GRB130919A

This page lists all entries on GRB130919A in GRBweb

Summary IPN Swift GCN 15232 GCN 15234 GCN 15235 GCN 15238

Summary table
Variable Value Source
T0 11:07:24 UTC GCN_circulars,Swift Det
ra 207.2810° Swift
decl -10.3530° Swift
pos_error 1.24e-02° Swift
T90 97.3 s Swift
T90_start 11:07:24 UTC Swift
fluence 1.40e-06 erg/cm² Swift
T100 97.3 s
GBM_located False
mjd 56554.463472222225 GCN_circulars,Swift Det
IPN table
GRB_name GRB130919A
ra 207.2875°
decl -10.3500°
pos_error 5.00e-02°
Swift table
GRB_name GRB130919A
t_trigger 11:07:24 UTC
ra 207.2810°
decl -10.3530°
pos_error 1.24e-02°
T90 97.3 s
fluence 1.40e-06 erg/cm²
GCN 15232 table
GRB_name GRB130919A
GCN_number 15232
Detection_method Swift Det
t_trigger 11:07:24 UTC
ra 207.2880°
decl -10.3550°
Circular_text TITLE: GCN CIRCULAR NUMBER: 15232 SUBJECT: GRB 130919A: Swift detection of a burst DATE: 13/09/19 11:18:50 GMT FROM: Hans Krimm at NASA-GSFC H. A. Krimm (CRESST/GSFC/USRA), A. A. Breeveld (UCL-MSSL), D. N. Burrows (PSU), P. A. Evans (U Leicester), N. Gehrels (NASA/GSFC), J. A. Kennea (PSU), C. B. Markwardt (NASA/GSFC), A. Melandri (INAF-OAB), K. L. Page (U Leicester), B. Sbarufatti (INAF-OAB/PSU), M. H. Siegel (PSU) and T. N. Ukwatta (MSU) report on behalf of the Swift Team: At 11:07:24 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 130919A (trigger=571271). The BAT on-board calculated location is RA, Dec 207.288, -10.355 which is RA(J2000) = 13h 49m 09s Dec(J2000) = -10d 21' 19" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a broad peak of at least 60 seconds duration. This was an image trigger, so the currently available light curve does not show significant structure. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 23:23 UT on 2013 December 7. There will thus be no XRT or UVOT data for this trigger before this time. Burst Advocate for this burst is H. A. Krimm (krimm 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 15234 table
GRB_name GRB130919A
GCN_number 15234
Detection_method Swift-BAT Det
ra 207.2810°
decl -10.3530°
Circular_text TITLE: GCN CIRCULAR NUMBER: 15234 SUBJECT: GRB 130919A, Swift-BAT refined analysis DATE: 13/09/20 02:27:56 GMT FROM: Hans Krimm at NASA-GSFC A. Y. Lien (NASA/GSFC/ORAU), S. D. Barthelmy (GSFC), J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU), M. Stamatikos (OSU), T. N. Ukwatta (MSU) (i.e. the Swift-BAT team): Using the data set from T-60 to T+243 sec from the recent telemetry downlink, we report further analysis of BAT GRB 130919A (trigger #571271) (Krimm, et al., GCN Circ. 15232). The BAT ground-calculated position is RA, Dec = 207.281, -10.353 deg which is RA(J2000) = 13h 49m 07.5s Dec(J2000) = -10d 21' 11.0" with an uncertainty of 1.6 arcmin, (radius, sys+stat, 90% containment). The partial coding was 77%. The burst came into the BAT field of view at ~T-60 seconds, following a pre-planned slew and another slew took it out of the field at around T+215 seconds. mask-weighted light curve shows a broad peak from T-30 s to T+70 s, with at least six subpeaks superimposed. T90 (15-350 keV) is 97.3 +- 25.1 sec (estimated error including systematics). The time-averaged spectrum from T-20.15 to T+108.07 sec is best fit by a power law with an exponential cutoff. This fit gives a photon index 0.54 +- 0.73, and Epeak of 71.7 +- 31.8 keV (chi squared 58.75 for 56 d.o.f.). For this model the total fluence in the 15-150 keV band is 1.4 +- 0.2 x 10^-6 erg/cm2 and the 1-sec peak flux measured from T-6.49 sec in the 15-150 keV band is 0.5 +- 0.1 ph/cm2/sec. A fit to a simple power law gives a photon index of 1.52 +- 0.14 (chi squared 65.60 for 57 d.o.f.). 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/571271/BA/
