Table A.2
Observations of the NaCo-ISPY PPD targets.
Target | Obs. date [yyyy-mm-dd] | Seeing(a) [″] | Airmass (min/max) | Field rot. [°] | AGPM | PSF stab. [%] | DIT(b) [s] | ToT(c) [min] | Comments(e) |
---|---|---|---|---|---|---|---|---|---|
V* V892 Tau | 2016-12-10 | 1.9 ± 0.5 | 1.7/2.3 | 50 | y | 13.4 | 0.35 | 130.6 | (1) |
HD 283571 | 2016-12-09 | 1.3 ± 0.4 | 1.7/2.0 | 42 | y | 7.0 | 0.35 | 104.4 | (1) |
V* HL Tau | 2018-10-19 | 0.7 ± 0.1 | 1.4/1.7 | 45 | y | 4.5 | 0.35 | 93.3 | (1) |
HD 31648 | 2017-11-01 | 0.8 ± 0.1 | 1.7/2.3 | 66 | y | 9.0 | 0.35 | 168.0 | |
HD 34282 | 2016-11-07 | 0.7 ± 0.2 | 1.0/1.2 | 118 | y | 4.6 | 0.25 | 135.4 | |
HD 35187 | 2019-01-15 | 0.7 ± 0.2 | 1.5/1.9 | 56 | y | 10.2 | 0.35 | 114.9 | |
HD 36112 | 2019-01-16 | 0.6 ± 0.1 | 1.6/1.8 | 63 | y | 2.0 | 0.35 | 131.8 | (1) |
HD 36910 | 2018-11-27 | 0.5 ± 0.1 | 1.5/2.0 | 69 | y | 1.9 | 0.35 | 175.6 | |
HD 37411 | 2017-11-02 | 0.6 ± 0.1 | 1.1/1.1 | 69 | y | 4.1 | 0.35 | 84.0 | |
HD 37806 | 2017-10-30 | 0.8 ± 0.2 | 1.1/1.2 | 55 | y | 5.1 | 0.35 | 78.8 | |
HD 38120 | 2017-10-29 | 0.5 ± 0.1 | 1.1/1.1 | 66 | y | 2.8 | 0.35 | 84.0 | |
V* NX Pup | 2018-02-22 | 0.5 ± 0.1 | 1.1/1.3 | 78 | y | 2.1 | 0.3 | 130.0 | |
HD 58647 | 2018-02-23 | 0.6 ± 0.1 | 1.0/1.2 | 126 | y | 4.1 | 0.3 | 123.5 | |
HD 72106 | 2016-12-12 | 0.6 ± 0.1 | 1.0/1.2 | 130 | n | 3.8 | 0.2 | 89.5 | |
V* TW Hya | 2016-05-03 | 0.8 ± 0.3 | 1.0/1.1 | 135 | y | 4.1 | 0.35 | 106.2 | (4) |
HD 97048 | 2016-05-02 | 0.6 ± 0.1 | 1.7/1.8 | 68 | y | 5.6 | 0.35 | 151.7 | |
HD 100453 | 2016-05-09 | 2.4 ± 0.6 | 1.2/1.3 | 85 | y | 13.4 | 0.25 | 97.5 | |
HD 100546 | 2017-03-15 | 0.8 ± 0.3 | 1.4/1.5 | 64 | y | 2.2 | 0.25 | 110.4 | (2) |
HD 101412 | 2017-03-17 | 0.7 ± 0.2 | 1.2/1.3 | 74 | y | 10.8 | 0.3 | 132.5 | (2) |
HD 104237 | 2017-05-16 | 1.0 ± 0.2 | 1.7/2.0 | 52 | y | 4.8 | 0.35 | 152.3 | |
PDS 70 | 2016-06-01 | 0.4 ± 0.1 | 1.0/1.2 | 84 | n | 5.3 | 0.2 | 61.7 | |
HD 139614 | 2017-05-01 | 0.6 ± 0.3 | 1.1/1.2 | 102 | y | 4.0 | 0.35 | 98.6 | (1) |
HD 141569 | 2019-04-13 | 0.6 ± 0.1 | 1.1/1.2 | 107 | y | 2.8 | 0.35 | 130.1 | |
V* IM Lup | 2017-05-15 | 1.2 ± 0.2 | 1.0/1.1 | 120 | n | 5.9 | 0.2 | 78.5 | |
HD 142666 | 2019-05-20 | 1 .1 ± 0.4 | 1.0/1.0 | 149 | y | 4.6 | 0.35 | 40.3 | |
HD 142527 | 2017-05-17 | 1.0 ± 0.2 | 1.1/1.2 | 108 | y | 8.0 | 0.35 | 129.5 | |
