J/ApJ/921/40 FIR properties of SFGs in GOODS-N & COSMOS fields (Kokorev+, 2021)

The evolving interstellar medium of star-forming galaxies, as traced by stardust. Kokorev V.I., Magdis G.E., Davidzon I., Brammer G., Valentino F., Daddi E., Ciesla L., Liu D., Jin S., Cortzen I., Delvecchio I., Gimenez-Arteaga C., Gomez-Guijarro C., Sargent M., Toft S., Weaver J.R. <Astrophys. J., 921, 40 (2021)> =2021ApJ...921...40K 2021ApJ...921...40K
ADC_Keywords: Galaxies, IR; Redshifts; Active gal. nuclei Keywords: High-redshift galaxies ; Submillimeter astronomy ; Infrared astronomy ; Astronomy software ; Galaxies ; Active galaxies ; Starburst galaxies Abstract: We analyze the far-infrared (FIR) properties of ∼5000 star-forming galaxies at z<4.5, drawn from the deepest, super-deblended catalogs in the GOODS-N and COSMOS fields. We develop a novel panchromatic spectral energy distribution fitting algorithm, Stardust, that models the emission from stars, active galactic nuclei (AGNs), and infrared dust emission, without relying on energy balance assumptions. Our code provides robust estimates of the UV- optical and FIR physical parameters, such as the stellar mass (M*), dust mass (Mdust), infrared luminosities (LIR) arising from AGN and star formation activity, and the average intensity of the interstellar radiation field (). Through a set of simulations we quantify the completeness of our data in terms of Mdust, LIR, and and subsequently characterize the distribution and evolution of these parameters with redshift. We focus on the dust-to-stellar mass ratio (fdust), which we parameterize as a function of cosmic age, stellar mass, and specific star formation rate. The fdust is found to increase by a factor of 10 from z=0 to z=2 and appears to remain flat at higher z, mirroring the evolution of the gas fraction. We also find a growing fraction of warm to cold dust with increasing distance from the main sequence, indicative of more intense interstellar radiation fields, higher star formation efficiencies, and more compact star-forming regions for starburst galaxies. Finally, we construct the dust mass functions (DMFs) of star-forming galaxies up to z=1 by transforming the stellar mass function to DMF through the scaling relations derived here. The evolution of fdust and the recovered DMFs are in good agreement with the theoretical predictions of the Horizon-AGN and IllustrisTNG simulations. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 272 4991 Structure of the best-fit catalog -------------------------------------------------------------------------------- See also: II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007) II/373 : The fourth UltraVISTA data release (DR4) (Moneti+, 2019) VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012) VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012) J/A+A/504/751 : GOODS-MUSIC catalog updated version (Santini+, 2009) J/AJ/142/111 : Total infrared brightness and SFR in M33 (Boquien+, 2011) J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011) J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011) J/ApJ/738/69 : SEDs of galaxies at 3.8<z<5 in GOODS (Shim+, 2011) J/MNRAS/423/197 : MIPS photometry for Herschel SAG2 Programs (Bendo+, 2012) J/ApJ/761/140 : Spectroscopy of Herschel-SPIRE galaxies (Casey+, 2012) J/ApJ/745/95 : Herschel FIR & submm phot. of KINGFISH sample (Dale+, 2012) J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012) J/A+A/551/A100 : Panchromatic SED of Herschel sources (Berta+, 2013) J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013) J/ApJ/768/74 : PHIBSS: CO obs. of star-forming galaxies (Tacconi+, 2013) J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014) J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016) J/ApJ/820/83 : ALMA galaxies in the COSMOS