J/MNRAS/460/4492 Nearby early-type galaxies catalog (Dabringhausen+, 2016)
An extensive catalogue of early-type galaxies in the nearby Universe.
Dabringhausen J., Fellhauer M.
<Mon. Not. R. Astron. Soc. 460, 4492 (2016)>
=2016MNRAS.460.4492D 2016MNRAS.460.4492D (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, nearby ; Galaxy catalogs ; Photometry ;
Radial velocities ; Morphology
Keywords: galaxies: abundances - galaxies: distances and redshifts -
galaxies: dwarf - galaxies: elliptical and lenticular, CD -
galaxies: kinematics and dynamics - galaxies: photometry
Description:
We present a catalogue of 1715 early-type galaxies from the
literature, spanning the luminosity range from faint dwarf spheroidal
galaxies to giant elliptical galaxies. The aim of this catalogue is to
be one of the most comprehensive and publicly available collections of
data on early-type galaxies. The emphasis in this catalogue lies on
dwarf elliptical galaxies, for which some samples with detailed data
have been published recently. For almost all of the early-type
galaxies included in it, this catalogue contains data on their
locations, distances, redshifts, half-light radii, the masses of their
stellar populations and apparent magnitudes in various passbands. Data
on metallicity and various colours are available for a majority of the
galaxies presented here. The data on magnitudes, colours,
metallicities and masses of the stellar populations is supplemented
with entries that are based on fits to data from simple stellar
population models and existing data from observations. Also, some
simple transformations have been applied to the data on magnitudes,
colours and metallicities in this catalog, in order to increase the
homogeneity of this data. Estimates on the Sersic profiles, internal
velocity dispersions, maximum rotational velocities, dynamical masses
and ages are listed for several hundreds of the galaxies in this
catalogue. Finally, each quantity listed in this catalogue is
accompanied with information on its source, so that users of this
catalogue can easily exclude data that they do not consider as
reliable enough for their purposes.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 104 1715 Different designations of the galaxies in this
catalogue in the literature
table2.dat 53 1715 Positions, distances and redshifts.
table5.dat 72 1715 Apparent magnitudes in the Johnson-Cousins
system
table6.dat 89 1715 Apparent magnitudes in the SDSS system.
table7.dat 72 1715 Solar luminosities in the Johnson-Cousins system
table8.dat 89 1715 Solar luminosities in the SDSS system
table9.dat 46 1715 Colours in the Johnson-Cousins system
table10.dat 60 1715 Colours in the SDSS system
table11.dat 112 1715 Radii, Sersic-indices, internal velocity
dispersions, rotational velocities, and
dynamical masses
table15.dat 63 1715 Properties of the stellar populations of the
galaxies
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 9 I4 --- NGC ?=0 Identification number of the galaxy in the
New General Catalog by Dreyer
(1888MmRAS..49....1D 1888MmRAS..49....1D, Cat. VII/118)
10- 13 A4 --- m_NGC Multiplicity index on NGC
15- 18 I4 --- IC ?=0 Identification number of the galaxy in the
Index Catalog by Dreyer (1895MmRAS..51..185D 1895MmRAS..51..185D,
Cat. VII/118)
20- 24 I5 --- UGC ?=0 Identification number of the galaxy in the
Uppsala General Catalogue of Galaxiesi
(Cat. VII/26)
25- 30 A6 --- m_UGC Multiplicity index on UGC
32- 37 I6 --- AGC ?=0 Identification number of the galaxy in the
Arecibo General Catalog
39- 45 I7 --- PGC ?=0 Identification number of the galaxy in the
Principal Galaxy Catalog (Cat. VII/237) (1)
47- 53 A7 --- CGCG ?=0 Identification code of the galaxy in the
Catalogue of Galaxies and Clusters of Galaxies
by Zwicky et al. (1968, Cat. VII/49)
54- 57 A4 --- m_CGCG Multiplicity index on CGCG
59- 62 I4 --- VCC ?=0 Identification number of the galaxy in the
Virgo Cluster Catalog by Binggeli et al.
