GRB140829A

This page lists all entries on GRB140829A in GRBweb

Summary Fermi GBM GCN 16758 GCN 16759

Summary table
Variable Value Source
GRB_name_Fermi GRB140829880
T0 21:07:26.442 UTC Fermi_GBM
ra 250.5589° GCN_circulars,Optical
decl 50.1287° GCN_circulars,Optical
T90 77.568 s Fermi_GBM
T90_error 2.064 s Fermi_GBM
T90_start 21:07:26.442 UTC Fermi_GBM
fluence 5.39e-06 erg/cm² Fermi_GBM
fluence_error 1.25e-07 erg/cm² Fermi_GBM
redshift 0.4830 GCN_circulars,Optical
T100 77.568 s
GBM_located False
mjd 56898.880167152776 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB140829880
trigger_name bn140829880
ra 255.5900°
decl 55.9300°
pos_error 4.86e+00°
datum 2014-08-29
t_trigger 21:07:27.466 UTC
T90 77.568 s
T90_error 2.064 s
T90_start 21:07:26.442 UTC
fluence 5.39e-06 erg/cm²
fluence_error 1.25e-07 erg/cm²
flux_1024 2.99e+00 erg/cm²/s
flux_1024_error 3.84e-01 erg/cm²/s
flux_1024_time 1.15e+01 erg/cm²/s
flux_64 8.20e+00 erg/cm²/s
flux_64_error 2.03e+00 erg/cm²/s
GCN 16758 table
GRB_name GRB140829A
GCN_number 16758
Detection_method Optical
ra 250.5589°
decl 50.1287°
redshift 0.4830
Circular_text TITLE: GCN CIRCULAR NUMBER: 16758 SUBJECT: GRB 140829A: iPTF optical observations DATE: 14/08/31 00:50:32 GMT FROM: Leo Singer at CIT/PTF L. P. Singer (Caltech), S. B. Cenko (NASA/GSFC), D. A. Perley (Caltech), and M. M. Kasliwal (Carnegie Observatories/Princeton), report on behalf of the intermediate Palomar Transient Factory (iPTF) collaboration: Fermi GBM triggered on GRB 140829A (Fermi trigger 431039250 / bn140829880) at 2014-08-29 21:07:27.47. At 2014-08-30 03:25:48, 6.3 hours after the burst, we began searching for optical counterparts using the Palomar 48-inch Oschin telescope (P48). We imaged 17 fields covering an area of 124 deg2, covering most of the 1-sigma statistical+systematic region of the final Fermi GBM localization. We estimate a 61% chance that these fields contain the true location of the source. Sifting through candidate variable sources using image subtraction and standard iPTF vetting procedures, we detected several faint optical transients. iPTF14ejs, at r=20.15+/-0.06 mag and possibly fading by 0.2+/-0.09 mag by 8.6 hours after the burst, is coincident with the galaxy SDSS J164214.15+500743.1. It is at the coordinates: RA(J2000) = 16h 42m 14.14s (250.558918 deg) Dec(J2000) = +50d 07' 43.3" (+50.128685 deg) We acquired a spectrum of iPTF14ejs using the Low Resolution Imaging Spectrometer (LRIS) on the Keck 10m telescope. A provisional reduction shows broad Balmer features characteristic of an AGN at a redshift of z=0.483, and therefore it is not a GRB afterglow. The remaining candidates do not show any clear photometric evolution over the course of our observations: iPTF14ejo, at r=20.32+/-0.07 mag, is coincident with the galaxy SDSS J173008.24+545502.8. It is at the coordinates: RA(J2000) = 17h 30m 08.26s (262.534415 deg) Dec(J2000) = +54d 55' 04.2" (+54.917842 deg) iPTF14eju, at r=20.66+/-0.12 mag, is 4.8" to the southwest of an r=18.43 unresolved point source that is present in archival iPTF images. It is at the coordinates: RA(J2000) = 17h 13m 25.08s (258.354509 deg) Dec(J2000) = +50d 10' 04.7" (+50.167985 deg) iPTF14ejp, at r=20.37+/-0.09 mag, is coincident with PGC 2393059. It is at the coordinates: RA(J2000) = 16h 56m 59.87s (254.249449 deg) Dec(J2000) = +51d 22' 21.7" (+51.372682 deg) iPTF14ejw, at r=20.27+/-0.10 mag, is coincident with the galaxy SDSS J164524.99+625127.7 . It is at the coordinates: RA(J2000) = 16h 45m 24.20s (251.350842 deg) Dec(J2000) = +62d 51' 27.7" (+62.857694 deg) iPTF14ejn, at r=20.31+/-0.07 mag, is coincident with the galaxy SDSS J172732.49+540754.0. It is at the coordinates: RA(J2000) = 17h 27m 32.49s (261.885373 deg) Dec(J2000) = +54d 07' 54.2" (+54.131732 deg) iPTF14ejv, at r=20.82+/-0.20 mag, is coincident with the galaxy SDSS J174853.28+580652.3. It is at the coordinates: RA(J2000) = 17h 48m 53.26s (267.221896 deg) Dec(J2000) = +58d 06' 52.8" (+58.114678 deg) The diagram http://www.its.caltech.edu/~lsinger/iptf/Fermi431039250.pdf shows the locations of our candidates and the P48 fields in relation to the Fermi GBM 1- and 2-sigma statistical+systematic contours.
GCN 16759 table
GRB_name GRB140829A
GCN_number 16759
Detection_method Fermi GBM Det
t_trigger 21:07:27.470 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 16759 SUBJECT: GRB 140829A: Fermi GBM Detection DATE: 14/08/31 20:50:38 GMT FROM: Matthew Stanbro at UAH/Fermi M. Stanbro (UAH) reports on behalf of the Fermi GBM Team: "At 21:07:27.47 UT on 29 August 2014, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 140829A (trigger 431039250 / 140829880). The GBM error circle was also observed with iPTF in search of an optical counterpart of the GRB; no credible counterpart was found (Singer et. al., 2014, GCN 16758). The GBM light curve consists of a double pulse with a duration (T90) of about 19 s (50-300 keV). The time-averaged spectrum from T0-3.1 s to T0+18.4 s is well fit by a power law function with an exponential high-energy cutoff. The power law index is -0.5 +/- 0.2 and the cutoff energy, parameterized as Epeak, is 324 +/- 43 keV. The event fluence (10-1000 keV) in this time interval is (5.12 +/- 0.41)E-06 erg/cm^2. The 1-sec peak photon flux measured starting from T0+11.52 s in the 10-1000 keV band is 2.9 +/- 0.4 ph/s/cm^2. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog."