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"26362 results found.
- GRB 210424.694: DDOTI Upper Limits on the Afterglow
- GRB 210422A: Swift-BAT refined analysis
- GRB 210420B: follow-up photometry of optical afterglow at INASAN/Simeiz
- GRB 210420B: Zeiss-1000 of Koshka optical observations
- GRB 210421A: Swift-BAT refined analysis
- GRB 210421B: Swift-XRT observations
- GRB 210420B: continued Tautenburg observations
- GRB 210421A: GECAM detection
- GRB 210421A: Swift/UVOT Upper Limits
- GRB 210420B: follow-up photometry of the optical afterglow at Konkoly
- GRB 210421A: MITSuME Akeno optical upper limits
- GRB 210420B: Swift-BAT refined analysis
- GRB 210421B: Swift/BAT-GUANO detection and arcminute localization
- GRB 210420B: Swift-XRT refined Analysis
- GRB 210421A: Swift-XRT refined Analysis
- Fermi GRB 210421C: Global MASTER-Net observations report
- GRB 210419C: Swift/UVOT Upper Limits
- GRB 210421A: Enhanced Swift-XRT position
- GRB 210420B: RATIR Optical and NIR Observations
- GRB 210420B: Tautenburg observations
- GRB 210420B: Swift/UVOT Detection
- GRB 210413B: MITSuME Okayama optical upper limits
- GRB 210419C: MITSuME Akeno optical upper limits
- GRB 210420B: DDOTI Detection of the Afterglow
- GRB 210421A: DDOTI Upper Limit
- GRB 210419C: Swift-BAT refined analysis
- GRB 210420B: Multiband photometry from NOT
- GRB 210420B: Montarrenti Observatory optical afterglow detection
- GRB 210421A: Swift detection of a burst
- GRB 210420B: Optical observations
- GRB 210420B: MASTER optical counterpart detection
- GRB 210419C: RATIR Optical and NIR Upper Limits
- GRB 210419C: Montarrenti Observatory Upper Limit
- GRB 210419A: Swift/UVOT Upper Limits
- GRB 210419C: Enhanced Swift-XRT position
- GRB 210419A: Swift-BAT refined analysis
- GRB 210419A: Swift-XRT refined Analysis
- GRB 210419C: Swift detection of a burst
- GRB 210419A: Enhanced Swift-XRT position
- GRB 210419A: LCO Optical Upper Limit
- GRB 210419A: Swift detection of a burst
- GRB 210413B: Swift-XRT observations
- GRB 210413B: LOAO optical upper limit
- GRB 210411C: A very significant early X-ray afterglow
- GRB 210413A: GECAM detection
- GRB 210411C: Swift/UVOT Detection
- GRB 210411C: Swift-BAT refined analysis
- GRB 210411C: Swift-XRT refined Analysis
- GRB 210410A: MITSuME Akeno optical upper limits
- Swift GRB 210411C: Global MASTER-Net observations report
- GRB 210411C: LCO Optical Afterglow Candidate
- GRB 210411C: Enhanced Swift-XRT position
- GRB 210411D: BALROG localization (Fermi Trigger 639851475 / GRB 210411688)
- GRB 210411C: Swift detection of a burst with an optical counterpart
- GRB 210410A: Swift-BAT refined analysis
- GRB 210410A: Swift-XRT refined Analysis
- GRB 210410A: Fermi GBM detection
- GRB 210410A: Swift/UVOT Upper Limits
- GRB 210406A: Swift-XRT observations
- GRB 210410A: RATIR Optical and NIR Observations
- GRB 210409A: GECAM detection
- GRB 210410A: Fermi-LAT detection
- Swift Triggers 1042031 and 1042032 are not astrophysical events
- GRB 210406A: Mondy optical afterglow candidate
- GRB 210406B: Fermi GBM detection
- Konus-Wind detection of GRB 210406A
- GRB 210406A: Fermi GBM detection
- GRB 210406A: Mondy optical upper limit
- GRB 210406A: Konkoly Obs. optical upper limit
- GRB 210406A: A long GRB detected by INTEGRAL
- GRB 210402A: MASTER prompt and follow up optical observation
- GRB 210402A: Swift/UVOT Upper Limits
- GRB 210402A: Fermi GBM detection
- GRB 210402A: Further NOT optical observations
- GRB 210402A: Swift-BAT refined analysis
- GRB 210404.141: DDOTI Upper Limits
- GRB 210207B: Prompt and very late time observations with HCT.
- GRB 210401A: GECAM detection
- GRB 210402A: NOT optical afterglow candidate
- GRB 210403A: Swift-BAT refined analysis
- GRB 210402A: LBT observations
- GRB 210402A: DDOTI Upper Limits
- GRB 210402A: Swift-XRT refined Analysis
- GRB 210402A: Montarrenti Observatory upper limit
- GRB 210402A: NOT optical upper limits
- GRB 210402A: Swift detection of a burst
- GRB 210401A: Fermi GBM Final Real-time Localization
- GRB 210328A: GECAM detection
- GRB 210330A: GECAM detection
- GRB 210328A: BALROG localization (Fermi Trigger / GRB 210328865)
- GRB 210326A: Insight-HXMT/HE detection
- GRB 210323A: Insight-HXMT/HE detection
- GRB 210323A: MASTER optical observation
- GRB 210323A: Swift-BAT refined analysis
- GRB 210324C: BALROG localization (Fermi Trigger 638308803 / GRB 210324833)
- Short GRB 210323A: GTC Observations
- GRB 210323A: Swift/UVOT Upper Limits
- GRB 210323A: Classification and redshift estimation
- GRB 210323A: Kitab optical upper limit
- GRB 210323A: Fermi GBM detection