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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"

37303 results found.

  1. GRB 080903: Swift-XRT Refined Analysis
  2. GRB 080903: Enhanced Swift-XRT position
  3. GRB 080903: optical observations
  4. GRB 080903: Liverpool Telescope observations
  5. GRB 080903: Astrotel-Caucasus optical observations
  6. GRB 080903: Optical afterglow candidate
  7. GRB 080903: ROTSE-III Optical Limits
  8. GRB 080903: Swift detection of a burst
  9. Recent VLA non-detection of SGR 0501+4516
  10. GRB 080830: Fermi Gamma-ray Burst Monitor detection
  11. SGR 0501+4516: Spin Down Rate and Inferred Dipole Magnetic Field
  12. SGR 0501+4516: preliminary results of the first XMM-Newton observation
  13. nIR observations of SGR 0501+4516
  14. INTEGRAL ToO observation of SGR0501+4516
  15. SGR 0501+4516: Confirmation of the NIR counterpart
  16. GRB080828: Swift/UVOT Upper Limits
  17. SGR 0501+4516: Detection of possible optical counterpart
  18. SGR 0501+4516: WHT observations of the possible near-infrared counterpart
  19. GRB080825B: Swift/UVOT Upper Limits
  20. GRB 080828: Swift-XRT detection of a possible X-ray afterglow
  21. Swift-BAT trigger 322590 is not a GRB
  22. VLA non-detection of SGR 0501+4516
  23. Radio Detection of SGR 0501+4516: Retraction
  24. Swift trigger 322590: BAT detection of a possible burst
  25. SGR 0501+4516: XMM-Newton monitoring schedule
  26. GRB 080828: SuperAGILE GRB Localization
  27. SGR 0501+4516: Decline in Activity
  28. Enhanced Swift-XRT position of SGR 0501+4516
  29. SGR 0501+4516: GMRT Radio Observation at 618 MHz
  30. SGR 0501+4516: Swift XRT measure of the spin period
  31. GRB080823: Fermi Gamma-ray Burst Monitor detection
  32. GRB 080824: Fermi Gamma Ray Burst Monitor detection
  33. Konus-Wind observation of GRB 080825B
  34. GRB080825C: GLAST Burst Monitor detection
  35. GRB 080825B: Swift-XRT team analysis
  36. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  37. Soft Gamma Repeater SGR 0501+4516: GBM Detection of multiple bursts
  38. Suzaku ToO Observation of SGR 0501+4516
  39. SGR 0501+4516: radio pulsar searches with GBT and WSRT
  40. GRB 080825B: GRB Localization by SuperAGILE
  41. Konus-Wind observations of new SGR 0501+4516
  42. INTEGRAL ToO Observation of SGR0501+4516
  43. Radio Detection of SGR 0501+4516
  44. SGR 0501+4516: MDM Optical Observations
  45. SGR 0501+4516: UKIRT detection of possible infra-red counterpart
  46. SGR 0501+4516: WSRT Radio Observations
  47. Trigger 321551: Continued Large Flaring of SGR 0501+4516
  48. New Soft Gamma Repeater 0501+4516 (GRB 080822): GLAST Burst Monitor detection
  49. SGR 0501+4516: optical observations
  50. Swift Trigger 321481: A Large Flare from SGR 0501+4516
  51. SGR 0501+4516: Swift-BAT refined analysis of the 3 discovery events
  52. Discovery of the Spin Period of the New Soft Gamma Repeater SGR 0501+4516
  53. GRB 080822B: Swift detection of a burst
  54. GRB080818B: GLAST Burst Monitor detection
  55. Third event from SGR 0501+4516
  56. New Soft Gamma Repeater 0501+4516 was GRB 080822
  57. GRB 080822: Swift detection of a short burst
  58. GLAST Burst Monitor detection of a GRB: 080816B
  59. GLAST Burst Monitor detection of GRB 080818
  60. GLAST Burst Monitor detection of GRB080817B
  61. GLAST Burst Monitor detection of GRB 080817
  62. GLAST Burst Monitor detection of GRB080816
  63. GRB080810 - optical observations
  64. GRB080810: optical observations
  65. GLAST Burst Monitor detection of GRB 080812
  66. Radio detection of GRB 080810 with the VLA
  67. GRB 080810: Konus-Wind and Swift/BAT joint spectral analysis
  68. GLAST Burst Monitor detection of GRB 080810
  69. GRB 080810: Liverpool and Faulkes North observations
  70. GRB 080810: RTT150 optical observations
  71. GRB080810: MITSuME optical observation
  72. GRB 080810: Swift/UVOT Refined Analysis
  73. GRB 080810: optical observations
  74. GRB 080810: Liverpool Telescope observations
  75. GRB 080810: Kanazawa optical observation
  76. GRB 080810: OSN follow-up
  77. GRB 080810: Observations from NOT
  78. GRB 080810: Swift-XRT Team refined analysis
  79. GRB 080810: Enhanced Swift-XRT position
  80. GRB 080810: KANATA optical-NIR observation, update
  81. GRB 080810: ROTSE-III Prompt Detection of Optical Counterpart
  82. GRB 080810: Keck/HIRES Spectroscopy
  83. GRB 080810 : optical observation with KANATA
  84. GRB 080810: Swift detection of a burst with a bright optical afterglow
  85. GRB 080723B: GROND upper limits
  86. GRB 080723B: XMM-Newton observation
  87. GRB 080805: VLT redshift update
  88. GRB 080805: Faulkes Telescope South optical observations
  89. GRB 080804: GROND observations
  90. GRB 080727B: Late VLT imaging
  91. GRB 080805: Swift-XRT Refined Analysis
  92. GRB 080805: Swift/UVOT Upper Limits
  93. GRB 080804: Swift-XRT Refined Analysis
  94. GRB 080804: Swift/UVOT Refined Analysis
  95. GRB 080804: Enhanced Swift-XRT position
  96. GRB080804: Gemini South redshift confirmation
  97. GRB 080804: Faulkes Telescope South observations
  98. GRB080805 optical limit by "Pi of the Sky"
  99. GRB 080805: VLT redshift
  100. GRB 080805: GROND detection of possible afterglow

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