J/A+A/547/A62        A catalogue of Paschen-line profiles        (Huang+, 2012)

A catalogue of Paschen-line profiles in standard stars. Huang W., Wallerstein G., Stone M. <Astron. Astrophys. 547, A62 (2012)> =2012A&A...547A..62H 2012A&A...547A..62H
ADC_Keywords: Atlases ; Line Profiles; Stars, early-type ; Stars, late-type Keywords: atlases ; line: profiles ; stars: early-type ; stars: late-type Abstract: We have assembled an atlas of line profiles of the Paschen Delta (P-δ) line at 10049Å for the use of stellar modelling. For a few stars we have substituted the Paschen Gamma (P-γ) line at 10938Å because the P-δ line blends with other features. Most of the targets are standard stars of spectral types from B to M. A few metal-poor stars have been included. For many of the stars we have also observed the Hydrogen Alpha (H-α) line so as to compare the profiles of lines originating from the meta-stable n=2 level with lines originating from the n=3 level. The greatest difference in line profile is found for high luminosity and cool stars where the departures from LTE in the population of the n=2 level is expected to be the greatest. For a few stars, sample line profiles have been calculated in the LTE approximation to demonstrate the usefulness of the tabulated and displayed catalogue. Description: This catalogue contains spectroscopic data of 90 stars. A wide variety of stars were observed at H-α and at P-δ. A few stars were observed at P-γ. Most of the data were obtained at the Dominion Astrophysical Observatory (DAO). The remainder of the data were obtained at the Apache Point Observatory. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file standard.dat 62 76 List of standard stars observed metalp.dat 60 15 List of metal-poor stars observed standard/* . 128 FITS files with spectrum of standard stars metalp/* . 15 FITS files with spectrum of metal-poor stars -------------------------------------------------------------------------------- See also: Byte-by-byte Description of file: standard.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD HD designation of star 8- 17 A10 --- SpType MK spectral type 20- 24 F5.2 [-] [Fe/H] ?=- Metallicity 26- 37 A12 --- H-Files Names of files with observed H-α spectra in subdirectory standard (1) 38- 49 A12 --- Pd-Files Names of files with observed P-δ spectra in subdirectory standard (1) 51- 62 A12 --- Pg-Files Names of files with observed P-γ spectra in subdirectory standard (1) -------------------------------------------------------------------------------- Note (1): Where applicable, file names begin with HD designation and are followed by an "h", "pd", "pg", or "e" which indicate H-α, P-δ, P-γ, or echelle, respectively. -------------------------------------------------------------------------------- Byte-by-byte Description of file: metalp.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- HD ? HD designation of star 8- 17 A10 --- BD BD designation of star 20- 26 A7 --- SpType MK spectral type 28- 32 F5.2 [-] [Fe/H] Metallicity 35- 46 A12 --- H-Files Names of files with observed H-α spectra in subdirectory metalp (1) 49- 60 A12 --- Pd-Files Names of files with observed P-δ spectra in subdirectory metalp (1) -------------------------------------------------------------------------------- Note (1): Where applicable, file names begin with HD designation and are followed by an "e" which indicates echelle. -------------------------------------------------------------------------------- Acknowledgements: Myra Stone, myrastone0(at)gmail.com
(End) Patricia Vannier [CDS] 10-Sep-2012
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