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 201014A: Swift-XRT refined Analysis
- Swift-BAT trigger 1000255: XRT afterglow detection of GRB 201014A
- GRB 201013A: Swift-XRT refined Analysis
- GRB 201006A: Chandra upper limit on the X-ray afterglow
- GRB 201008A: Swift-XRT observations
- IceCube-200926A: Upper limits from Insight-HXMT Observations
- Swift-XRT observations of IceCube 201007A
- GRB 201006A: Swift-XRT refined Analysis
- GRB 201001A: Swift-XRT refined Analysis
- Swift-XRT observations of IceCube 200929A
- Swift-XRT observations of IceCube 200926A
- GRB 200925B: Swift-XRT refined analysis update
- GRB 200925B: Swift-XRT refined Analysis
- GRB 200922A: Swift-XRT refined Analysis
- GRB 200914A: Swift-XRT further observations
- Swift-XRT observations of IceCube 200916A
- GRB 200917A: Swift-XRT refined Analysis
- Swift-XRT observations of IceCube 200911A
- GRB 200914A: Swift-XRT observations
- GRB 200907B: Swift-XRT refined Analysis
- GRB 200906A: LBT near-infrared upper limit
- GRB 200906A: Swift-XRT refined Analysis
- GRB 200901B: Swift-XRT refined Analysis
- GRB 200901A: Swift-XRT refined Analysis
- GRB 200901A: Swift-XRT observations
- GRB 200829A: Swift-XRT refined Analysis
- GRB 200826A: Swift-XRT afterglow detection
- Swift Trigger 992444 is due to detector noise
- Swift Trigger 992444: a possible GRB 200821A
- GRB 200819A: Swift-XRT refined Analysis
- Swift Trigger 990358 is due to detector noise
- Swift Trigger 989458 is due to detector noise
- GRB 200809B: Swift-XRT afterglow detection
- GRB 200806A: Swift-XRT refined Analysis
- GRB 200803A: Swift-XRT afterglow detection
- GRB 200729A: Swift-XRT refined Analysis
- GRB 200714E: Swift-XRT afterglow detection
- GRB 200716C: Swift-XRT refined analysis correction
- GRB 200716C: Swift-XRT refined Analysis
- GRB 200715A: Swift-XRT afterglow detection
- GRB 200714E: Swift-XRT observations
- GRB 200713A: Swift-XRT refined Analysis
- GRB 200711A: Swift-XRT refined Analysis
- GRB 200709B/HAWC-200907A: Swift-XRT further observations
- GRB 200709B: Swift-XRT observations
- GRB 200630A: Swift-XRT refined Analysis
- GRB 200623A: Swift XRT further observations
- GRB 200623A: Swift-XRT observations
- Swift-XRT observations of IceCube 200615A
- Fermi GRB 200616A: Global MASTER-Net observations report
- GRB 200613A: Swift-XRT afterglow detection
- GRB 200613A: Fermi-LAT detection
- GRB 200612A: Swift-XRT refined Analysis
- GRB 200529A: Swift-XRT refined Analysis
- GRB 200528A: Swift-XRT refined Analysis
- GRB 200528A: Swift/UVOT Upper Limits
- GRB 200524A: Swift-XRT afterglow detection
- GRB 200522A: Swift-XRT refined Analysis
- GRB 200517A: Swift-XRT Confirmation of afterglow
- GRB 200519A: Swift-XRT refined Analysis
- GRB 200517A: Swift-XRT afterglow detection
- GRB 200512A: Swift-XRT refined Analysis
- GRB 200509A: Swift-XRT refined Analysis
- GRB 200424A: Swift-XRT afterglow detection
- SGR 1935+2154 the Insight-HXMT observation plan
- GRB 200424A: Swift/UVOT Upper Limits
- GRB 200425A: Swift-XRT refined Analysis
- GRB 200424A: Swift-XRT observations
- GRB 200412B: Swift XRT confirmation of afterglow and UVOT upper limits
- GRB 200405B: Further Swift-XRT observations
- GRB 200412B: Swift-XRT afterglow detection
- GRB 200411A: Swift-XRT refined Analysis
- LIGO/Virgo S200225q: Swift XRT observations, 1 X-ray sources
- LIGO/Virgo S200224ca: Swift XRT observations, 8 X-ray sources
- GRB 200410A: Swift-XRT refined Analysis
- GRB 200409A: Swift-XRT refined Analysis
- GRB 200405B: Swift-XRT observations
- GRB 200325B: further Swift-XRT observations
- GRB 200325B: Swift-XRT and UVOT observations
- GRB 200324A: Swift-XRT refined Analysis
- Chandra observations of GW170817 at 2.5 years since merger (All epochs 4 of 4)
- GW170817: Continued X-ray emission detected with Chandra at 940 days post-merger
- LIGO/Virgo S200316bj: No counterpart candidates in Fermi-LAT observations
- LIGO/Virgo S200213t: Continued Swift UVOT and XRT observations of ZTF20aamvmzj (AT2020cja)
- LIGO/Virgo S200311bg: No significant counterpart candidates in Fermi-LAT observations
- Chandra observations of GW170817 ~ 2.5 years since merger (epoch 1 of 4)
- GRB 200306C: Swift-XRT refined Analysis
- GRB 200306A: Swift-XRT refined Analysis
- GRB 200303A: Swift-XRT refined Analysis
- LIGO/Virgo S200302c: No significant counterpart candidates in Fermi-LAT observations
- GRB 200228B: Swift-XRT refined Analysis
- GRB 200227A: Swift-XRT refined Analysis
- LIGO/Virgo S200225q: No counterpart candidates in Fermi-LAT observations
- LIGO/Virgo S200224ca: No counterpart candidates in Fermi-LAT observations
- GRB 200219C: Swift-XRT afterglow confirmation
- GRB 200224A: Swift-XRT refined Analysis
- GRB 200219C: Swift-XRT afterglow detection
- LIGO/Virgo S200213t: Swift UVOT and XRT observations of ZTF20aamvmzj (AT2020cja)
- LIGO/Virgo S200219ac: No counterpart candidates in Fermi-LAT observations
- GRB 200219A: Swift-XRT refined Analysis correction