(1985, Cat. J/AJ/90/1681)
64- 67 I4 --- GMP ?=0 Identification number of the galaxy in the
catalogue of galaxies in the Coma cluster
by (Goodwin et al., 1983, Cat. VII/42)
69- 71 I3 --- FCC ?=0 Identification number of the galaxy in the
Fornax Cluster Catalog by (Ferguson, 1989,
Cat. VII/180)
73- 74 I2 --- LLH ?=0 Identification number of the galaxy in the
catalogue of Virgo cluster galaxies by
Lieder et al. (2012, Cat. J/A+A/538/A69)
76- 79 A4 --- CCC ?=0 Identification code of the galaxy in the
catalogue of Centaurus cluster galaxies by
Misgeld et al. (2009, Cat. J/A+A/496/683)
81- 83 I3 --- HCC ?=0 Identification number of the galaxy in the
Hydra Cluster Catalog by Misgeld et al.
(2008, Cat. J/A+A/486/697)
85- 86 I2 --- A496 ?=0 Identification number of the galaxy in the
catalogue of galaxies in the galaxy cluster
Abell 496 by Chilingarian et al.
(2008, Cat. J/A+A/486/85)
88-104 A17 --- OName Other names or designations for the galaxies.
The dwarf galaxies in the Local Group are
often only known by those names
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Note (1): This is the primary identification used for the objects listed in
HyperLeda (Marakov et al., 2014A&A...570A..13M 2014A&A...570A..13M)
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 7 I2 h RAh Right ascension (J2000.0)
9- 10 I2 min RAm Right ascension (J2000.0)
12- 15 F4.1 s RAs Right ascension (J2000.0)
17 A1 --- DE- Declination sign (J2000.0)
18- 19 I2 deg DEd Declination (J2000.0)
21- 22 I2 arcmin DEm Declination (J2000.0)
24- 25 I2 arcsec DEs Declination (J2000.0)
27 I1 --- r_RAh [1/2] Source for right ascension and
declination (1)
29- 35 F7.3 Mpc Dist Mean redshift independent distance of
the galaxy
37- 38 I2 --- o_Dist Number of individual estimates from which D is
estimated
40- 42 I3 --- r_Dist (1-4 101-107) Source for Dist (2)
44- 49 I6 km/s RV ?=0 Radial velocity of the galaxy
51- 53 I3 --- r_RV (1-5 101-107) Source for RV (3)
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Note (1): References for position as follows:
1 = NASA/IPAC Extragalactic Database (NED)
2 = Chilingarian et al. (2008, Cat. J/A+A/486/85)
Note (2): References for distances as follows:
1 = NED
2 = Cappellari et al. (2013, Cat. J/MNRAS/413/813)
3 = Toloba et al. (2012A&A...548A..78T 2012A&A...548A..78T)
4 = Guerou et al. (2015ApJ...804...70G 2015ApJ...804...70G)
101 = directly with Eq. 1 from the z of the galaxy
102 = galaxy is considered a member of the Virgo Cluster, and the estimate for
its distance is based on that membership. The distance of the galaxy
is then considered to be 16.5Mpc.
103 = galaxy is considered to be a member one of the galaxy clusters NGC 383,
NGC 507, Abell 262, Cancer, Abell 1367, Coma, Pegasus or Abell 2634,
and the estimate for its distance is based on that membership.
The heliocentric velocity, vhel of those galaxy clusters is given in
Scodeggio et al. (1998, Cat. J/AJ/116/2728)
104 = for galaxies that Chilingarian et al. (2008, Cat. J/A+A/486/85) consider
members of the galaxy cluster Abell 496, with a distance of 133Mpc.
105 = galaxy is considered to be a member of the Fornax Galaxy Cluster, and
the estimate for its distance is based on that membership. The distance
to the Fornax Cluster considered to be 18.967Mpc.
106 = galaxy is considered to be a member of the Hydra Galaxy Cluster, and the
estimate for its distance is based on that membership. The distance
to the Hydra Cluster is considered to be 47.206Mpc
107 = galaxy is considered to be a member of the Centaurus Galaxy Cluster,
and the estimate for its distance is based on that membership. The
distance to the Centaurus Cluster is considered to be 45.290Mpc.
Note (3): References for radial velocities as follows:
1 = NED
2 = Kourkchi et al. (2012MNRAS.420.2835K 2012MNRAS.420.2835K)
3 = Chilingarian et al. (2008, Cat. J/A+A/486/85)
4 = Hyper-Leda
5 = Scodeggio et al. (1998, Cat. J/AJ/116/2728)
101 = calculated from Eq. (1) from a redshift-independent estimate of Dist
102 = galaxy is considered to be a member of the Local Group, and its value
for RV has been set to 0km/s
103 = galaxy is considered to be a member of the Virgo Cluster, and its value
for RV has been calculated with Eq. (1) using the distance to the Virgo
Cluster. The distance to the Virgo Cluster is 16.5Mpc according to
Mei et al. (2007, Cat. J/ApJ/655/144), leading to RV=1172km/s.
104 = galaxy is considered to be a member of the Fornax Cluster, and its value
for RV has been calculated with Eq. (1) using the distance to the
Fornax Cluster. The distance to the Fornax Cluster is 18.967Mpc
according to Freedman et al. (2001ApJ...553...47F 2001ApJ...553...47F), leading to
RV=1347km/s.
105 = galaxy is considered to be a member of the Hydra Cluster, and its value
for RV has been calculated with Eq. (1) using the distance to the
Hydra Cluster. The distance to the Hydra Cluster is 47.206Mpc according
to Mieske et al. (2005A&A...438..103M 2005A&A...438..103M), leading to RV=3352km/s.
106 = galaxy is considered to be a member of the Centaurus Cluster, and its
value for RV has been calculated with Eq. (1) using the distance to
the Centaurus Cluster. The distance to the Centaurus Cluster is
45.290Mpc according to Mieske et al. (2005A&A...438..103M 2005A&A...438..103M), leading to
RV=3216km/s.
107 = galaxies in the Local Group with whose RV have been set to 0km/s,
since their true RV is unknown
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Byte-by-byte Description of file: table5.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 10 F5.2 mag Umag ?=-9.99 Galaxy apparent Johnson U-band
magnitude (G1)
12- 16 F5.2 mag e_Umag ?=-9.99 Uncertainty of Umag
18- 21 I4 --- r_Umag ?=0 (0-2 1002, 1010, 1012) Source for Umag (G2)
23- 27 F5.2 mag Bmag ?=-9.99 Galaxy apparent Johnson B-band
magnitude (G1)
29- 33 F5.2 mag e_Bmag ?=-9.99 Uncertainty of Bmag
35- 38 I4 --- r_Bmag ?=0 (0-5 1002, 1012) Source for Bmag (G2)
40- 44 F5.2 mag Vmag ?=-9.99 Galaxy apparent Johnson V-band
magnitude (G1)
46- 50 F5.2 mag e_Vmag ?=-9.99 Uncertainty of Vmag
52- 55 I4 --- r_Vmag ?=0 (0/10 1023) Source for Vmag (G2)
57- 61 F5.2 mag Imag ?=-9.99 Galaxy apparent Cousins I-band
magnitude (G1)
63- 67 F5.2 mag e_Imag ?=-9.99 Uncertainty of Imag
69- 72 I4 --- r_Imag ?=0 (0-7, 1005, 1040, 1045) Source for Imag (G2)
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Byte-by-byte Description of file: table6.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 10 F5.2 mag umag ?=-9.99 Galaxy apparent SDSS u-band magnitude (G1)
12- 16 F5.2 mag e_umag ?=-9.99 Uncertainty of umag
18- 21 I4 --- r_umag ?=0 (0-2, 1002, 1012) Source for umag (G3)
23- 27 F5.2 mag gmag ?=-9.99 Galaxy apparent SDSS g-band magnitude (G1)
29- 33 F5.2 mag e_gmag ?=-9.99 Uncertainty of gmag
35- 38 I4 --- r_gmag ?=0 (0-2, 1002, 1012) Source for gmag (G3)
40- 44 F5.2 mag rmag ?=-9.99 Galaxy apparent SDSS r-band magnitude (G1)
46- 50 F5.2 mag e_rmag ?=-9.99 Uncertainty of rmag
52- 55 I4 --- r_rmag ?=0 (0-2 1004 1030 1034) Source for rmag (G3)
57- 61 F5.2 mag imag ?=-9.99 Galaxy apparent SDSS i-band magnitude (G1)
63- 67 F5.2 mag e_imag ?=-9.99 Uncertainty of imag
69- 72 I4 --- r_imag ?=0 (0-2 1004) Source for imag (G3)
74- 78 F5.2 mag zmag ?=-9.99 Galaxy apparent SDSS z-band magnitude (G1)
80- 84 F5.2 mag e_zmag ?=-9.99 Uncertainty of zmag
86- 89 I4 --- r_zmag ?=0 (0-2 1004) Source for zmag (G3)
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Byte-by-byte Description of file: table7.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 10 F5.2 Lsun ULum ?=-9.99 U-band luminosity of the galaxy (G1)
12- 16 F5.2 Lsun e_ULum ?=-9.99 Uncertainty of ULum
18- 21 I4 --- r_ULum ?=0 (0-2 1002 1010 1012) Source for ULum (G2)
23- 27 F5.2 Lsun BLum ?=-9.99 B-band luminosity of the galaxy (G1)
29- 33 F5.2 Lsun e_BLum ?=-9.99 Uncertainty of BLum
35- 38 I4 --- r_BLum ?=0 (0-5 1002 1012) Source for BLum (G2)
40- 44 F5.2 Lsun VLum ?=-9.99 V-band luminosity of the galaxy (G1)
46- 50 F5.2 Lsun e_VLum ?=-9.99 Uncertainty of VLum
52- 55 I4 --- r_VLum ?=0 (0-10 1023) Source for VLum (G2)
57- 61 F5.2 Lsun ILum ?=-9.99 I-band luminosity of the galaxy (G1)
63- 67 F5.2 Lsun e_ILum ?=-9.99 The uncertainty of ILum
69- 72 I4 --- r_ILum ?=0 (0-7 1005 1040 1045) Source for ILum (G2)
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Byte-by-byte Description of file: table8.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 10 F5.2 Lsun uLum ?=-9.99 Galaxy SDSS u-band luminosity (G1)
12- 16 F5.2 Lsun e_uLum ?=-9.99 Uncertainty of uLum
18- 21 I4 --- r_uLum ?=0 (0-2 1002 1012) Source for uLum (G3)
23- 27 F5.2 Lsun gLum ?=-9.99 Galaxy SDSS g-band luminosity (G1)
29- 33 F5.2 Lsun e_gLum ?=-9.99 Uncertainty of gLum
35- 38 I4 --- r_gLum ?=0 (0-2 1002 1012) Source for gLum (G3)
40- 44 F5.2 Lsun rLum ?=-9.99 Galaxy SDSS r-band luminosity (G1)
46- 50 F5.2 Lsun e_rLum ?=-9.99 Uncertainty of rLum
52- 55 I4 --- r_rLum ?=0 (0-2 1004 1030 1034) Source for rLum (G3)
57- 61 F5.2 Lsun iLum ?=-9.99 Galaxy SDSS i-band luminosity (G1)
63- 67 F5.2 Lsun e_iLum ?=-9.99 Uncertainty of iLum
69- 72 I4 --- r_iLum ?=0 (0-2 1004) Source for iLum (G3)
74- 78 F5.2 Lsun zLum ?=-9.99 Galaxy SDSS z-band luminosity (G1)
80- 84 F5.2 Lsun e_zLum ?=-9.99 Uncertainty of zLum
86- 89 I4 --- r_zLum ?=0 (0-1 1004) Source for zLum (G3)
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Byte-by-byte Description of file: table9.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 10 F5.2 mag U-B ?=-9.99 Galaxy Johnson U-B-colour index (G1)
