==========================================================================
VII/282 T-RECS. Tiered Radio Extragalactic Continuum Simulation (Bonaldi+, 2018)
The following files can be converted to FITS (extension .fit or fit.gz)
agnsdeep.dat agnsmedi.dat agnswide.dat
sfgsdeep.dat sfgsmedi.dat sfgswide*.dat
==========================================================================
drwxr-xr-x 257 cats archive 8192 Feb 8 10:28 [Up]
drwxr-xr-x 4 cats archive 4096 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 384 Nov 4 2019 .message
-r--r--r-- 1 cats archive 12558 Nov 4 2019 ReadMe
-r--r--r-- 1 cats archive 6320435 Oct 31 2019 agnsdeep.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 137987864 Oct 31 2019 agnsmedi.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1002111423 Oct 31 2019 agnswide.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
drwxr-xr-x 2 cats archive 4096 Oct 31 2019 fits
-r--r--r-- 1 cats archive 227368060 Oct 31 2019 sfgsdeep.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 2328724584 Oct 31 2019 sfgsmedi.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 510409910 Oct 31 2019 sfgswide1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 9674307 Oct 31 2019 sfgswide10.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1841878310 Oct 31 2019 sfgswide2.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 4079056778 Oct 31 2019 sfgswide3.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 6162195541 Oct 31 2019 sfgswide4.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 2811978966 Oct 31 2019 sfgswide5.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 583794180 Oct 31 2019 sfgswide6.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 66464430 Oct 31 2019 sfgswide7.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 45434764 Oct 31 2019 sfgswide8.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 31306413 Oct 31 2019 sfgswide9.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :VII/282 T-RECS. Tiered Radio Extragalactic Continuum Simulation (Bonaldi+, 2018)
================================================================================
The Tiered Radio Extragalactic Continuum Simulation (T-RECS).
Bonaldi A., Bonato M., Galluzzi V., Harrison I., Massardi M., Kay S.,
De Zotti G., Brown M.L.
<Mon. Not. R. Astron. Soc., 482, 2-19 (2019)>
=2019MNRAS.482....2B
=2018yCat.7282....0B
================================================================================
ADC_Keywords: Models ; Radio continuum ; Active gal. nuclei ;
Star Forming Region
Keywords: radio continuum: galaxies -
galaxies: luminosity function, mass function -
large-scale structure of Universe
Abstract:
We present the Tiered Radio Extragalactic Continuum Simulation
(T-RECS): a new simulation of the radio sky in continuum, over the
150MHz-20GHz range. T-RECS models two main populations of radio
galaxies: Active Galactic Nuclei (AGNs) and Star-Forming Galaxies
(SFGs), and corresponding sub-populations, following Bonato et al.
(2017). Our model also includes polarised emission over the full
frequency range, which has been characterised statistically for each
population using the available in- formation (e.g., Hales et al.,
2014MNRAS.440.3113H; Galluzzi et al. 2018MNRAS.475.1306G; Sun & Reich
2012A&A...543A.127S). We model the clustering properties in terms of
probability distributions of hosting halo masses, and use lightcones
extracted from a high-resolution cosmological simulation to determine
the positions of haloes. This limits the sky area for the simulations
including clustering to a 25deg^2^ field of view. We compare
luminosity functions, number counts in total intensity and
polarization, and clustering properties of our outputs to the most
recent compilation of data and find a very good agreement. We deliver
a set of simulated catalogues, as well as the code to produce them,
which we believe will be very useful for simulating observations and
predicting results from deep radio surveys with existing and
forthcoming radio facilities, such as the Square Kilometre Array
(SKA).
Description:
AGN and SFG catalogs,
"deep" tier (1 square degrees, 1nJy flux limit imposed at 1.4GHz),
"medium" tier (25 square degrees, 10 nJy flux limit imposed at 1.4GHz)
and "wide" tier (400 square degrees, 100nJy flux limit imposed at 1.4GHz).
The description of the models and the simulation is in the paper.