GRB230816A

This page lists all entries on GRB230816A in GRBweb

Summary IPN Swift GCN 34450 GCN 34453 GCN 34456 GCN 34457 GCN 34458 GCN 34459 GCN 34460 GCN 34462 GCN 34469 GCN 34470 GCN 34473 GCN 34474

Summary table
Variable Value Source
T0 16:08:48 UTC GCN_circulars,Swift Det
ra 328.4455° Swift
decl 37.8548° Swift
pos_error 2.85e-04° Swift
T90 20.48 s Swift
T90_start 16:08:48 UTC Swift
fluence 7.70e-07 erg/cm² Swift
T100 20.48 s
GBM_located False
mjd 60172.67277777778 GCN_circulars,Swift Det
IPN table
GRB_name GRB230816A
ra 328.3750°
decl 37.8333°
pos_error 5.00e-02°
Swift table
GRB_name GRB230816A
t_trigger 16:08:48 UTC
ra 328.4455°
decl 37.8548°
pos_error 2.85e-04°
T90 20.48 s
fluence 7.70e-07 erg/cm²
GCN 34450 table
GRB_name GRB230816A
GCN_number 34450
Detection_method Swift Det
t_trigger 16:08:48 UTC
ra 328.3750°
decl 37.8280°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34450 SUBJECT: GRB 230816A: Swift detection of a burst DATE: 23/08/16 16:24:41 GMT FROM: David Palmer at LANL M. H. Siegel (PSU), S. Dichiara (PSU), R. A. J. Eyles-Ferris (U Leicester), J.D. Gropp (PSU), J. A. Kennea (PSU), F. E. Marshall (NASA/GSFC), M. J. Moss (GWU), K. L. Page (U Leicester), D. M. Palmer (LANL), T. M. Parsotan (GSFC/UMBC/CRESSTII), B. Sbarufatti (INAF-OAB) and M. A. Williams (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 16:08:48 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 230816A (trigger=1185673). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 328.375, +37.828 which is RA(J2000) = 21h 53m 30s Dec(J2000) = +37d 49' 43" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a single-peaked structure with a duration of about 25 sec. The peak count rate was ~1900 counts/sec (15-350 keV), at ~0 sec after the trigger. The XRT began observing the field at 16:10:18.4 UT, 90.2 seconds after the BAT trigger. Using promptly downlinked data we find a fading, uncatalogued X-ray source with an enhanced position: RA, Dec 328.44552, 37.85549 which is equivalent to: RA(J2000) = 21h 53m 46.92s Dec(J2000) = +37d 51' 19.8" with an uncertainty of 1.9 arcseconds (radius, 90% containment). This location is 223 arcseconds from the BAT onboard position. This position may be improved as more data are received; the latest position is available at https://www.swift.ac.uk/sper. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density in excess of the Galactic value (2.90 x 10^21 cm^-2, Willingale et al. 2013), with an excess column of 3.7 (+3.48/-2.91) x 10^21 cm^-2 (90% confidence). UVOT took a finding chart exposure of 150 seconds with the White filter starting 93 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 none of the XRT error circle. 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 0.311. Burst Advocate for this burst is M. H. Siegel (siegel AT swift.psu.edu). 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/)
GCN 34453 table
GRB_name GRB230816A
GCN_number 34453
Detection_method Optical
ra 328.4454°
decl 37.8544°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34453 SUBJECT: GRB 230816A: Nanshan/HMT optical afterglow detection DATE: 23/08/16 18:15:50 GMT FROM: Dong Xu at NAOC/CAS S.Q. Jiang, S.Y. Fu, X. Liu, T.H. Lu, Z.P. Zhu, D. Xu (NAOC), X. Gao (Urumqi No.1 Senior High School), J.Z. Liu (XAO) report: We observed the field of GRB 230816A detected by Swift (Siegel et al., GCN 34450) using the HMT-0.5m telescope located at Nanshan, Xinjiang, China. Observations started at 16:10:20 UT on 2023-08-16, i.e., 92 s after the Swift/BAT trigger, we obtained a serise of 3x20, 3x40, 4x60, 12x90 s frames without any filter. An uncatalogued optical source is detected in our stacked image at coordinates R.A. (J2000) = 21:53:46.9 Dec. (J2000) = +37:51:15.9 2.23 arcsec away from the center of the XRT error circle (radius: 1.9 arcsec, 90% containment; Siegel et al., GCN 34450) with m(r) = 19.6 +/- 0.18 mag(AB) at 24.6 min post-burst, calibrated with the nearby PanSTAR field in the Sloan r-filter and the magnitude is not corrected for Galactic extinction. We thus think this OT is the optical afterglow of the burst.
