al. 2008, PASP 120, 405) mounted at the 2.2 m MPG telescope at ESO La Silla Observatory (Chile). Observations started at 00:44 UT on 28-08-2017, 19.5 hours after the GRB trigger. They were performed at an average seeing of 1.5" and at an average airmass of 1.0. A point source is present within the 4.9" Swift-XRT error circle (Marshall et al., GCN #21718) in the g'r'i'z' GROND images, consistent with the ePESSTO position reported by Lyman et al. (GCN #21728). Based on a total exposure time of 36 min in g'r'i'z' and 30 min in JHK, the estimated preliminary magnitudes and upper limits (all in AB system) are g' = 22.8 +/- 0.1 mag r' = 21.9 +/- 0.1 mag i' = 21.6 +/- 0.1 mag z' = 21.4 +/- 0.1 mag J > 21.1 mag H > 20.6 mag K > 20.1 mag Given magnitudes are calibrated against GROND zeropoints as well as 2MASS field stars and are not corrected for the expected Galactic foreground extinction corresponding to a reddening of E_(B-V)=0.09 mag in the direction of the burst (Schlafly & Finkbeiner 2011). A second fainter source is also detected within the XRT error circle at around 2.3" west of the ePESSTO afterglow candidate. No statement can be made at this time on the variability of either source. I acknowledge the excellent help provided by the support astronomer in La Silla, Markus Rabus, in obtaining these data.
GCN 21730 table
GRB_name GRB170827A
GCN_number 21730
Detection_method Swift-XRT Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 21730 SUBJECT: GRB 170827A: Swift-XRT refined Analysis DATE: 17/08/28 13:23:16 GMT FROM: Antonino D'Ai at IASF-PA A. D'Ai (IASF-PA), V. D'Elia (ASDC), F. E. Marshall (NASA/GSFC) reports on behalf of the Swift-XRT team: We have analysed 1.1 ks of XRT data for GRB 170827A (Marshall et al. GCN Circ. 21718), from 113 s to 17.3 ks after the BAT trigger. The data comprise 165 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 initial light curve from T0+130s to T0+295s can be modelled with a power-law decay with a decay index of alpha=1.19 (+/-0.08). In the following observation at T0+16.1 ks the afterglow is not detected with a 3-sigma upper limit of 1.6 x 10^-2 count^-1 s^-1. A spectrum formed from the WT mode data can be fitted with an absorbed power-law with a photon spectral index of 2.23 (+0.06, -0.05). The best-fitting absorption column is 1.46 (+/-0.15) x 10^21 cm^-2, in excess of the Galactic value of 1.2 x 10^21 cm^-2 (Willingale et al. 2013). The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 3.0 x 10^-11 (4.2 x 10^-11) erg cm^-2 count^-1. A summary of the WT-mode spectrum is thus: Total column: 1.46 (+/-0.15) x 10^21 cm^-2 Galactic foreground: 1.2 x 10^21 cm^-2 Excess significance: 3.0 sigma Photon index: 2.23 (+0.06, -0.05) Given the lack of detection in the second observation, no reliable estimate of the X-ray count rate for the following days is possible. The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00769567. This circular is an official product of the Swift-XRT team.
GCN 21743 table
GRB_name GRB170827A
GCN_number 21743
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 21743 SUBJECT: GRB170827A: Further GROND follow-up observations DATE: 17/08/29 07:29:05 GMT FROM: Patricia Schady at MPE/Swift P. Schady (MPE Garching) reports I re-observed the field of GRB 170827A (Swift trigger 769567; Marshall et al., GCN #21718) simultaneously in g'r'i'z'JHK with GROND (Greiner et al. 2008, PASP 120, 405) on 29-08-2017, 1.8 days after the GRB trigger and 1 day after the first set of GROND observations (Schady, GCN #21729) . Observations were performed at an average seeing of 1.4" and at an average airmass of 1.0. The two point sources detected within the 4.9" XRT error circle (Marshall et al., GCN #21718) in the first epoch of GROND observations (Schady, GCN #21729) are still seen in the second epoch of GROND observations and they remain at the same magnitude. Neither of these sources are therefore likely to be the optical counterpart of GRB 170827A. I acknowledge the excellent help provided by the support astronomer in La Silla, Markus Rabus, in obtaining these data.
GCN 21807 table
GRB_name GRB170827A
GCN_number 21807
Detection_method LCO
Circular_text TITLE: GCN CIRCULAR NUMBER: 21807 SUBJECT: GRB 170827A: LCO Observations DATE: 17/09/04 11:43:05 GMT FROM: Antonino Cucchiara at UVI A. Cucchiara, D. Morris, J. Staff, and B. Gendre (U. Virgin Islands) report on behalf of a larger collaboration: "On August 27.71 UT (T_0 +12.0h) we began observing the center of the field of GRB 170827A (Marshall et al. GCN 21718, D'Ai et al. GCN 21730) using the Las Cumbres Observatory 1m telescope located in Sutherland Observatory. We performed a series of 5x240s observations in SDSS r' and i’ bands for a total of 20 minutes on sky in each filter at average airmass of 1.05. In the full median stacked images we identified no optical counterpart within the center of the Swift-XRT refined position or at the ePESSTO NTT optical counterpart location (Evans et al. GCN 21413, Lyman et al. GCN 21728) at the following 3-sigma limits: r' > 20.6 mag i' > 19.6 mag These values are consistent with the limits and detections reported by other observatories (D'Avanzo et al. GCN 21721, Schady et al. GCN 21729, 21743). These magnitudes are calibrated against nearby USNO-B1 sources, converted in SDSS bands, and not corrected for Galactic extinction."