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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"

28049 results found.

  1. GRB 080905C: Fermi GBM detection
  2. SGR J0501+4516: radio pulsar searches with GBT and WSRT
  3. Swift trigger 324362 (LS I +61 303 ?)
  4. GRB080905A: Swift/UVOT Upper Limits
  5. GRB 080905B: Watcher optical detection
  6. GRB 080904: Fermi Gamma-ray Burst Monitor detection
  7. GRB 080905B: Fermi Gamma-ray Burst Monitor detection
  8. GRB 080905A: Fermi Gamma-ray Burst Monitor detection
  9. GRB 080905A: MITSuME Akeno optical upper limits
  10. GRB 080906: Refined Swift/UVOT Observations
  11. GRB 080906: Swift-XRT Refined Analysis
  12. GRB 080906, Swift-BAT refined analysis
  13. GRB 080905A: optical afterglow
  14. GRB 080906: GROND observations of the optical/NIR afterglow
  15. GRB 080905B: Refined UVOT Analysis
  16. GRB 080905B: VLT redshift
  17. GRB 080905A: NOT and VLT observations
  18. GRB 080905B: Enhanced Swift-XRT position
  19. GRB 080905B, Swift-BAT refined analysis
  20. GRB 080905A, Swift-BAT refined analysis
  21. GRB 080906: Swift detection of a burst with optical afterglow
  22. GRB 080905A: Swift-XRT Refined Analysis
  23. GRB080825C: Fermi-LAT observations
  24. GRB 080905B: Swift detection of a burst with possible optical counterpart
  25. GRB 080905: Swift detection of a probably-short burst
  26. GRB 080903: Swift/UVOT Observations
  27. GRB 080903: Swift-XRT Refined Analysis
  28. GRB 080903: Enhanced Swift-XRT position
  29. GRB 080903, Swift-BAT refined analysis
  30. GRB 080903: optical observations
  31. GRB 080903: Liverpool Telescope observations
  32. GRB 080903: Optical afterglow candidate
  33. GRB 080903: TAROT Calern observatory optical observations
  34. GRB 080903: Swift detection of a burst
  35. GRB 080830: Fermi Gamma-ray Burst Monitor detection
  36. SGR 0501+4516: Spin Down Rate and Inferred Dipole Magnetic Field
  37. SGR 0501+4516: preliminary results of the first XMM-Newton observation
  38. nIR observations of SGR 0501+4516
  39. SGR 0501+4516: Confirmation of the NIR counterpart
  40. GRB080828: Swift/UVOT Upper Limits
  41. SGR 0501+4516: Detection of possible optical counterpart
  42. GRB080825B: Swift/UVOT Upper Limits
  43. GRB 080828: Swift-XRT detection of a possible X-ray afterglow
  44. VLA non-detection of SGR 0501+4516
  45. Swift trigger 322590: BAT detection of a possible burst
  46. GRB 080828: SuperAGILE GRB Localization
  47. Enhanced Swift-XRT position of SGR 0501+4516
  48. SGR 0501+4516: GMRT Radio Observation at 618 MHz
  49. GRB080823: Fermi Gamma-ray Burst Monitor detection
  50. GRB 080824: Fermi Gamma Ray Burst Monitor detection
  51. Konus-Wind observation of GRB 080825B
  52. GRB080825C: GLAST Burst Monitor detection
  53. GRB 080825B: Swift-XRT team analysis
  54. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  55. Suzaku ToO Observation of SGR 0501+4516
  56. SGR 0501+4516: radio pulsar searches with GBT and WSRT
  57. GRB 080825B: GRB Localization by SuperAGILE
  58. Radio Detection of SGR 0501+4516
  59. GRB 080822B, Swift-BAT refined analysis
  60. SGR 0501+4516: Astrotel-Caucasus optical observations
  61. SGR 0501+4516: UKIRT detection of possible infra-red counterpart
  62. New Soft Gamma Repeater 0501+4516 (GRB 080822): GLAST Burst Monitor detection
  63. SGR 0501+4516: optical observations
  64. SGR 0501+4516: Swift-BAT refined analysis of the 3 discovery events
  65. Discovery of the Spin Period of the New Soft Gamma Repeater SGR 0501+4516
  66. GRB080818B: GLAST Burst Monitor detection
  67. GRB 080822: Swift detection of a short burst
  68. GLAST Burst Monitor detection of a GRB: 080816B
  69. GLAST Burst Monitor detection of GRB 080818
  70. GLAST Burst Monitor detection of GRB080817B
  71. GLAST Burst Monitor detection of GRB 080817
  72. GLAST Burst Monitor detection of GRB080816
  73. GRB080810 - optical observations
  74. GLAST Burst Monitor detection of GRB 080812
  75. Radio detection of GRB 080810 with the VLA
  76. GRB 080810: Konus-Wind and Swift/BAT joint spectral analysis
  77. GLAST Burst Monitor detection of GRB 080810
  78. First GLAST Burst Monitor GRB Circulars
  79. GRB 080810: Swift/UVOT Refined Analysis
  80. GRB 080810: Liverpool Telescope observations
  81. GRB 080810: Kanazawa optical observation
  82. GRB 080810: OSN follow-up
  83. GRB 080810: Swift-XRT Team refined analysis
  84. GRB 080810: Enhanced Swift-XRT position
  85. GRB 080810: KANATA optical-NIR observation, update
  86. GRB 080810: ROTSE-III Prompt Detection of Optical Counterpart
  87. GRB 080810, Swift-BAT refined analysis
  88. GRB 080810 : optical observation with KANATA
  89. GRB 080810: Swift detection of a burst with a bright optical afterglow
  90. GRB 080723B: GROND upper limits
  91. GRB 080723B: XMM-Newton observation
  92. GRB 080805: Faulkes Telescope South optical observations
  93. GRB 080804: GROND observations
  94. GRB 080727B: Late VLT imaging
  95. GRB 080805: Swift-XRT Refined Analysis
  96. GRB 080805: Swift/UVOT Upper Limits
  97. GRB 080804: Swift-XRT Refined Analysis
  98. GRB 080804: Swift/UVOT Refined Analysis
  99. GRB 080805, Swift-BAT refined analysis
  100. GRB 080804, Swift-BAT refined analysis

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