12- 16 F5.2 mag e_U-B ?=-9.99 Uncertainty of U-B
18 I1 --- r_U-B [0/2]?=0 Source for U-B (G2)
20- 24 F5.2 mag B-V ?=-9.99 Galaxy Johnson B-V-colour index (G1)
26- 30 F5.2 mag e_B-V ?=-9.99 Uncertainty of B-V
32 I1 --- r_B-V [0/5]?=0 Source for B-V (G2)
34- 38 F5.2 mag V-I ?=-9.99 Galaxy Johnson-Cousins V-I-colour
index (G1)
40- 44 F5.2 mag e_V-I ?=-9.99 Uncertainty of V-I
46 I1 --- r_V-I [0/7]?=0 Source for V-I (G2)
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Byte-by-byte Description of file: table10.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 10 F5.2 mag u-g ?=-9.99 SDSS u-g-colour of the galaxy (G1)
12- 16 F5.2 mag e_u-g ?=-9.99 Uncertainty of u-g
18 I1 --- r_u-g [0/2]?=0 Source for u-g (G3)
20- 24 F5.2 mag g-r ?=-9.99 SDSS g-r-colour of the galaxy (G1)
26- 30 F5.2 mag e_g-r ?=-9.99 Uncertainty of g-r
32 I1 --- r_g-r [0/2]?=0 Source for g-r (G3)
34- 38 F5.2 mag g-i ?=-9.99 SDSS g-i-colour of the galaxy (G1)
40- 44 F5.2 mag e_g-i ?=-9.99 The uncertainty of g-i
46 I1 --- r_g-i [0/2]?=0 Source for g-i (G3)
48- 52 F5.2 mag g-z ?=-9.99 SDSS g-z-colour of the galaxy (G1)
54- 58 F5.2 mag e_g-z ?=-9.99 Uncertainty of g-z
60 I1 --- r_g-z [0/1]?=0 Source for g-z (G3)
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Byte-by-byte Description of file: table11.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 13 F8.1 pc Re ?=-9.9 Effective half-light radius of the
galaxy
15- 21 F7.1 pc e_Re ?=-9.9 Uncertainty of Re
23- 24 I2 --- r_Re [0/15]?=0 Source for Re (1)
26- 29 F4.1 --- sersic ?=-9.9 Best-fitting Sersic-index of the galaxy
31- 34 F4.1 --- e_sersic ?=-9.9 Uncertainty of the Sersic index
36 I1 --- r_sersic [0/5]?=0 Source for the Sersic index (2)
38- 42 F5.1 km/s sige ?=-9.9 Internal velocity dispersion within Re
of the galaxy
44- 47 F4.1 km/s E_sige ?=-9.9 Positive uncertainty of sige
49- 52 F4.1 km/s e_sige ?=-9.9 Negative uncertainty of sige
54- 56 I3 --- r_sige ?=0 (0-14 101) Source for sige (3)
58- 62 F5.1 km/s sig0 ?=-9.9 Internal velocity dispersion at the
centre of the galaxy
64- 67 F4.1 km/s E_sig0 ?=-9.9 Positive uncertainty of sig0
69- 72 F4.1 km/s e_sig0 ?=-9.9 Negative uncertainty of sig0
74- 76 I3 --- r_sig0 ?=0 (0-2 101) Source for sig0 (4)
78- 82 F5.1 km/s vrot ?=-9.9 Rotational velocity of the galaxy
84- 87 F4.1 km/s E_vrot ?=-9.9 Positive uncertainty of vrot
89- 92 F4.1 km/s e_vrot ?=-9.9 Negative uncertainty of vrot
94 I1 --- r_vrot [0/6]?=0 Source for vrot (5)
96-101 F6.2 [Msun] logMdyn ?=-99.99 Estimate for the dynamical mass of the
galaxy (logarithm to the base of 10 of Mdyn)
103-108 F6.2 [Msun] e_logMdyn ?=-99.99 Logarithmic uncertainty to the value
on Mdyn
110-112 I3 --- r_logMdyn ?=0 (0-1 101) Source for the estimates on
Mdyn (6)
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Note (1): References for Re as follows:
0 = no data available
1 = galaxy is included in the ATLAS3D survey, and that Re has been taken from
Cappellari et al. (2013, Cat. J/MNRAS/413/813)
2 = based on the data in Bender et al. (1992ApJ...399..462B 1992ApJ...399..462B)
3 = based on the angular Re in the g-band in Ferrarese et al.
