J/ApJS/252/18  Low-surface-brightness galaxies from DES Y3  (Tanoglidis+, 2021)

Shadows in the dark: low-surface-brightness galaxies discovered in the Dark Energy Survey. Tanoglidis D., Drlica-Wagner A., Wei K., Li T.S., Sanchez J., Zhang Y., Peter A.H.G., Feldmeier-Krause A., Prat J., Casey K., Palmese A., Sanchez C., DeRose J., Conselice C., Gagnon L., Abbott T.M.C., Aguena M., Allam S., Avila S., Bechtol K., Bertin E., Bhargava S., Brooks D., Burke D.L., Rosell A.C., Kind M.C., Carretero J., Chang C., Costanzi M., da Costa L.N., De Vicente J., Desai S., Diehl H.T., Doel P., Eifler T.F., Everett S., Evrard A.E., Flaugher B., Frieman J., Garcia-Bellido J., Gerdes D.W., Gruendl R.A., Gschwend J., Gutierrez G., Hartley W.G., Hollowood D.L., Huterer D., James D.J., Krause E., Kuehn K., Kuropatkin N., Maia M.A.G., March M., Marshall J.L., Menanteau F., Miquel R., Ogando R.L.C., Paz-Chinchon F., Romer A.K., Roodman A., Sanchez E., Scarpine V., Serrano S., Sevilla-Noarbe I., Smith M., Suchyta E., Tarle G., Thomas D., Tucker D.L., Walker A.R. (The DES Collaboration) <Astrophys. J. Suppl. Ser., 252, 18 (2021)> =2021ApJS..252...18T 2021ApJS..252...18T
ADC_Keywords: Galaxies, photometry; Optical; Surveys; Morphology Keywords: Sky surveys ; Low surface brightness galaxies Abstract: We present a catalog of 23790 extended low-surface-brightness galaxies (LSBGs) identified in ∼5000°2 from the first three years of imaging data from the Dark Energy Survey (DES). Based on a single-component Sersic model fit, we define extended LSBGs as galaxies with g-band effective radii Reff(g)>2.5" and mean surface brightness µeff(g)>24.2mag/arcsec2. We find that the distribution of LSBGs is strongly bimodal in (g-r) versus (g-i) color space. We divide our sample into red (g-i≥0.60) and blue (g-i<0.60) galaxies and study the properties of the two populations. Redder LSBGs are more clustered than their blue counterparts and are correlated with the distribution of nearby (z<0.10) bright galaxies. Red LSBGs constitute ∼33% of our LSBG sample, and ∼30% of these are located within 1° of low-redshift galaxy groups and clusters (compared to ∼8% of the blue LSBGs). For nine of the most prominent galaxy groups and clusters, we calculate the physical properties of associated LSBGs assuming a redshift derived from the host system. In these systems, we identify 41 objects that can be classified as ultradiffuse galaxies, defined as LSBGs with projected physical effective radii Reff>1.5kpc and central surface brightness µ0(g)>24.0mag/arcsec2. The wide-area sample of LSBGs in DES can be used to test the role of environment on models of LSBG formation and evolution. Description: The Dark Energy Survey (DES) is an optical-near-infrared imaging survey covering ∼5000°2 of the southern Galactic cap using the Dark Energy Camera (DECam) on the 4-m Blanco Telescope at the Cerro Tololo Inter-American Observatory (CTIO). We use data collected from the first three years of DES observing (DES Y3 Gold; 2013-August -- 2016-February). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 99 82 Characteristics of the most prominent density peaks and their association tabled1.dat 494 23790 Extended low-surface-brightness galaxy catalog -------------------------------------------------------------------------------- See also: VII/110 : Rich Clusters of Galaxies (Abell+ 1989) VII/180 : Galaxies in Fornax Cluster and five nearby groups (Ferguson+ 1990) II/371 : The Dark Energy Survey (DES): Data Release 2 (Abott+, 2021) J/A+AS/134/59 : The central Fornax Cluster. I. Galaxy phot. (Hilker+ 1999) J/A+A/425/367 : REFLEX Galaxy Cluster Survey catalogue (Boehringer+, 2004) J/MNRAS/355/1303 : Rmag surface brightness of HIDEEP galaxies (Minchin+, 2004) J/MNRAS/357/819 : Colours and HI line observations in Virgo (Sabatini+, 2005) J/A+A/459/679 : RB photometry of LSBG in Coma (Adami+, 2006) J/MNRAS/410/166 : Morphological types from Galaxy Zoo 1 (Lintott+, 2011) J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012) J/ApJ/776/80 : PAndAS view of Andromeda satellites. I. (Martin+, 2013) J/ApJ/813/L15 : Dwarf galaxies in Fornax cluster from NGFS (Munoz+, 2015) J/AJ/149/171 : 2MASS galaxy group catalog (Tully, 2015) J/ApJ/833/167 : PAndAS view of Andromeda satellites. II. (Martin+, 2016) J/A+A/608/A142 : Fornax Deep Survey with VST. III. LSB gal. (Venhola+, 2017) J/MNRAS/470/1512 : Faint LSB galaxy cand. in Perseus cluster (Wittmann+, 2017) J/ApJ/855/142 : Next Generation Fornax