Extended Data Table 1 Optical-NIR observations of the counterpart and host galaxy of GRB 211211A

From: A kilonova following a long-duration gamma-ray burst at 350 Mpc

  1. Asterisk * indicates magnitudes of the transient after subtracting the model afterglow flux as described in Methods. Magnitudes corrected for foreground galactic extinction according to AV = 0.048 mag (ref. 84). All upper limits newly published in this work are given at the 3σ level. References: (1) This work, (2)156, (3)157, (4)158, (5)159, (6)160, (7)161, (8)162, (9)163, (10)66, (11)81. This table is available in a machine-readable format in the Supplementary Information.
  2. Source data
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