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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"

3798 results found.

  1. GRB081008: Swift/UVOT observations
  2. GRB 081008: Swift detection of a burst with optical afterglow
  3. GRB 081008: ROTSE-III Detection of Optical Counterpart
  4. GRB 081007: Swift detection of a burst with optical afterglow
  5. Trigger 324561: IGR J08408-4503 detected by Swift
  6. GRB 080916A: GROND lightcurve
  7. GRB 080916C: GROND Detection of the Optical Afterglow Candidate
  8. GRB080916A: Refined Swift/UVOT Observations
  9. GRB 080916A, Swift-BAT refined analysis
  10. GRB 080916: REM detection of the NIR afterglow
  11. GRB 080916: REM candidate afterglow
  12. GRB 080916: Swift detection of a burst with optical afterglow
  13. GRB 080915B, Swift-BAT refined analysis
  14. GRB 080913, Swift-BAT refined analysis
  15. Swift-BAT/-XRT refined analysis on trigger 324362 (LS I +61 303)
  16. GRB 080905B: Watcher optical detection
  17. GRB 080905B: Swift detection of a burst with possible optical counterpart
  18. GRB 080903, Swift-BAT refined analysis
  19. GRB 080830: Fermi Gamma-ray Burst Monitor detection
  20. INTEGRAL ToO observation of SGR0501+4516
  21. SGR 0501+4516: Decline in Activity
  22. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  23. GRB 080825B - optical counterpart candidate
  24. SGR 0501+4516: Swift-BAT refined analysis of the 3 discovery events
  25. GRB 080727C, Swift-BAT refined analysis
  26. GRB 080727B: Swift/UVOT Upper Limits
  27. GRB 080727B, Swift-BAT refined analysis
  28. GRB 080727: Swift detection of a burst
  29. GRB 080721: UVOT Follow-Up Observations
  30. GRB 080721 : Lulin Optical follow-ups
  31. GRB 080721: Swift detection of a burst with a bright optical counterpart.
  32. Refined analysis of Swift Trigger 316063, is IGR J08408-4503
  33. GRB 080613B - NOT optical and IR nondetections
  34. GRB 080605, Swift-BAT refined analysis
  35. GRB 080605, Swift-BAT refined analysis
  36. GRB 080605: MASTER VWF 46 s AT observation
  37. GRB 080605: Swift detection of a burst with an optical afterglow
  38. GRB 080603B, Swift-BAT refined analysis
  39. Swift analysis of BAT Slew Survey event (Trigger=009)
  40. GRB080521(?): detection of possible burst from BAT slew data and XRT ToO
  41. GRB 080520, Swift-BAT refined analysis
  42. GRB 080514B: Suzaku WAM observation of the prompt emission
  43. GRB 080515, Swift-BAT refined analysis
  44. GRB 080515: Swift detection of a burst
  45. GRB080506: Swift/UVOT observations
  46. GRB 080506, Swift-BAT refined analysis
  47. GRB080503, RIMOTS optical upper limit
  48. GRB 080506: TLS afterglow detection in VRIZ
  49. GRB 080506: Swift detection of a burst with optical afterglow
  50. GRB 080503: Swift detection of a short burst
  51. GRB080430: Optical observation in AsU CAS Ondrejov & Brno
  52. GRB 080420?: Swift detection of a possible short burst
  53. GRB 080413B, Swift-BAT refined analysis
  54. GRB 080409: Swift detection of a burst
  55. GRB080330: Swift XRT refined analysis
  56. Konus-Wind observation of GRB 080328
  57. GRB080330: LOAO R-band Detection
  58. GRB 080320: Swift XRT refined analysis
  59. GRB 080320: J detection with FLAMINGOS
  60. GRB 080320: Gemini-N optical afterglow
  61. GRB 080319B: Gemini-South photometry
  62. GRB 080320 - SDSS Pre-Burst Observations
  63. GRB 080319D: MASTER-VWF-Kislovodsk optical observation
  64. GRB 080319C: MASTER-VWF-Kislovodsk optical observation
  65. GRB 080319b light curve by Pi-of-the-Sky
  66. GRB 080319b prompt optical observation by Pi-of-the-Sky
  67. Swift Trigger 306616 is not a GRB
  68. GRB080310: Optical observation by MITSuME telescope
  69. GRB080229, optical upper limit
  70. GRB080307: Optical upper limits
  71. GRB 080218B, Swift-BAT refined analysis
  72. GRB 080218B: Swift detection of a burst
  73. GRB 080212, Swift-BAT refined analysis
  74. GRB 080210: Super-LOTIS observations
  75. GRB 080207, Swift-BAT refined analysis
  76. GRB 080207, Swift-BAT refined analysis
  77. GRB 080205: Swift detection of a burst
  78. GRB 080123: Early afterglow detection with BATSS (BAT Slew Survey)
  79. GRB 080123 : Suzaku WAM observation of the prompt emission
  80. GRB 080123: Swift detection of a short burst
  81. Swift-BAT refined analysis of short GRB 071227
  82. GRB 071227: Swift detection of a burst
  83. GRB 071122: MASTER optical observation
  84. GRB 071118: Swift detection of a burst
  85. GRB071112C: Errata of MITSuME Ic band photometry
  86. GRB071112C MITSuME Okayama Optical Observation
  87. GRB 071112C: Swift detection of a burst with an optical counterpart
  88. GRB071101: Optical and NIR upper limits by KANATA
  89. GRB071028: Xinglong EST V-band upper limit
  90. GRB071021: MARGE Optical Limits
  91. GRB071020, optical upper limit
  92. GRB071021: MITSuME Okayama Optical Upper Limits
  93. GRB 071018: Swift-XRT observation
  94. GRB 071011, Swift-BAT refined analysis
  95. GRB 071010B, Swift-BAT refined analysis
  96. GRB071008: Swift-XRT observation
  97. GRB 071003, Swift-BAT refined analysis
  98. GRB 071003: Swift detection of a bright burst
  99. Recent SGR1806-20 Activity
  100. GRB 070920B, Swift-BAT refined analysis

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