GCN 34456 table
GRB_name GRB230816A
GCN_number 34456
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 34456 SUBJECT: GRB 230816A: SAO RAS optical observations DATE: 23/08/16 19:26:01 GMT FROM: Moskvitin Alexander at SAO RAS A. S. Moskvitin and O. I. Spiridonova (SAO RAS), report on behalf of the GRB follow-up team. We observed the field of the GRB 230816A (Siegelet al., GCN 34450) with the 1-m telescope of SAO RAS Zeiss-1000 equipped with the CCD photometer. We obtained 8 x 300 sec. images in Rc band on August 16, 17:45:41 -- 18:35:29 UT. The OT (Jiang et al., GCN 34453) is clearly detected in our stacked frame with the coordinates R.A. (J2000) = 21:53:46.9, Decl.(J2000) = +37:51:16.7 (+/- 0".5) and the brightness of R = 21.0 +/- 0.1 (t_mid - t0 = 2.030h = 0.0846d). This preliminary photometry is based on nearby USNO-B1 stars (R2 mag), the magnitude is not corrected for MW extinction.
GCN 34457 table
GRB_name GRB230816A
GCN_number 34457
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 34457 SUBJECT: GRB 230816A: TShAO and Assy optical observations DATE: 23/08/16 20:29:24 GMT FROM: Alexei Pozanenko at IKI, Moscow N. Pankov (HSE, IKI), I. Reva (FAI), V. Kim (FAI), A. Pozanenko (IKI), S. Belkin (IKI) report on behalf of the GRB-IKI-FuN. We observed the field of the GRB 230816A (Siegel et al., GCN 34450) with Zeiss-1000 telescope of Tien-Shan Observatory (TShAO) and AZT-20 telescope of Assy Observatory. We clearly detect the afterglow (Jiang et al., GCN 34453; Moskivitin et al., GCN 34456) in the stacked images. Preliminary photometry is following Date UT start t-T0 Filter Exp. OT Err. UL(3sigma) (mid, days) (s) 2023-08-16 16:21:24 0.034787 R 25*180 19.57 0.10 22.3 2023-08-16 17:26:29 0.072354 r' 53*60 21.10| 0.025 23.5 The photometry is based on nearby stars of USNO-B1.0 and PanSTARRS-DR1 catalogues. RA Dec R2 r' 328.5043802 +37.8674441 16.47 16.8245 328.3579777 +37.8706420 17.04 17.1589 328.4483771 +37.8290610 15.45 15.3054
GCN 34458 table
GRB_name GRB230816A
GCN_number 34458
Detection_method Other
ra 328.4459°
decl 37.8546°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34458 SUBJECT: GRB 230816A: AKO Optical Observations DATE: 23/08/16 20:58:15 GMT FROM: Mohammad Odeh at Al Khatim Observatory M44 Mohammad Odeh, Nada Odeh, Osama Ghannam, Anas Mohammad, and Khalfan Al-Noaimy, report on behalf of Al-Khatim Observatory (AKO) operated by the International Astronomical Center in Abu Dhabi, UAE: We observed the field of the GRB 230816A (Siegel et al., GCN 34450) with our 0.36m f/7.7 robotic telescope. We obtained 21 x 180 sec. images in a clear filter on 16 August, from 19:05 to 20:36 UT. We detected the afterglow (Jiang et al., GCN 34453; Moskivitin et al., GCN 34456; Pankov et al., GCN 34457) in our stacked images with the coordinates (J2000) R.A.= 21:53:47.01, Dec.= +37:51:16.7 and the brightness of Mv = 20.6 +/- 0.27 (t_mid - t0 = 3.7 hours). The magnitude is not corrected for galactic extinction.
