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"3283 results found.
- GRB 190202A: Swift-XRT refined Analysis
- GRB 190129B: Swift-XRT candidate afterglow detection
- GRB 190123A: Swift-XRT refined Analysis
- GRB 190114B: Swift-XRT refined Analysis
- GRB 190114C: Swift-XRT refined Analysis
- GRB 190114A: Swift-XRT refined Analysis
- GRB 190109B: Swift-XRT refined Analysis
- GRB 190109A: Swift-XRT refined Analysis
- GRB 190106A: Swift-XRT refined Analysis
- GRB 190103B: Swift-XRT refined Analysis
- GRB 181225A: further Swift-XRT observations
- GRB 181228A: Swift-XRT refined Analysis
- GRB 181222B: Swift follow-up observations of MASTER optical transient J204928.79+245744.0
- GRB 181225A: Swift observations and X-ray candidate afterglow
- GRB 181213A: Swift-XRT refined Analysis
- GRB 181203A: Swift/UVOT Upper Limits
- GRB 181203A: Swift-XRT refined Analysis
- GRB 181201A: Swift/UVOT Detection
- GRB 181202A: Swift-XRT refined Analysis
- GRB 181201A: Swift-XRT afterglow detection
- GRB 181126A: No Ks-band afterglow detection with Keck I
- GRB 181126A: Swift-XRT refined Analysis
- GRB 181123B: Swift-XRT refined Analysis
- Swift Trigger 872470: further Swift analysis
- GRB 181110A: Swift-XRT refined Analysis
- GRB 181103A: Swift-XRT refined Analysis
- GRB 181030A: Swift-XRT refined Analysis
- GRB 181022A: Swift-XRT refined Analysis
- GRB 181023A: Swift-XRT refined Analysis
- GRB 181020A: Swift-XRT refined Analysis
- GRB 181013A: Swift detection of a probable burst
- GRB 181010A: Swift-XRT refined Analysis
- GRB 181003A: Swift-XRT afterglow detection
- GRB 181002A: Swift-XRT refined Analysis
- GRB 180930A: Swift-XRT refined Analysis
- GRB 180925A: Swift-XRT refined Analysis
- GRB 180924A: Swift-XRT refined Analysis
- GRB 180914B: Swift-XRT afterglow detection
- GRB 180914A: Swift-XRT observations
- GRB 180905A: Swift-XRT refined Analysis
- GRB 180904A: Swift-XRT refined Analysis
- GRB 180829A: Swift-XRT observations
- GRB 180828A: Swift-XRT refined Analysis
- GRB 180823A: Swift-XRT refined Analysis
- GRB 180821A: Swift-XRT refined Analysis
- GRB180806A: confirmation of the X-ray afterglow
- GRB 180818B: Swift-XRT refined Analysis
- GRB 180818A: Swift-XRT refined Analysis
- Chandra X-ray observations of GW170817 at 1 year post-merger: increasingly rapid fading
- GRB 180812A: Swift-XRT refined Analysis
- GRB 180809B: Swift-XRT refined Analysis
- Swift Trigger 852625: Swift/BAT/XRT/UVOT observations
- GRB 180809B: Swift/UVOT Detection
- GRB 180809A: Swift-XRT afterglow detection
- GRB 180806A: Swift-XRT afterglow detection
- GRB 180805A: Swift-XRT refined Analysis
- GRB 180805B: Swift-XRT refined Analysis
- GRB 180728A: Swift-XRT refined Analysis
- GRB 180727A: Swift-XRT refined Analysis
- GRB 180722A: Swift-XRT observations
- GRB 180718B: Swift-XRT observations
- GRB 180718A: Swift-XRT observations
- GRB 180720C: Swift-XRT refined Analysis
- GRB 180721A: Swift-XRT refined Analysis
- GRB 180720B: Swift-XRT refined Analysis
- GRB 180715A: Swift-XRT observations
- GRB 180715A: Swift-XRT observations
- GRB 180709A: Swift-XRT refined Analysis
- GRB 180703A: Swift-XRT afterglow detection
- GRB 180705A: Swift-XRT refined Analysis
- GRB 180706A: Swift-XRT refined Analysis
- GRB 180704A: Swift-XRT refined Analysis
- GRB 180703A: Swift-XRT observations
- GRB 180630A: Swift-XRT refined Analysis
- GRB 180626A: Swift-XRT refined Analysis
- GRB 180624A: Swift-XRT refined Analysis
- GRB 180623A: Swift-XRT refined Analysis
- GRB 180613A: Afterglow confirmation and added photometry
- GRB 180620B: Swift-XRT refined Analysis
- GRB 180620A: Swift-XRT refined Analysis
- GRB 180618A: Swift-XRT refined Analysis
- GRB 180614A: Swift-XRT refined Analysis
- GRB 180613A: Possible IR afterglow
- GRB 180613A: Swift-XRT refined Analysis
- GRB 180602A: Swift-XRT refined Analysis
- GRB 180514A: Swift-XRT refined Analysis
- GRB 180512A: Swift-XRT refined Analysis
- GRB 180510B: Swift-XRT refined Analysis
- GRB 180510A: Swift-XRT refined Analysis
- Chandra observations of GW170817 reveal a fading afterglow
- Chandra observations of GW170817 260 days since merger: first statistically significant evidence for an X-ray decay
- GRB 180504A: Swift-XRT refined Analysis
- GRB 180425A: Swift-XRT refined Analysis
- GRB 180418A: Swift-XRT refined Analysis
- GRB 180409A: Swift-XRT afterglow detection
- GRB 180411A: Swift-XRT refined Analysis
- GRB 180410A: Swift-XRT refined Analysis
- GRB 180409A: Swift-XRT observations
- Chandra observations of GRB161219B 400 days after the explosion
- GRB 180404A: Swift-XRT refined Analysis