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"
2623 results found.
- GRB 140311C: MASTER optical observations
- GRB 140311C: Swift-XRT and UVOT observations
- Fermi416242156: possible iPTF counterpart
- GRB 140226A/iPTF14yb: Mondy optical observations
- GRB 140219A: Mondy optical observations of XRT source #5
- Konus-Wind observation of GRB 140226A
- IPN triangulation of GRB 140226A, a possible GRB counterpart to iPTF14yb
- iPTF14yb: Swift-XRT detection
- GRB 140219A: Xuyi and Nanshan upper limits
- GRB 140209A, Swift-BAT refined analysis
- GRB 140209A: optical observations
- GRB 140206A: theoretical prediction of redshift and of supernova occurrence
- GRB 140110A: Second Follow-up Swift-XRT Observation
- GRB 140104B: Further Swift XRT observations
- GRB 140108A: theoretical prediction of redshift and of supernova occurrence
- GRB 140105A/Fermi410578384: MASTER-Net early optical observations
- Fermi410578384: iPTF optical afterglow candidates for a possible short GRB
- GRB 131202A: theoretical estimation of the redshift
- GRB 060614: theoretical derivation of the redshift and need for deeper search of the host galaxy
- GRB 131128A: Swift detection of a burst
- GRB 131122A: i-band observations from NOT
- IPN Triangulation of GRB 131118A
- GRB 130925A: HST imaging
- GRB 131108A: 1.23m CAHA optical candidate
- GRB 131108A: Swift detection of a possible X-ray afterglow
- GRB 131103A: Swift detection of a burst
- GRB 131024C: ICSP discovery of a burst in X-rays by balloon borne study
- IPN Triangulation of GRB 131028A (long/bright)
- Swift Trigger 575905/possible GRB 131026A: Swift-XRT observations
- Swift Trigger 575905: a possible GRB
- IPN triangulation of GRB 131011B (Swift Trigger 574266)
- IPN Triangulation of GRB 131014A
- GRB 131014A: RATIR Optical and NIR Observations
- GRB 131014A: NOT afterglow candidate
- GRB 131014A: Nanshan optical observations
- GRB 131014A: Swift detection of a possible X-ray afterglow
- Fermi403206457: continued P60 observations and fading behavior
- Fermi403206457: iPTF detection of a possible optical afterglow
- GRB 130925A: Possible signatures of binary nature in the afterglow - Request for observations
- GRB131004A: TNG Redshift confirmation
- GRB131004A: Magellan Redshift
- GRB 131004A: TNG optical afterglow confirmation
- GRB 130925A: continuing Swift/XRT monitoring
- Konus-Wind observation of GRB 130925A
- Observation of possible GRB/TDE 130925A by INTEGRAL/SPI-ACS: three activity episodes
- Fermi GBM detection of GRB 130925A and a possible precursor
- GRB 130925A: Swift-XRT refined Analysis
- GRB 130831A: Maidanak optical observations, possible emerging Supernova
- GRB 130913A detected in ground analysis of Swift-BAT data
- GRB 130912A: REM optical/NIR upper limits
- GRB 130907A: Early Tautenburg detections, red afterglow
- GRB 130907A: Skynet DSO-14/Yerkes-41 detections of a possible afterglow
- Swift follow-up results of the possible weak INTEGRAL GRB
- Swift follow-up of an INTEGRAL possible weak GRB
- Swift Trigger 569022: a possible GRB
- IPN triangulation of GRB 130828A
- IPN triangulation of GRB130821A
- GRB 130821A: Swift-XRT observation
- Refined IPN Triangulation of GRB 130812B
- GRB 130806A: Swift detection of a burst
- GRB130803A: GROND detection of possible host
- GRB 130722A: Swift/UVOT Detection
- GRB 130626A: Retraction of possible X-ray afterglow
- GMRT radio detection of GRB 130702A
- GRB 130702A: Maidanak optical observations
- GRB 130702A (= Fermi 394416326): correction of the GCN #14988 title
- GRB 130702A: NOT spectroscopy and redshift of the nearby bright galaxy
- Fermi GRB 130702A: Swift XRT and UVOT observations
- GRB 130702A / Fermi394416326 : Fermi-LAT detection of a burst
- Fermi394416326: FTN detection
- Fermi394416326: iPTF detection of a possible optical afterglow
- GRB 130627B: Possible Swift-XRT afterglow detection
- GRB 130626A: Swift-XRT possible detection and UVOT upper limits
- GRB 130603B: Analogy with GRB 090510A and possible connection with a supernova
- GRB 130603B: Detection of possible afterglow/kilonova in HST observations
- GMRT radio observation of GRB 130603B
- GRB 130606A: Errata Ks magnutide in GCN 14792
- Swift/UVOT observations of GRB130603A
- Swift Trigger 556533 is probably not an astrophysical event
- GRB 130518A: Swift XRT and UVOT possible afterglow
- GRB 130427A: Continued RATIR Optical and NIR Observations - Photometric Evidence for a New Component
- GRB 130427A: Skynet detections of a possible supernova
- GRB 130514B Swift-BAT observations
- GRB 130515A: GROND Observations
- GRB 130427A: Tautenburg 2nd epoch: No break, no clear SN
- GRB 130427A: host galaxy observations
- GRB 130505B: Swift Candidate Afterglow
- Refined IPN Triangulation of GRB 130502B
- Konus-Wind observation of GRB 130504C
- GRB 130504C: Swift-XRT observations
- GRB 130502B: possible TNG counterpart
- Trigger 555096: Swift detection of a possible burst
- GRB 130427A: Pan-STARRS 1 optical observations
- GRB 130427A: Predictions about the occurrence of a supernova
- GRB 130427A: GMRT radio detection
- GRB 130427A: photo-z of possible SDSS host galaxy
- GRB 130427A: high energy gamma-ray detection by AGILE
- GRB 130427A: Nishi-Harima NIR Observations
- GRB 130427A: P60 early nondetection
- Trigger 554491: Swift detection of a spike possibly from Sgr A*