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"15722 results found.
- GRB 241127A: SVOM/GRM observation
- GRB 241127A: LCOGT (40-cm) optical counterpart detection
- Swift GRB241127.91: Global MASTER-Net OT detection
- EP241126a: WFST Observations
- GRB 241127A: Swift detection of a burst with an optical counterpart
- Swift GRB241127.91: Global MASTER-Net OT detection
- EP241126a: Optical Upper limits with Kinder observations
- EP trigger ID 01709122294: 1.6m Mephisto multi-band optical observations
- EP241126a: EP-FXT follow-up observation update
- EP241126a: GSP detects optical counterpart
- EP241126a: TRT optical counterpart detection
- LIGO/Virgo/KAGRA S241125n: COLIBRÍ Upper Limits on Optical Counterparts to Two of the Swift/XRT Sources
- GRB 241113B: EP-FXT afterglow detection
- LIGO/Virgo/KAGRA S241125n: DDOTI Optical Upper Limits
- LIGO/Virgo/KAGRA S241125n: Gaoyazi/GOT optical observations
- SVOM/GRM detection of a short burst from SGR 1830
- LIGO/VIRGO/KAGRA S241125n: GROWTH-India telescope optical observations
- GRB 241026A: radio detection with the VLA
- EP241125a: Optical upper limit with Kinder observations
- LIGO/Virgo/KAGRA S241125n: COLIBRÍ Upper Limits on a Optical Counterpart at the BAT Position
- LIGO/Virgo/KAGRA S241125n: Kinder optical upper limit in the BAT error region
- GRB 241113B: SVOM/VT optical afterglow observations
- GRB 241105A: ATCA radio detection
- GRB 241026A: VIRT Optical Upper Limit
- GRB 241025A: VIRT Optical Upper Limit
- GRB241120A: OHP/T193 optical observations
- EP241021a and EP241026b: Keck/LRIS spectroscopic observations
- EP trigger ID 01709065118: Keck/LRIS spectroscopic observations
- EP-WXT trigger 01709018832: Lick/Kast spectroscopy with the 3 m Shane telescope
- GRB 241120A: Mondy and AbAO optical observations
- EP241119a: Optical upper limits with Kinder observations
- EP241119a: GIT optical upper limits
- GRB 241113A: Possible ATCA Radio detection
- GRB 241112B: Mephisto further optical observations
- GRB 241117A: SVOM/GRM observation of a short burst with extended emission
- EP241115a/GRB 241115D: Optical upper limits with Kinder observations
- GRB 241115A: Mephisto upper limits
- GRB 241113B: Mephisto upper limits
- GRB 241115D / EP 241115a: SVOM/GRM observation
- GRB 241115A: LCOGT Optical Upper Limits
- EP 241113a: LBT possible optical counterpart
- GRB 241113B: KAIT Optical Afterglow Candidate
- GRB 241113A: J-band observations with WINTER
- GRB 241030A: LCO optical observation
- GRB 241113A: 1.6m Mephisto and 50cm array optical upper limits
- GRB 241113A: KAIT optical observations
- GRB 241113B: SVOM/GRM observation
- EP241107a: SOAR upper limits
- GRB 241113A: REM detection of the optical/NIR afterglow
- GRB 241113A: LCO optical observations
- GRB 241112B: GMG Optical Upper Limit
- GRB241113A: LCOGT (40-cm) optical counterpart detection
- GRB 241113A: MASTER010615.66-224018.2 optical counterpart detection
- GRB 241113A: Swift detection of a burst with an optical counterpart
- SVOM/GRM detection of a short burst from SGR 1E1841-045
- GRB 241105A: ATCA Radio Upper Limits
- GRB 241112B: AbAO optical upper limit
- GRB 241107A: GROWTH-India telescope optical upper limit
- GRB 241112B: Optical afterglow detection confirmation in revisiting the Mephisto data
- GRB 241112B: LCO optical detection of the SVOM/VT candidate
- GRB 241112B: SVOM/GRM observation
- GRB 241112B: SVOM/VT afterglow detection
- GRB 241112B: Mephisto optical upper limits
- GRB 241112B: GOTO optical upper limits
- GRB 241030B: TESS detection of optical counterpart
- EP241107a: AbAO optical upper limit
- GRB 241108A: Further COLIBRÍ Upper Limits on the Optical Counterpart
- EP241107A: MASTER optical observations of xray transient
- EP241107a: KAIT optical observations
- GRB 241030A: TESS observations
- GRB 241108A: COLIBRÍ Upper Limits on the Optical Counterpart
- EP241107a: Kinder optical follow-up observations
- GRB 241025A: radio detection with the VLA
- EP241107a: AKO Optical Afterglow Follow-Up Observations
- EP241107a: GSP detects optical counterpart
- EP241107a: Gemini-South spectroscopic confirmation (z = 0.456)
- GRB 241105A: EP-FXT follow-up observations
- EP241107a: FTW Optical and NIR observations of the optical counterpart
- GRB 241105A: ePESSTO+ NTT optical afterglow detection
- EP241107a: GIT optical observations
- EP241107a: SVOM/C-GFT optical observations
- EP241107a: AKO Optical Afterglow Detection
- GRB 241025A: LBT optical observations
- GRB241105A: Gemini-South Optical Afterglow Detection
- GRB 241105A: VLT/FORS2 optical afterglow rapid fading
- GRB 241105A: Swift/UVOT Detection
- EP241101a: CrAO ZTSH optical observations
- GRB 241030A: optical afterglow detection from the INAF Asiago Observatory
- GRB 241105A: BOOTES-7 optical detection
- GRB 241030A: Mondy optical observations
- GRB 241105A: Fermi GBM Observation of a Short Burst with Extended Emission
- GRB 241105A: SVOM/VT optical afterglow observations
- GRB 241105A: Swift-XRT afterglow detection
- GRB 241105A: VLT/FORS2 spectroscopic redshift z = 2.681
- GRB 240511A: LCO upper limits
- GRB 241105A: Swift/BAT-GUANO arcminute localization of a short burst
- GRB 241104A: NOT optical non-detection
- GRB 241105A: GOTO tentative optical counterpart candidate
- GRB 241104A: SVOM/VT optical candidate
- GRB 241104A/EP241104a: Optical upper limits with Kinder observations