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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"

27015 results found.

  1. GRB 080906: Swift detection of a burst with optical afterglow
  2. GRB080825C: Fermi-LAT observations
  3. GRB 080905B: Swift detection of a burst with possible optical counterpart
  4. GRB 080905: Swift detection of a probably-short burst
  5. GRB 080903: Swift/UVOT Observations
  6. GRB 080903: Swift-XRT Refined Analysis
  7. GRB 080903, Swift-BAT refined analysis
  8. GRB 080903: Astrotel-Caucasus optical observations
  9. GRB 080903: TAROT Calern observatory optical observations
  10. GRB 080903: ROTSE-III Optical Limits
  11. GRB 080903: Swift detection of a burst
  12. GRB 080830: Fermi Gamma-ray Burst Monitor detection
  13. Swift-BAT trigger 322590 is not a GRB
  14. Swift trigger 322590: BAT detection of a possible burst
  15. SGR 0501+4516: XMM-Newton monitoring schedule
  16. SGR 0501+4516: Decline in Activity
  17. GRB080823: Fermi Gamma-ray Burst Monitor detection
  18. GRB 080824: Fermi Gamma Ray Burst Monitor detection
  19. GRB080825C: GLAST Burst Monitor detection
  20. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  21. Soft Gamma Repeater SGR 0501+4516: GBM Detection of multiple bursts
  22. GRB 080822B, Swift-BAT refined analysis
  23. SGR 0501+4516: UKIRT detection of possible infra-red counterpart
  24. Trigger 321551: Continued Large Flaring of SGR 0501+4516
  25. New Soft Gamma Repeater 0501+4516 (GRB 080822): GLAST Burst Monitor detection
  26. Swift Trigger 321481: A Large Flare from SGR 0501+4516
  27. SGR 0501+4516: Swift-BAT refined analysis of the 3 discovery events
  28. GRB 080822B: Swift detection of a burst
  29. GRB080818B: GLAST Burst Monitor detection
  30. Third event from SGR 0501+4516
  31. New Soft Gamma Repeater 0501+4516 was GRB 080822
  32. GRB 080822: Swift detection of a short burst
  33. GLAST Burst Monitor detection of a GRB: 080816B
  34. GLAST Burst Monitor detection of GRB 080818
  35. GLAST Burst Monitor detection of GRB080817B
  36. GLAST Burst Monitor detection of GRB 080817
  37. GLAST Burst Monitor detection of GRB080816
  38. GLAST Burst Monitor detection of GRB 080812
  39. GRB 080810: Konus-Wind and Swift/BAT joint spectral analysis
  40. GLAST Burst Monitor detection of GRB 080810
  41. First GLAST Burst Monitor GRB Circulars
  42. GRB 080810: Swift/UVOT Refined Analysis
  43. GRB 080810: Kanazawa optical observation
  44. GRB 080810: Swift-XRT Team refined analysis
  45. GRB 080810: KANATA optical-NIR observation, update
  46. GRB 080810: ROTSE-III Prompt Detection of Optical Counterpart
  47. GRB 080810, Swift-BAT refined analysis
  48. GRB 080810: Swift detection of a burst with a bright optical afterglow
  49. GRB 080723B: XMM-Newton observation
  50. GRB 080805: Swift/UVOT Upper Limits
  51. GRB 080804: Swift/UVOT Refined Analysis
  52. GRB 080805, Swift-BAT refined analysis
  53. GRB 080804, Swift-BAT refined analysis
  54. GRB080805 optical limit by "Pi of the Sky"
  55. GRB 080805: Swift detection of a burst
  56. GRB 080804: Swift detection of a burst with optical afterglow
  57. GRB 080804: ROTSE-III Detection of Optical Counterpart
  58. GRB 080802: Swift/UVOT Upper Limits
  59. GRB 080802: UVI Telescope Upper Limit
  60. GRB 080802, Swift-BAT refined analysis
  61. GRB 080802: Swift detection of a probable burst
  62. GRB 080727C: Suzaku WAM observation of the prompt emission
  63. GRB 080727C: TAROT Calern observatory optical observations
  64. GRB 080727B: GROND redshift limit
  65. GRB 080727C, Swift-BAT refined analysis
  66. GRB 080727C: Swift/UVOT Upper Limits
  67. Konus-Wind observation of GRB 080727B
  68. GRB 080727C: Swift XRT refined analysis
  69. GRB080727C: RTT150 optical observations
  70. GRB 080727C: Swift detection of a burst
  71. Swift detection of XTE J1701-407
  72. GRB 080727B: Swift/UVOT Upper Limits
  73. BAT Trigger 318150 is not a GRB
  74. GRB 080727B: Swift-XRT refined analysis
  75. GRB 080727B, Swift-BAT refined analysis
  76. GRB 080727A, Swift-BAT refined analysis
  77. GRB 080727A: Swift-XRT refined analysis
  78. GRB080727A: Swift/UVOT Upper Limits
  79. GRB 080727B: Swift detection of a bright burst
  80. GRB 080727: Swift detection of a burst
  81. GRB 080725, Swift-BAT refined analysis
  82. GRB 080725: REM prompt observations
  83. GRB 080725: Swift detection of a burst
  84. GRB 080723A: Swift/UVOT Upper Limits
  85. GRB 080723B - Swift-XRT refined analysis
  86. GRB 080723B - Swift-XRT position
  87. GRB 080723, Swift-BAT refined analysis
  88. GRB 080723A: Swift-XRT refined analysis
  89. GRB 080723B: Detection and Localization by SuperAGILE
  90. GRB 080723: Swift detection of a burst
  91. GRB 080721: UVOT Follow-Up Observations
  92. Konus-Wind observation of GRB 080721
  93. GRB 080721: Swift-XRT refined analysis
  94. GRB 080721, Swift-BAT refined analysis
  95. GRB 080721: Swift/UVOT Photometric Redshift
  96. GRB 080721: Swift detection of a burst with a bright optical counterpart.
  97. Retraction of Swift Trigger 317393
  98. Trigger 317393: Swift detection of a possible GRB
  99. Trigger 317205: Swift detection of an outburst from XTE J1701-407
  100. GRB 080714: GROND confirmation of the optical/NIR afterglow

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