GCN 34459 table
GRB_name GRB230816A
GCN_number 34459
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 34459 SUBJECT: GRB 230816A: Tautenburg observations DATE: 23/08/16 21:06:26 GMT FROM: Sylvio Klose at TLS Tautenburg S. Klose, S. Melnikov, B. Stecklum, A. Nicuesa Guelbenzu, F. Ludwig (all TLS Tautenburg) report: We observed the field of GRB 230816A (Siegel et al., GCN 34450) with the Tautenburg 1.34m Schmidt telescope equipped with the TAUKAM 6kx6k CCD camera and using the Sloan filter set. For the optical transient discovered by Jiang et al. (GCN 34453) we measure the following preliminary magnitudes: r = 21.75 +/- 0.25 (midtime: August 16, 2023, 20:23:11 UT), i = 20.33 +/- 0.08 (midtime: August 16, 2023, 20:34:05 UT), calibrated against USNO stars in the field. The photometry will still be improved by calibrating the data via a nearby Pan-STARRS field.
GCN 34460 table
GRB_name GRB230816A
GCN_number 34460
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 34460 SUBJECT: GRB230816A: Possible host and GIT detection of optical counterpart DATE: 23/08/16 22:08:37 GMT FROM: Vishwajeet Swain at IIT Bombay R. Kumar (IITB), R. Sharma (IITB), V. Swain (IITB), A. Salgundi (IITB), H. Kumar (IITB), G. Waratkar(IITB), V. Bhalerao (IITB), G. C. Anupama(IIA), S. Barway (IIA) and K. Angail (IAO) report on behalf of the GIT team: We observed the field of GRB 230816A detected by SWIFT (Siegel et al., GCN 34450) with 0.7m GROWTH-India Telescope (GIT). We started observations at 16:40:00 UT, i.e., 31.2 mins after the Swift/BAT trigger. We obtained 5 frames in the r' band of 300 sec each. After image subtraction, we detected a source in our stacked image at RA 21:53:46.96, Dec: +37:51:16.08 with an uncertainty of 0.67 arcsec - coincident with the reported afterglow (Jiang et al., GCN 34453), and 3.75 arsec away from center of the XRT error circle (Siegel et al., GCN 34450). We note that there is a faint source (m_r ~ 23.0) nearly coincident with the counterpart in the Pan-STARRS1 images, which could be a host of this GRB. Our image subtraction ensures that this source flux does not affect out photometric measurements. There is no minor planet present at this position. The photometric results are as follows: ---------------------------------------------------------------------- JD (mid) | T_mid-T0 (mins) | Exposure (sec) | Filter | Magnitude (AB) | ---------------------------------------------------------------------- 2460173.202193 | 42.35 | 5 x 300 | r' | 20.61 +/- 0.06 | ---------------------------------------------------------------------- Our results are consistent with other reports (Jiang et al. GCN 34453, Moskvitin et al., GCN 34456, Pankov et al., GCN 34457, Odeh et al., GCN 34458, Klose et al., GCN 34459). We encourage photometric for further confirmation and spectroscopic follow-up for redshift measurement. The magnitudes are calibrated against PanSTARRS DR1 (Chambers et al., 2016) and are not corrected for Galactic extinction. The GROWTH India Telescope (GIT; Kumar et al. 2022) is a 70-cm telescope with a 0.7-degree field of view, set up by the Indian Institute of Astrophysics (IIA) and the Indian Institute of Technology Bombay (IITB) with funding from DST-SERB and IUSSTF. It is located at the Indian Astronomical Observatory (Hanle), operated by IIA. We acknowledge funding by the IITB alumni batch of 1994, which partially supports the operations of the telescope. Telescope technical details are available at https://sites.google.com/view/growthindia/.
