Table 1
Selection of 23 RRLs in the northern hemisphere observed with the SOPHIE spectrograph at OHP, with their mean magnitude in band V (mV), exposure time (∆t), and number of spectra acquired.
Name | mV | ∆t (s) | N | Maximum gap | Nrebound | < S/N > | Refs RV | Refs Teff | Refs photometry |
---|---|---|---|---|---|---|---|---|---|
V0341 Aql(†) | 10.89 | 900 | 13 | 0.17 | 2 | 22.0 | 35 | ||
X Ari(†) | 8.97 | 600 | 25 | 0.27 | 3 | 26.0 | 6 (⋆) | 12,13 | 21 (⋆),24 (⋆),30 (⋆),33,35 |
RS Boo(†, B) | 9.73 | 600 | 11 | 0.42 | 3 | 26.0 | 8 (⋆) | 12 (⋆),13,16 | 26 (⋆) |
RR Cet(*) | 9.15 | 600 | 10 | 0.22 | 3 | 25.0 | 9 (⋆),10 | 12,14,16 | 28 (⋆),29,30 (⋆),33 |
W CVn(‡) | 11.18 | 900 | 19 | 0.08 | 4 | 25.0 | 5 | 12 | 23,27,35 |
UY Cyg(‡) | 11.10 | 900 | 16 | 0.19 | 7 | 17.0 | 23 (⋆),27 (⋆),30 (⋆),35 | ||
DX Del(*) | 9.52 | 600 | 6 | 0.67 | 3 | 31.0 | 1,10 (⋆) | 12 (⋆),14 (⋆),15,16(⋆) | 17(⋆) ,29,30 (⋆),32,34 (⋆) |
SU Dra(‡) | 9.27 | 600 | 19 | 0.18 | 8 | 29.0 | 9,11 | 13 | 28 (⋆),30 (⋆) |
SW Dra(‡) | 10.55 | 600 | 19 | 0.12 | 7 | 22.0 | 2,7 | 12(⋆) | 19 (⋆), 25 (⋆), 30(⋆) |
RX Eri(‡) | 9.22 | 600 | 18 | 0.12 | 7 | 25.0 | 9 | 12 (⋆),14 (⋆) | 28 (⋆),30 (⋆),33,35 |
SV Eri | 9.96 | 900 | 4 | 0.62 | 0 | 24.0 | 12 | 23,30,33,35 | |
VX Her(*, B) | 11.31 | 900 | 7 | 0.56 | 4 | 28.0 | 12,14,16 | 23,27,30,35 | |
WZ Hya(*) | 10.27 | 900 | 9 | 0.43 | 3 | 16.0 | 23 | ||
RR Leo(‡) | 9.94 | 900 | 25 | 0.11 | 9 | 22.0 | 9 | 12,14 | 28,30,35 |
SS Leo(†) | 11.00 | 900 | 12 | 0.45 | 6 | 19.0 | 4 (⋆) | 22 (⋆),35 | |
TT Lyn(‡) | 9.51 | 600 | 24 | 0.09 | 7 | 33.0 | 1, 9 | 12 | 17,18,28 (⋆),30 (⋆),35 |
AV Peg(‡) | 9.87 | 600 | 22 | 0.13 | 7 | 21.0 | 9 | 12 (⋆),14 | 28 (⋆),30 (⋆),31,35 |
CG Peg | 11.13 | 900 | 2 | 0.92 | 0 | 18.0 | |||
VY Ser(†) | 9.73 | 600 | 17 | 0.18 | 4 | 24.0 | 13,15 (⋆),16 | 20,22(⋆) ,26,35,36 (⋆) | |
AB UMa(‡) | 10.88 | 900 | 18 | 0.09 | 4 | 26.0 | 27,30 (⋆) | ||
TU UMa(‡) | 9.26 | 600 | 24 | 0.09 | 7 | 32.0 | 1,9 | 12(⋆) | 17 (⋆),18 (⋆),28 (⋆),30(⋆) ,33,35 |
UU Vir(†) | 9.90 | 900 | 10 | 0.24 | 3 | 22.0 | 1,8,9 | 12,13 | 17,18,26,28,30,35 |
BN Vul(‡) | 11.13 | 900 | 23 | 0.10 | 6 | 24.0 | 23,35 |
Notes. The maximum gap and Nrebound are two criteria that we used to select RV curves that are sufficiently well covered. The three last columns list the references for the RV, effective temperature, and photometric data. Star symbols(⋆) indicate the data sets that were effectively used in the model fitting. (‡)Refers to complete RV curves, (†)to satisfactorily covered RV curves, and (*)to incomplete RV curves. (B) Indicates the stars that exhibit the Blazhko effect. The absence of any symbol indicates that there are too few observations.
References. (1) Barnes et al. (1988); (2) Cacciari et al. (1987); (3) Carney & Latham (1984); (4) Fernley et al. (1990); (5) Fernley et al. (1993); (6) Jones et al. (1987a); (7) Jones et al. (1987b); (8) Jones et al. (1988); (9) Liu & Janes (1989); (10) Meylan et al. (1986); (11) Varsavsky (1960); (12) Andrievsky et al. (2018); (13) Andrievsky et al. (2020); (14) Andrievsky et al. (2021); (15) Takeda et al. (2006); (16) Takeda (2022); (17) Barnes et al. (1988); (18) Barnes et al. (1992); (19) Cacciari et al. (1987); (20) Carney & Latham (1984); (21) Fernley et al. (1989); (22) Fernley et al. (1990); (23) Fernley et al. (1993); (24) Jones et al. (1987a); (25) Jones et al. (1987b); (26) Jones et al. (1988); (27) Layden et al. (2019); (28) Liu & Janes (1989); (29) Meylan et al. (1986); (30) Monson et al. (2017); (31) Paczyński (1965); (32) Paczyński (1966); (33) Preston & Paczynski (1964); (34) Skillen et al. (1989); (35) Sturch (1966); (36) Varsavsky (1960).
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