GCN Circulars
GCN Circulars are rapid astronomical bulletins submitted by and distributed to community members worldwide. They are used to share discoveries, observations, quantitative near-term predictions, requests for follow-up observations, or future observing plans related to high-energy, multi-messenger, and variable or transient astrophysical events. See the documentation for help with subscribing to or submitting Circulars.
To navigate to a specific circular, enter the associated Circular ID (e.g. 'gcn123', 'Circular 123', or '123').
Advanced Search
To narrow the search results, use advanced search syntax. This allows for specifying which circular field to search (submitter, subject, and/or body). For additional information, refer to the advanced search documentation.
Advanced Search Examples (click to copy):
subject:"Swift"body:"GRB"submitter:"Judith Racusin"15717 results found.
- EP250321a: SVOM/VT optical observation
- EP 250321A: Optical counterpart detection by LCO.
- EP250321a: Kinder optical follow-up observations
- GRB 250321A: Swift/UVOT Upper Limits
- GRB 250320B: SVOM/GRM observation of a long burst
- EP250321a: LCO optical counterpart detection
- EP250321a: Swift-XRT detection of an X-ray source
- EP250321A: COLIBRÍ Optical Observations
- EP250321a: VLT/X-shooter redshift z = 4.368
- EP250321a: REM optical/NIR afterglow detection
- EP250321a: BOOTES-5/JGT optical afterglow detection
- EP250321a: TRT optical counterpart detection
- GRB 250321A: GOTO optical upper limits
- EP250226a/GRB 250226A: KAIT optical observations
- GRB 250309B: Proof-of-concept for Joint ZTF+EP Experiment
- GRB 250317B: Mondy AZT-33IK Continued Optical Observations
- GRB 250317B: SVOM/COLIBRI (F-GFT) follow-up observations
- GRB 250314A: ATCA radio upper limits
- EP250302a: VLA observations
- GRB 250317B: OHP/T193 continued follow-up
- GRB 250317C: SVOM/GRM observation of a long burst
- GRB 250317B: Leavitt Observatory optical upper limit
- GRB 250309B/AT2025dws: further ATCA observations
- GRB 250317B: Mondy AZT-33IK Optical Observations
- GRB 250317B: NOT optical observations suggest an optical plateau phase
- GRB 250317B: OHP/T193 optical observations
- GRB250312A: Swift/UVOT Upper Limits
- GRB 250317B: REM optical/NIR observations
- GRB 250317B: Swift-XRT observations
- GRB 250316A: Swift/UVOT Upper Limits
- GRB 250314A: REM optical/NIR upper limits
- GRB 250316A: AbAO AS-32 Optical Upper Limit
- EP 250317B: Fading optical counterpart detection by LCO
- GRB 250317B: LCO detection of the fading optical afterglow
- GRB 250317B: SVOM/VT detection of an optical candidate from VHF data
- GRB 250317B: SVOM/F-GFT (COLIBRÍ) Detection of a Fading Optical Counterpart
- GRB 250314A: GTC z-band upper limit and updated photo-z ~ 7.27
- GRB 250315A/EP250315A: Fermi-GBM Sub-Threshold Detection
- EP250315a: refined analysis of the EP-WXT and EP-FXT observations
- GRB 250314A: Swift/UVOT Upper Limits
- GRB 250314A: Swift XRT Detection
- EP250315a: optical counterpart candidate detected by Gemini North
- GRB 250226A: Mondy AZT-33IK and Koshka Zeiss-1000 Optical Upper Limits
- GRB 250314A: NOT near-infrared candidate counterpart
- GRB250314A: SVOM/VT lack of bright optical candidate from VHF data
- EP250304a: Pan-STARRS r and i-band imaging and photometry
- EP trigger ID 01709061302: Lick/Kast spectroscopy with the 3 m Shane telescope
- GRB 250309B: PRIME near-infrared upper limits in 2nd epoch
- EP250304a: SVOM/VT optical observation
- ATCA detection of the radio counterpart of GRB 250309B-AT2025dws
- EP250302a: Chandra X-ray Detection
- GRB 250309B/AT2025dws: Daochen/RC-10 optical counterpart observation
- GRB 241213A: VIRT Optical Upper Limit
- GRB 241228A: VIRT Optical Upper Limit
- GRB 250311A/EP250311a: Optical upper limits with Kinder observations
- GRB 250309B: 1.3m DFOT Optical observations
- GRB 250309B: PRIME near-infrared detection
- GRB 250311A/EP250311a: TRT optical upper limit
- IceCube-250309A: MITSuME Akeno and Seimei/TriCCS optical observations
- GRB 250309B: SVOM/VT optical observation
- GRB 250309B / AT2025dws: further SAO RAS optical observations
- IceCube-250309A: Upper limits from Fermi-GBM Observations
- EP250308a: 1.6m Mephisto optical upper limits
- GRB 250309B / AT2025dws: KMTNet-CTIO optical observations
- IPN triangulation of GRB 250309B
- GRB 250309B/AT2025dws : COLIBRÍ Detection of the Optical Counterpart
- GRB 250309B: Swift-XRT refined Analysis
- GRB 250309B / IceCube-250309A: GECAM-B observations
- Liverpool Telecope observations of AT 2025dws / GRB 250309B
- GRB 250309B / AT2025dws: SAO RAS optical observations
- GRB 250309B / AT2025dws: Swift-UVOT detection
- AT 2025dws, likely optical counterpart of GRB 250309B: LCO confirmation of fast fading
- GRB250309B: One candidate counterpart from the Zwicky Transient Facility
- IceCube-250309A: No candidates from the Zwicky Transient Facility
- EP250308a: GSP optical upper limit
- EP250308a: FTW optical and NIR upper limits
- EP250308a: NOT optical upper limit
- EP250304a: MeerKAT detection of a possible radio counterpart
- EP250302a:Xinglong optical observations
- GRB250101A: Radio upper limits from VLA observations
- GRB 250305A: SVOM/GRM observation of a burst
- EP250302a: Optical Observations at CrAO and SAO RAS
- GRB 250219A: SVOM/C-GFT optical upper limit at early phase
- EP 250304A: Optical counterpart detection by LCO
- EP250302A: 1.3m DFOT optical afterglow detection
- EP250304a: refined analysis of the EP-WXT and EP-FXT observations
- EP250304a: REM NIR upper limits
- EP250304a: Swift/UVOT detection of an optical counterpart with a rising light curve
- EP250302a: Mondy Continued Optical Observations
- EP250304a: VLT/X-shooter redshift z = 0.200
- EP250304a: Swift-XRT detection of a fading X-ray source
- EP250304a: TRT optical counterpart detection
- EP250302a: SVOM/VT optical observation
- EP250302a: SAO RAS optical observations
- EP250302a : GIT optical follow-up
- EP250225a: the candidate optical counterpart is an AGN
- EP250302a: Kinder optical follow-up observations
- EP250302a: Swift/UVOT detection
- EP250302a: NUTTelA-TAO Early Measurments
- EP250302a: optical observation from the INAF Asiago Observatory