Open Access

Table A.1

Standard ATs configurations used in VLTI/MATISSE observations of 3 Puppis.

3 Pup observation
Night | Time (UTC)
VLTI
config.
AT stations
position
Projected baseline length
B(m)
2020-02-15 100h33m01s Small A0-B2-D0-C1 Bmin = 11.26 19.89 22.54 23.31 29.36 33.80
2020-02-20 | 04h54m 13s Medium K0-G2-D0-J3 36.06 56.22 56.81 57.65 79.36 92.69
2020-02-27 | 04h08m 18s Large A0-G1-J2-J3 51.18 83.86 103.93 113.50 118.58 130.02
2024-03-10 | 00h57m35s Extended A0-B5-J2-J6 48.47 111.96 129.11 167.34 169.42 Bmax = 201.43
2024-03-10 | 04h46m33s Extended A0-B5-J2-J6 48.19 73.61 91.69 144.57 167.93 184.39

Notes. The starting observation time of 3 Puppis is given in the UTC convention and with the units of hours:minutes:seconds. Bmax and Bmin are respectively the longest and the shortest projected baseline separation lengths used during the observations. The so called ‘large’ configuration in this table refers to the old VLTI baseline configuration (config.), that is to say before the ESO call for proposal P112. The ‘extended’ baseline configuration has been offered to the community since 2023.

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