J/A+A/530/A31    Stellar parameters in 10 globular cluster fields  (Lane+, 2011)

AAOmega spectroscopy of 29351 stars in fields centered on ten Galactic globular clusters. Lane R.R., Kiss L.L., Lewis G.F., Ibata R.A., Siebert A., Bedding T.R., Szekely P., Szabo G.M. <Astron. Astrophys. 530, A31 (2011)> =2011A&A...530A..31L 2011A&A...530A..31L
ADC_Keywords: Clusters, globular ; Spectroscopy ; Effective temperatures ; Abundances ; Equivalent widths ; Radial velocities ; Rotational velocities Keywords: globular clusters: general - Galaxy: halo Abstract: Here we publish the extracted stellar parameters from a recent large spectroscopic survey of ten globular clusters. A brief review of the project is also presented. Stellar parameters have been extracted from individual stellar spectra using both a modified version of the Radial Velocity Experiment (RAVE) pipeline and a pipeline based on the parameter estimation method of RAVE. We publish here all parameters extracted from both pipelines. We calibrate the metallicity and convert this to [Fe/H] for each star and, furthermore, we compare the velocities and velocity dispersions of the Galactic stars in each field to the Besanc,on Galaxy model. We find that the model does not correspond well with the data, indicating that the model is probably of little use for comparisons with pencil beam survey data such as this. Description: Various stellar parameters were extracted, using two different reduction pipelines, from individual stellar spectra obtained with AAOmega on the Anglo-Australia Telescope. These spectra were obtained from ten fields centered on Galactic globular clusters, namely M4, M12, M22, M30, M53, M55, M68, NGC 288, NGC 6752 and 47 Tuc. Stellar parameters provided include the radial velocity, sum of the equivalent widths of the calcium triplet lines, equatorial coordinates, I magnitude, V magnitude, effective temperature, surface gravity, metallicity, rotational velocity, J magnitude, H magnitude, K magnitude, distance from the cluster centre, position angle with respect to the cluster centre and whether each star was determined to be a member of the cluster. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 121 28244 Parameters from the RAVE pipeline for all fields table2.dat 118 8788 Parameters from the KISS pipeline for fields centered on M22, M30, M53, M68 table3.dat 147 20563 Parameters from the KISS pipeline for fields centered on 47 Tuc, M4, M12, M55, NGC 288, NGC 6752 -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) III/257 : RAVE second data release (Zwitter+, 2008) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Cluster Cluster at centre of field (e.g. 47tuc) 9- 25 F17.15 rad RArad Right Ascension (J2000) 27- 44 F18.15 rad DErad Declination (J2000) 46- 50 F5.2 mag Imag Estimated I magnitude 52- 61 A10 --- Field Field name (G2) 63- 65 I03 --- Fib AAOmega fibre number (G2) 67- 74 F8.2 km/s HRV Heliocentric radial velocity 76- 82 F7.2 km/s e_HRV Heliocentric radial velocity uncertainty 84- 89 I6 K Teff Effective temperature 91- 95 F5.2 [cm/s2] logg Logarithm of the surface gravity 97-101 F5.2 --- [m/H] Uncalibrated metallicity 103-107 F5.2 --- [a/Fe] α element abundance 109-112 F4.2 km/s xi Microturbulence velocity ξ 114-117 I4 km/s Vrot Rotational velocity, v.sin(i) 119-121 A3 --- Mm [yes no] Member of cluster (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Cluster Cluster at centre of field (e.g. M22) 10- 19 A10 --- Field Field name (G2) 21- 23 I03 --- Fib AAOmega fibre number (G2) 25- 32 F8.3 km/s HRV Heliocentric radial velocity 34- 40 F7.3 km/s e_HRV Heliocentric radial velocity uncertainty 42- 46 F5.2 0.1nm W(CaT) Sum of the equivalent widths of the calcium triplet lines 48- 59 F12.8 deg RAdeg Right Ascension (J2000) 61- 72 F12.8 deg DEdeg Declination (J2000) 74- 79 F6.3 mag Imag Estimated I magnitude 81- 85 I5 K Teff Effective temperature 87- 89 F3.1 [cm/s2] logg Logarithm of the surface gravity 91- 94 F4.1 --- [m/H] Uncalibrated metallicity 96- 98 I3 km/s Vrot Rotational velocity, v.sin(i) 100-105 F6.1 arcsec Dist Distance from the cluster centre 107-114 F8.3 deg PA [-180/180] Position angle of distance vector 116-118 A3 --- Mm [yes no] Member of cluster (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Cluster Cluster at centre of field (e.g. NGC6752) 10- 19 A10 --- Field Field name (G2) 21- 23 I03 --- Fib AAOmega fibre number (G2) 25- 32 F8.3 km/s HRV Heliocentric radial velocity 34- 40 F7.3 km/s e_HRV Heliocentric radial velocity uncertainty 42- 47 F6.2 0.1nm W(CaT) Sum of the equivalent widths of the calcium triplet lines 49- 60 F12.8 deg RAdeg Right Ascension (J2000) 62- 73 F12.8 deg DEdeg Declination (J2000) 75- 80 F6.3 mag Imag Estimated I magnitude 82- 87 F6.3 mag Vmag Estimated V magnitude 89- 93 I5 K Teff Effective temperature 95- 97 F3.1 [cm/s2] logg Logarithm of the surface gravity 99-102 F4.1 --- [m/H] Uncalibrated metallicity 104-106 I3 km/s Vrot Rotational velocity, v.sin(i) 108-113 F6.3 mag Jmag 2MASS/J magnitude (Cat. II/246) 115-120 F6.3 mag Hmag 2MASS/H magnitude (Cat. II/246) 122-127 F6.3 mag Kmag 2MASS/Ks magnitude (Cat. II/246) 129-134 F6.1 arcsec Dist Distance from the cluster centre 136-143 F8.3 deg PA [-180/180] Position angle 145-147 A3 --- Mm [yes no] Member of cluster (G1) -------------------------------------------------------------------------------- Global notes: Note (G1): Denotes whether the star was classified as a member or not in Papers 1, 2 & 3. * Paper 1 : Lane et al., 2009MNRAS.400..917L 2009MNRAS.400..917L * Paper 2 : Lane et al., 2010MNRAS.401.2521L 2010MNRAS.401.2521L, 2010ApJ...711L.122L 2010ApJ...711L.122L * Paper 3 : Lane et al., 2010MNRAS.406.2732L 2010MNRAS.406.2732L Note (G2): Stars are identified as [field]_[fibre number], where [field] is the field name and [fibre number] is the AAOmega fibre (e.g. ngc50246b380 designates the field ngc5024_6b and fibre number 380). -------------------------------------------------------------------------------- Acknowledgements: Richard Lane, rlane(at)astro-udec.cl History: 03-May-2011: on-line data 20-Apr-2018: in table2, Vmag corrected in Imag
(End) Richard Lane [Univ. de Concepcion], Patricia Vannier [CDS] 14-Apr-2011
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