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Table 1

Observing log for the β Pic CRIRES+ observations.

Date Mode DIT NDIT Nfr ρb RVb ρc RVc BV(a)
(s) Nfr (mas) (km/s) (mas) (km/s) (km/s)
29 Nov. 2022 L3262 30 1 120 536 11.0±0.3 11 −0.4±3.9 2.44
23 Dec. 2022 L3262 30 1 120 539 11.1±0.3 23 −6.0±3.8 −0.95
23 Dec. 2022 M4318 10 6 52 539 11.1±0.3 23 −6.0±3.8 −0.95
25 Dec. 2022 L3340 30 1 120 539 11.1±0.3 29 −6.4±3.8 −1.23
31 Dec. 2022 L3426 60 1 60 539 11.1±0.3 32 −7.6±3.7 −2.08
22 Jan. 2023 M4318 10 6 56 541 11.1±0.3 54 −11.7±3.3 −4.91
15 Feb. 2023 L3340 60 1 60 544 11.2±0.3 72 −15.2±2.9 −7.13
25 Feb. 2023 M4318 10 6 56 544 11.2±0.3 81 −16.4±2.6 −7.70
27 Sep. 2023 L3340 30 1 128 557 11.4±0.3 149 −20.2±0.5 7.94
9 Oct. 2023 L3262 60 1 60 557 11.4±0.3 149 −19.8±0.5 7.52
12 Oct. 2023(b) L3426 60 1 124 557 11.4±0.3 149 −19.7±0.5 7.36
13 Oct. 2023(b) M4318 10 6 104 557 11.4±0.3 149 −19.6±0.5 7.30
1 Nov. 2023 M4318 10 6 56 558 11.4±0.3 147 −18.9±0.5 5.81

Notes. (a)Nfr: number of frames in the run. ρ: Star-planet separation. RVb and RVc: expected planet RV relative to the star for planets b and c. BV: barycentric velocity of Earth relative to β Pic.(b)Two OBs in the same mode were executed contiguously on these nights, the OB pairs are merged and count as single observations here.

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