GCN 34462 table
GRB_name GRB230816A
GCN_number 34462
Detection_method Swift-XRT Det
ra 328.4457°
decl 37.8550°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34462 SUBJECT: GRB 230816A: Enhanced Swift-XRT position DATE: 23/08/17 03:20:23 GMT FROM: Phil Evans at U of Leicester P.A. Evans, M.R. Goad, J.P. Osborne and A.P. Beardmore (U. Leicester) report on behalf of the Swift-XRT team. Using 1206 s of XRT Photon Counting mode data and 1 UVOT images for GRB 230816A, 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 = 328.44568, +37.85495 which is equivalent to: RA (J2000): 21h 53m 46.96s Dec (J2000): +37d 51' 17.8" with an uncertainty of 2.3 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.
GCN 34469 table
GRB_name GRB230816A
GCN_number 34469
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 34469 SUBJECT: GRB 230816A: Osservatorio Astronomico "Nastro Verde" optical observations DATE: 23/08/17 19:51:04 GMT FROM: Nello Ruocco at Osservatorio Nastro Verde - Sorrento (Naples) - Italy - MPC Code C82 Nello Ruocco at Osservatorio Nastro Verde - Sorrento (Naples) - Italy in a large collaboration with: M.G. Dainotti (National Astronomical Observatory of Japan), Y. Niino (Tokyo University, Institute of Astronomy), K. Kalinowski (Aarhus University, Department of Physics and Astronomy), B. De Simone (Universita' degli Studi Di Salerno) report: We observed the field of GRB 230816A (Siegel et al., GCN 34450) with telescope of Nastro Verde Observatory - Sorrento (Naples), Italy. Member of: AAVSO - American Association of Variable Star Observers. UAI/SSV - Unione Astrofili Italiani/sezione stelle variabili. AstroCampania Associazione The observations started at 18:55 UT of 2023/08/16, after about 2,45 hours after the GRB trigger, at the end of twilight with clear skies, with principal telescope SC 0.35 f/10 with focal reduced + CCD Sbig ST10 XME I took 25 image of 240 sec each. All images are unfiltered, calibrated with masterdark and masterflat,stacked with Tycho Tracker software We have detected a faint source of magnitude 19.1 G at the enhanced position reported by Swift-XRT (Siegel et al., GCN 34450, P.A. Evans et al., GCN 34462) and by optical telescopes ( A. S. Moskvitin et al GCN 34456., N. Pankov et al GCN 34457., Mohammad Odeh et al GCN 34458., S. Klose et al GCN 34459., R. Kumar et al GCN 34460) at following position RA (J2000) 21h 53m 46.87s Decl. (J2000) +37° 51' 14.7" Photometry and astrometry on stack of 13 images each of 240 sec GRB 230816A KC2023 08 16.88481 21 53 46.87 +37 51 14.7 19.1 G C82 Magnitudes were estimated with the GAIA DR2 cat. and are not corrected for galactic dust extinction. The message may be cited.
GCN 34470 table
GRB_name GRB230816A
GCN_number 34470
Detection_method Swift-XRT Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 34470 SUBJECT: GRB 230816A: Swift-XRT refined Analysis DATE: 23/08/17 21:21:12 GMT FROM: Phil Evans at U of Leicester M.G. Bernardini (INAF-OAB), J. D. Gropp (PSU), S. Dichiara (PSU), J.A. Kennea (PSU), K.L. Page (U. Leicester), A.P. Beardmore (U. Leicester), E. Ambrosi (INAF-IASFPA) , M. Capalbi (INAF-IASFPA) and P.A. Evans report on behalf of the Swift-XRT team: We have analysed 3.9 ks of XRT data for GRB 230816A, from 97 s to 91.3 ks after the BAT trigger. The data are entirely in Photon Counting (PC) mode. The light curve can be modelled with a power-law decay with a decay index of alpha=1.44 (+0.27, -0.43). A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.66 (+0.31, -0.14). The best-fitting absorption column is consistent with the Galactic value of 2.9 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 4.4 x 10^-11 (5.6 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 2.9 (+/-1.2) x 10^21 cm^-2 Galactic foreground: 2.9 x 10^21 cm^-2 Excess significance: <1.6 sigma Photon index: 1.66 (+0.31, -0.14) The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/01185673. This circular is an official product of the Swift-XRT team.