Survey. II. (Eigenthaler+, 2018) J/ApJ/857/104 : Low surface brightness galaxies from HSC-SSP (Greco+, 2018) J/ApJ/859/52 : NGFS. III. Gal. in outer regions (Ordenes-Briceno+, 2018) J/A+A/620/A165 : Fornax Deep Survey with VST. IV. Dwarf gal. (Venhola+, 2018) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations ------------------------------------------------------------------------------- 1- 2 I2 --- Seq [1/82] Peak Number 4- 16 F13.9 deg RAdeg [-60/90.4] Peak Right Ascension (J2000) 18- 30 F13.9 deg DEdeg [-62.8/3.2] Peak Declination (J2000) 32- 47 A16 --- Assoc Best Association Name 49- 59 F11.7 deg RAAdeg [-58.6/90.5] Association Right Ascension (J2000) 61- 70 F10.6 deg DEAdeg [-61.5/3.2] Association Declination (J2000) 72- 79 F8.5 --- z [-0.84/0.1]?=-1 Redshift for association (1) 81- 86 F6.2 Mpc Dist [18.97/430]?=-1 Distance to association (1) 88- 92 F5.2 Mpc e_Dist [1.3/31]?=-1 Uncertainty in Dist (1) 94- 95 I2 --- NLSBG [13/68] Number of LSBGs<0.5deg from peak center 97- 99 A3 --- Qual Association quality (I=very good, II=good, III=not so good) -------------------------------------------------------------------------------- Note (1): Redshift and distance values from NED. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tabled1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- ID [0/23789] Object sequential identifier 7- 15 I9 --- Coadd [61426632/618665124] Coadd object identifier 17- 26 F10.6 deg RAdeg [0.0048/360] Right Ascension, decimal degrees, SourceExtractor (J2000) 28- 37 F10.6 deg DEdeg [-68.2/5.4] Declination, decimal degrees, SourceExtractor (J2000) 39- 51 F13.9 deg RAGdeg [0.0046/360] Right Ascension, decimal degrees, galfitm (J2000) 53- 65 F13.9 deg DEGdeg [-68.2/5.4] Declination, decimal degrees, galfitm (J2000) 67- 73 F7.5 mag E(B-V) [0.002/0.22] Reddening, E(B-V) Schlegel+ (1998ApJ...500..525S 1998ApJ...500..525S) 75- 85 F11.9 --- ellSE [0.0014/0.8] Isophotal ellipticity, SourceExtractor 87- 97 F11.9 --- ellG [2.9e-7/0.85] Isophotal ellipticity, galfitm 99- 107 F9.6 mag gmagSE [15.8/22.8] g-band MAG_AUTO, SourceExtractor 109- 119 F11.9 mag e_gmagSE [0.0019/0.2] Uncertainty in gmagSE 121- 129 F9.6 mag rmagSE [15.5/22.5] r-band MAG_AUTO, SourceExtractor 131- 141 F11.9 mag e_rmagSE [0.002/0.2] Uncertainty in rmagSE 143- 152 F10.7 mag imagSE [15.35/22.3] i-band MAG_AUTO, SourceExtractor 154- 164 F11.9 mag e_imagSE [0.003/0.3] Uncertainty in imagSE 166- 175 F10.7 arcsec gRadSE [2.5/22] SourceExtractor FLUX_RADIUS g-band 177- 186 F10.7 arcsec rRadSE [1.59/21.9] SourceExtractor FLUX_RADIUS r-band 188- 197 F10.7 arcsec uRadSE [1/21.7] SourceExtractor FLUX_RADIUS i-band 199- 207 F9.6 mag gmagG [15.4/22.5] g-band, galfitm 209- 219 F11.9 mag e_gmagG [0.002/0.4] Uncertainty in gmagG 221- 229 F9.6 mag rmagG [15.19/22.2] r-band, galfitm 231- 241 F11.9 mag e_rmagG [0.002/0.3] Uncertainty in rmagG 243- 252 F10.7 mag imagG [15.1/22.3] i-band, galfitm 254- 264 F11.9 mag e_imagG [0.003/0.4] Uncertainty in imagG 266- 275 F10.8 --- n [0.2/5] Sersic index 277- 287 F11.9 --- e_n [0.0015/1.11] Uncertainty in n 289- 298 F10.7 kpc gReff [2.5/43.8] Physical effective radius, g-band 300- 310 F11.9 kpc e_gReff [0.017/2.9] Uncertainty in gReff 312- 321 F10.7 kpc rReff [2/41.1] Physical effective radius, r-band 323- 333 F11.9 kpc e_rReff [0.012/2.6] Uncertainty in rReff 335- 344 F10.7 kpc iReff [1.26/38.8] Physical effective radius, i-band 346- 356 F11.9 kpc e_iReff [0.015/2.7] Uncertainty in iReff 358- 370 F13.8 --- gchi2 [0.47/7716] χ^2, loc, g-band 372- 384 F13.8 --- rchi2 [0.33/3346] χ^2, loc, r-band 386- 398 F13.8 --- ichi2 [0.2/2183] χ^2, loc, i-band 400- 408 F9.6 mag/arcsec2 gmu [24.2/27.2] Mean surface brightness, g-band 410- 418 F9.6 mag/arcsec2 rmu [22.66/26.4] Mean surface brightness, r-band 420- 428 F9.6 mag/arcsec2 imu [21/26.3] Mean surface brightness, i-band 430- 440 F11.8 mag/arcsec2 gmu0 [15.63/26.3] Central surface brightness, g-band 442- 452 F11.8 mag/arcsec2 rmu0 [13.69/25.72] Central surface brightness, r-band 454- 464 F11.8 mag/arcsec2 imu0 [12.1/25.5] Central surface brightness, i-band 466- 474 F9.6 mag/arcsec2 gmuSE [23.6/27.1] Mean surface brightness, g-band, SourceExtractor 476- 484 F9.6 mag/arcsec2 rmuSE [21.74/26.5] Mean surface brightness, r-band, SourceExtractor 486- 494 F9.6 mag/arcsec2 imuSE [19.4/26.3] Mean surface brightness, i-band, SourceExtractor -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 19-Apr-2022
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