GRB250430A
This page lists all entries on GRB250430A in GRBweb
Summary Swift GCN 40292 GCN 40294 GCN 40295 GCN 40299 GCN 40302 GCN 40303 GCN 40304 GCN 40305 GCN 40307 GCN 40308 GCN 40310 GCN 40311 GCN 40312 GCN 40316 GCN 40318 GCN 40321 GCN 40323
Summary table | ||
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Variable | Value | Source |
T0 | 17:31:21 UTC | GCN_circulars,Swift Det |
ra | 233.3869° | Swift |
decl | -18.1184° | Swift |
pos_error | 1.42e-04° | Swift |
GBM_located | False | |
mjd | 60795.730104166665 | GCN_circulars,Swift Det |
Swift table | ||
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GRB_name | GRB250430A | |
t_trigger | 17:31:21 UTC | |
ra | 233.3869° | |
decl | -18.1184° | |
pos_error | 1.42e-04° |
GCN 40292 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40292 | |
Detection_method | Swift Det | |
t_trigger | 17:31:21 UTC | |
ra | 233.4280° | |
decl | -18.0830° | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40292
SUBJECT: GRB 250430A: Swift detection of a burst with optical counterpart
DATE: 25/04/30 18:07:07 GMT
FROM: Tyler Parsotan at NASA GSFC |
GCN 40294 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40294 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40294
SUBJECT: GRB 250430A: Kanata optical upper limit
DATE: 25/04/30 18:52:29 GMT
FROM: Koji Kawabata at HASC,Hiroshima U |
GCN 40295 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40295 | |
Detection_method | Swift-BAT Det | |
ra | 233.3873° | |
decl | -18.1183° | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40295
SUBJECT: GRB 250430A: AKO Optical Afterglow Detection
DATE: 25/04/30 19:20:09 GMT
FROM: Mohammad Odeh at Al Khatim Observatory M44 |
GCN 40299 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40299 | |
Detection_method | Swift-XRT Other | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40299
SUBJECT: EP250430a/GRB 250430A: Einstein Probe WXT detection of the X-ray prompt emission
DATE: 25/05/01 08:11:44 GMT
FROM: EP Team at NAOC/CAS |
GCN 40302 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40302 | |
Detection_method | MITSuME | |
Circular_text | TITLE: GCN CIRCULAR NUMBER: 40302 SUBJECT: GRB 250430A : MITSuME Akeno optical upper limits DATE: 25/05/01 11:06:05 GMT FROM: hagio.h.ffca@m.isct.ac.jp H. Hagio, I. Takahashi, M. Sasada, H. Seki, S. Joshima, Y. Kubo, A. Ochi, R. Kato, Y. Yatsu and N. Kawai (Science Tokyo) report on behalf of the MITSuME collaboration: We observed the field of GRB 240430A detected by Swift/BAT (Parsotan et al. GCN 40292) with the optical three-color (g', Rc, and Ic) CCD cameras attached to the MITSuME 50-cm telescope Akeno. The observation started at 2025-04-30 17:31:53 UT (32 seconds after the Swift/BAT trigger). We stacked the images with good conditions. We did not detect any obvious point sources at the position reported by Parsotan et al., GCN 40292, Odeh et al., GCN 40295, Wang et al., GCN 40299, and Garnichey et al., GCN 40301. We obtained the 5-sigma limits of the stacked images as follows: T0+[min] | MID-UT | T-EXP[sec] | 5-sigma limits ------------------------------------------------------------------------------------------------ 15.1 | 2025-04-30 17:46:27 | 620 | g'>18.2, Rc>18.2, Ic>17.8 78.5 | 2025-04-30 18:29:51 | 2880 | g'>19.3, Rc>19.6, Ic>19.0 ------------------------------------------------------------------------------------------------ T0+ : Elapsed time after the trigger T-EXP: Total Exposure time We used the PS1 catalog for flux calibration. The catalog magnitudes in PS1 g, r and i bands were converted to our g', Rc and Ic band magnitudes following Tonry et al. (2012), Table 6. The magnitudes are expressed in the AB system. The images were processed in real-time through the MITSuME GPU reduction pipeline (Niwano et al. 2021, PASJ; https://github.com/MNiwano/Eclaire). |
GCN 40303 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40303 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40303
SUBJECT: GRB 250430A: Bassano Bresciano Observatory upper limit
DATE: 25/05/01 13:33:33 GMT
FROM: Ulisse Quadri at Bassano Bresciano Observatory |
GCN 40304 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40304 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR NUMBER: 40304 SUBJECT: GRB 250430A: Leavitt Observatory optical upper limit DATE: 25/05/01 14:02:45 GMT FROM: leavittob@gmail.com L. Moretti, E. Pavoni (Leavitt Observatory, Italy) Members of: GRB/UAI - Gamma Ray Burst Section of Unione Astrofili Italiani ATA - Associazione Tuscolana di Astronomia 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), report: We observed the field of the GRB 250430A / EP250430a (Parsotan et al., GCN 40292; Wang et al., GCN 40299) with our RC telescope (D=250 mm, F/D=8) of Leavitt Observatory, Manciano, Italy. The observations started approximately 6 hours after the Swift/BAT trigger time, with good weather conditions. We utilized the astropy package (Astropy Collaboration et al., 2022ApJ...935..167A) to align and stack 25 individual frames of 120 sec each, with a median time of 2025-04-30T23:29:41 (UTC). All images