//////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 31661 SUBJECT: GRB 220302A: Swift detection of a burst DATE: 22/03/02 07:57:49 GMT FROM: Kim Page at U.of Leicester E. Troja (NASA/GSFC/UMCP), C. Gronwall (PSU), K. L. Page (U Leicester), D. M. Palmer (LANL) and T. M. Parsotan (GSFC/UMBC/CRESSTII) report on behalf of the Neil Gehrels Swift Observatory Team: At 07:40:19 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 220302A (trigger=1094950). Swift did not slew to the burst. The BAT on-board calculated location is RA, Dec 301.432, +49.389 which is RA(J2000) = 20h 05m 44s Dec(J2000) = +49d 23' 20" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a complex structure with a duration of about 20 sec. The peak count rate was ~1156 counts/sec (15-350 keV), at ~2 sec after the trigger. Swift is currently restarting after a reaction wheel failure, so automatic slews to GRBs are turned off. Therefore there will be no XRT or UVOT observations at this time. Burst Advocate for this burst is E. Troja (nora.gsfc AT gmail.com). 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/) //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 31662 SUBJECT: Swift GRB 220302A: Global MASTER-Net observations report DATE: 22/03/02 08:36:31 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs V. Lipunov, V.Kornilov, E.Gorbovskoy, K.Zhirkov, N.Tyurina, P.Balanutsa, A.Kuznetsov, D. Vlasenko, G.Antipov, D.Zimnukhov, V.Senik, T.Pogrosheva, E.Minkina, A.Chasovnikov, V.Topolev, V.Grinshpun, D.Kuvshinov, D. Cheryasov (Lomonosov Moscow State University, SAI, Physics Department), R. Podesta, C.Lopez, F. Podesta, C.Francile (Observatorio Astronomico Felix Aguilar OAFA), R. Rebolo, M. Serra (The Instituto de Astrofisica de Canarias), D. Buckley (South African Astronomical Observatory), O.A. Gres, N.M. Budnev (Irkutsk State University, API), B.L.Carrasco, J.R.Valdes,V.Chavushyan, C.J.Martinez, V.M.Patino Alvarez, M.L.H.Rodriguez (INAOE, OAGH) A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory), A. Gabovich, V.Yurkov (Blagoveschensk Educational State University) MASTER-OAGH robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in Mexico (OAGH National Institute for Astrophysics, Optics and Electronics) was pointed to the Swift GRB 220302A ( E. Troja et al., GCN 31661) errorbox 2514 sec after notice time and 2575 sec after trigger time at 2022-03-02 08:23:15 UT, with upper limit up to 16.6 mag. The observations began at zenith distance = 87 deg. The sun altitude is -63.3 deg. The galactic latitude b = 9 deg., longitude l = 84 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=1899637 We obtain a following upper limits. Tmid-T0 | Site |Filt.| Expt. | Limit| Comment _________|_____________________|_____|_______|______|________ 2606 | MASTER-OAGH | C | 60 | 15.8 | 2687 | MASTER-OAGH | C | 60 | 15.0 | 2769 | MASTER-OAGH | C | 60 | 15.7 | 3051 | MASTER-OAGH | C | 60 | 16.6 | 3133 | MASTER-OAGH | C | 60 | 15.8 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 31664 SUBJECT: GRB 220302A: Swift afterglow detection DATE: 22/03/02 17:03:47 GMT FROM: Kim Page at U.of Leicester E. Troja (NASA/GSFC/UMCP), C. Gronwall (PSU), J. A. Kennea (PSU), K. L. Page (U Leicester), D. M. Palmer (LANL), T. M. Parsotan (GSFC/UMBC/CRESSTII) and A. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: Continuing the recovery from the Reaction Wheel anomaly, Swift has performed a follow-up observation of GRB 220302A which occurred at 07:40:19 UT (Troja et al., GCN 31661). The XRT began observing the field at 16:41:18.7 UT, 32459.3 seconds after the BAT trigger. Using promptly downlinked data we find an uncatalogued X-ray source located at RA, Dec 301.43151, 49.38868 which is equivalent to: RA(J2000) = 20h 05m 43.56s Dec(J2000) = +49d 23' 19.2" with an uncertainty of 4.7 arcseconds (radius, 90% containment). This location is 1.6 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 https://www.swift.ac.uk/sper. We cannot determine whether the source is fading at the present time. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density consistent with the Galactic value of 3.44 x 10^21 cm^-2 (Willingale et al. 2013). UVOT took a finding chart exposure of 150 seconds with the White filter starting 32463 seconds after the BAT trigger. No credible afterglow candidate has been found in the initial data products. The 2.7'x2.7' sub-image covers 100% of the XRT error circle. The typical 3-sigma upper limit has been about 19.6 mag. 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 0.216. Burst Advocate for this burst is E. Troja (nora.gsfc AT gmail.com). 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/) //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 31666 SUBJECT: GRB 220302A: Enhanced Swift-XRT position DATE: 22/03/02 23:50:27 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 1271 s of XRT Photon Counting mode data and 2 UVOT images for GRB 220302A, 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 = 301.43044, +49.38699 which is equivalent to: RA (J2000): 20h 05m 43.30s Dec (J2000): +49d 23' 13.1" with an uncertainty of 2.9 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: 31669 SUBJECT: GRB 220302A: BOOTES-5/JGT optical upper limit DATE: 22/03/03 17:13:47 GMT FROM: Youdong HU at IAA-CSIC Y.-D. Hu, E. Fernandez-Garcia, T.-R. Sun, A. J. Castro-Tirado, M.D. Caballero-Garcia and R. Sanchez-Ramirez (IAA-CSIC), D. Hiriart and W. H. Lee (UNAM), C. J. Perez del Pulgar and I. Carrasco (UMA), I. H. Park (SKKU) on behalf of a larger collaboration, report: Following the detection of GRB 220302A by Swift (Troja et al. GCNC 31661), the BOOTES-5/JGT 0.6m robotic telescope at Observatorio Astronomico Nacional in San Pedro Martir (Mexico) automatically started to observe the GRB localization starting on Mar 2 at 12:59 UT (~5.3 hours after trigger). In the co-added image (5 x 60 s exposures in the clear filter), no optical afterglow is detected within the Swift/XRT error region (Troja et al. GCNC 31664, Osborne et al. GCNC 31666) down to 20.3 mag. This non-detection is consistent with the UVOT (Troja et al. GCNC 31664) and MASTER observation (Lipunov et al. GCNC 31662). We thank the staff at Observatorio Astronomico Nacional in San Pedro Martir for their excellent support. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 31673 SUBJECT: GRB 220302A: Swift-XRT refined Analysis DATE: 22/03/04 06:42:37 GMT FROM: Phil Evans at U of Leicester M. Perri (SSDC & INAF-OAR), V. D'Elia (SSDC & INAF-OAR), A. D'Ai (INAF-IASFPA), J. D. Gropp (PSU), J.A. Kennea (PSU), A. Tohuvavohu (U. Toronto), P.A. Evans (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester) and E. Troja report on behalf of the Swift-XRT team: We have analysed 3.4 ks of XRT data for GRB 220302A (Troja et al. GCN Circ. 31661), from 32.5 ks to 160.8 ks after the BAT trigger. The data are entirely in Photon Counting (PC) mode. The enhanced XRT position for this burst was given by Osborne et al. (GCN Circ. 31666). The light curve can be modelled with a power-law decay with a decay index of alpha=0.7 (+0.5, -0.4). The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/01094950. This circular is an official product of the Swift-XRT team. //////////////////////////////////////////////////////////////////////// TITLE: GCN CIRCULAR NUMBER: 31682 SUBJECT: GRB 220302A: Swift/UVOT Upper Limits DATE: 22/03/05 03:37:18 GMT FROM: Mike Siegel at PSU/Swift MOC M. H. Siegel (PSU) and E. Troja (NASA/GSFC/UMCP) report on behalf of the Swift/UVOT team: The Swift/UVOT began settled observations of the field of GRB 220302A 32464 s after the BAT trigger (Troja et al., GCN Circ. 31661). No optical afterglow consistent with the XRT position (Osborne et al. GCN Circ. 31666) 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 subsequent exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white_FC 32464 32614 147 >19.9 white 32464 32614 147 >19.9 v 32621 33528 885 >19.2 m2 33533 34194 651 >19.7 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.217 in the direction of the burst (Schlegel et al. 1998).