J/ApJS/250/17   NGVS. XXXIV. Ultracompact dwarf galaxies in Virgo   (Liu+, 2020)

The Next Generation Virgo Cluster Survey. XXXIV. Ultracompact dwarf galaxies in the Virgo cluster. Liu C., Cote P., Peng E.W., Roediger J., Zhang H., Ferrarese L., Sanchez-Janssen R., Guhathakurta P., Yang X., Jing Y., Alamo-Martinez K., Blakeslee J.P., Boselli A., Cuilandre J.-C., Duc P.-A., Durrell P., Gwyn S., Jordan A., Ko Y., Lancon A., Lim S., Longobardi A., Mei S., Mihos J.C., Munoz R., Powalka M., Puzia T., Spengler C., Toloba E. <Astrophys. J. Suppl. Ser., 250, 17 (2020)> =2020ApJS..250...17L 2020ApJS..250...17L
ADC_Keywords: Clusters, galaxy; Photometry, ugriz ; Photometry, infrared ; Magnitudes, absolute ; Radial velocities Keywords: Ultracompact dwarf galaxies ; Globular star clusters ; Galaxy nuclei ; Dwarf elliptical galaxies ; Virgo Cluster ; Galaxy formation Abstract: We present a study of ultracompact dwarf (UCD) galaxies in the Virgo cluster based mainly on imaging from the Next Generation Virgo Cluster Survey (NGVS). Using ∼100deg2 of u*giz imaging, we have identified more than 600 candidate UCDs, from the core of Virgo out to its virial radius. Candidates have been selected through a combination of magnitudes, ellipticities, colors, surface brightnesses, half-light radii, and, when available, radial velocities. Candidates were also visually validated from deep NGVS images. Subsamples of varying completeness and purity have been defined to explore the properties of UCDs and compare to those of globular clusters and the nuclei of dwarf galaxies with the aim of delineating the nature and origins of UCDs. From a surface density map, we find the UCDs to be mostly concentrated within Virgo's main subclusters, around its brightest galaxies. We identify several subsamples of UCDs-i.e., the brightest, largest, and those with the most pronounced and/or asymmetric envelopes-that could hold clues to the origin of UCDs and possible evolutionary links with dwarf nuclei. We find some evidence for such a connection from the existence of diffuse envelopes around some UCDs and comparisons of radial distributions of UCDs and nucleated galaxies within the cluster. Description: The primary source of data used in this study is the Next Generation Virgo cluster Survey (NGVS; Ferrarese+ 2012ApJS..200....4F 2012ApJS..200....4F). The survey footprint covers the two main subclusters of Virgo (A and B, centered on M87 and M49, respectively) out to their virial radii (i.e., R200=5.38° for Virgo A and 3.33° for Virgo B). The NGVS imaging consists of short and long exposures, where the former can be used to find ultracompact dwarf (UCD) galaxies brighter than g∼18.5mag. All the NGVS fluxes are obtained with the MegaCam/WirCam instruments on the CFHT (Canada France Hawaii Telescope). In addition to the imaging that forms the basis of this study, there are many past spectroscopic programs targeting the Virgo cluster that we can draw upon. Ferrarese+ 2012ApJS..200....4F 2012ApJS..200....4F summarized the relevant programs for Virgo compact stellar systems (i.e., GCs, UCDs, and dE, Ns) as of 2012; these include radial velocity measurements from various Multiple Mirror Telescope (MMT)/Hectospec, Magellan/IMACS, Very Large Telescope/VIMOS, and Anglo-Australian Telescope (AAT)/AAOmega programs (see the paper for details). Since then, a number of NGVS-motivated spectroscopic programs have been undertaken (see Section 2.1). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 145 828 Photometric properties of ultracompact dwarf (UCD) candidates table4.dat 108 828 Structural properties and other information for UCD candidates -------------------------------------------------------------------------------- See also: II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012) J/AJ/90/1681 : The Virgo Cluster Catalog (VCC) (Binggeli+, 1985) J/A+AS/134/75 : Central Fornax Cluster. II. Galaxy spectrosc. (Hilker+ 1999) J/ApJ/559/812 : Globular cluster system in M87 (Hanes+, 2001) J/A+A/383/823 : Radial velocities of UCOs in Fornax (Mieske+, 2002) J/ApJ/591/850 : Radial velocities of M49 globular clusters (Cote+, 2003) J/ApJS/153/223 : ACS Virgo Cluster Survey. I. (Cote+, 2004) J/A+A/418/445 : FCOS UCD galaxies radial velocities (Mieske+, 2004) J/ApJS/164/334 : ACS Virgo Cluster Survey. VI (Ferrarese+, 2006) J/ApJS/171/101 : GCs in the ACS Virgo cluster survey (Jordan+, 2007) J/ApJ/655/144 : ACS Virgo Cluster Survey. XIII. (Mei+, 2007) J/A+A/472/111 : Centaurus Compact Object Survey (Mieske+, 2007) J/AJ/136/2295 : Ultra-compact dwarf cand. in Abell S0740 (Blakeslee+, 2008) J/A+A/485/657 : Physical param. of Wolf-Rayet galaxies (Brinchmann+, 2008) J/AJ/135/1567 : Bright star clusters in M51 (Hwang+, 2008) J/ApJS/180/54 : GC candidates in ACS Virgo survey. (Jordan+, 2009) J/AJ/142/199 : Sizes and luminosities of stellar systems (Brodie+, 2011) J/ApJ/737/86 : UCD galaxies in the Coma cluster (Chiboucas+, 2011) J/ApJS/197/33 : The M87 globular cluster system (Strader+, 2011) J/MNRAS/422/885 : Ultracompact dwarf galaxies in Perseus (Penny+, 2012) J/ApJ/760/87 : Globular clusters of M60 with HST (Strader+, 2012) J/MNRAS/428/389 : SLUGGS GCs in early-type galaxies (Pota+, 2013) J/A+A/570/A69 : GALEX Ultraviolet Virgo Cluster Survey. IV. (Boselli+, 2014) J/AJ/148/32 : Globular cluster candidates in NGC 3115 (Jennings+, 2014) J/MNRAS/443/1151 : AIMSS Project. I. Compact Stellar Systems (Norris+, 2014) J/ApJ/806/133 : Virgo cluster ETGs: GC and galaxy diffuse light (Li+, 2015) J/ApJ/812/34 : Properties of UCD cand. in M87/M49/M60 regions (Liu+, 2015) J/MNRAS/450/1962 : M60 SLUGGS and Gemini/GMOS combined study (Pota+, 2015) J/ApJ/802/30 : NGVS VI. Ultra-compact dwarfs in M87 (Zhang+, 2015) J/ApJS/227/12 : NGVS XXV. Virgo GCs photometry (Powalka+, 2016) J/A+A/586/A102 : UCDs in the halo of NGC1399 (Voggel+, 2016) J/AJ/153/114 : GCs in 27 nearby ETGs from the SLUGGS survey (Forbes+, 2017) J/ApJ/835/212 : Wide-field spectrosc. survey of GCs in Virgo (Ko+, 2017) J/ApJ/858/102 : Gemini/NIFS and HST obs. of the galaxy M59-UCD3 (Ahn+, 2018) J/A+A/625/A50 : Ultra compact dwarf galaxies catalog (Fahrion+, 2019) http://astrowww.phys.uvic.ca/~lff/NGVS/ : NGVS home page Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq [1/828] Sequential identification number 5- 15 A11 --- Name Ultracompact dwarf (UCD) galaxy name 17- 21 A5 --- --- [NGVS-] 22- 40 A19 --- NGVS Object name in NGVS catalog (JHHMMSS.ss+DDMMSS.s) 42- 42 A1 --- Tobs Exposure time (l=long exposure data; s=short exposure data) 44- 54 F11.7 deg RAdeg [181.71/193.37] Right Ascension (J2000) 56- 65 F10.7 deg DEdeg [4.84/18.19] Declination (J2000) 67- 71 F5.3 mag E(B-V) [0.016/0.07] Galactic extinction according to Schlegel+ 1998ApJ...500..525S 1998ApJ...500..525S 73- 78 F6.3 mag g0mag [15.3/21.5] Galactic extinction-corrected, aperture-corrected CFHT