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Spectroscopic stellar parameters for 582 FGK stars in the HARPS volume-limited sample. Revising the metallicity-planet correlation
To understand the formation and evolution of solar-type stars andplanets in the solar neighborhood, we need to obtain their stellarparameters with high precision. We present a catalog of precise stellarparameters for low-activity FGK single stars in a volume-limited samplefollowed by the HARPS spectrograph in the quest to identify extra-solarplanets. The spectroscopic analysis was completed assuming LTE with agrid of Kurucz atmosphere models and using the ARES code to perform anautomatic measurement of the line equivalent widths. The results arecompared with different independent methods and also with other valuesfound in the literature for common stars. Both comparisons areconsistent and illustrate the homogeneity of the parameters derived byour team. The derived metallicities of this sample reveal a somewhatdifferent distribution for the present planet hosts, but still indicatesthe already known higher frequency of planets observed for the moremetal-rich stars. We combine the results derived in this sample with theone from the CORALIE survey to present the largest homogeneousspectroscopic study of the metallicity-giant-planet relation using atotal of 1830 stars.Full Table 1 is only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/533/A141
| Bayesian inference of stellar parameters and interstellar extinction using parallaxes and multiband photometry
Astrometric surveys provide the opportunity to measure the absolutemagnitudes of large numbers of stars, but only if the individualline-of-sight extinctions are known. Unfortunately, extinction is highlydegenerate with stellar effective temperature when estimated frombroad-band optical/infrared photometry. To address this problem, Iintroduce a Bayesian method for estimating the intrinsic parameters of astar and its line-of-sight extinction. It uses both photometry andparallaxes in a self-consistent manner in order to provide anon-parametric posterior probability distribution over the parameters.The method makes explicit use of domain knowledge by employing theHertzsprung-Russell Diagram (HRD) to constrain solutions and to ensurethat they respect stellar physics. I first demonstrate this method byusing it to estimate effective temperature and extinction from BVJHKdata for a set of artificially reddened Hipparcos stars, for whichaccurate effective temperatures have been estimated from high-resolutionspectroscopy. Using just the four colours, we see the expected strongdegeneracy (positive correlation) between the temperature andextinction. Introducing the parallax, apparent magnitude and the HRDreduces this degeneracy and improves both the precision (reduces theerror bars) and the accuracy of the parameter estimates, the latter byabout 35 per cent. The resulting accuracy is about 200 K in temperatureand 0.2 mag in extinction. I then apply the method to estimate theseparameters and absolute magnitudes for some 47 000 F, G, K Hipparcosstars which have been cross-matched with Two-Micron All-Sky Survey(2MASS). The method can easily be extended to incorporate the estimationof other parameters, in particular metallicity and surface gravity,making it particularly suitable for the analysis of the 109stars from Gaia.
| The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars
The Henry Draper Extension Charts (HDEC), published in the form offinding charts, provide spectral classification for some 87000 starsmostly between 10th and 11th magnitude. This data, being highlyvaluable, as yet was practically unusable for modern computer-basedastronomy. An earlier pilot project (Roeser et al. 1991) demonstrated apossibility to convert this into a star catalogue, using measurements ofcartesian coordinates of stars on the charts and positions of theAstrographic Catalogue (AC) for subsequent identification. We presenthere a final HDEC catalogue comprising accurate positions, propermotions, magnitudes and spectral classes for 86933 stars of the HenryDraper Extension Charts.
| Dwarf K and M stars in the southern hemisphere.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972AJ.....77..486U&db_key=AST
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| Takýmyýldýz: | Oglak |
| Sað Açýklýk: | 20h53m49.50s |
| Yükselim: | -18°47'21.5" |
| Görünürdeki Parlaklýk: | 9.627 |
| Uzaklýk: | 38.344 parsek |
| özdevim Sað Açýklýk: | 104.5 |
| özdevim Yükselim: | -91.7 |
| B-T magnitude: | 11.125 |
| V-T magnitude: | 9.751 |
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