J/MNRAS/494/2090    Group galaxies in ALFALFA survey             (Jones+, 2020)

The HI mass function of group galaxies in the ALFALFA survey. Jones M., Hess K.M., Adams E.A.K., Verdes-Montenegro L. <Mon. Not. R. Astron. Soc. 494, 2090 (2020)> =2020MNRAS.494.2090J 2020MNRAS.494.2090J (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs ; H I data Keywords: galaxies: groups: general - galaxies: luminosity function - mass function - radio lines: galaxies Abstract: We estimate the HI mass function (HIMF) of galaxies in groups based on thousands of ALFALFA (Arecibo Legacy Fast ALFA survey) HI detections within the galaxy groups of four widely used SDSS (Sloan Digital Sky Survey) groups catalogues. Although differences between the catalogues mean that there is no one definitive group galaxy HIMF, in general we find that the low-mass slope is flat, in agreement with studies based on small samples of individual groups, and that the 'knee' mass is slightly higher than that of the global HIMF of the full ALFALFA sample. We find that the observed fraction of ALFALFA galaxies in groups is approximately 22 per cent. These group galaxies were removed from the full ALFALFA source catalogue to calculate the field HIMF using the remaining galaxies. Comparison between the field and group HIMFs reveals that group galaxies make only a small contribution to the global HIMF as most ALFALFA galaxies are in the field, but beyond the HIMF 'knee' group galaxies dominate. Finally we attempt to separate the group galaxy HIMF into bins of group halo mass, but find that too few low-mass galaxies are detected in the most massive groups to tightly constrain the slope, owing to the rarity of such groups in the nearby Universe where low-mass galaxies are detectable with existing HI surveys. Description: These four tables list the ALFALFA galaxies (by AGC number) from Haynes et al. 2018 (J/ApJ/861/49) which were matched to the four optical galaxy groups catalogues used in this work: Berlind et al. 2009 (http://lss.phy.vanderbilt.edu/groups/dr7/), Tempel et al. 2014 (J/A+A/566/A1/v180_gr), Yang et al. 2012 (https://gax.sjtu.edu.cn/data/Group.html), and Lim et al. 2017 (https://gax.sjtu.edu.cn/data/Group.html). The tables also include the groups within the survey volume considered by do not contain any galaxies detected in ALFALFA. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file berlind.dat 34 2792 ALFALFA galaxies in Berlind et al. 2009 groups tempel.dat 34 5885 ALFALFA galaxies in Tempel et al. 2014 groups yang.dat 34 3292 ALFALFA galaxies in Yang et al. 2012 groups lim.dat 34 4358 ALFALFA galaxies in Lim et al. 2017 groups -------------------------------------------------------------------------------- See also: J/ApJ/861/49 : ALFALFA extragalactic HI source catalog (Haynes+, 2018) J/A+A/566/A1 : Flux- and volume-limited groups for SDSS galaxies (Tempel+ 2014) https://gax.sjtu.edu.cn/data/Group.html : Group Catalogues for 2dFGRS & SDSS SDSS_DR7 Home Page http://lss.phy.vanderbilt.edu/groups/dr7 : Groups and Clusters in the SDSS Home Page Byte-by-byte Description of file: berlind.dat lim.dat tempel.dat yang.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- AGC ? ID number corresponding to the ALFALFA 100% release (J/ApJ/861/49) 8- 12 I5 --- GN Group ID number (1) 14- 18 F5.1 Mpc dist Hubble distance of group (h=0.7) 20- 24 F5.2 [Msun] log(MHI) ? log(HI mass) of galaxy assuming distance above 26- 30 F5.1 km/s W50 ? Observed velocity width at 50% of peak on either side (J/ApJ/861/49) 32 I1 --- comp [0/1]? Flag indicating if above the ALFALFA completeness limit 34 I1 --- prox [0/1]? Flag indicating if the ALFALFA galaxy was matched to the group only by a proximity match -------------------------------------------------------------------------------- Note (1): Group ID number from: berlind.dat : Berlind et al., 2009 Mr18 catalogue (http://lss.phy.vanderbilt.edu/groups/dr7/) tempel.dat : Tempel et al., 2014 catalogue (J/A+A/566/A1/v180_gr) yang.dat : Yang et al., 2012 SDSS DR7 model B catalogue (https://gax.sjtu.edu.cn/data/Group.html) https://gax.sjtu.edu.cn/data/data1/Group_SDSS7/group_DR7.tar.gz lim_.dat : Lim et al., 2017 SDSS+M group catalogue (https://gax.sjtu.edu.cn/data/Group.html) https://gax.sjtu.edu.cn/data/data1/Group_LowZ/catalogs.tgz -------------------------------------------------------------------------------- Acknowledgements: Michael Jones, mjones(at)iaa.es
(End) Patricia Vannier [CDS] 12-Mar-2020
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