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Table 2.

Log of the observations of Gaia BH3 (LS II +14 13) and the interferometric calibrator (BD+08 4132) with GRAVITY.

Starting UT date MJD Target Cal/ Obj/ Exp. Instrumental setup AM σ τ0
−60000 Sci Sky (s) (Res, Pol, Mode) (″) (ms)
2024-06-03T08:09:17 464.3400 LS II +14 13 Sci (OSOO) 389 Med, Split, Single 1.32 0.51 3.5
2024-06-03T08:49:05 464.3678 BD+08 4132 Cal (SO) 389 Med, Split, Single 1.31 0.29 2.6
2024-06-23T07:33:20 484.3150 LS II +14 13 Sci OSOO 376 Med, Comb, Single 1.41 0.54 2.3
2024-06-23T08:10:10 484.3406 BD+08 4132 Cal SO 376 Med, Comb, Single 1.41 0.73 2.3
2024-06-23T08:30:14 484.3545 LS II +14 13 Sci (O)SOOO 414 High, Comb., Single 1.61 0.58 2.3
2024-06-23T09:14:18 484.3851 BD+08 4132 Cal OS 414 High, Comb, Single 1.81 0.78 2.3
2024-07-18T06:16:05 509.2614 LS II +14 13 Sci OSOO 376 Med, Comb, Dual 1.45 0.32 7.5
2024-07-18T06:52:52 509.2868 BD+08 4132 Cal OS 376 Med, Comb, Single 1.51 0.49 5.4

Notes. The listed exposure time “Exp.” is the shutter-open time for one object (O) or sky (S) series. The data files in parentheses are affected by instrumental problems (see Sect. 2 and App. A). The instrumental setup includes the spectral resolution (medium or high), the polarization (split or combined), and the field configuration (single or dual). The term “AM” refers to the airmass, σ to the DIMM seeing, and τ0 to the coherence time.

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