J/ApJS/245/10  A catalog of galaxies in direction of Perseus  (Wittmann+, 2019)

A catalog of galaxies in the direction of the Perseus cluster. Wittmann C., Kotulla R., Lisker T., Grebel E.K., Conselice C.J., Janz J., Penny S.J. <Astrophys. J. Suppl. Ser., 245, 10 (2019)> =2019ApJS..245...10W 2019ApJS..245...10W
ADC_Keywords: Galaxy catalogs; Clusters, galaxy; Photometry, UBVRI; Extinction; Colors; Morphology; Cross identifications Keywords: catalogs; galaxies: clusters: individual (Perseus); galaxies: dwarf; galaxies: photometry Abstract: We present a catalog of 5437 morphologically classified sources in the direction of the Perseus galaxy cluster core, among them 496 early-type low-mass galaxy candidates. The catalog is primarily based on V-band imaging data acquired with the William Herschel Telescope, which we used to conduct automated source detection and derive photometry. We additionally reduced archival Subaru multiband imaging data in order to measure aperture colors and perform a morphological classification, benefiting from 0.5" seeing conditions in the r-band data. Based on morphological and color properties, we extracted a sample of early-type low-mass galaxy candidates with absolute V-band magnitudes in the range of -10 to -20mag. In the color-magnitude diagram, the galaxies are located where the red sequence for early-type cluster galaxies is expected, and they lie on the literature relation between absolute magnitude and Sersic index. We classified the early-type dwarf candidates into nucleated and nonnucleated galaxies. For the faint candidates, we found a trend of increasing nucleation fraction toward brighter luminosity or higher surface brightness, similar to what is observed in other nearby galaxy clusters. We morphologically classified the remaining sources as likely background elliptical galaxies, late-type galaxies, edge-on disk galaxies, and likely merging systems and discussed the expected contamination fraction through non-early-type cluster galaxies in the magnitude-size surface brightness parameter space. Our catalog reaches its 50% completeness limit at an absolute V-band luminosity of -12mag and a V-band surface brightness of 26mag/arcsec2. This makes it the largest and deepest catalog with coherent coverage compared to previous imaging studies of the Perseus cluster. Description: We performed the source detection and photometry in our V-band mosaic of the Perseus cluster core, which we presented and described in Wittmann+ (2017, J/MNRAS/470/1512 --see their Figure 1 and Figure 1 in this paper). The mosaic is based on imaging data acquired with the prime focus imaging platform at the William Herschel Telescope (WHT; program 2012B/045; PI: T. Lisker). The observations were carried out 2012 November 12 and 13. The WHT data constitute our primary data set that we used to establish the catalog. We additionally reduced archival Subaru HSC data in the g, r, and z bands, which served as an auxiliary data set to improve the quality of the catalog. The HSC data set was compiled from a number of mostly overlapping observations taken under two different proposals in 2014 September and November, obtained from the Subaru-Mitaka-Okayama-Kiso Archive (SMOKA; Baba+ 2002ASPC..281..298B 2002ASPC..281..298B). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table6.dat 252 5437 The Perseus Cluster Catalog (PCC) table7.dat 275 139 The PCC literature crossmatch; updated version by the author -------------------------------------------------------------------------------- See also: VII/42 : GMP catalogue: galaxies in the Coma cluster (Godwin+ 1983) VII/180 : Galaxies in Fornax Cluster and five nearby groups (Ferguson+ 1990) V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012) J/AJ/90/1681 : The Virgo Cluster Catalog (VCC) (Binggeli+, 1985) J/A+AS/139/141 : Galaxies in the Perseus Cluster (Brunzendorf+, 1999) J/AJ/117/75 : BR photom. in Coma, A2199 & AWM5 clusters (Conselice+, 1999) J/A+A/430/411 : B-band photometry of ellipticals in Virgo (Gavazzi+, 2005) J/A+A/490/923 : Morphology of gal. in Coma cluster direction (Michard+, 2008) J/A+A/496/683 : Early-type galaxies in the Centaurus cluster (Misgeld+, 2009) J/A+A/538/A69 : Virgo early-type galaxies optical properties (Lieder+, 2012) J/MNRAS/422/885 : Ultracompact dwarf galaxies in Perseus (Penny+, 2012) J/MNRAS/445/2385 : HST/ACS Coma Cluster Survey. X. (den Brok+, 2014) J/MNRAS/443/1151 : AIMSS Project. I. Compact Stellar Systems (Norris+, 2014) J/ApJ/813/L15 : Dwarf galaxies in Fornax cluster from NGFS (Munoz+, 2015) J/ApJS/225/11 : Subaru-UDGs in the Coma cluster (Yagi+, 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 (NGFS) II. (Eigenthaler+, 2018) J/ApJ/859/52 : NGFS III. Dwarf 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: table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [PCC-] 5- 8 I04 --- PCC [1/5437] Perseus Cluster Catalog number 10- 16 F7.4 deg RAdeg [49.2/50.1] Right Ascension (J2000) 18- 24 F7.4 deg DEdeg [41.1/41.8] Declination (J2000) 26- 30 F5.2 mag Vmag [14/24.3] Integrated WHT V band apparent magnitude; corrected for extinction 32- 39 F8.2 mag e_Vmag [0/0.7]?=-9999 Uncertainty in Vmag 41- 45 F5.2 arcsec R50 [0.1/15.3] Half-light radius 47- 54 F8.2 arcsec e_R50 [0/1.2]?=-9999 Uncertainty in R50 (1) 56- 60 F5.2 mag/arcsec2 mu50 [15.8/26.8] Effective V-band surface brightness within R50; corrected for extinction 62- 69 F8.2 mag/arcsec2 e_mu50 [0/1]?=-9999 Uncertainty in mu50; propagated from e_Vmag and e_R50 71- 74 F4.2 --- n [0.05/4] Sersic index 76- 83 F8.2 --- e_n [0/3.8]?=-9999 Uncertainty in n (2) 85- 92 F8.2 --- b/a [0.1/1]?=-9999 Axis ratio (3) 94-101 F8.2 --- e_b/a [0/1]?=-9999 Uncertainty in b/a (4) 103-109 F7.1 deg PA [-90/90]?=-9999 Position angle (5) 111-117 F7.1 deg e_PA [0/89.3]?=-9999 Uncertainty in PA (5) 119-122 F4.2 mag Av [0.3/0.6] V-band galactic foreground extinction 124-124 I1 --- pFlag [1/9] Photometry processing flag (6) 126-130 I5 --- rFlag [0/1]?=-9999 Residual flag (1=residuals) (7) 132-132 I1 --- bgFlag [0/2]? Background flag (8) 134-141 F8.2 mag (g-r)1 [-0.7/2.3]?=-9999 The (g-r) aperture 1 color index (9) 143-150 F8.2 mag e_(g-r)1 [0/1]?=-9999 Uncertainty in (g-r)1 152-159 F8.2 mag (r-z)1 [-0.7/3.4]?=-9999 The (r-z) aperture 1 color index (9) 161-168 F8.2 mag e_(r-z)1 [0/1]?=-9999 Uncertainty in (r-z)1 170-177 F8.2 mag (g-r)2 [-0.8/2]?=-9999 The (g-r) aperture 2 color index (10) 179-186 F8.2 mag e_(g-r)2 [0/1]?=-9999 Uncertainty in (g-r)2 188-195 F8.2 mag (r-z)2 [-0.2/1.9]?=-9999 The (r-z) aperture 2 color index (10) 197-204 F8.2 mag e_(r-z)2 [0.01/1]?=-9999 Uncertainty in (r-z)2 206-210 I5 --- (g-r)f [0/1]?=-9999 The (g-r) flag (0=not contaminated) (11) 212-216 I5 --- (r-z)f [0/1]?=-9999 The (r-z) flag (0=not contaminated) (11) 218-225 F8.2 mag Ag [0.4/0.7]?=-9999 g-band galactic foreground extinction 227-234 F8.2 mag Ar [0.3/0.5]?=-9999 r-band galactic foreground extinction 236-243 F8.2 mag Az [0.1/0.3]?=-9999 z-band galactic foreground extinction 245-246 I2 --- mFlag [1/11] Morphology flag (12) 248-252 I5 --- nFlag [1/4]?=-9999 Nucleation flag (13) -------------------------------------------------------------------------------- Note (1): For sources fitted with GALFIT with free R50 parameter (pflag=1-5,7) Note (2): For sources fitted with GALFIT with free Sersic n parameter (pflag=1). Note (3): For sources fitted with GALFIT (pflag=1-8). Note (4): For sources fitted with GALFIT with free b/a parameter (pflag=1-4). Note (5): For sources fitted with GALFIT and b/a<0.9. North/Up=0, East/Left=90. Note (6): Photometry processing flag as follows: 1 = GALFIT: Sersic fit with free parameters. 