J/ApJS/141/503      Radial Velocities for 889 late-type stars  (Nidever+, 2002)

Radial velocities of 889 late-type stars Nidever D.L., Marcy G.W., Butler R.P., Fischer D.A., Vogt S.S. <Astrophys. J. Suppl. Ser. 141, 503 (2002)> =2002ApJS..141..503N 2002ApJS..141..503N
ADC_Keywords: Stars, late-type ; Radial velocities Keywords: stars: fundamental parameters; late-type; kinematics - techniques: radial velocities; spectroscopic - catalogs: binaries: spectroscopic Abstract: We report radial velocities for 844 FGKM-type main sequence and subgiant stars and 45 K giants, most of which had either low-precision velocity measurements or none at all. These velocities differ from the standard stars of Udry et al. (1999IAUCo.170..354U 1999IAUCo.170..354U) by 0.035km/s (RMS) for the 26 FGK standard stars in common. The zero-point of our velocities differs from that of Udry et al.: <Vpresent-VUdry≥+0.053km/s. Thus these new velocities agree with the best known standard stars both in precision and zero-point, to well within 0.1km/s. Nonetheless, both these velocities and the standards suffer from three sources of systematic error, namely, convective blueshift, gravitational redshift, and spectral type mismatch of the reference spectrum. These systematic errors are here forced to be zero for G2V stars by using the Sun as reference, with Vesta and day sky as proxies. But for spectral types departing from solar, the systematic errors reach 0.3km/s in the F and K stars and 0.4km/s in M dwarfs. Multiple spectra were obtained for all 889 stars during four years, with the HIRES echelle spectrometer (Vogt et al., 1994, , Proc. Soc. Photo-Opt. Instr. Eng., 2198, 362) on the 10m Keck I telescope and with the "Hamilton" echelle spectrometer fed by either the 3m Shane or the 0.6m Coude Auxilliary (CAT) Telescopes (Vogt, 1987PASP...99.1214V 1987PASP...99.1214V), and 782 of them exhibit velocity scatter less than 0.1km/s. These stars may serve as radial velocity standards if they remain constant in velocity. We found 11 new spectroscopic binaries and report orbital parameters for them. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 50 782 Radial velocities of stable stars with RMS<100m/s table2.dat 75 107 Radial velocities of stars with RMS >0.1km/s table3.dat 125 15 Orbital parameters of 15 stars with companions table4.dat 40 30 Stars with linear trends -------------------------------------------------------------------------------- See also: III/21 : General catalogue of stellar radial velocity (Wilson, 1953) III/190 : WEB Catalog of Radial Velocities (Duflot+ 1995) III/213 : General Catalog of mean radial velocities (Barbier-Brossat+, 2000) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Primary name 14- 25 A12 --- AName Alternative name 27- 29 A3 --- Ref [NSO M] Stellar spectrum used as the template (NSO: National Solar Observatory or M: M dwarf composite) 31- 37 I7 JD Date Mean time of observation 39- 42 I4 d DeltaT ?=0 Span of observations (1) 44- 50 I7 m/s Mean barycentric radial velocity -------------------------------------------------------------------------------- Note (1): Stars with only one observation were put in the table even though the RMS scatter is not defined. They can be distinguished by DeltaT=0. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Name Primary name 14- 25 A12 --- AName Alternative name 27- 29 A3 --- Ref [NSO M] Stellar spectrum used as the template (NSO: National Solar Observatory, M: M dwarf) 31- 41 F11.3 d JD Time of observation 43- 48 I6 m/s RV Barycentric radial velocity 50- 56 I7 d Mean time of observation 58- 61 I4 d DeltaT Span of observations (1) 63- 67 I5 m/s RMS RMS scatter of velocity of all observations 69- 71 I3 --- o_RV Number of observations 73- 74 A2 --- Com [AL CO] Comments (2) -------------------------------------------------------------------------------- Note (1): Stars with only one observation were put in the table even though the RMS scatter is not defined. They can be distinguished by DeltaT=0. Note (2): Comments on stars with companion orbit or linears trends: L: velocity varies linearly with time (see table4.dat) CO: a companion and its orbit were found C: a published companion exists but an orbit is not given here A: the star is chromospherically active based on the emission reversal seen at the Ca II H&K lines in our spectrum -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Primary name 11- 19 F9.4 d Per Orbital period 21- 29 F9.4 d e_Per rms uncertainty on Per 31- 35 F5.2 km/s K Velocity semi-amplitude 37- 40 F4.2 km/s e_K rms uncertainty on K 42- 45 F4.2 --- Ecc Eccentricity 47- 51 F5.3 --- e_Ecc ? rms uncertainty on Ecc 52 A1 --- n_Ecc [f] f: fixed 54- 56 I3 deg omega Longitude of periastron 58- 61 F4.1 deg e_omega rms uncertainty on omega 63- 73 F11.3 d T0 Time of periastron passage 75- 82 F8.4 d e_T0 rms uncertainty on T0 84- 87 F4.2 solMass M1 Mass of the primary 89- 93 F5.1 --- M2,min Minimum mass of the secondary, in Jupiter mass 95- 98 F4.2 AU amin Minimum semi-major axis 100-107 F8.6 solMass f(M) Mass function = (M2*sini)3/(M1+M2)2 109-125 A17 --- Ref References (1) -------------------------------------------------------------------------------- Note (1): References: 1: Duquennoy & Mayor, 1991A&A...248..485D 1991A&A...248..485D 2: Martin et al., 1998A&AS..133..149M 1998A&AS..133..149M 3: Blazit et al., 1987A&AS...71...57B 1987A&AS...71...57B 4: Kamper, 1987AJ.....93..683K 1987AJ.....93..683K 5: Wagman, 1949AJ.....54Q.138W 1949AJ.....54Q.138W 6: Beavers & Salzer, 1983PASP...95...79B 1983PASP...95...79B 7: Kamper & Lyons, 1981JRASC..75...56K 1981JRASC..75...56K 8: Halbwachs et al., 2000A&A...355..581H 2000A&A...355..581H 9: Mazeh et al., 1996, Cat. J/ApJ/466/415 10: Oetik er et al., 2001PASP..113..703O 2001PASP..113..703O 11: Mayor et al., 1997IAUCo.161..313M 1997IAUCo.161..313M 12: McCarthy 1986; in Astrophysics of Brown Dwarfs, ed. M.C. Kafatos, R.S. Harrinton and S.P Maran (Cambridge University Press), p. 9. 13: Barbieri et al., 1996A&A...315..418B 1996A&A...315..418B 14: Henry & McCarthy, 1993, Cat. J/AJ/106/773 15: Marcy & Moore, 1989ApJ...341..961M 1989ApJ...341..961M 16: McCarthy & Henry, 1987ApJ...319L..93M 1987ApJ...319L..93M 17: Lippincott & Borgman, 1978PASP...90..330L 1978PASP...90..330L -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 A9 --- Name Primary name (HD name) 10 A1 --- n_Name [ab] Note on Name (1) 12- 21 A10 --- AName Alternate name (HIP name) 23- 30 F8.3 m/s/d Slope Slope of the radial velocity 32- 36 F5.3 m/s/d e_Slope rms uncertainty on Slope 38- 39 I2 --- Nobs Number of observations -------------------------------------------------------------------------------- Note (1): a: Exhibits some additional positive curvature b: Exhibits some additional negative curvature -------------------------------------------------------------------------------- Acknowledgements: David Nidever
(End) Patricia Bauer [CDS] 10-Apr-2002
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line