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"
3078 results found.
- GRB 240225B: Swift-XRT observations
- Transient EPW20240219aa: Kp-band imaging observations with NIRES
- GRB 240222A: Swift-XRT refined Analysis
- GRB 240218A: LBT H-band detection
- Konus-Wind detection of GRB 240218A
- GRB 240218A: Swift-XRT refined Analysis
- Fermi GRB 240216A: Global MASTER-Net observations report
- GRB 240128A: Further Swift-XRT observations
- GRB240204A: Swift/UVOT Upper Limits
- GRB 240128A: Swift-XRT observations
- GRB 240122A: Swift/UVOT Upper Limits
- GRB 240123A: Swift-XRT refined Analysis
- GRB 240122A: Swift-XRT afterglow detection
- GRB 240118A: Swift-XRT afterglow detection
- GRB 240112C: Swift-XRT refined Analysis
- GRB 231220A: Swift-UVOT upper limit
- GRB 240101B: Swift-XRT refined Analysis
- GRB 240102A: Swift-XRT refined Analysis
- GRB 240101B: Swift/UVOT Upper Limits
- GRB 240101A: Swift-XRT refined Analysis
- GRB 231230A: Swift-XRT refined Analysis
- Fermi trigger No 725592555: Global MASTER-Net observations report
- GRB 231222B: Swift-XRT afterglow detection
- GRB 231220A: Swift-XRT follow-up observations
- GRB 231216A: Swift-XRT refined Analysis
- GRB 231215A: Swift-XRT refined Analysis
- GRB 231214A: Swift-XRT refined Analysis
- GRB 231210B: Swift-XRT refined Analysis
- GRB 231205B: Swift-XRT refined Analysis
- GRB 231129C: Swift-XRT afterglow detection
- GRB 231129B: Swift-XRT observations
- GRB 231129C: Swift-XRT observations
- GRB 231129A: Swift-XRT refined Analysis
- GRB 231123C: Insight-HXMT/HE detection
- GRB 231115A: XMM-Newton observation
- GRB 231117A: GTC Near-Infrared Observations
- GRB 231117A: Swift-XRT refined Analysis
- GRB 231118A: Swift-XRT refined Analysis
- GRB 231115A: NuSTAR Follow-Up Observations
- GRB 231115A: Swift-XRT and Swift-UVOT observations
- GRB 231115A: archival Chandra X-ray observations
- GRB 231110A: Swift-UVOT Upper Limits
- GRB 231111A: Swift-XRT refined Analysis
- GRB 231110A: Swift-XRT afterglow detection
- GRB 231104A: Swift-XRT refined Analysis
- GRB 231017A: Swift-XRT observations
- GRB 230906A: optical counterpart
- GRB 230911A: Swift-XRT afterglow detection
- GRB 230911C: Swift-XRT refined Analysis
- GRB 230906A: Chandra detection of the X-ray afterglow
- GRB 230906A: Swift/UVOT Upper Limits
- GRB 230906A: Swift-XRT observations
- GRB 230812B: Chandra late-time detection of the X-ray afterglow
- GRB 230903A: Swift-XRT refined Analysis
- GRB 230827B: Swift-XRT afterglow detection
- GRB 230826A: Swift-XRT refined Analysis
- GRB 230824B: AstroSat CZTI detection
- GRB 230818A: Swift-XRT refined Analysis
- GRB 230816A: Swift-XRT refined Analysis
- GRB230815A: Swift/UVOT upper limits
- GRB 230815A: Swift-XRT refined Analysis
- GRB 230812B: Swift-XRT afterglow detection
- GRB 230812B: Improved Swift/XRT localization
- GRB 230805B: Swift-XRT refined Analysis
- GRB 230802A: Swift-XRT refined Analysis
- GRB 230728A: Swift-XRT refined Analysis
- GRB 230723B: Swift-XRT refined Analysis
- Swift-XRT position for GRB 230723B
- IceCube-230707A: No candidates detected by Swift-XRT
- GRB 230707A: Swift-XRT observations
- GRB 230628E: Swift-XRT refined Analysis
- GRB 230623A: Swift-XRT observations
- GRB 230622A: Swift-XRT refined Analysis
- GRB 230618A: Swift-XRT refined Analysis
- GRB 230616A: Swift-XRT observations
- GRB 230506B: Chandra localization of the X-ray afterglow
- GRB 230606A: Swift-XRT refined Analysis
- LIGO/Virgo S230518h: Swift XRT observations, 8 X-ray sources
- GRB 230512A: Swift-XRT observations
- GRB 230510A: Swift-XRT refined Analysis
- GRB 230506C: Swift-XRT refined Analysis
- GRB 230506C: Swift/UVOT Upper Limits
- GRB 230506B: Swift-XRT refined Analysis
- GRB 230506C: Swift-XRT analysis
- GRB 230427A: Swift-XRT refined Analysis
- GRB 230423A: Swift-XRT refined Analysis
- GRB 230420A: Swift-XRT refined Analysis
- GRB 230414B: Swift-XRT refined Analysis
- GRB 230409B: Swift-XRT refined Analysis
- GRB 230405B: Swift-XRT refined Analysis
- GRB 230307A: Chandra late-time detection of the X-ray afterglow
- GRB 230328B: 3.6m DOT multiband optical observation
- GRB 230328B: Swift-XRT refined Analysis
- GRB 230325A: Swift-XRT refined Analysis
- GRB 230322B: Swift-XRT refined Analysis
- GRB 230307A: INTEGRAL upper limit on Hard X-ray afterglow
- GRB 230307A: Swift/UVOT detection
- GRB 230307A: Swift-XRT afterglow detection
- GRB 230307A: Swift/BAT upper limits on the early afterglow
- GRB 230307A: Swift-XRT observations