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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').
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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.

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subject:"Swift"
body:"GRB"
submitter:"Judith Racusin"

4252 results found.

  1. GRB 080928: GROND DETECTION
  2. GRB 080925: Fermi GBM Detection
  3. SGR 0501+4516: preliminary results of the Suzaku ToO observation
  4. GRB 080915B, Swift-BAT refined analysis
  5. SGR 0501+4516 : P200 i-band observations
  6. GRB 080905C: Fermi GBM detection
  7. SGR J0501+4516: radio pulsar searches with GBT and WSRT
  8. Swift Trigger 324122 is again known source Swift J1842.5-1124
  9. GRB 080906: Swift detection of a burst with optical afterglow
  10. Recent VLA non-detection of SGR 0501+4516
  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. SGR 0501+4516: Detection of possible optical counterpart
  17. SGR 0501+4516: WHT observations of the possible near-infrared counterpart
  18. VLA non-detection of SGR 0501+4516
  19. Radio Detection of SGR 0501+4516: Retraction
  20. SGR 0501+4516: XMM-Newton monitoring schedule
  21. SGR 0501+4516: Decline in Activity
  22. SGR 0501+4516: Proximity to supernova remnant HB9
  23. Enhanced Swift-XRT position of SGR 0501+4516
  24. SGR 0501+4516: GMRT Radio Observation at 618 MHz
  25. SGR 0501+4516: Swift XRT measure of the spin period
  26. SGR 0501+4516: Fermi GBM (formerly GLAST Burst Monitor) observations of three exceptionally intense outbursts
  27. Soft Gamma Repeater SGR 0501+4516: GBM Detection of multiple bursts
  28. Suzaku ToO Observation of SGR 0501+4516
  29. SGR 0501+4516: radio pulsar searches with GBT and WSRT
  30. Konus-Wind observations of new SGR 0501+4516
  31. INTEGRAL ToO Observation of SGR0501+4516
  32. Radio Detection of SGR 0501+4516
  33. SGR 0501+4516: MDM Optical Observations
  34. SGR 0501+4516: Astrotel-Caucasus optical observations
  35. SGR 0501+4516: UKIRT detection of possible infra-red counterpart
  36. SGR 0501+4516: WSRT Radio Observations
  37. Trigger 321551: Continued Large Flaring of SGR 0501+4516
  38. SGR 0501+4516: optical observations
  39. Swift Trigger 321481: A Large Flare from SGR 0501+4516
  40. SGR 0501+4516: Swift-BAT refined analysis of the 3 discovery events
  41. Discovery of the Spin Period of the New Soft Gamma Repeater SGR 0501+4516
  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 080727B: Late VLT imaging
  46. Trigger 317393: Swift detection of a possible GRB
  47. Trigger 317205: Swift detection of an outburst from XTE J1701-407
  48. GRB 080710, Swift-BAT refined analysis
  49. GRB 080710: Swift detection of a burst
  50. GRB 080707: Swift detection of a burst
  51. GRB 080702B : Burst detected in BAT during Swift slew
  52. GRB 080701: Swift detection of a burst
  53. GRB 080613B: Swift detection of a burst
  54. GRB 080604: Swift detection of a burst with an optical afterglow
  55. SGR 1627-41: Chandra/RXTE/Swift Observations Scheduled
  56. Konus-Wind observation of reactivation of SGR 1627-41
  57. Reactivation of SGR 1627-41
  58. GRB 080515: KPNO 4m NIR afterglow detection
  59. GRB 080506: NAYUTA Optical Observation
  60. GRB080430: Optical observation in AsU CAS Ondrejov & Brno
  61. GRB 080426: Swift detection of a possibly short burst
  62. GRB 080413A: MOA-II optical afterglow observations
  63. GRB 080330, SMARTS optical/IR afterglow observations
  64. GRB 080319A: UVOT Observations
  65. GRB 080319C: Swift-XRT Team Refined Analysis
  66. GRB 080319C: Swift detection of a burst with an optical afterglow
  67. GRB080310: Super-LOTIS suggestion of brightening
  68. GRB080307, optical upper limit
  69. GRB 080307: retraction of UVOT candidate
  70. GRB 080303A: ROTSE-III Optical Limits
  71. GRB080229: Possible optical afterglow
  72. UVOT analysis for GRB080229
  73. GRB 080218: Swift detection of a burst
  74. GRB 080207, Swift-BAT refined analysis
  75. GRB 080207, Swift-BAT refined analysis
  76. GRB 080129: Swift-XRT refined analysis
  77. GRB 080129: Gemini-South Imaging Observations
  78. Konus-Wind observation of GRB 080122
  79. GRB 080121: Swift-BAT detection of a very weak, short burst
  80. IPN triangulation of very bright GRB 071125
  81. Disregard the "GRB 071126" position
  82. GRB 071118: Swift detection of a burst
  83. GRB 071101: Swift detection of a burst
  84. GRB 071028: Swift-XRT Team refined analysis
  85. GRB 071028: Swift detection of a burst
  86. GRB071020, optical upper limit
  87. GRB 071017: a SHORT GRB detected by INTEGRAL
  88. GRB071010B: Swift/XRT detection
  89. GRB 070911, SMARTS optical/IR afterglow observations
  90. GRB 070920B: ROTSE-III Early Optical Limits
  91. INTEGRAL ToO observations of SGR1806-20
  92. GRB 070920b, SMARTS optical observation
  93. SGR1806-20: Swift-BAT detection of enhanced activity
  94. GRB 070911: Swift XRT refined analysis
  95. GRB 070911, Swift-BAT refined analysis
  96. Intense burst from SGR 1806-20 detected on September 7
  97. GRB 070810: ROTSE-III Detection of Optical Counterpart
  98. GRB 070809: ROTSE-III Optical Limits
  99. GRB 070808: Xinglong TNT optical Upper Limit
  100. GRB070808: Optical observations with KANATA

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