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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"

23435 results found.

  1. GRB 110921A: Swift/UVOT Observations
  2. GRB 110921A: NOT observations
  3. GRB 110921A: TNT astrometry
  4. GRB 110918A: submm observations from APEX
  5. GRB 110921A: optical observations in Mt. Terskol and Maidanak observatories
  6. GRB 110921A: Enhanced Swift-XRT position
  7. GRB 110921A: Swift detection of a burst
  8. GRB 110915B : X-ray afterglow confirmation
  9. GRB 110918A: Swift/UVOT Detection of the Optical Counterpart
  10. GRB 110918A optical observation
  11. GRB 110918A: GROND detection of the afterglow candidate
  12. GRB 110918A: INT optical detection of Swift candidate afterglow
  13. GRB 110918A: Swift-XRT observations
  14. Swift detection of short bursts from PSR J1647-4552
  15. GRB 110915A: Konus-Wind and Swift/BAT joint spectral analysis
  16. IPN triangulation of GRB 110918A (long duration, extremely intense)
  17. GRB 110915B: GROND Observations of the Optical/NIR Afterglow Candidate
  18. GRB 110915A: Swift/UVOT Upper Limits
  19. GRB 110915B: Swift/UVOT Upper Limits
  20. GRB 110915A: GROND Upper limits
  21. GRB 110915B: Afterglow candidate from OSN
  22. GRB 110915A: Deep Near-IR Limits from Magellan
  23. GRB 110915B: XRT afterglow candidate
  24. GRB 110915A: Deep Gemini-South i/z-band imaging
  25. GRB110915A MITSuME Okayama J-band upper-limit
  26. GRB 110915A: MITSuME Okayama and Ishigakijima Optical upper limits
  27. GRB 110915A: NOT observations
  28. GRB 110915A: 1.23m CAHA I-band observations
  29. GRB 110915A: Enhanced Swift-XRT position
  30. GRB 110915A: GMG optical upper limit
  31. GRB 110915A: MASTER-Net early limit
  32. GRB 110915A: Swift detection of a burst
  33. GRB 110825A: Further Swift/XRT Observations
  34. GRB 110731A: SAO RAS and Terskol observations
  35. GRB 110906A(?): Burst detection (unconfirmed) from Swift-BAT slew data
  36. GRB 110905A: Swift detection of a burst
  37. GRB 110903A: Fermi GBM observation
  38. GRB 110903A: Swift/UVOT Upper Limits
  39. GRB 110903A: Swift-XRT observations
  40. GRB 110903A: a long GRB detected by INTEGRAL
  41. GRB 110820A: optical upper limit
  42. Trigger 502024: Swift detection of KS 1741-293
  43. Swift detection of an SGR burst from Swift J1834.9-0846
  44. GRB 110825A: Suzaku WAM observation of the prompt emission
  45. GRB 110825A: GMG optical observation
  46. GRB110825A: ROTSE early time optical limit
  47. GRB 110827A, Swift-BAT refined analysis
  48. GRB 110825A: optical afterglow candidate
  49. GRB 110827A: Swift detection of a burst
  50. GRB 110825A: field inspection and possible host galaxy
  51. GRB110825A: Swift target of opportunity observation
  52. IPN triangulation of GRB110825A (very intense, long-duration)
  53. Swift-BAT Trigger 501485 is noise
  54. IPN triangulation of GRB 110820B (very long duration, extremely intense)
  55. GRB 110820A: Swift/UVOT Upper Limits
  56. GRB 110820A: Position udpate + 2nd epoch data
  57. GRB 110820A: CQUEAN izY Observation
  58. GRB110820A: MITSuME Ishigakijima Optical Upper Limits
  59. GRB 110820A: Enhanced Swift-XRT position
  60. GRB 110820A: CrAO optical upper limit
  61. GRB 110820A: Swift detection of a burst
  62. GRB 110818A: Swift/UVOT Upper Limits
  63. GRB 110818A: Enhanced Swift-XRT position
  64. GRB 110818A: Optical afterglow and redshift from VLT/X-shooter
  65. GRB 110818A: Swift-XRT refined Analysis
  66. GRB 110815A: Swift-XRT and UVOT refined Analysis
  67. GRB 110818A: Swift detection of a burst
  68. IPN triangulation of GRB110815A (long, intense)
  69. GRB 110801A: Konus-Wind and Swift/BAT joint spectral analysis
  70. GRB 110801A: optical observations at Mt. Terskol observatory
  71. GRB 110812A: SuperAGILE localization of a long GRB.
  72. IPN triangulation of GRB 110808B (short/hard/intense)
  73. A new photometric resource for GRB observers
  74. RXTE Discovery of the Spin Period of Swift J1834.9-0846
  75. GRB 110808A: Swift/UVOT Detection
  76. GRB 110808A: VLT/X-shooter spectroscopy
  77. GRB 110808A: Enhanced Swift-XRT position
  78. GRB 110808A: Swift detection of a burst with optical counterpart
  79. Fermi GBM detection of a SGR-like burst
  80. GRB 110807A: SAO RAS observations
  81. GRB 110807A: Swift detection of a burst or a posible new SGR
  82. GRB 110726A: two epochs of SAO RAS optical observations
  83. IPN triangulation of GRB110802A (short/hard burst)
  84. GRB 110801A: optical observations in CrAO
  85. EVLA observation for Fermi burst GRB 110721A
  86. GRB 110801A: SAO RAS optical observations
  87. GRB110801A: MITSuME Ishigakijima Optical Observation at 1 day after the burst
  88. GRB 110801A: MASTER OT observations
  89. Swift/UVOT observations of GRB110801A
  90. GRB 110801A: Afterglow redshift from 10.4m GTC
  91. GRB110801A: MITSuME Ishigakijima Optical Observation
  92. GRB 110801A: Enhanced Swift-XRT position
  93. GRB 110801A: Swift detection of a burst with an optical counterpart
  94. GRB 110731A / EVLA upper limits
  95. GRB110731A: MITSuME Ishigakijima Optical Upper Limits
  96. GRB110731A: Swift/UVOT Observations
  97. GRB 110731A: NOT photometry
  98. GRB 110731A: Enhanced Swift-XRT position
  99. GRB 110731A: Swift detection of a burst with an optical counterpart
  100. Sw J1644+57 (GRB 110328A): Continued VLBA Observations

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