g-band magnitude (1) 80- 84 F5.3 mag e_g0mag [0/0.014] Uncertainty in g0mag 86- 91 F6.3 mag Kmag [11.99/19.03]? UKIDSS K-band magnitude (2) 93- 97 F5.3 mag e_Kmag [0.001/0.35]? Uncertainty in Kmag 99-104 F6.3 mag (u*-g)0 [-0.16/1.76]? u*-g color index (3) 106-110 F5.3 mag e_(u*-g)0 [0.001/0.03]? Uncertainty in (u*-g)0 112-117 F6.3 mag (g-i)0 [-1.23/1.35]? g-i color index (3) 119-123 F5.3 mag e_(g-i)0 [0.001/0.017]? Uncertainty in (g-i)0 125-130 F6.3 mag (g-z)0 [-1.18/1.67] g-z color index (3) 132-136 F5.3 mag e_(g-z)0 [0.001/0.05] Uncertainty in (g-z)0 138-143 F6.3 mag Denv [-2.11/0.69] Envelop parameter Δenv (4) 145-145 I1 --- UCD? [0/1] Object flag (1=confirmed or possible UCD; 0=contaminant) -------------------------------------------------------------------------------- Note (1): Galactic extinction-corrected, aperture-corrected g-band magnitude found within a 16 pixels (∼3") diameter aperture. For details, see Liu+ 2015, Cat. J/ApJ/812/34 Note (2): Lawrence+ (2007MNRAS.379.1599L 2007MNRAS.379.1599L -- see II/319) UKIDSS K-band magnitude within a 3-arcsec diameter aperture. Note (3): Color indices measured in an 8-pixel (∼1.5") diameter aperture, Galactic extinction corrected. Note (4): Envelop parameter, Δenv≡g16-g32, where g16 and g32 are magnitudes in 16- and 32-pixel diameter apertures; -------------------------------------------------------------------------------- Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Ultracompact dwarf (UCD) galaxy name 13- 18 F6.2 mag BMAG [-15.3/-9.2]? Absolute B band magnitude (5) 20- 25 F6.2 mag VMAG [-14.6/-8.6]? Absolute V band magnitude (5) 27- 31 F5.2 pc rh [11/96.7] Weighted mean half-light radius (6) 33- 36 F4.2 pc e_rh [0.01/9.1] Uncertainty in rh 38- 40 F3.1 [Msun] Mstar [5.3/8.9] log of stellar mass 42- 47 I6 km/s HRV [-420/222826]? Heliocentric radial velocity (7) 49- 81 A33 --- r_HRV Source for HRV (8) 83- 83 I1 --- Cl [1/6] Class parameter (9) 85- 85 I1 --- Env [0/1] Envelope (1=has obvious envelope) 87- 88 A2 --- Meth Selection method (10) 90-108 A19 --- OName Altenative names, if available -------------------------------------------------------------------------------- Note (5): Absolute magnitudes calculated using the transformation equations, B=u*-0.8116(u*-g)+0.1313, and V=g-0.2906(u*-g)+0.0885 (Lupton 2005; http://www.sdss3.org/dr10/algorithms/sdssUBVRITransform.php#Lupton2005) and a distance modulus of 31.1mag from Mei+ 2007ApJ..655...144M 2007ApJ..655...144M and Blakeslee+ 2009ApJ..694...556B 2009ApJ..694...556B Note (6): Weighted mean half-light radius in the g and i bands, or rh=rh,g if an i-band measurement is not available. Note (7): Heliocentric radial velocity or weighted mean value if multiple measurements are available. Note (8): The source of our adopted HRV measurement as follows: SDSS = Abolfathi+ 2018ApJS..235...42A 2018ApJS..235...42A NED = NASA/IPAC Extragalactic Database; SIMBAD = SIMBAD Astronomical Database (Wenger+ 2000A&AS..143....9W 2000A&AS..143....9W) VCC = The Virgo Cluster Catalog; Binggeli+ 1985, J/AJ/90/1681 NTT17 = NTT 2017 program; AAT12 = Anglo-Australian Telescope (AAT)/AAOmega 2012 program; MMT09 = Multiple Mirror Telescope (MMT)/Hectospec 2009 program; Toloba2018 = Toloba et al. 2018ApJ...856L..31T 2018ApJ...856L..31T Ko2017 = Ko et al. 2017, J/ApJ/835/212 MMT14 = Multiple Mirror Telescope (MMT)/Hectospec 2014 program; Keck = Keck program; C03 = Cote et al. 2003, J/ApJ/591/850 