(2006, Cat. J/ApJS/164/334)
4 = based on the angular Re in Toloba et al. (2014ApJS..215...17T 2014ApJS..215...17T)
5 = based on the angular Re in Geha et al. (2003AJ....126.1794G 2003AJ....126.1794G)
6 = galaxy is part of the Coma cluster and its Re is based on the physical
Re published by Kourkchi et al. (2012MNRAS.420.2835K 2012MNRAS.420.2835K)
7 = galaxies in the cluster Abell 496 whose Re are based on their angular Re
in Chilingarian et al. (2008, Cat. J/A+A/486/85).
8 = Re is based on the angular Re of galaxies published in
Scodeggio et al. (1998, Cat. J/AJ/116/2728)
9 = part of the Virgo cluster and its Re is based on the angular Re from
Ferguson (1989. Cat. VII/180)
10 = Re is estimated from angular semi-major axes published by
McConnachie (2012, Cat. J/AJ/144/4) on galaxies in the Local Group.
11 = galaxy is part of the Virgo cluster and its Re is based on the physical
Re published by Lieder et al. (2012, Cat. J/A+A/538/A69)
12 = Hydra cluster whose Re is based on the angular Re in
Misgeld et al. (2008, Cat. J/A+A/486/697)
13 = galaxies in the Centaurus cluster whose Re is based on their angular Re
in Misgeld et al. (2009, Cat. J/A+A/496/683)
14 = galaxies in the Virgo cluster whose for Re is based on their angular Re
in Toloba et al. (2014ApJS..215...17T 2014ApJS..215...17T)
15 = Re is based on the values for the physical Re published by
Guerou et al. (2015ApJ...804...70G 2015ApJ...804...70G)
Note (2): References for Sersic-index as follows:
0 = no data available
1 = from Krajnovic et al. (2013MNRAS.432.1768K 2013MNRAS.432.1768K)
2 = from Toloba et al. (2014ApJS..215...17T 2014ApJS..215...17T)
3 = from Geha et al. (2003AJ....126.1794G 2003AJ....126.1794G)
4 = from Kourkchi et al. (2012MNRAS.420.2835K 2012MNRAS.420.2835K)
5 = from Guerou et al. (2015ApJ...804...70G 2015ApJ...804...70G)
Note (3): References for sige as follows:
0 = no data available
1 = galaxy is included in the ATLAS3D survey and value is taken from
Cappellari et al. (2013, Cat. J/MNRAS/413/813)
2 = fromForbes et al. (2011MNRAS.413.2665F 2011MNRAS.413.2665F)
3 = from Guerou et al. (2015ApJ...804...70G 2015ApJ...804...70G)
4 = from Toloba et al. (2014ApJS..215...17T 2014ApJS..215...17T)
5 = from Geha et al. (2003AJ....126.1794G 2003AJ....126.1794G)
6 = from Kourkchi et al. (2012MNRAS.420.2835K 2012MNRAS.420.2835K)
7 = from Chilingarian et al. (2008, Cat. J/A+A/486/85)
8 = from Scodeggio et al. (1998, Cat. J/AJ/116/2738)
9 = from Thomas et al. (2005, Cat. J/ApJ/621/673)
10 = from Matkovic et al. (2009, Cat. J/ApJ/691/1862)
11 = from Sanchez-Blazquez et al. (2006A&A...457..809S 2006A&A...457..809S)
12 = galaxy is part of the Local Group and sige is based on the internal
velocity dispersion given in McConnachie (2012, Cat. J/AJ/144/4)
13 = galaxy is part of the Local group and that its value is taken from
HyperLeda
14 = from Koleva et al. (2011MNRAS.417.1643K 2011MNRAS.417.1643K)
101 = no value for sige has been published, while a value for sig0 is
available. It is then assumed that sige=sig0, if Re≤1kpc.
