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"15741 results found.
- GRB 241029A: Xinglong-2.16m optical afterglow confirmation
- GRB 241029A: Mephisto observations
- EP 241026b: LBT possible optical counterpart (brightening source)
- GRB 241029A: TRT optical afterglow candidate detection
- GRB 241029A: SVOM/GRM observation
- GRB 240821A: Keck/LRIS spectroscopic observations
- EP241021a: Gemini-South detection of optical rebrightening
- GRB 241026A: TNOT optical counterpart detection
- GRB 241025A (EP241025a): Optical afterglow observations with the Tsinghua-Nanshan Optical Telescope
- GRB 241026A: LBT redshift confirmation
- GRB 241025A: further SAO RAS optical observations
- GRB 241026A: BTA and Zeiss-1000 optical observations
- GRB 241026A: SVOM/GRM observation
- EP241026B: GROWTH-India Telescope optical upper limit
- GRB 241026A: GROWTH-India Telescope optical observations
- GRB 241026A: J-band observations with WINTER
- GRB 241025A: SAO RAS optical observations
- GRB 241026A: Las Cumbres optical detection
- GRB 241025A: Mondy optical observations
- EP241021a: SOAR observations of the optical counterpart
- EP241021a: further SAO RAS optical observations
- EP 241026b: LBT optical observations
- EP241021a: e-MERLIN radio observation
- GRB 241026A: KAIT optical observations
- GRB 241026A: COLIBRÍ Detection of the Optical Counterpart
- GRB 241026A: SAO RAS observations of possible optical afterglow
- GRB241025A: 1.3m DFOT optical afterglow detection
- EP241021a: optical follow-up observations with Xinglong Observatory
- GRB 241025A: optical photometry from Konkoly
- GRB 241025A: GROWTH-India Telescope optical observations
- GRB 241025A: COLIBRÍ Detection of the Afterglow
- GRB 241025A: GRANDMA and Kilonova-Catcher optical afterglow detections and upperlimits
- EP241021a: Optical and NIR observations of counterpart with the Fraunhofer Telescope at Wendelstein Observatory
- EP241021a: Optical and NIR observations of counterpart with the Fraunhofer Telescope at Wendelstein Observatory
- EP241021a: optical follow-up observations with the Liverpool Telescope
- GRB 241025A : SVOM/VT optical afterglow observations
- EP241021a: Liverpool Telescope optical follow-up observations
- GRB 241001A: JWST spectroscopic identification of a supernova counterpart
- GRB 241025A: NOT spectroscopic redshift of z = 4.20
- GRB 241025A: TRT optical afterglow observation
- GRB 241025A: Swift detection of a burst with an optical counterpart
- EP241021a: GTC OSIRIS+ spectroscopy of the optical counterpart
- GRB 241001A: ATCA radio observations
- GRB 241010A: VIRT Optical Upper Limit
- EP241021a: VLT/FORS2 redshift z = 0.75
- EP241021a: SAO RAS optical observations
- EP241021a: KAIT optical observations
- EP241021a: EP-FXT follow-up observation update
- EP241021a: Optical counterpart observations with the Liverpool Telescope
- EP241021a: 1.3m DFOT Optical observations
- EP241021a: GSP detects optical candidate counterpart
- EP241021a: Optical upper limits with Kinder observations
- EP241021a: TRT optical observations
- GRB 241018A: SVOM/C-GFT optical observations
- EP241021a: NOT likely optical counterpart
- GRB241017A: 1.3m DFOT optical upper limit
- GRB 241018A: 1.3m DFOT Optical upper limit
- GRB 241018A: EP-FXT afterglow detection
- EP241021a: GOTO optical upper limits
- GRB 241018A/sb24101802: Mephisto optical upper limit
- GRB 241017A/sb24101702: Mephisto optical upper limit
- GRB 241018A: BOOTES-4/MET optical upper limit
- GRB 241018A: Mondy optical upper limit
- GRB 241018A: GROWTH-India telescope optical upper limit
- GRB241018A: XingLong Optical Upper Limit
- GRB 241018A: Swift-XRT observations
- GRB 241018A: REM optical/NIR upper limits
- GRB 241018A: NOT optical observations
- GRB 241017A: SVOM/VT follow-up and optical upper limit
- GRB 241018A: SVOM/VT follow-up and optical candidate
- GRB 241018A: LCO/0.4m optical upper limits
- GRB 241006A: VIRT Optical Upper Limit
- GRB 240727A: VIRT Optical Upper Limit
- GRB241017a: Liverpool Telescope observations of XRT uncatalogued sources
- GRB 241017A: GROWTH-India Telescope optical upper limit
- GRB 240916A: radio detection with the VLA
- GRB 241009A: LCO optical upper limits
- GRB 241009A: GRANDMA optical upper limits
- GRB 241010A: JinShan optical observations and potential host galaxy
- GRB 241010A: J-band observations with WINTER
- GRB 241010A: LCO optical observations
- GRB 241010A: Swift detection of a burst with an optical counterpart
- GRB 241002B: Swift-XRT afterglow detection
- GRB 241002A: NOT optical upper limits
- IceCube-241006A: No candidates from the Zwicky Transient Facility
- GRB 241006A: GRANDMA optical upper limits
- EP240930a / GRB 240930B: CrAO ZTSH optical upper limit
- GRB 241002B: PRIME near-infrared detection in 3rd epoch
- GRB 240910A: LBT optical observations
- GRB 241006A: Swift/UVOT Upper Limits
- GRB 241006A: SVOM/VT follow-up and optical upper limit
- GRB 241001A: Swift-XRT afterglow detection
- GRB 240930B: SVOM/C-GFT optical upper limit
- GRB 241002B: PRIME near-infrared detection in 2nd epoch
- GRB 241002B: Swift-XRT observations
- GRB 241002C: SVOM/C-GFT optical upper limit
- GRB 241002B: PRIME near-infrared detection
- GRB 241001A : SVOM/VT optical detection
- GRB 241002B: GOTO24gpc/AT 2024xbg follow-up observations update
- GRB 241002B: ULL-ASTRO-MASTER LCOGT 0.4m + QHY600 detection of the GOTO optical counterpart candidate AT 2024xbg / GOTO24gpc