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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"

19938 results found.

  1. Recent VLA non-detection of SGR 0501+4516
  2. SGR 0501+4516: Spin Down Rate and Inferred Dipole Magnetic Field
  3. SGR 0501+4516: preliminary results of the first XMM-Newton observation
  4. nIR observations of SGR 0501+4516
  5. INTEGRAL ToO observation of SGR0501+4516
  6. SGR 0501+4516: Confirmation of the NIR counterpart
  7. GRB080828: Swift/UVOT Upper Limits
  8. SGR 0501+4516: Detection of possible optical counterpart
  9. SGR 0501+4516: WHT observations of the possible near-infrared counterpart
  10. GRB080825B: Swift/UVOT Upper Limits
  11. GRB 080828: Swift-XRT detection of a possible X-ray afterglow
  12. Swift-BAT trigger 322590 is not a GRB
  13. VLA non-detection of SGR 0501+4516
  14. Radio Detection of SGR 0501+4516: Retraction
  15. Swift trigger 322590: BAT detection of a possible burst
  16. SGR 0501+4516: XMM-Newton monitoring schedule
  17. SGR 0501+4516: Decline in Activity
  18. SGR 0501+4516: Proximity to supernova remnant HB9
  19. Enhanced Swift-XRT position of SGR 0501+4516
  20. SGR 0501+4516: GMRT Radio Observation at 618 MHz
  21. SGR 0501+4516: Swift XRT measure of the spin period
  22. GRB 080825B: Swift-XRT team analysis
  23. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  24. Soft Gamma Repeater SGR 0501+4516: GBM Detection of multiple bursts
  25. Suzaku ToO Observation of SGR 0501+4516
  26. SGR 0501+4516: radio pulsar searches with GBT and WSRT
  27. Konus-Wind observations of new SGR 0501+4516
  28. INTEGRAL ToO Observation of SGR0501+4516
  29. Radio Detection of SGR 0501+4516
  30. SGR 0501+4516: MDM Optical Observations
  31. GRB 080822B, Swift-BAT refined analysis
  32. SGR 0501+4516: Astrotel-Caucasus optical observations
  33. SGR 0501+4516: UKIRT detection of possible infra-red counterpart
  34. SGR 0501+4516: WSRT Radio Observations
  35. Trigger 321551: Continued Large Flaring of SGR 0501+4516
  36. New Soft Gamma Repeater 0501+4516 (GRB 080822): GLAST Burst Monitor detection
  37. SGR 0501+4516: optical observations
  38. Swift Trigger 321481: A Large Flare from SGR 0501+4516
  39. SGR 0501+4516: Swift-BAT refined analysis of the 3 discovery events
  40. Discovery of the Spin Period of the New Soft Gamma Repeater SGR 0501+4516
  41. GRB 080822B: Swift detection of a burst
  42. Third event from SGR 0501+4516
  43. GRB 080822 (SGR 0501+4516): archival optical observations
  44. New Soft Gamma Repeater 0501+4516 was GRB 080822
  45. GRB 080822: Swift detection of a short burst
  46. Radio detection of GRB 080810 with the VLA
  47. GRB 080810: Konus-Wind and Swift/BAT joint spectral analysis
  48. GLAST Burst Monitor detection of GRB 080810
  49. GRB 080810: Swift/UVOT Refined Analysis
  50. GRB 080810: D50 optical observation
  51. GRB 080810: Kanazawa optical observation
  52. GRB 080810: Swift-XRT Team refined analysis
  53. GRB 080810: Enhanced Swift-XRT position
  54. GRB 080810: ROTSE-III Prompt Detection of Optical Counterpart
  55. GRB 080810, Swift-BAT refined analysis
  56. GRB 080810: Swift detection of a burst with a bright optical afterglow
  57. GRB 080723B: XMM-Newton observation
  58. GRB 080727B: Late VLT imaging
  59. GRB 080805: Swift-XRT Refined Analysis
  60. GRB 080805: Swift/UVOT Upper Limits
  61. GRB 080804: Swift-XRT Refined Analysis
  62. GRB 080804: Swift/UVOT Refined Analysis
  63. GRB 080805, Swift-BAT refined analysis
  64. GRB 080804, Swift-BAT refined analysis
  65. GRB 080804: Enhanced Swift-XRT position
  66. GRB 080804: Faulkes Telescope South observations
  67. GRB080805 optical limit by "Pi of the Sky"
  68. GRB 080805: Swift detection of a burst
  69. GRB 080804: Swift detection of a burst with optical afterglow
  70. GRB 080804: ROTSE-III Detection of Optical Counterpart
  71. GRB 080802: Swift/UVOT Upper Limits
  72. GRB 080802: Swift-XRT Refined Analysis
  73. GRB 080802, Swift-BAT refined analysis
  74. GRB 080802: Swift detection of a probable burst
  75. GRB 080727C: Suzaku WAM observation of the prompt emission
  76. GRB 080727C: TAROT Calern observatory optical observations
  77. GRB 080727B: GROND redshift limit
  78. GRB 080727C, Swift-BAT refined analysis
  79. GRB 080727C: Swift/UVOT Upper Limits
  80. Konus-Wind observation of GRB 080727B
  81. GRB 080727C: Swift XRT refined analysis
  82. GRB 080727C: Enhanced Swift-XRT position
  83. GRB080727C: RTT150 optical observations
  84. GRB 080727C: Swift detection of a burst
  85. Swift detection of XTE J1701-407
  86. GRB 080727B: Swift/UVOT Upper Limits
  87. BAT Trigger 318150 is not a GRB
  88. GRB 080727B: Swift-XRT refined analysis
  89. GRB 080727B, Swift-BAT refined analysis
  90. GRB 080727A, Swift-BAT refined analysis
  91. GRB 080727A: Swift-XRT refined analysis
  92. GRB080727A: Swift/UVOT Upper Limits
  93. GRB 080727B: Enhanced Swift-XRT position
  94. GRB 080727A: Enhanced Swift-XRT position
  95. GRB 080727B: Swift detection of a bright burst
  96. GRB 080727: Swift detection of a burst
  97. GRB 080725, Swift-BAT refined analysis
  98. GRB 080723A: optical upper limit
  99. GRB080723B: Swift/UVOT Upper Limits
  100. GRB 080725: Swift detection of a burst

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