J/ApJS/256/41       Grid of synthetic spectra for subdwarfs     (Pacheco+, 2021)

A grid of synthetic spectra for subdwarfs: Non-LTE line-blanketed atmosphere models. Pacheco T.A., Diaz M.P., Levenhagen R.S., Coelho P.R.T. <Astrophys. J. Suppl. Ser. 256, 41 (2021)> =2021ApJS..256...41P 2021ApJS..256...41P (SIMBAD/NED BibCode)
ADC_Keywords: Stars, subdwarf ; Models ; Spectroscopy Keywords: stellar atmospheres - spectral energy distribution - stellar spectral lines - subdwarf stars Abstract: A new grid of detailed atmosphere model spectra for hot and moderately cool subdwarf stars is presented. High-resolution spectra and synthetic photometry are calculated in the range from 1000Å to 10,000Å using Non-LTE fully line- blanketed atmosphere structures. Our grid covers eight temperatures within 10000<Teff[K]<65000, three surface gravities in the range 4.5<logg[cgs]<6.5, two helium abundances matching two extreme helium-rich and helium-poor scenarios, and two limiting metallicity boundaries regarding both solar ([Fe/H]=0) and Galactic halo ([Fe/H]=-1.5 and [alpha/Fe]=+0.4). Besides its application in the determination of fundamental parameters of subdwarfs in isolation and in binaries, the resulting database is also of interest for population synthesis procedures in a wide variety of stellar systems. Description: 96 spectra in FITS (2-D data) covering wavelength between 1000 and 10000Å with microturbulent velocity = 10km/s and rotation velocity = 0. $1 wavelength in angstrom $2 flux in erg/cm2/s/Hz From filename: The number after t is Teff and the number after g is log g. The suffix represents the chemical abundances: sol_Hepoor ([Fe/H]=0 and He-poor); sol_Herich ([Fe/H]=0 and He-rich); lowZ_Hepoor ([Fe/H]=-1.5, [alpha/Fe]=+0.4 and He-poor); or lowZ_Herich ([Fe/H]=-1.5, [alpha/Fe]=+0.4 and He-rich). The reference for each He value (log(nHe/nH)) as a function of Teff is available at paper's table 2 as follow: 10000K: He rich = -3.81 and He poor = -4.98 15000K: He rich = -3.13 and He poor = -4.35 20000K: He rich = -2.46 and He poor = -3.72 25000K: He rich = -1.78 and He poor = -3.09 30000K: He rich = -1.22 and He poor = -2.42 35000K: He rich = -0.43 and He poor = -1.83 45000K: He rich = +0.92 and He poor = -0.57 65000K: He rich = +3.62 and He poor = +1.95 Example: t10000g+4.5sol_Hepoor.spec is the spectrum with 10000K, log g=+4.5, solar abundance and He-poor. How to read data from python3: --------------------------------------------------------------------- ≫>from astropy.io import fits ≫>hdr = fits.getheader('./t25000g+4.5lowZHepoorhr.fit') #Header ≫>hdl = fits.getdata('./t25000g+4.5lowZHepoorhr.fit') #Data ≫>w = hdl['WAVELENGTH'] ≫>f = hdl['FLUX'] File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 60 96 List of fits spectra sp/* . 96 Individual fits spectra -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 31 A31 --- FileName Name of the spectrum file in subdirectory sp 33- 37 I5 K Teff [10000/65000] Effective temperature 39- 42 F4.1 [cm/s2] logg Surface gravity, +4.5, +5.5 or +6.5 44- 47 F4.1 [-] [Fe/H] Metallicity (0 for solar abundance) 49- 52 F4.1 [-] [alpha/Fe] ? [alpha/Fe] abundance 54- 60 A7 --- He He-poor or He-rich (1) -------------------------------------------------------------------------------- Note (1): Reference for each He value (log(nHe/nH)) as a function of Teff as follows: 10000K = He rich = -3.81 and He poor = -4.98 15000K = He rich = -3.13 and He poor = -4.35 20000K = He rich = -2.46 and He poor = -3.72 25000K = He rich = -1.78 and He poor = -3.09 30000K = He rich = -1.22 and He poor = -2.42 35000K = He rich = -0.43 and He poor = -1.83 45000K = He rich = +0.92 and He poor = -0.57 65000K = He rich = +3.62 and He poor = +1.95 -------------------------------------------------------------------------------- Acknowledgements: Thayse Pacheco, thayse.pacheco(at)usp.br
(End) Thayse Pacheco [USP, Brazil], Patricia Vannier [CDS] 30-Sep-2021
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