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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"

22913 results found.

  1. GRB 080129: GROND detection in all bands, and fading
  2. GRB 080129: GROND detection of the optical/NIR afterglow, and fading
  3. GRB 080129: Enhanced Swift-XRT position
  4. GRB 080129: Gemini-South Imaging Observations
  5. GRB 080129 (?): UVOT Upper Limits
  6. GRB 080129 (?): Swift detection of a possible burst
  7. GRB 080121: Upper limit on X-ray afterglow
  8. GRB 080121: Swift/UVOT upper limits
  9. SNe 2008D and 2007uy: Chandra Detections
  10. GRB 080121: Enhanced Swift-XRT position
  11. IPN triangulation of GRB080122
  12. GRB 080121: Nearby SDSS galaxies
  13. GRB 080121: Swift-BAT detection of a very weak, short burst
  14. GRB 080123: Swift/UVOT refined analysis
  15. GRB 080123: Enhanced Swift-XRT position
  16. GRB 080123: Swift detection of a short burst
  17. GRB 080120: GROND confirmation of the optical afterglow
  18. VLA radio upper limit on GRB 080120
  19. UVOT detection of GRB080120
  20. GRB080120: Swift XRT position
  21. GRB 080120: a long GRB detected by INTEGRAL
  22. Transient XRF 080109 / SN 2008D: Mount Abu NIR observations
  23. NGC 2770B has the same redshift as NGC 2770
  24. Swift UVOT Monitoring of the SN 2008D Brightening (Transient in NGC 2770)
  25. XRF 080109 / SN 2008D: UKIRT JHK imaging
  26. optical observations, XRT in NGC 2770
  27. XRF 080109/SN 2008D: PROMPT Optical Imaging
  28. Gemini-South observations of XRF 080109 / SN 2008D
  29. Swift observations of the X-ray transient in NGC 2770 (aka SN2008D)
  30. Discovery of Radio Emission from Transient in NGC 2770
  31. XRF 080109 in NGC2770: NIR observations at TNG
  32. XRB 080109/SN 2008D: Early decline in brightness and change in colors
  33. XRB 080109/SN 2008D:PAIRITEL NIR observations and t_0 from Swift
  34. XRF 080109 in NGC2770: Detectable Superluminal Motion
  35. Spectroscopic classification of SN 2008D (Transient in NGC 2770)
  36. Refined Swift-XRT analysis of the transient in NGC 2770
  37. Refined Swift UVOT Analysis of SN 2008D (Transient in NGC 2770)
  38. Early OT detection of XRF in NGC 2770 in Asiago frames
  39. Possible XRF in NGC 2770 - NOT observations of the optical counterpart
  40. Bright X-ray Transient in NGC 2770 - A low-luminosity XRF?
  41. GRB 071227: optical afterglow
  42. Further Swift-BAT analysis of GRB 071227
  43. Konus-Wind observation of GRB 071227
  44. GRB 071227: Swift-XRT refined analysis
  45. GRB 071227: VLT probable redshift of the candidate host galaxy
  46. GRB 071227: Magellan observations
  47. GRB071227: Swift/UVOT refined analysis
  48. GRB 071227: REM NIR and Optical observations
  49. GRB 071227: Swift detection of a burst
  50. GRB 070429B: Possible UVOT Detection of an Optical Afterglow
  51. GRB 071208?: Swift detection of a possible burst
  52. GRB 071125: Suzaku WAM observation of the prompt emission
  53. GRB 070429B: Probable host galaxy and redshift
  54. GRB 071129, Swift-BAT refined analysis
  55. GRB 071129: Swift detection of a burst
  56. Konus-Wind and Konus-A observations of GRB 071125
  57. IPN triangulation of very bright GRB 071125
  58. GRB 071126: Enhanced Swift-XRT position
  59. GRB071122: Swift/UVOT Observations
  60. GRB071104: NIR Afterglow Candidate at TNG
  61. GRB 071122 Swift-XRT refined analysis
  62. GRB 071122: P60 Optical Afterglow Candidate
  63. GRB 071122: ROTSE-III Optical Limits
  64. GRB 071122: Swift detection of a burst
  65. GRB 071118: P60 Observations
  66. GRB071118 MITSuME OAO optical observation
  67. GRB 071118: Observations from OSN
  68. GRB 071117: VLT observations and probable redshift
  69. Swift/UVOT observations of GRB071118
  70. Swift XRT follow-up observations of GRB071008
  71. Swift/UVOT upper limits for GRB 071117
  72. GRB071118: Swift XRT refined analysis
  73. GRB 071117: Gemini Optical Afterglow Discovery
  74. GRB 071118, Swift-BAT refined analysis
  75. GRB 071117: TAROT La Silla observatory optical observations
  76. GRB 071112B: Gemini Image Differencing
  77. GRB 071118: Swift detection of a burst
  78. GRB 071117: Gemini Observations
  79. VLT FORS2 observations of short hard GRB071112B
  80. GRB 071117: Initial Swift/UVOT observations
  81. GRB 071117: Swift detection of a bright burst
  82. Swift detection of MXB 0656-072
  83. GRB 071112C: Optical and NIR data observed with KANATA
  84. GRB 071112C MITSuME Akeno early optical observation
  85. GRB 071112C: SARA upper limit
  86. GRB 071112C : Second Epoch Lulin R-band observations
  87. GRB071112C MITSuME Okayama Optical Observation
  88. GRB 071112C: Swift-BAT refined analysis
  89. GRB 071112C: Swift XRT refined analysis
  90. GRB 071112C: Optical observations at Crni Vrh
  91. Swift UVOT upper limits of GRB071112B
  92. GRB 071112B: Gemini Optical Imaging
  93. GRB 071112B: Swift-XRT preliminary analysis
  94. GRB 071112C: Palomar Pre-Imaging
  95. GRB 071112C : Lulin R-band observation
  96. GRB 071112C: TAROT Calern observatory optical observations
  97. Swift XRT follow-up observations of GRB071028B
  98. GRB071112C Xinglong_TNT_and_EST_afterglow observations
  99. GRB 071112C: Optical and NIR afterglows observed with KANATA
  100. GRB 071112B: ROTSE-III Rapid Optical Limits

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