Table A.1
O−C residuals for RS Puppis.
JD⊙ | E | O−C | 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 O−C 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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