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"
3041 results found.
- GRB 100414A: Swift-XRT detection of a possible X-ray afterglow
- GRB 100413A: Swift-XRT Refined Analysis
- Spin down rate and inferred dipole magnetic field of the new soft gamma-ray repeater SGR 1833-0832
- Swift/BAT trigger 417974 (GRB100401A): Swift/XRT observations
- GRB 100316A: R-band limit
- GRB 100331B: Swift/XRT possible afterglow candidate
- SGR 1833-0832: Archival Chandra Observations
- Possible pulsation period in SGR 1833-0832
- Discovery of the Spin Period of SGR 1833-0832
- Probable SGR 1833-0832: Swift-XRT refined analysis
- Swift-XRT refined position of the probable new SGR 1833-0832
- GRB 100316D: Swift XRT enhanced position and further refined analysis
- GRB 100316B: Swift-XRT refined analysis
- GRB 100316C: Swift-XRT team refined analysis
- GRB 100316A: Swift-XRT refined analysis
- GRB 100305A: Swift-XRT refined analysis
- GRB 100305A: PAIRITEL NIR Upper Limits
- GRB 100302A: Swift-XRT refined analysis
- GRB 100219A: XRT refined analysis
- GRB 100216A: Swift/UVOT Observations
- GRB 100216A: XRT Refined Analysis
- GRB 100213B: PAIRITEL NIR Upper Limits
- GRB 100213B: Swift XRT refined analysis
- GRB 100212A: Swift XRT refined analysis
- GRB 100206A: PAIRITEL Photometry of Host Candidate
- GRB 100206A: NOT NIR observations
- GRB 100206A: Swift-XRT refined analysis
- GRB 100205A: Swift XRT refined analysis
- GRB 100203A: Swift XRT and UVOT refined analyses
- GRB 100115A: Swift-XRT refined analysis
- GRB 100117A: Swift-XRT refined analysis
- GRB 100115A: Swift-XRT candidate afterglow
- GRB 100111A: PAIRITEL NIR Upper Limits
- GRB 100103A: Swift-XRT team refined analysis
- GRB 100103A: Swift/XRT position
- Swift Trigger 381591 is probably not a burst
- GRB 091230: Swift-XRT observation
- Swift Trigger 381434 is not a GRB
- GRB 091221 : IRSF NIR upper limit
- GRB 091117: Swift-XRT late time observations
- GRB 091221: Swift-XRT refined analysis
- GRB 091221: Enhanced Swift-XRT position
- Swift trigger 379449 (possible GRB) is not a burst
- GRB091208A: Swift/UVOT refined analysis
- GRB 091208A: Swift-XRT observations
- GRB 091208B: Swift-XRT refined analysis
- GRB091202: Swift-XRT refined analysis
- Konus-Wind observation of very long GRB 091123
- GRB 091130B: Swift-XRT team refined analysis
- Swift trigger 377436 (possible GRB 091130A) is not a burst
- GRB 091127: Swift-XRT afterglow detection and analysis
- GRB 091117: Swift-XRT observations
- GRB 091117: Evidence for Variability of XRT Source #1
- GRB 091117: Swift XRT refined analysis
- GRB091111: Swift XRT refined analysis
- GRB 091109B: Swift-XRT Team refined analysis
- GRB 091109: Swift-XRT refined analysis
- GRB 091104: Swift XRT Refined Analysis
- GRB091026 : IRSF NIR upper limit
- GRB 091102: Swift-XRT refined analysis
- GRB 091026: Swift-XRT refined analysis
- GRB 091024: Swift-XRT team refined analysis
- GRB 091020: Swift-XRT refined analysis
- GRB 091018: Swift XRT refined analysis
- GRB 091018: miniTAO/ANIR Observations
- GRB 091010: Swift-XRT refined analysis
- GRB 091010: Swift-XRT position
- GRB 091003: Swift-XRT confirmation of fading afterglow
- GRB 091003: Swift XRT analysis
- GRB 090929A: Swift-XRT non-detection
- GRB 090929B: Swift-XRT refined analysis
- GRB090926A: Swift-XRT refined analysis
- GRB090904B : IRSF NIR upper limit
- GRB 090916: Swift-XRT upper limit
- GRB 090915: Swift-XRT detection of a fading X-ray counterpart
- GRB 090827: Confirmation of the X-ray afterglow
- GRB 090912: Swift-XRT refined analysis
- GRB 090823: Swift XRT confirmation of the X-ray afterglow
- GRB 090904A: Swift-XRT refined analysis
- GRB 090904B: Swift XRT Refined Analysis
- GRB 090904A: Enhanced Swift XRT position
- GRB090902B: Swift XRT refined analysis
- GRB 090902B: Enhanced Swift-XRT position
- Swift Trigger 361477, called GRB090831B, is probably not real.
- GRB 090831C: Swift XRT Refined Analysis
- GRB 090827: Swift XRT and UVOT observations
- GRB 090823: Swift XRT possible detection of the X-ray afterglow
- GRB 090817: Swift/UVOT Observations of a Host Galaxy Candidate
- GRB 090817: Confirmation of the X-ray afterglow
- GRB 090815C: Swift refined analysis
- GRB 090817: Swift-XRT observations
- GRB 090814B: Confirmation of the X-ray afterglow
- GRB 090814B: Swift/UVOT Upper Limits
- GRB 090814B: Swift-XRT detection of a possible afterglow.
- GRB 090814A: Swift-XRT Team Refined Analysis
- GRB 090813: Swift-XRT refined analysis
- GRB 090812: Swift XRT refined analysis
- GRB 090809: Swift-XRT refined analysis
- GRB 090807: Swift-XRT refined analysis
- GRB 090728: Swift XRT refined analysis