GCN 34473 table
GRB_name GRB230816A
GCN_number 34473
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 34473 SUBJECT: GRB 230816A: SVOM/C-GFT optical detection DATE: 23/08/18 13:41:54 GMT FROM: Chao Wu at NAOC Liping Xin (NAOC), Chao Wu (NAOC), Zhe Kang (CHO), Xuhui Han (NAOC), Huali Li (NAOC), Xiaomeng Lu (NAOC), Damien Turpin(CEA), Zhenwei Li (CHO),Pinpin Zhang (NAOC),Ruosong Zhang (NAOC),Yulei Qiu (NAOC),You Lv (CHO),Jing Wang(GXU), Cordier Bertrand (CEA) and Jianyan Wei (NAOC) on behalf of SVOM GRB team We observed the burst GRB230816A (Siegel et al. GCN Circ. 34450) on 16:15:38 UT, Aug. 16th, 2023, about 6.9 minutes after the Swift trigger with C-GFT (Chinese Ground Follow-up Telescope in SVOM mission) in System Test Mode (STM). C-GFT is located at Jilin (long.=126.33 deg, lat.=43.8243778 deg), Changchun Observatory, National Astronomical Observatories, CAS. It has FOV of 1.5 deg X 1.5 deg with a 4k*4k CMOS detector mounted on the primary focus of 1.2-meter-aperure telescope. A series of g and r band images were obtained. The exposure time was 10 seconds for each frame. The optical afterglow reported (Jiang et al., GCN 34453, Moskvitin et al., GCN 34456., Pankov et al.,GCN 34457, Odeh et al., GCN 34458Klose et al., GCN 34459., Kumar et al., GCN 34460; Ruocco et al., GCN 34469) was also clearly detected by our stacked r-band image (100 * 10 seconds). The brightness was estimated to be about 20.1 +/-0.2 magnitude in r-band with the midtime of about 34 min after the burst, after calibration with nearby USNO R2 catalogs. More detailed analysis is continuing. We thank the observation assistant Bowen Li at Jilin observatory for their excellent support. This message may be cited.
GCN 34474 table
GRB_name GRB230816A
GCN_number 34474
Detection_method Swift-BAT Det
ra 328.4530°
decl 37.8530°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34474 SUBJECT: GRB 230816A: Swift-BAT refined analysis DATE: 23/08/18 18:04:02 GMT FROM: Tyler Parsotan at NASA GSFC A. Y. Lien (U Tampa), S. D. Barthelmy (GSFC), H. A. Krimm (NSF), S. Laha (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Parsotan (GSFC/UMBC), T. Sakamoto (AGU), M. Stamatikos (OSU) (i.e. the Swift-BAT team): Using the data set from T-239 to T+303 sec from the recent telemetry downlink, we report further analysis of BAT GRB 230816A (trigger #1185673) (Siegel, et al., GCN Circ. 34450). The BAT ground-calculated position is RA, Dec = 328.453, 37.853 deg which is RA(J2000) = 21h 53m 48.8s Dec(J2000) = +37d 51' 12.1" with an uncertainty of 1.2 arcmin, (radius, sys+stat, 90% containment). The partial coding was 98%. The mask weighted light curve shows a fast rise exponential decay type single peak. T90 (15-350 keV) is 20.48 +- 4.94 sec (estimated error including systematics). The time-averaged spectrum from T-5.60 to T+21.08 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.43 +- 0.14. The fluence in the 15-150 keV band is 7.7 +- 0.7 x 10^-07 erg/cm2. The 1-sec peak photon flux measured from T+0.60 sec in the 15-150 keV band is 1.0 +- 0.1 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/1185673/BA/