HD 143006 | 2019-04-12 | 0.9 ± 0.2 | 1.0/1.2 | 162 | y | 3.7 | 0.35 | 114.3 | |
V* MY Lup | 2018-06-04 | 1.0 ± 0.2 | 1.0/1.2 | 114 | n | 7.1 | 0.2 | 100.8 | |
2MASS J1604 | 2016-05-31 | 0.8 ± 0.1 | 1.0/1.1 | 147 | n | 6.3 | 0.2 | 65.0 | (2), (3) |
HD 144432 | 2019-05-19 | 1.0 ± 0.1 | 1.0/1.1 | 165 | y | 6.2 | 0.35 | 67.7 | (2) |
TYC 7851 | 2018-06-06 | 0.6 ± 0.1 | 1.0/1.1 | 111 | n | 3.4 | 0.2 | 76.8 | |
HD144668 | 2017-06-16 | 0.7 ± 0.1 | 1.0/1.1 | 61 | y | 18.6 | 0.35 | 53.7 | (2) |
HD 145263 | 2019-05-25 | 1 .1 ± 0.1 | 1.0/1.0 | 179 | n | 3.2 | 0.2 | 45.4 | (5) |
Elias 2-27 | 2019-04-14 | 0.4 ± 0.1 | 1.0/1.2 | 192(d) | n | 6.8 | 0.2 | 63.3 | (1) |
WLY 2-48 | 2016-07-31 | 0.6 ± 0.1 | 1.0/1.1 | 55 | y | 4.5 | 0.35 | 63.0 | (2) |
EM* AS209 | 2019-07-20 | 0.8 ± 0.2 | 1.0/1.3 | 135 | n | 1.8 | 0.2 | 152.0 | (1) |
HD 152404 | 2019-05-18 | 0.8 ± 0.1 | 1.0/1.2 | 95 | y | 5.6 | 0.35 | 79.9 | |
V* KK Oph | 2016-08-01 | 0.5 ± 0.1 | 1.0/1.1 | 171 | y | 5.1 | 0.35 | 98.6 | |
HD 158643 | 2019-06-24 | 0.8 ± 0.1 | 1.0/1.0 | 168 | y | 12.5 | 0.3 | 46.0 | |
HD 163296 | 2019-07-13 | 0.5 ± 0.1 | 1.0/1.0 | 151(d) | y | 3.0 | 0.35 | 48.4 | |
HD 319139 | 2016-05-03 | 0.5 ± 0.2 | 1.0/1.1 | 161 | y | 28.4 | 0.35 | 106.2 | |
HD 169142 | 2017-05-18 | 0.6 ± 0.1 | 1.0/1.2 | 107 | y | 3.7 | 0.35 | 109.7 | |
V* R CrA | 2018-06-06 | 0.6 ± 0.1 | 1.0/1.2 | 120 | y | 22.8 | 0.1082 | 47.5 | |
V* T CrA | 2017-05-15 | 1.2 ± 0.2 | 1.0/1.1 | 122 | y | 4.7 | 0.35 | 106.8 | |
HD 179218 | 2016-05-02 | 0.8 ± 0.3 | 1.3/1.6 | 64 | y | 3.0 | 0.35 | 126.1 |
Notes.(a) DIMM (Differential Image Motion Monitor) seeing.(b) DIT = Detector integration time, i.e., exposure time per image frame.(c) ToT = Time on Target.(d) Passage through the sky region around zenith not accessible to the VLT telescopes.(e) (1) Only unsaturated PSF frames taken at the beginning of the observing sequence were used; (2) Only unsaturated PSF frames taken at the end of the observing sequence were used; (3) The first 21 cubes were not used; (4) only 2 quadrants before and after the observing sequence were used; (5) one cube was removed from the unsaturated PSF sequence because the star was not well-centered in the quadrant. (f) 2MASS J16042165–2130284. (g)TYC 7851–810–1.
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