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Table A.1

OC residuals for RS Puppis.

JD E OC W Reference
−2.4 × 106 [d]

15 050.6 977 85.1 1 Innes & Gill (1903)
15 424.6 968 85.7 1 Gerasimovic (1927)
16 830.1 934 80.5 1 Gerasimovic (1927)
18 277.9 899 76.2 1 Gerasimovic (1927)
19 723.4 864 69.5 1 Gerasimovic (1927)
20 963.2 834 64.6 1 Gerasimovic (1927)
22 824.1 789 58.5 1 Gerasimovic (1927)
26 006.61 712 46.24 1 Voûte (1939)
26 379.42 703 45.64 1 Voûte (1939)
26 752.55 694 45.36 1 Voûte (1939)
27 042.15 687 44.53 1 Voûte (1939)
27 456.32 677 43.80 1 Voûte (1939)
278 28.94 668 43.01 1 Voûte (1939)
28 201.64 659 42.30 1 Voûte (1939)
34 451.700 508 27.366 1 Eggen et al. (1957)
34 533.607 506 26.293 2 Walraven et al. (1958)
34 864.914 498 25.680 2 Eggen et al. (1957)
35 196.511 490 25.357 1 Irwin (1961)
37 513.865 434 19.271 3 Westerlund (1963)
37 638.297 431 19.233 3 Mitchell et al. (1964)
40 701.394 357 12.070 3 Pel (1976)
40 949.305 351 11.041 3 Pel (1976)
41 405.313 340 10.659 1 Dean et al. (1977)
41 735.214 332 8.640 2 Madore (1975)
41 776.643 331 8.579 3 Dean et al. (1977)
42 065.736 324 7.242 3 Dean et al. (1977)
42 438.472 315 6.568 2 Dean et al. (1977)
44 055.085 276 5.071 2 Harris (1980)
44 428.140 267 4.716 1 Moffett & Barnes (1984)
44 967.089 254 4.295 3 Moffett & Barnes (1984)
47 951.011 182 0.937 3 ESA (1997)
48 240.973 175 0.469 3 ESA (1997)
48 448.945 170 0.991 3 ESA (1997)
48 739.114 163 0.730 3 ESA (1997)
49 111.661 154 0.133 1 AAVSO
49 360.599 148 0.135 1 Walker & Williams
49 527.027 144 0.333 1 AAVSO
49 817.467 137 0.343 3 Berdnikov (1995, 2008)
50 108.216 130 0.662 3 Bersier (2002)
50 357.203 124 0.709 3 Berdnikov (1995, 2008)
50 522.961 120 0.507 3 Bersier (2002)
50 564.680 119 0.736 1 Berdnikov (1995, 2008)
51 270.917 102 1.643 1 Berdnikov (1995, 2008)
51 644.316 93 1.632 2 Berdnikov (1995, 2008)
51 976.659 85 2.055 3 Berdnikov (1995, 2008)
52 350.347 76 2.333 3 Berdnikov (1995, 2008)
52 640.475 69 2.031 3 Berdnikov (1995, 2008)
52 681.984 68 2.050 3 Pojmanski (2002)
53 014.205 60 2.351 2 Berdnikov (1995, 2008)
53 055.383 59 2.039 3 Pojmanski (2002)
53 096.193 58 1.359 3 Berdnikov (1995, 2008)
53 551.918 47 0.694 2 Tabur
53 842.397 40 0.743 2 AAVSO
53 842.461 40 0.807 3 Tabur
53 842.495 40 0.841 2 Pojmanski (2002)
5 4091.419 34 0.825 3 present work
54 132.197 33 0.113 3 AAVSO
54 215.229 31 0.165 3 Tabur
54 215.264 31 0.200 3 Pojmanski (2002)
54 505.241 24 0.253 3 Pojmanski (2002)
54 546.574 23 0.410 3 Tabur
54 546.611 23 0.373 3 AAVSO
54 588.094 22 0.380 2 present work
54 837.503 16 0.089 3 Pojmanski (2002)
54 878.846 15 0.058 2 AAVSO
55 127.522 9 0.322 1 Pojmanski (2002)
55 252.067 6 0.247 2 AAVSO
55 252.640 −6 −0.241 3 Kervella et al. (2014)
55 293.713 5 0.091 2 present work
55 335.074 4 0.220 3 present work
55 501.254 0 0.000 3 present work
55 625.868 3 0.144 2 AAVSO
56 041.317 13 0.693 3 AAVSO
56 373.179 21 0.635 3 AAVSO

Notes. JD is the heliocentric moment of maximum brightness. E is the epoch number as calculated from the ephemeris C = 2 455 501.254 + 41.49 × E. W is the weight assigned to the OC value (1, 2, or 3 depending on the quality of the light curve). The symbol in the references indicates unpublished data.

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