Strong Hα emission and signs of accretion in a circumbinary planetary mass companion from MUSE

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Volume 638 (June 2020)

A&A, 638 (2020) L6

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Table B.1.

Hα EWs of the three components, A, B, and (AB)b, in the Delorme 1 system during the observation.

UT time	EW_A, Hα	EW_B, Hα	EW_(AB)b, Hα
(hh:mm)	(Å)	(Å)	(Å)
02:55	−68.6 ± 0.3	−32.1 ± 0.1	… ^(a)
03:03	−60.3 ± 0.1	−29.7 ± 0.1	−112 ± 10
03:10	−49.9 ± 0.0	−25.0 ± 0.5	−99 ± 11
03:18	−49.5 ± 0.4	−31.6 ± 0.2	−166 ± 8
03:25	−46.1 ± 0.3	−32.0 ± 0.5	−147 ± 5
03:33	−44.7 ± 0.3	−33.7 ± 0.1	−120 ± 9
04:57	−38.1 ± 0.3	−30.6 ± 1.0	−200 ± 21
05:05	−37.9 ± 0.1	−29.4 ± 0.1	−156 ± 35
05:12	−37.2 ± 0.4	−33.4 ± 0.2	−118 ± 11
05:21	−39.3 ± 0.5	−32.7 ± 0.0	−124 ± 5
05:28	−41.8 ± 0.1	−31.8 ± 0.4	−141 ± 16
05:36	−38.5 ± 0.1	−34.8 ± 0.3	−157 ± 6

Notes. Negative values indicate emission. See Fig. B.2 for a graphical representation of this table.

^(a)

Missing value because this cube was excluded from the analysis of the companion (Sect. 2).

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