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"11394 results found.
- Konus-Wind observation of GRB 100423A
- GRB 100418A: Terskol optical observations
- GRB 100425A: Swift XRT refined analysis
- GRB 100424A: Liverpool Telescope Upper Limits
- GRB 100425A: GROND afterglow observation
- GRB 100424A: D50 optical limits
- GRB 100424A: GROND Upper Limits
- GRB 100424A: Swift-XRT refined analysis
- GRB 100425A: Swift detection of a burst
- GRB 100424A, Swift-BAT refined analysis
- GRB 100420A: GRT Optical Observation
- GRB 100418A: ROVOR optical measurements at 35 hours
- Swift Trigger 420256: ROTSE-III Optical Limits
- Radio afterglow detection of GRB 100418A with the EVLA
- GRB 100418A: Continued PAIRITEL NIR Observations
- GRB 100418A: WSRT Radio Detection
- GRB 100418A: RTT150 optical observations
- GRB100420A: MITSuME optical upper limits
- GRB 100414A: CFHT optical observations
- GRB 100420A: SARA Upper Limits
- GRB 100418A: RTT150 observations during the optical afterglow maximum
- GRB 100418A: SMA submm detection
- GRB 100420A: ROTSE-III Optical Limits
- GRB 100418A: Swift-XRT Refined Analysis
- GRB100414A: SAO RAS optical observations
- GRB 100418A: ROTSE-III Optical Limits
- GRB 100418A: Swift detection of a burst with a possible optical afterglow
- GRB 100414A: Suzaku WAM observation of the prompt emission
- Konus-Wind observation of GRB 100414B
- GRB 100415A: MAXI/GSC detection of a probable GRB
- GRB 100414A: Fermi GBM detection
- GRB100414A: Fermi LAT detection
- Konus-Wind observation of GRB 100413A
- Tentative redshift of GRB100413A from X-ray data
- GRB 100413A: Swift-XRT Refined Analysis
- GRB 100413: xinglong TNT optical upper limit
- GRB 100413A: MASTER-Net optical observations
- GRB 100413A: Swift detection of a burst
- Spin down rate and inferred dipole magnetic field of the new soft gamma-ray repeater SGR 1833-0832
- GRB100401A: GROND Upper Limits
- MASTER observations on the Swift second trigger on LS V +44 17
- GRB 100331B: Swift/XRT possible afterglow candidate
- GRB 100331B: SuperAGILE Localization of a Long GRB
- INTEGRAL trigger 5994 / GRB 100331A: GROND detection of a variable source
- Konus-Wind observation of GRB 100324B
- GRB 100331A: A long GRB detected by INTEGRAL
- Konus-Wind observation of GRB 100322A
- Short X-ray Transient detected by MAXI/GSC
- Fermi/GBM and Swift/BAT detection of a burst from SGR 1806-20
- GRB 100325A: Fermi LAT detection
- GRB 100324A: GROND observations
- SGR 1833-0832: Swift/UVOT Upper Limits
- SGR 1833-0832: Archival Chandra Observations
- SGR 1833-0832 is pulsed at 7.56 seconds
- SGR 1833-0832 is pulsed at 7.56 seconds
- Possible pulsation period in SGR 1833-0832
- Discovery of the Spin Period of SGR 1833-0832
- GRB 100319A: correction to GCN 10527
- Probable SGR 1833-0832: Swift-XRT refined analysis
- Probable SGR 1833-0832: Enhanced Swift-XRT position
- Swift-XRT refined position of the probable new SGR 1833-0832
- Swift-BAT refined analysis of the probable new SGR 1833-0832
- GRB 100219A: MASTER-Net optical alert observations
- GRB 100319A: Swift detection of a burst; possible SGR
- GRB 100316D: Further Gemini observations
- GRB 100316B: Swift-XRT refined analysis
- Tentative redshift of GRB100316D from X-ray data
- GRB 100316C: Swift-XRT team refined analysis
- GRB 100316D: Swift XRT refined analysis
- GRB 100316A: Swift-XRT refined analysis
- GRB 100316A: Swift-BAT refined analysis
- GRB 100316B: Swift-BAT refined analysis
- GRB 100316C: BOOTES-3 observations
- XRF 100315A: MAXI/GSC detection of a short X-ray transient
- GRB 100316C: Swift detection of a burst
- GRB 100316B: Swift detection of a burst with optical counterpart
- GRB 100305A: Super-LOTIS early observations
- GRB 100305A: Swift-XRT refined analysis
- GRB 100305A Optical Observations
- GRB 100305A: Swift detection of a burst
- GRB 100302A: Swift-XRT refined analysis
- GRB 100302A: Optical observations at Crni Vrh
- GRB 100302A: Swift detection of a burst
- GRB 100224A SHB found in ground analysis of BAT data
- GRB 100225A: Fermi LAT detection
- GRB 100225A: Fermi GBM detection
- GRB
- GRB 100219A: XRT refined analysis
- GRB 100219A - Gemini South Spectroscopy
- GRB100219A Akeno and Okayama MITSuME Optical Observation
- GRB 100219A: GROND observations
- GRB 100219A: Swift detection of a burst
- GRB 100213B: Swift XRT refined analysis
- GRB 100213A: SARA observations
- GRB 100205A: Keck limits on an underlying host galaxy
- GRB 100206A: YNAO-GMG observations
- GRB 100206A: WHT candidate afterglow
- GRB 100205A: Swift XRT refined analysis
- GRB 100205A: Swift detection of a burst
- Short X-ray Transient detected by MAXI/GSC