IMACS16 = Megallan/IMACS 2016 program; S11 = Strader et al. 2011ApJS..197...33S 2011ApJS..197...33S Note (9): Class parameter as follows: 1 = probable UCD (612 occurrences); 2 = dwarf nucleus (41 occurrences); 3 = background galaxy (132 occurrences); 4 = blended object (12 occurrences); 5 = star (14 occurrences); 6 = star-forming region (17 occurrences). Note (10): Selection method (See Table 2) as follows: m1 = Radial velocity cut (HRV<3500km/s) + half-light radius (rh) cut; m2 = gz color selection + surface brightness (muge) cut + g band half-light radius (rhg) cut; m3 = gzK color selection + surface brightness (muge) cut + half-light radius (rh) cut; m4 = gzK color selection + surface brightness (muge) cut + g band half-light radius (rhg) cut; m5 = u*gz color selection + surface brightness (muge) cut + half-light radius (rh) cut; m6 = u*gz color selection + surface brightness (muge) cut + g band half-light radius (rhg) cut; m7 = u*gzK color selection + surface brightness (muge) cut + half-light radius (rh) cut; m8 = u*gzK color selection + surface brightness (muge) cut + g band half-light radius (rhg) cut. -------------------------------------------------------------------------------- History: From electronic version of the journal References: Ferrarese et al. Paper I. 2012ApJS..200....4F 2012ApJS..200....4F Paudel et al. Paper IV. 2013ApJ...767..133P 2013ApJ...767..133P Zhu et al. Paper V. 2014ApJ...792...59Z 2014ApJ...792...59Z Zhang et al. Paper VI. 2015ApJ...802...30Z 2015ApJ...802...30Z Cat. J/ApJ/802/30 Sanchez-Janssen et al. Paper VII. 2016ApJ...820...69S 2016ApJ...820...69S Durrell et al. Paper VIII. 2014ApJ...794..103D 2014ApJ...794..103D Grossauer et al. Paper IX. 2015ApJ...807...88G 2015ApJ...807...88G Liu et al. Paper X. 2015ApJ...812...34L 2015ApJ...812...34L Cat. J/ApJ/812/34 Raichoor et al. Paper XI. 2014ApJ...797..102R 2014ApJ...797..102R Guerou et al. Paper XII. 2015ApJ...804...70G 2015ApJ...804...70G Ferrarese et al. Paper XIII. 2016ApJ...824...10F 2016ApJ...824...10F Ferrarese et al. Paper XIV. 2020ApJ...890..128F 2020ApJ...890..128F Cat. J/ApJ/890/128 Raichoor et al. Paper XV. 2014ApJ...797..102R 2014ApJ...797..102R Toloba et al. Paper XVI. 2016ApJ...822...51T 2016ApJ...822...51T Sun et al. Paper XVII. 2019ApJ...885..145S 2019ApJ...885..145S Cantiello et al. Paper XVIII. 2018ApJ...856..126C 2018ApJ...856..126C Lokhorst et al. Paper XIX. 2016ApJ...819..124L 2016ApJ...819..124L Licitra et al. Paper XX. 2016ApJ...829...44L 2016ApJ...829...44L Cat. J/ApJ/829/44 Parroni et al. Paper XXI. 2017ApJ...848..114P 2017ApJ...848..114P Paudel et al. Paper XXII. 2017ApJ...834...66P 2017ApJ...834...66P Sanchez-Janssen et al. Paper XXIII. 2019ApJ...878...18S 2019ApJ...878...18S Cat. J/ApJ/878/18 Roediger et al. Paper XXIV. 2017ApJ...836..120R 2017ApJ...836..120R Powalka et al. Paper XXV. 2016ApJS..227...12P 2016ApJS..227...12P Cat. J/ApJS/227/12 Powalka et al. Paper XXVI. 2017ApJ...844..104P 2017ApJ...844..104P Fantin et al. Paper XXVIII. 2017ApJ...843...53F 2017ApJ...843...53F Lim et al. Paper XXX. 2020ApJ...899...69L 2020ApJ...899...69L Longobardi et al. Paper XXXI. 2018ApJ...864...36L 2018ApJ...864...36L Powalka et al. Paper XXXII. 2018ApJ...856...84P 2018ApJ...856...84P Liu et al. Paper XXXIV. 2020ApJS..250...17L 2020ApJS..250...17L This catalog
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 02-Nov-2020
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