are unfiltered and were processed by a single data processing pipeline based on astropy package (Astropy Collaboration et al., 2022ApJ...935..167A). In the stacked frame, we did not found any optical uncatalogued object within the Swift error circle. Mid-Time (UTC) Rc limit Error 2025-04-30T23:29:41 >20.32 +/- 0.01 This upper limit is consistent with other observations reported by K. S. Kawabata et al. (GCN Circular 40294), Mohammad Odeh et al. (GCN Circular 40295), Andrea Saccardi et al (GCN Circular 40301), H. Hagio et al. (GCN Circular 40302), Quadri et al. (GCN 40303). Our photometry is in the AB system and is not corrected for galactic dust extinction. Magnitudes were estimated with the Pan-STARRS cat. and converted using Lupton (2005) equations. The message may be cited. Reference: https://leavittobservatory.altervista.org |
GCN 40305 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40305 | |
Detection_method | Swift-BAT Det | |
Circular_text | TITLE: GCN CIRCULAR NUMBER: 40305 SUBJECT: GRB 250430A: DDOTI Optical Observations DATE: 25/05/01 14:06:36 GMT FROM: sahil.atri@students.uniroma2.eu Sahil Atri (U Roma), Rosa L. Becerra (U Roma), Alan M. Watson (UNAM), Camila Angulo Valdez (UNAM), Sahil Atri (U Roma), Nat Butler (ASU), Simone Dichiara (Penn State University), Tsvetelina Dimitrova (ASU), Alexander Kutyrev (GSFC/UMD), William H. Lee (UNAM), and Océlotl López (UNAM), Margarita Pereyra (UNAM) and Eleonora Troja (U Roma) report: We observed the field of the Swift/BAT GRB 250430A (Parsotan et al., GCN Circ. 40292) with the DDOTI/OAN wide-field imager at the Observatorio Astronómico Nacional on the Sierra of San Pedro Martir (http://ddoti.astroscu.unam.mx) on the night of 2025-05-01 UTC. DDOTI observed the Swift/UVOT error region (Parsotan et al., GCN Circ. 40292) from 05:23 UTC to 10:43 UTC (from T+11.9 h to T+17.4 h after the trigger) with a total exposure of 2.3 hours, alternating with other scientific programs. Comparing our observations to the USNO-B1 and PanSTARRS PS1 DR2 catalogues, we detect no any uncatalogued source at the position reported by Parsotan et al., (GCN Circ. 40292); Odeh et al., (GCN Circ. 40295); Wang et al., (GCN Circ. 40299); Garnichey et al., (GCN Circ. 40301); Hagio et al., (GCN Circ. 40302); Quadri (GCN Circ. 40303) and Moretti (GCN Circ. 40304) down to a 3-sigma limiting AB magnitude of: w > 20.6 We thank the staff of the Observatorio Astronómico Nacional on the Sierra of San Pedro Mártir. |
GCN 40307 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40307 | |
Detection_method | correction | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40307
SUBJECT: GRB 250430A: NUTTelA-TAO Early Measurements
DATE: 25/05/01 17:08:43 GMT
FROM: Toktarkhan Komesh at Nazarbayev University |
GCN 40308 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40308 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40308
SUBJECT: GRB 250430A / EP250430a: J-band upper limits with WINTER
DATE: 25/05/01 17:50:27 GMT
FROM: Geoffrey Mo at MIT |
GCN 40310 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40310 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40310
SUBJECT: GRB 250430A: KAIT optical observations
DATE: 25/05/01 21:27:09 GMT
FROM: Weikang Zheng at UC Berkeley |
GCN 40311 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40311 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40311
SUBJECT: GRB 250430A: SVOM/VT optical observations
DATE: 25/05/02 03:29:23 GMT
FROM: SVOM_group |
GCN 40312 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40312 | |
Detection_method | Swift-BAT Det | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40312
SUBJECT: GRB 250430A: Calapai Observatory, Massa S. Giorgio (Messina), upper limit
DATE: 25/05/02 06:35:58 GMT
FROM: Giovanni Calapai at Calapai Astronomical Observatory, Massa S. Giorgio, Messina, Italy |
GCN 40316 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40316 | |
Detection_method | Optical | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40316
SUBJECT: GRB 250430A: Optical Observations via Virtual Telescope Project, Italy
DATE: 25/05/02 11:22:42 GMT
FROM: Gianluca Masi at Virtual Telescope Project |
GCN 40318 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40318 | |
Detection_method | Swift-XRT Det | |
ra | 233.3870° | |
decl | -18.1185° | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40318
SUBJECT: GRB 250430A: Enhanced Swift-XRT position
DATE: 25/05/02 11:57:52 GMT
FROM: Phil Evans at U of Leicester |
GCN 40321 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40321 | |
Detection_method | Swift-UVOT Det | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40321
SUBJECT: GRB 250430A: Swift/UVOT Detection
DATE: 25/05/02 12:22:02 GMT
FROM: Alice Breeveld at MSSL-UCL |
GCN 40323 table | ||
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GRB_name | GRB250430A | |
GCN_number | 40323 | |
Detection_method | Swift-XRT Other | |
Circular_text | TITLE: GCN CIRCULAR
NUMBER: 40323
SUBJECT: GRB 250430A: Swift-XRT refined Analysis
DATE: 25/05/02 13:27:07 GMT
FROM: Phil Evans at U of Leicester |