2 = GALFIT: Sersic fit with free parameters but constrained n=4. 3 = GALFIT: Sersic fit with fixed n (derived from Petrosian concentration r90/r50, see this paper, Sect. 4.3). 4 = GALFIT: Sersic fit with fixed n and position. 5 = GALFIT: Sersic fit with fixed n and b/a=0.1. 6 = GALFIT: Sersic fit with fixed n, R50=0.5pix, and b/a=1. 7 = GALFIT: Sersic fit with fixed n, position, and b/a=0.1. 8 = GALFIT: Sersic fit with fixed n, position, R50=0.5pix, and b/a=1. 9 = Petrosian photometry. Note (7): For sources fitted with GALFIT (pflag=1-8). 0 = No residuals after subtracting GALFIT model. 1 = Residuals. Note (8): Background flag as follows: 0 = Background fitted with GALFIT. 1 = SExtractor BACK_SIZE = 256 pixels background map. 2 = SExtractor BACK_SIZE = 32 pixels background map. Note (9): Color corrected for extinction (r_aper1=1R50 for sources with R50>4pix, r_aper1=4pix for sources with R50≤4pix). Note (10): Color corrected for extinction (only for sources with R50>4pix, where r_aper2=2R50). Note (11): Flag for sources with (g-r)1 and / or (g-r)2 colors. 0 = Color not contaminated. 1 = Color possibly comtaminated through bleeding trails of bright stars within 3 arcsec. Note (12): Morphology flag as follows: 1 = Likely dE/ETG cluster candidate. 11 = Possible dE/ETG cluster candidate. 2 = Likely background ETG or unresolved source. 3 = Cluster or background LTG. 4 = Cluster or background galaxy with possibly weak substructure. 5 = Likely cluster or background edge-on disk galaxy. 6 = Likely merging system. Note (13): For likely or possible dE/ETG cluster candidates (mflag=1, mflag=11). Nucleation flag as follows: 1 = Nucleated. 2 = Non-nucleated. 3 = Unsure. 4 = Bulge / Bright central source. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [PCC-] 5- 8 I04 --- PCC [27/5423] Perseus Cluster Catalog number 10- 16 F7.4 deg RAdeg [49.2/50.1] PCC Right Ascension (J2000) 18- 24 F7.4 deg DEdeg [41.2/41.8] PCC Declination (J2000) 26- 35 A10 --- [CG99] Conselice & Gallagher 1999, J/AJ/117/75 identifier; <[CG99] SA426-NN> in Simbad 37- 46 F10.4 deg RA1deg [49.9/50]? LIT1 Right Ascension (J2000) 48- 57 F10.4 deg DE1deg [41.4/41.6]? LIT1 Declination (J2000) 61- 63 I3 --- [BM99] [137/278]? Identifier from Brunzendorf & Meusinger 1999, J/A+AS/139/141 65- 74 F10.4 deg RA2deg [49.3/50]? LIT2 Right Ascension (J2000) 76- 85 F10.4 deg DE2deg [41.2/41.7]? LIT2 Declination (J2000) 87- 96 A10 --- --- [[CGW2003_ ]] 97-110 A14 --- [CGW2003] Conselice+ 2003AJ....125...66C 2003AJ....125...66C identifier (JHHMMSS.s+DDMM) 112-121 F10.4 deg RA3deg [49.7/50]? LIT3 Right Ascension (J2000) 123-132 F10.4 deg DE3deg [41.3/41.6]? LIT3 Declination (J2000) 134-139 A6 --- LIT4 Penny & Conselice 2008MNRAS.383..247P 2008MNRAS.383..247P identifier (<[CGW2003] NN> in Simbad) 141-150 F10.4 deg RA4deg [49.7/50]? LIT4 Right Ascension (J2000) 152-161 F10.4 deg DE4deg [41.3/41.6]? LIT4 Declination (J2000) 166-167 I2 --- LIT5 [12/78]? Penny+ 2012, J/MNRAS/422/885 ID; <[PFC2012] UCDNN> in Simbad 169-178 F10.4 deg RA5deg [49.7/50]? LIT5 Right Ascension (J2000) 180-189 F10.4 deg DE5deg [41.4/41.6]? LIT5 Declination (J2000) 194-195 I2 --- [WLA2017] [1/89]? Wittmann+ 2017, J/MNRAS/470/1512 identifier 197-206 F10.4 deg RA6deg [49.2/50.1]? LIT6 Right Ascension (J2000) 208-217 F10.4 deg DE6deg [41.2/41.8]? LIT6 Declination (J2000) 219-246 A28 --- NED NED identifier 248-257 F10.4 deg RA7deg [49.2/50.1]? LIT7 Right Ascension (J2000) 259-268 F10.4 deg DE7deg [41.2/41.7]? LIT7 Declination (J2000) 270-275 I6 km/s Vel [2886/125580]? NED velocity -------------------------------------------------------------------------------- History: From electronic version of the journal for Table 6. Table 7 sent by the author. Acknowledgements: Carolin Wittmann
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 17-Mar-2020
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