{
  "bibcode": "2019GCN.25589....1D",
  "body": "A. de Ugarte Postigo (HETH/IAA-CSIC and DARK/NBI), M. Bremer (IRAM), D. \nA. Kann (HETH/IAA-CSIC), S. Schulze (Weizmann), C. C. Thoene, M. Blazek, \nK. Bensch, J. F. Agui (all HETH/IAA-CSIC), L. Izzo (DARK/NBI), D. A. \nPerley (LJMU), S. Martin (ALMA), I. de Gregorio-Monsalvo (ESO), M. \nMichalowski (AOI-AMU), D. B. Malesani (DARK/NBI, DAWN/NBI) R. \nSanchez-Ramirez (INAF-IAPS) report:\n\nWe observed the afterglow of GRB 190829A (Fermi GBM team, GCN #25551; \nDichiara et al., GCN #25552), at a redshift of z = 0.0785 (Valeev et al. \nGCN #25565) with NOEMA at 90 GHz. Observations started at 01:26 UT on 31 \nAugust, 29.48 hrs after the GRB. The afterglow is well detected and had \na flux density of 6.3 mJy at 90 GHz.\n\nWe derive the following refined coordinates for the afterglow:\n\nRA. (J2000): 02:58:10.510\nDec (J2000): -08:57:28.44\n\nwith an error of +/- 0\".1.",
  "circularId": 25589,
  "createdOn": 1567263695000,
  "email": "kann@iaa.es",
  "subject": "GRB 190829A: NOEMA detection of the mm afterglow",
  "submitter": "Alexander Kann at IAA-CSIC  <kann@iaa.es>",
  "eventId": "GRB 190829A"
}