GCN 15235 table
GRB_name GRB130919A
GCN_number 15235
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 15235 SUBJECT: GRB 130919A: Skynet PROMPT-CTIO optical upper limits DATE: 13/09/20 04:04:19 GMT FROM: Adam S. Trotter at UNC-Chapel Hill/PROMPT/Skynet A. Trotter, D. Reichart, J. Haislip, A. LaCluyze, J. Moore, N. Frank, K. Ivarsen, M. Nysewander, A. Foster, T. Berger, H. T. Cromartie, R. Egger, M. Maples, and J. A. Crain report: Skynet observed the Swift-BAT localization of GRB 130919A (Krimm et al., GCN 15232; Lien et al., GCN 15234, Swift trigger=571271) with three 16" telescopes of the PROMPT array at CTIO, Chile (V, R, and I bands). Starting at 2013-09-19, 23:29 UT and continuing until 2013-09-20, 00:00 UT (t=12.40-12.93h post-trigger), Skynet took a total of 49 160s exposures, at high airmass >3. In stacked images, we do not detect any uncatalogued optical source in any band in or near the Swift-BAT error circles. The 3-sigma limiting magnitudes of our images are: ================================== tmid scope expos fil limit ================================== 12.67h Prompt5 12x160s I >19.44 12.55h Prompt4 7x160s R >19.24 12.63m Prompt1 10x160s V >19.54 ================================== Magnitudes are in the Vega System, calibrated to 8 APASS-DR7 stars in the field. Magnitudes have not been corrected for line-of-sight Milky Way dust extinction, with expected E(B-V)=0.057 (Schlegel et al. 1998). No further Skynet observations are scheduled.
GCN 15238 table
GRB_name GRB130919A
GCN_number 15238
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 15238 SUBJECT: Fermi Trigger 401326696: MASTER prompt optical observations DATE: 13/09/21 12:42:39 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs H. Levato and C. Saffe Instituto de Ciencias Astronomicas, de la Tierra y del Espacio (ICATE) C. Mallamaci, C. Lopez and F. Podest Observatorio Astronomico Felix Aguilar (OAFA) E. Gorbovskoy, V. Lipunov, V. Kornilov, D. Denisenko, A. Kuznetsov, D. Kuvshinov, A. Belinski, N. Tyurina, N. Shatskiy, P. Balanutsa, D. Zimnukhov, V.V. Chazov Lomonosov Moscow State University, Sternberg Astronomical Institute A. Tlatov, A.V. Parhomenko, D. Dormidontov, V. Sennik Kislovodsk Solar Station of the Pulkovo Observatory K. Ivanov, S. Yazev, N.M. Budnev, O. Gres, O. Chuvalaev, V.A. Poleshchuk Irkutsk State University V. Yurkov, Yu. Sergienko, D. Varda, E. Sinyakov Blagoveschensk Educational State University, Blagoveschensk V. Krushinski, I. Zalozhnich, A. Popov, A. Bourdanov, A. Punanova Ural Federal University MASTER-ICATE robotic very wide field cameras (FOV=2x384 square degrees, D=72mm, f/1.2, 1 pix = 22 arcsec, http://observ.pereplet.ru) located in Argentina (Observatorio Astronomico Felix Aguilar, http://93.180.27.230:8080/) synchronously observed 35% part of FERMI GRB130919A (trigger 401326696) error box before, during and after the trigger. Since 40 sec after the trigger cameras pointed to FERMI alert our FOV cover 95% part of error box. We haven't found optical transient within FERMI error-box our first (5 s exposure) set. The 5-sigma upper limit has been about 12.0 mag. The 5-sigma upper limit on coadd first 30 images is about 13.0 mag. The first seconds movie locate here http://master.sai.msu.ru/static/GRB130919A.gif Our cameras are continuously imaging the sky with 5 sec exposures. The more accurat error box (by IPN) is requied. The message may be cited.