J/A+A/580/A43   Global HI content from a stacking experiment     (Gereb+, 2015)

From star-forming galaxies to AGN: the global HI content from a stacking experiment. Gereb K., Morganti R., Oosterloo T.A., Hoppmann L., Staveley-Smith L. <Astron. Astrophys. 580, A43 (2015)> =2015A&A...580A..43G 2015A&A...580A..43G
ADC_Keywords: Galaxies, spectra ; Radio lines Keywords: radio lines: galaxies Abstract: We study the atomic neutral hydrogen (HI) content of ∼1600 galaxies up to z∼0.1 using stacking techniques. The observations were carried out with the Westerbork Synthesis Radio Telescope (WSRT) in the area of the SDSS South Galactic Cap (SSGC), where we selected a galaxy sample from the SDSS spectroscopic catalog. Multi-wavelength information is provided by SDSS, NVSS, GALEX, and WISE. We use the collected information to study HI trends with color, star-forming, and active galactic nuclei (AGN) properties. Using near-UV (NUV)-r colors, galaxies are divided into blue cloud, green valley and red sequence galaxies. Description: We present the atomic neutral hydrogen (HI) stacked spectra of different galaxy populations selected by colour and/or AGN/star-forming properties. The HI observations were carried out with the Westerbork Synthesis Radio Telescope (WSRT) in the redshift range 0<z<0.12. In the observed volume, about 1600 galaxies have available Sloan Digital Sky Survey (SDSS) spectroscopic measurement and accompanying multi-wavelength data. Galaxy populations are defined using the multi-wavelength information. The HI spectra of a selected population are de-redshifted to the rest frame frequency of HI (1420.4MHz) according to the SDSS redshift, and co-added in redshift/luminosity bins. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 156 34 *List of fits spectra fits/* . 34 Individual fits spectra -------------------------------------------------------------------------------- Note on list.dat: spectra are from 1.40 to 1.44GHz. -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Nx [260] Number of Frequencies 5- 6 I2 Kibyte size [15] Size of the file 8- 47 A40 --- FileName Name of the fits file in subdirectory fits 49-156 A108 --- Title Title of the file -------------------------------------------------------------------------------- Acknowledgements: Katinka Gereb, kgereb(at)swin.edu.au
(End) K. Gereb [Swinburne Univ. of Technology], P. Vannier [CDS] 29-Jul-2015
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