survey field (Scoville+, 2016) J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017) J/ApJS/233/22 : xCOLD GASS catalog (Saintonge+, 2017) J/ApJ/853/172 : "Super-deblended" dust emission in galaxies. I. (Liu+, 2018) J/ApJ/864/56 : "Super-deblended" dust em. in gal. II. COSMOS (Jin+, 2018) J/ApJS/236/30 : Herschel-ATLAS (H-ATLAS) DR2 (Maddox+, 2018) J/ApJS/235/34 : Deep JVLA imaging of GOODS-N at 20cm (Owen, 2018) J/A+A/609/A30 : Monochromatic conversion factors to LIR (Schreiber+, 2018) J/A+A/627/A132 : GAS II. UV luminosity functions & IR excess (Cousin+, 2019) J/ApJS/244/40 : A3COSMOS. I. ALMA continuum photometry catalogs (Liu+, 2019) J/A+A/643/A2 : ALPINE DR1 merged catalog (Bethermin+, 2020) J/A+A/644/A144 : Dusty star-forming galaxies (Donevski+, 2020) J/ApJ/909/56 : A galaxy sample with CO detections (Liu+, 2021) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Cat [1/2] Catalog identifier (1) 3- 10 I8 --- ID [6/20010955] Object identifier in Cat 12- 22 F11.7 deg RAdeg [149.3/189.6] Right Ascension (J2000) 24- 33 F10.7 deg DEdeg [1.6/62.5] Declination (J2000) 35 I1 --- Area [0/1] The goodArea flag in the parent catalogs 37- 41 F5.3 --- z [0.005/7.5] Redshift used in fitting 43 I1 --- f_z [0/2]? Redshift type (2) 45- 52 E8.2 Lsun LIR [0/4.04e+13] Total FIR luminosity (3) 54- 62 E9.2 Lsun e_LIR [0/8.1e+12]?=-99 Uncertainty in LIR 64- 71 E8.2 Lsun LAGN [0/2e+13] AGN luminosity 73- 81 E9.2 Lsun e_LAGN [0/8.3e+12]?=-99 Uncertainty in LAGN 83- 90 E8.2 Lsun LIRdr [0/3.3e+13] Luminosity from DL07 (Draine & Li 2007ApJ...657..810D 2007ApJ...657..810D) template 92-100 E9.2 Lsun e_LIRdr [0/5.5e+12]?=-99 Uncertainty in LIRdr 102-109 E8.2 Msun Mdust [0/4.4e+10] Dust mass predicted by best-fit DL07 (Draine & Li 2007ApJ...657..810D 2007ApJ...657..810D) template 111-118 E8.2 Msun e_Mdust [1/7.7e+21]?=-99 Uncertainty in Mdust 120-128 E9.2 --- delGDR [53.4/9.8e+20]?=-99 Gas-to-dust-ratio 130 A1 --- f_delGDR i=infinite value 132-140 E9.2 Msun Mgas [0/6.5e+26]?=-99 Gas mass computed from DelGDR & Mdust 142-150 E9.2 Msun e_Mgas [0/1.4e+25]?=-99 Uncertainty in Mgas 152 A1 --- f_Mgas i=infinite value 154-162 E9.2 Msun Mstar [0/1.9e+14]?=-99 Stellar mass (4) 164-170 F7.2 um lamLast [53.2/1180.5] Last band that has an S/N>3 detection (λlast) given in rest frame 172-178 F7.2 --- chi2 [0/1988] The χ2 of best-fit coefficients 180-187 E8.2 --- fAGN [0/0.92] AGN fraction, LAGN/LIR 189-197 E9.2 --- e_fAGN [0/1.8]?=-99 Uncertainty in fAGN 199-207 E9.2 --- fgas [0/18400]?=-99 Gas fraction computed as Mgas/Mdust 209-217 E9.2 --- fgasFMR [-0.00022/1.1e+20]? Gas fraction assuming delGDR=100 219 A1 --- f_fgasFMR i=infinite value 221-225 F5.2 --- Umin [0.1/50] Best fit Umin value 227-232 F6.4 --- gamma [0/0.5] Best fit γ value 234-235 I2 --- qpah [0/10] Index of the best fit qPAH value 237-244 E8.2 --- U [0/373] Average radiation field intensity 246-253 E8.2 --- e_U [0/219] Uncertainty in U 255-262 E8.2 --- delMS [0/4590] Star formation ratio (5) 264-272 E9.2 --- e_delMS [0/207]?=-99 Uncertainty in delMS -------------------------------------------------------------------------------- Note (1): Catalog as follows: 1 = The GOODS-N field (Liu+ 2018, J/ApJ/853/172 ; <[LDD2018] NNNNN> in Simbad ; 585 occurrences). 2 = The COSMOS field (Jin+ 2018, J/ApJ/864/56). (4406 occurrences) Note (2): Redshift type as follows: 1 = spectroscopic (552 occurrences) 0 = photometric (4364 occurrences) 2 = zphot from EAZY (75 occurrences) Note (3): Obtained as the sum between AGN and DL07 components. Note (4): Equal to the value in the original catalog. Note (5): SFR/SFRMS where SFR=LIR,drainex10-10 and SFRMS is given by Schreiber+ (2015A&A...575A..74S 2015A&A...575A..74S). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 03-Feb-2023
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