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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"
  1. GRB080913: Swift/UVOT Upper Limits
  2. GRB 080913: GROND photo-z
  3. GRB 080913, Swift-BAT refined analysis
  4. GRB 080913: VLT/FORS2 observations
  5. GRB 080913: REM NIR early observations
  6. GRB 080913: Enhanced Swift-XRT position
  7. GRB 080913: GROND observation of a high-z optical/NIR afterglow candidate
  8. GRB 080913: Swift detection of a burst
  9. GRB 080906: Watcher observations
  10. Swift-BAT/-XRT refined analysis on trigger 324362 (LS I +61 303)
  11. GRB 080906B: Fermi GBM detection
  12. GRB 080905C: Fermi GBM detection
  13. SGR J0501+4516: radio pulsar searches with GBT and WSRT
  14. Swift trigger 324362 (LS I +61 303 ?): XRT
  15. GRB 080905B: Photometric Redshift for the 2MASS Galaxy
  16. Swift trigger 324362 (LS I +61 303 ?)
  17. GRB080905A: Swift/UVOT Upper Limits
  18. GRB 080905B: Watcher optical detection
  19. GRB 080904: Fermi Gamma-ray Burst Monitor detection
  20. GRB 080905B: Fermi Gamma-ray Burst Monitor detection
  21. GRB 080905A: Fermi Gamma-ray Burst Monitor detection
  22. GRB 080905A: Enhanced Swift-XRT position
  23. GRB 080905A: MITSuME Akeno optical upper limits
  24. Swift Trigger 324122 is again known source Swift J1842.5-1124
  25. Swift Trigger 324116 is known source again
  26. Swift Trigger 324112 is known source Swift J1842.5-1124
  27. GRB 080906: Refined Swift/UVOT Observations
  28. GRB 080906: Swift-XRT Refined Analysis
  29. GRB 080906, Swift-BAT refined analysis
  30. GRB 080905A: optical afterglow
  31. GRB 080906: GROND observations of the optical/NIR afterglow
  32. GRB 080905B: Swift-XRT Refined Analysis
  33. GRB 080905B: Refined UVOT Analysis
  34. GRB 080905B: VLT redshift
  35. GRB 080905A: NOT and VLT observations
  36. GRB 080905B: Enhanced Swift-XRT position
  37. GRB 080905B, Swift-BAT refined analysis
  38. GRB 080905A, Swift-BAT refined analysis
  39. GRB 080906: Swift detection of a burst with optical afterglow
  40. GRB 080905A: Swift-XRT Refined Analysis
  41. GRB 080825C: Fermi GBM Spectral Analysis
  42. GRB080825C: Fermi-LAT observations
  43. GRB 080905B: Swift detection of a burst with possible optical counterpart
  44. GRB 080905: R & I-band optical observations
  45. GRB 080905: Swift detection of a probably-short burst
  46. GRB 080903: Swift/UVOT Observations
  47. GRB 080903: Swift-XRT Refined Analysis
  48. GRB 080903: Enhanced Swift-XRT position
  49. GRB 080903, Swift-BAT refined analysis
  50. GRB 080903: optical observations
  51. GRB 080903: Liverpool Telescope observations
  52. GRB 080903: Astrotel-Caucasus optical observations
  53. GRB 080903: Optical afterglow candidate
  54. GRB 080903: TAROT Calern observatory optical observations
  55. GRB 080903: ROTSE-III Optical Limits
  56. GRB 080903: Swift detection of a burst
  57. Recent VLA non-detection of SGR 0501+4516
  58. GRB 080830: Fermi Gamma-ray Burst Monitor detection
  59. SGR 0501+4516: Spin Down Rate and Inferred Dipole Magnetic Field
  60. SGR 0501+4516: preliminary results of the first XMM-Newton observation
  61. nIR observations of SGR 0501+4516
  62. INTEGRAL ToO observation of SGR0501+4516
  63. SGR 0501+4516: Confirmation of the NIR counterpart
  64. GRB080828: Swift/UVOT Upper Limits
  65. SGR 0501+4516: Detection of possible optical counterpart
  66. SGR 0501+4516: WHT observations of the possible near-infrared counterpart
  67. GRB080825B: Swift/UVOT Upper Limits
  68. GRB 080828: Swift-XRT detection of a possible X-ray afterglow
  69. Swift-BAT trigger 322590 is not a GRB
  70. VLA non-detection of SGR 0501+4516
  71. Radio Detection of SGR 0501+4516: Retraction
  72. Swift trigger 322590: BAT detection of a possible burst
  73. SGR 0501+4516: XMM-Newton monitoring schedule
  74. GRB 080828: SuperAGILE GRB Localization
  75. SGR 0501+4516: Decline in Activity
  76. SGR 0501+4516: Proximity to supernova remnant HB9
  77. Enhanced Swift-XRT position of SGR 0501+4516
  78. SGR 0501+4516: GMRT Radio Observation at 618 MHz
  79. SGR 0501+4516: Swift XRT measure of the spin period
  80. GRB080823: Fermi Gamma-ray Burst Monitor detection
  81. GRB 080824: Fermi Gamma Ray Burst Monitor detection
  82. GRB 080825B: pseudo-z= 0.83 from prompt emission spectrum
  83. Konus-Wind observation of GRB 080825B
  84. GRB080825C: GLAST Burst Monitor detection
  85. GRB 080825B: Swift-XRT team analysis
  86. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  87. Soft Gamma Repeater SGR 0501+4516: GBM Detection of multiple bursts
  88. GRB080825: Afterglow confirmation and redshift estimate
  89. Suzaku ToO Observation of SGR 0501+4516
  90. GRB 080825B - optical counterpart candidate
  91. SGR 0501+4516: radio pulsar searches with GBT and WSRT
  92. GRB 080825B: GRB Localization by SuperAGILE
  93. Konus-Wind observations of new SGR 0501+4516
  94. INTEGRAL ToO Observation of SGR0501+4516
  95. Radio Detection of SGR 0501+4516
  96. SGR 0501+4516: MDM Optical Observations
  97. GRB 080822B, Swift-BAT refined analysis
  98. SGR 0501+4516: Astrotel-Caucasus optical observations
  99. SGR 0501+4516: UKIRT detection of possible infra-red counterpart
  100. SGR 0501+4516: WSRT Radio Observations

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