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"
16217 results found.
- GRB 241115A: Swift detection of a burst
- EP 241113a: LBT possible optical counterpart
- LIGO/Virgo/KAGRA S241114bi: Identification of a GW compact binary merger candidate
- GRB 241113A: PRIME near-infrared upper limits
- GRB 241113B: J-band upper limit from WINTER
- GRB 241113A: J-band observations with WINTER
- EP241113a : J-band observations with WINTER
- GRB 241030A: LCO optical observation
- GRB 241113B: Swift-XRT observations
- GRB 241113A: 1.6m Mephisto and 50cm array optical upper limits
- EP241113b/GRB 241113B: EP detection of GRB 241113B
- EP241113a: EP on-board trigger and autonomous follow-up observation
- GRB 241113A: Swift/UVOT Detection
- GRB 241113A: REM detection of the optical/NIR afterglow
- GRB 241113A: LCO optical observations
- GRB 241112B: GMG Optical Upper Limit
- GRB 241113A: Enhanced Swift-XRT position
- GRB241113A: LCOGT (40-cm) optical counterpart detection
- GRB 241113A: Swift detection of a burst with an optical counterpart
- SVOM/GRM detection of a short burst from SGR 1E1841-045
- GRB 241105A: ATCA Radio Upper Limits
- GRB 241112B: AbAO optical upper limit
- GRB 241107A: GROWTH-India telescope optical upper limit
- GRB 241112B: Optical afterglow detection confirmation in revisiting the Mephisto data
- GRB 241112B: Swift-XRT afterglow detection
- GRB 241112B: LCO optical detection of the SVOM/VT candidate
- GRB 241112B: Mephisto optical upper limits
- GRB 241112B: GOTO optical upper limits
- GRB 241107A: INTEGRAL IBIS localization
- EP241107a: EP-FXT follow-up observations
- LIGO/Virgo/KAGRA S241109bn: ATLAS observations and discovery of the potential counterpart AT2024aawt
- IPN triangulation of GRB 241107A (short/hard)
- LIGO/Virgo/KAGRA S241109bn: Upper limits from EP-WXT observations
- LIGO/Virgo/KAGRA S241109bn: Coverage and upper limits from MAXI/GSC observations
- INTEGRAL detection of a burst from 1E 1841-045
- EP241107a: AbAO optical upper limit
- GRB 241108A: Further COLIBRÍ Upper Limits on the Optical Counterpart
- EP241109a: confirmation of a stellar flare by BOOTES-7
- EP241109a: EP on-board trigger and autonomous follow-up observation
- EP241107A: MASTER optical observations of xray transient
- EP241107a: KAIT optical observations
- GRB 241108A: COLIBRÍ Upper Limits on the Optical Counterpart
- EP241107a: Kinder optical follow-up observations
- GRB 241025A: radio detection with the VLA
- EP241107a: AKO Optical Afterglow Follow-Up Observations
- GRB 241105A: EP-FXT follow-up observations
- GRB 241105A: SVOM/GRM observation
- EP241107a: OHP/T193 photometric and spectroscopic observations
- GRB 241105a: PRIME near-infrared upper limits
- GRB 241105A: ePESSTO+ NTT optical afterglow detection
- EP241107a: GIT optical observations
- EP241107a: SVOM/C-GFT optical observations
- EP241107a: AKO Optical Afterglow Detection
- GRB 241025A: LBT optical observations
- EP241107a: EP on-board trigger and autonomous follow-up observation
- GRB 241105A: VLT/FORS2 optical afterglow rapid fading
- GRB 241105A: Swift/UVOT Detection
- GRB 241105A: Swift-XRT afterglow detection
- GRB 241104A: Swift-XRT observations
- GRB 240511A: LCO upper limits
- GRB 241104A: SVOM/VT optical candidate
- GRB 241104A/EP241104a: Optical upper limits with Kinder observations
- GRB 241104A: COLIBRÍ Upper Limits on the Optical Counterpart
- EP241104a: EP detection of GRB 241104A X-ray emission
- GRB 241010A: host galaxy redshift z = 0.977
- EP241101a NUTTelA-TAO / BSTI Measurements 2024-11-02
- GRB 240821A: further radio observations with the VLA
- EP241101a: EP-FXT observations update
- EP241103a: GIT optical upper limit
- EP241021a: OHP/T193 further optical observations
- LIGO/Virgo/KAGRA S241102br: OHP/T193 optical observations
- EP241103a: Swift XRT detection and improved X-ray position
- EP241021a: continued SOAR observations
- EP241101a: Optical upper limits with Kinder observations
- EP241101a: OHP/T193 optical observations
- EP241103a: EP observation update
- LIGO/Virgo/KAGRA S241102br: EP-WXT X-ray follow-up and flux limits
- GRB 241030A: Swift-UVOT observations of the optical prompt flare
- EP241103A: LCO optical observations
- EP241103a: an X-ray transient detected by Einstein Probe
- Kinder optical follow-up observations of EP241021a, EP241026b, and EP241030a/GRB241030A
- GRB241030A: OHP/T193 optical observations
- EP241030a: Futher EP-FXT observation of the X-ray Afterglow of GRB 241030A
- EP241101a: EP-WXT detection of a fast X-ray transient
- GRB 241101A: FRAM-ORM optical limit
- GRB 241030A/EP241030a: TNOT observations of the optical counterpart
- GRB 241101A: Swift-BAT refined analysis
- GRB 241030A: further SAO RAS optical observations
- GRB 241030A: Optical Observations via Virtual Telescope Project
- EP241021a: Liverpool Telescope optical follow-up observations
- GRB 241026A: SAO RAS optical observations
- EP241030a: EP/FXT observation of GRB 241030A X-ray Afterglow
- GRB 241030B: NUTTelA-TAO / BSTI Optical Limits
- EP241021a: OHP/T193 optical observations
- GRB 241030A: Palomar 1-m telescope COSMOS optical observations
- GRB 241030B: Montarrenti Observatory optical upper limit
- EP241026b: Liverpool Telescope optical follow-up
- GRB 241030A: SAO RAS optical observations
- EP241021a: AMI-LA radio detection
- GRB 241030B : GIT optical upper limits