TITLE: GCN CIRCULAR NUMBER: 29834 SUBJECT: GRB 210419C: Swift detection of a burst DATE: 21/04/20 00:45:40 GMT FROM: Michael Moss at George Washington U M. J. Moss (GWU), V. D'Elia (SSDC & INAF-OAR), C. Gronwall (PSU), J.D. Gropp (PSU), J. A. Kennea (PSU), N. J. Klingler (PSU), N. P. M. Kuin (UCL-MSSL), S. Laha (GSFC/UMBC/CRESST), A. Y. Lien (GSFC/UMBC), F. E. Marshall (NASA/GSFC), M. H. Siegel (PSU) and A. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 23:27:49 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 210419C (trigger=1044236). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 212.968, 35.999 which is RA(J2000) = 14h 11m 52s Dec(J2000) = +35d 59' 56" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). Currently, we only have limited BAT light curve data. The available light curve from ~T+110 s to ~T+400 s does not show any significant structure. Due to lack of data, we do not have an accurate XRT position. However our current best estimate for the GRB position is RA/Dec(J2000) = 212.96009, +36.0096, which is equivalent to: RA(J2000): 14h 11m 50.4s Dec(J2000): 36d 00m 34.6s Uncertainty of this position is unclear. We await ground processed data to report an accurate position for this GRB. UVOT took a finding chart exposure of ​95​ seconds with the ​U​ filter starting​ around 340 ​seconds after the BAT trigger. No credible afterglow candidate has been found in the initial data products. The 2.7'x2.7' sub-image covers 100% of the XRT error circle. The typical 3-sigma upper limit has been about 19.6 mag. The 8'x8' region for the list of sources generated on-board covers 100% of the XRT error circle. The list of sources is typically complete to about 18 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.0​1​. Burst Advocate for this burst is M. J. Moss (mikejmoss3 AT gmail.com). Please contact the BA by email if you require additional information regarding Swift followup of this burst. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone (see Swift TOO web site for information: http://www.swift.psu.edu/)