Open Access

Table 1

Summary of the SPHERE/IRDIS observations of PDS 70 used in this work, sorted by date.

Date Strategy Program Filter Coronagraph [sec] Number of frames(b) Seeing(c) [″] ΔPA(d) [°]
2015-05-06 ADI 095.C−0298(A) H23 N_ALC_YJH_S 64 16 1.25 36.0
2015-06-04 ADI 095.C−0298(B) H23 N_ALC_YJH_S 64 16 1.33 40.0
2016-03-26 PDI 096.C−0333(A) J N_ALC_YJ_S 64 35 1.83 -
2018-01-25 ADI 1100.C−0481(D) K12 N_ALC_YJH_S 96 30 1.07 95.7
2019-03-11 ADI 1100.C−0481(L) K12 N_ALC_Ks 96 16 0.7 49.0
2019-04-13 ADI 1100.C−0481(M) K12 N_ALC_YJ_S 96 15 0.53 71.3
2019-07-13 PDI 1100.C−0481(T) Ks n/a 64 [66,69](e) [0.9,0.69] -
2019-08-09 PDI 0102.C−0916(B) H N_ALC_YJH_S 64 37 1.58 -
2021-07-16 PDI 60.A−9001(S) H [N_NS_CLEAR, N_ALC YJH_S] 16 [17,49](f) [0.65,0.83] -

Notes.(a) Exposure time of OBJECT frames.(b) Number of frames in cubes.(c) Average seeing from ESO Astronomical Site Monitoring (ASM,, https://www.eso.org/asm/ui/publicLog).(d) Maximum parallactic angle variation.(e) Program split into two parts to improve image quality, due to the variation in observing conditions.(f) Program split into two parts, due to different coronagraph settings.

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