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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"

19356 results found.

  1. VLT/UVES observations of GRB060418
  2. GRB060418: Swift XRT Team Refined Analysis
  3. GRB060418: Magellan/MIKE Spectroscopic Redshift
  4. GRB 060418: Swift detection of a burst with bright x-ray and optical afterglow
  5. SGR 1900+14: Refined analysis of the Swift-BAT outburst
  6. GRB060413: Swift/UVOT upper limits
  7. SGR 1900+14: Swift detection of an outburst
  8. GRB 060413: Refined analysis of the Swift-BAT burst
  9. GRB 060413: XRT refined analysis
  10. GRB 060413: No Optical Afterglow in Swift/UVOT TDRSS Data
  11. GRB 060413: Swift detection of a burst
  12. GRB060403: XRT refined analysis
  13. GRB 060403: Swift/UVOT upper limits
  14. SGR 1900+14: BAT observations
  15. GRB 060403: Refined analysis of the Swift-BAT burst
  16. GRB060403: Swift XRT refined position
  17. Konus-Wind observation of the recent SGR 1900+14 activity. Will
  18. GRB 060403: Swift detection of a burst
  19. GRB060331: Swift/UVOT upper limits
  20. Swift XRT observations of the HETE transient H4043
  21. SGR 1900+14: bright burst detected by Konus-Wind on March 28
  22. SGR 1900+14: Swift-BAT detection of a cluster of outbursts
  23. SGR 1900+14: Swift-BAT detection of a bright outburst
  24. GRB 060323 : WIDGET simultaneous optical observations
  25. GRB 060322: Confirmation of Swift XRT afterglow
  26. GRB060323: optical limit
  27. SGR 1900+14: CORRECTION to GCN 4923
  28. SGR 1900+14: Refined Swift-BAT analysis of the renewed activity
  29. SGR 1900+14: Swift detection of renewed activity
  30. GRB060323: NOT optical observations
  31. GRB 060322: IAC80 optical observations
  32. GRB 060322: Swift XRT afterglow candidate
  33. GRB 060323: Swift/UVOT Observations
  34. GRB060323: NOT observations
  35. GRB 060323: Refined analysis of the Swift-BAT burst
  36. GRB 060323: Swift XRT refined analysis
  37. GRB 060323: Swift/XRT position
  38. GRB 060322: Refined analysis of the Swift-BAT burst
  39. GRB060323 - SDSS Pre-Burst Observations
  40. GRB 060323: Swift detection of a burst with a possible optical afterglow
  41. GRB 060322: Swift-BAT detection of a 200-sec burst
  42. GRB 060319: IAC-80 optical observations
  43. GRB060319: Swift XRT refined analysis
  44. GRB060319: Swift/UVOT upper limits
  45. GRB 060319: Swift-BAT refined analysis
  46. GRB060319: Swift/XRT position
  47. GRB 060319: Swift detection of a burst
  48. Konus-Wind observation of GRB 060313
  49. GRB 060313: Further analysis of the Swift-BAT bright short hard burst
  50. GRB 060313: Swift/UVOT Observations
  51. GRB 060313: Swift-XRT team refined analysis
  52. GRB 060313: Refined analysis of the Swift-BAT bright short hard burst
  53. GRB 060313: Swift XRT position
  54. GRB060313: optical and near infrared observations with REM
  55. GRB 060313: Swift-BAT detection of a bright short hard burst
  56. GRB060312: Swift UVOT observation
  57. GRB 060312: Refined analysis of the Swift-BAT burst
  58. GRB 060312: Swift XRT team refined analysis
  59. GRB060306: APO Ks-band Imaging Observations
  60. GRB 060312: ROTSE-III Optical Limits
  61. GRB 060312: Swift detection of a burst
  62. Bright short hard GRB 060303: IPN localization and Konus spectrum
  63. GRB060218: analysis of the XMM-Newton observation
  64. Swift/UVOT observations of GRB060306
  65. GRB 060306: Swift-BAT refined analysis
  66. GRB 060306: Swift-XRT team refined analysis
  67. GRB 060306: Swift detection of a bright burst
  68. GRB060218: Ep,i - Eiso correlation
  69. GRB 060223b: Swift/UVOT Upper Limits
  70. GRB 060223B: Swift XRT possible afterglow
  71. GRB 060223B: Swift-BAT refined analysis
  72. GRB 060223a: Swift/UVOT refined analysis
  73. GRB 060223: Swift XRT Team preliminary analysis
  74. GRB 060218/SN 2006aj: Swift-BAT fluence and peak flux
  75. GRB 060223B: Swift detection of a bright burst
  76. GRB 060223: Swift-BAT refined analysis
  77. GRB 060223: Swift/UVOT Confirmation of Optical Afterglow
  78. GRB 060223: Swift detection of a burst
  79. GRB 060219: Swift-BAT refined analysis
  80. GRB 060218: Further refined analysis of the Swift-BAT burst
  81. GRB 060218: Likely an underluminous GRB
  82. GRB 060219: SDSS galaxy inside XRT error circle
  83. GRB060218: UV Detection and Light Curves
  84. GRB 060219: Swift/UVOT Upper Limits
  85. GRB 060219: Swift-XRT Team refined analysis
  86. GRB 051221B: Swift-XRT Team Refined Analysis
  87. GRB 060219: Partial refined analysis of the Swift-BAT burst
  88. GRB 060219: Swift-XRT position typo correction
  89. GRB 060219: Swift-XRT position
  90. GRB 060218: optical/nIR observations at La Palma
  91. GRB 060219: Swift-BAT detection of a weak burst
  92. Oddball GRB 060218, transient or GRB?
  93. GRB060218: Swift/XRT Team preliminary analysis of the possible burst
  94. Brightening of the Optical Counterpart of the Possible GRB 060218
  95. GRB 060218: MDM Observations
  96. GRB 060218A: ROTSE-III Possible Optical Flare
  97. GRB060218: Swift/XRT refined position of a possible burst
  98. Preliminary refined analysis of the Swift-BAT trigger 191157
  99. Further UVOT Observations of the Candidate Optical Afterglow for GRB 060218
  100. GRB 060211B: Swift/UVOT Upper Limits

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