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Table 3

ICRS positions of HD 7977 from various catalogues and our own measurements based on several photographic surveys (see 3.3 for details).

RA epoch Dec epoch Source RA(s) 1h 20m Dec (arcsec) +61° 52′ RA error (s) Dec error (arcsec) Reference Used
1842.0 1842.0 Argelander(a) 31s.69 57″.7 0.01 0″.1 1 *
1875.0 1875.0 Argelander(a) 31s.69 57″.8 0.01 0″.1 2 *
1877.1 1877.1 H+G Krueger(a) 31s.95 56″.6 0.01 0″.1 3
1903.94 1903.94 VO (a) 31s.676 57″.40 0.022 0″.195 4 *
1903.94 1903.94 our VO (c) 31s.627 57″.51 0.019 0″.17 This paper *
1903.94 1903.94 our VO (c) 31s.675 57″.17 0.024 0″.15 This paper *
1929.8 1929.9 AGK2 (a) 31s.56 57″.3 0.01 0″.1 5 *
1933.69 1932.62 PPM (a) 31s.617 57″.18 0.016 0″.11 6
1943.816 1944.427 ACRS (a) 31s.597 57″.25 0.022 0″.195 7 *
1950.0 1950.0 SAO (a) 31s.482 57″.64 0.024 0″.360 8
1951.81 1951.81 AGK3U (a) 31s.586 57″.35 0.015 0″.106 9 *
1954.8 1954.8 our POSSI-E(b) 31s.5684 56″.863 0.0097 0″.043 This paper *
1954.8 1954.8 our POSSI-O(b) 31s.5530 56″.867 0.0051 0″.036 This paper *
1983.123 1983.123 FONAC(a) 31s.6095 57″.075 0.0047 0″.057 10 *
1983.9 1983.9 our Pal-QV(b) 31s.6270 56″.798 0.0038 0″.030 This paper *
1989.68 1989.02 UCAC4(a) 31s.6252 57″.061 0.0018 0″.027 11 *
1989.8 1989.8 our POSSII-J(b) 31s.5826 57″.169 0.0038 0″.016 This paper *
1991.00 1991.01 PPMX(a) 31.6539 57″.045 0.0011 0″.008 12
1991.10 1991.19 Tycho-2 (a) 31s.5956 57″.044 0.0011 0″.008 13 *
1991.8 1991.8 our POSSII-F (b) 31s.5805 57″.063 0.0027 0″.012 This paper *
1993.8 1993.8 our POSSII-N (b) 31s.5877 57″.127 0.0022 0″.008 This paper *
2000.0 2000.0 ACT (a) 31s.5929 57″.010 0.0009 0″.006 14
2003.672 2003.672 UCAC5 (a) 31.61012 57″.0661 0.00003 0″.0003 15 *
2013.550 2013.550 URAT1 (a) 31s.5924 57″.189 0.0016 0″.011 16 *
2015.0 2015.0 Gaia DR1 (a) 31s.596488 57″.07803 0.000031 0″.00030 17
2015.5 2015.5 Gaia DR2 (a) 31s.5965293 57″.0780133 0.0000032 0″.0000261 18
2016.0 2016.0 Gaia DR3 (a) 31s.5965296 57″.0779238 0.0000028 0″.0000236 19 *

Notes. The first three columns present the Right Ascension and Declination epochs, and the data source; the next four columns contain positions and their uncertainties. The eighth column gives references, and in the last column, the values we used in the proper motion estimation are marked with an asterisk. (a)Star catalogue. (b)Scanned photographic plate astrometry. (c)Measured photographic plate astrometry.

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