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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.

Search for Circulars by submitter, subject, or body text (e.g. 'Fermi GRB').
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"

37530 results found.

  1. Fermi 403206457 / GRB 131011A: AAO optical observations
  2. GRB 131014A: RATIR Optical and NIR Observations
  3. GRB 131014A: Enhanced XRT position
  4. Konus-Wind observation of GRB 131014A
  5. GRB 131014A: NOT afterglow candidate
  6. GRB 131014A: Nanshan optical observations
  7. GRB 131014A: Swift detection of a possible X-ray afterglow
  8. GRB 131014A Tiled Swift observations
  9. GRB 131014A: Fermi-LAT detection
  10. GRB 131014A: Fermi GBM detection
  11. GRB 131011A: Fermi GBM detection
  12. iPTF 13dsw/Fermi403206457: X-Shooter redshift
  13. Swift-XRT detection of iPTF 13dsw/Fermi403206457
  14. GRB 131011A: GROND afterglow observations
  15. Fermi403206457: continued P60 observations and fading behavior
  16. Fermi403206457: Weihai optical upper limit
  17. Fermi403206457: NOT optical observations
  18. Fermi403206457: iPTF detection of a possible optical afterglow
  19. Trigger 574266 is not a Swift detection of a known source
  20. GRB 130925A: Possible signatures of binary nature in the afterglow - Request for observations
  21. GRB 130831A: Continued RATIR Optical and NIR Observations
  22. GRB 130831A: VLT/FORS2 spectroscopic detection of a supernova
  23. GRB 131004A: MOSFIRE NIR imaging
  24. GRB 131004A: Correction to XRT refined analysis
  25. GRB 131004A: Skynet PROMPT/DSO-14 upper limits
  26. GRB 131004A, Swift-BAT refined analysis
  27. GRB 131004A: Fermi GBM observation
  28. GRB 131004A: CARMA 93 GHz upper limit
  29. GRB 131004A: Swift/UVOT Detection
  30. GRB 131004A: RATIR Optical and NIR Upper Limits
  31. GRB 131004A: Swift-XRT refined Analysis
  32. GRB131004A: TNG Redshift confirmation
  33. GRB 131004A: GROND observations of the afterglow
  34. GRB 131004A: Enhanced Swift-XRT position
  35. GRB131004A: Magellan Redshift
  36. GRB 131004A: Liverpool Telescope optical afterglow observations
  37. GRB 131004A: TNG optical afterglow confirmation
  38. GRB 131004A: optical afterglow from the NOT
  39. GRB 131004A: Swift detection of a burst (may be short)
  40. GRB 131002A, Swift-BAT refined analysis
  41. GRB 130925A: 3mm observations with CARMA
  42. GRB 131002A: Fermi GBM observation
  43. GRB 130925A/Sw J0244-2609: mm observations at PdBI
  44. GRB 131002B, Swift-BAT refined analysis
  45. GRB 131002B: GROND upper limits
  46. GRB 131002B: Swift-XRT Refined Analysis
  47. GRB 131002B: Swift/UVOT Upper Limits
  48. GRB 131002A: Swift/UVOT Detection
  49. GRB 131001A, Swift-BAT refined analysis
  50. GRB 131002A: Swift-XRT refined Analysis
  51. GRB 131002B: Enhanced Swift-XRT position
  52. GRB 131002A: ISON-NM optical observations
  53. Swift J1242.9-3530, Swift-BAT refined analysis
  54. GRB 131001A: Swift UVOT and XRT Upper Limits
  55. GRB 131002A: Enhanced Swift-XRT position
  56. NuSTAR observations of GRB 130925A
  57. Fermi Gamma-ray Burst Monitor trigger 402405063 / 131002466 is not a GRB
  58. GRB 131002B: Swift detection of a burst
  59. GRB 131002A: Swift detection of a burst
  60. GRB 131002A: Faulkes Telescope North optical afterglow
  61. GRB 131001A detected in ground analysis of Swift-BAT data
  62. GRB 130925A: continuing Swift/XRT monitoring
  63. Swift Operations in the event of a US Government shutdown
  64. IPN Observations of GRB 130925A
  65. US Government shutdown may impact GRB operation of GCN
  66. GRB 130930A: Swift detection of a burst
  67. GRB 130929A: Swift/UVOT Upper Limits
  68. GRB 130831A: Continued RATIR Optical and NIR Observations
  69. GRB 130929A: Swift-XRT refined Analysis
  70. GRB 130929A, Swift-BAT refined analysis
  71. GRB 130929A: Enhanced Swift-XRT position
  72. GRB 130929A: TAROT La Silla observatory optical observations
  73. GRB 130929A: Swift detection of a burst
  74. Fermi LAT Upper Limits on GRB 130925A
  75. GRB 130925A: Swift/UVOT Detection of the Host Galaxy
  76. GRB 130925A: Swift/UVOT Upper Limits
  77. GRB 130925A: sub-mm non-detection with SMA
  78. GRB 130925A: optical upper limit
  79. GRB 130925A: Continued RATIR Optical and NIR Observations
  80. GRB 130925A: Fermi GBM Detection
  81. Konus-Wind observation of GRB 130925A
  82. Observation of possible GRB/TDE 130925A by INTEGRAL/SPI-ACS: three activity episodes
  83. GRB 130925A: RATIR Optical and NIR Observations
  84. GRB 130925A Swift-BAT refined analysis
  85. GRB 130925A: Historical non-detection from Rosat-HRI
  86. Fermi GBM detection of GRB 130925A and a possible precursor
  87. GRB 130925A: Swift-XRT refined Analysis
  88. GRB 130925A: Initial Similarities to Swift J1644+57
  89. GRB 130925A: TAROT La Silla observatory optical observations
  90. GRB 130925A: Enhanced Swift-XRT position
  91. GRB 130925A: VLT/X-shooter redshift
  92. GRB 130925A: VLT/UVES observations
  93. GRB 130925A: MAXI/GSC detection
  94. GRB 130925A: GROND afterglow candidate
  95. GRB 130925A: Swift detection of a burst
  96. IPN Triangulation of SGR-like burst 130913 - probable association with SGR/AXP 1E1841-045
  97. GRB 130831A: RTT150 optical observations
  98. GRB 130702A: RTT150 optical observations
  99. GRB 130831A: RATIR Confirmation of NIR/Optical Afterglow Flattening
  100. GRB 130903A: optical observations

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