If Re>1 kpc, sige is calculated from sig0 with Eq. (11).
Note (4): References for sig0 as follows:
0 = no data available
1 = galaxy is included in the ATLAS3D survey, and that the value for sig0 is
taken from Cappellari et al. (2013, Cat. J/MNRAS/413/813)
2 = value is taken from Bender et al. (1992ApJ...399..462B 1992ApJ...399..462B)
101 = no value has been published, while a value for sige is available.
It is then assumed that sig0=sige, if Re≤1kpc.
If Re>1kpc, sig0 is calculated from sige with Eq. (12).
Note (5): References for vrot as follows:
0 = no available data
1 = galaxy is included in the ATLAS3D survey and the estimate of vrot is
based on the data given in Emsellem et al. (2011, Cat J/MNRAS/414/888)
2 = from Toloba et al. (2014ApJS..215...17T 2014ApJS..215...17T)
3 = from Geha et al. (2003AJ....126.1794G 2003AJ....126.1794G)
4 = based on the values for the rotational velocities from
McConnachie (2012, Cat. J/AJ/144/4)
5 = from HyperLeda
6 = from Scodeggio et al. (1998, Cat. J/AJ/116/2738)
Note (6): References for vrot logMdyn as follows:
0 = no available data
1 = galaxy is included in the ATLAS3D survey, and that the value for Mdyn is
taken from Cappellari et al. (2013, Cat. J/MNRAS/413/813).
101 = Mdyn is calculated with Eq. (13) from the data on Re, n and sig0 in
Table 11
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Byte-by-byte Description of file: table15.dat
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Bytes Format Units Label Explanations
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1- 4 I4 --- Seq Running number of the galaxy in this catalogue
6- 9 F4.1 Gyr t ?=-9.9 SSP-equivalent age of the stellar
population of the galaxy
11- 14 F4.1 Gyr E_t ?=-9.9 Positive uncertainty of t
16- 19 F4.1 Gyr e_t ?=-9.9 Negative uncertainty of t
21 I1 --- r_t [0/8]?=0 Source for t (1)
23- 27 F5.2 [Sun] [Z/H] ?=99.99 SSP-equivalent metal abundance
(logarithm to the base of 10) of the galaxy
29- 33 F5.2 [Sun] E_[Z/H] ?=99.99 Positive logarithmic uncertainty of
[Z/H]
35- 39 F5.2 [Sun] e_[Z/H] ?=99.99 Negative uncertainty of [Z/H]
41- 44 I4 --- r_[Z/H] ?=0 (0/8 101 1020) Source for the estimate
of [Z/H] (1)
46- 51 F6.2 [Msun] logMs ?=-99.99 Mass of the stellar population of the
galaxy (logarithm to the base of 10 of Ms)
53- 58 F6.2 [Msun] e_logMs ?=-99.99 Logarithmic uncertainty to the values
of Ms
60- 63 I4 --- r_logMs ?=0 (0/1 1000 1010 1011 1020 1021) Source for
the estimate of Ms (3)
--------------------------------------------------------------------------------
Note (1): References for t and [Z/H] as follows:
0 = no data available
1 = galaxy is included in the ATLAS3D survey, and that the quoted value for t
is taken from Cappellari et al. (2013, Cat. J/MNRAS/413/813)
2 = from Thomas et al. (2005, Cat. J/ApJ/621/673)
3 = galaxy is part of the Coma Cluster and its t is taken from
Matkovic et al. (2009, Cat. J/ApJ/691/1862)
4 = galaxy is part of the Coma Cluster and its t is taken from
Sanchez-Blazquez et al. (2006A&A...457..809S 2006A&A...457..809S)
5 = galaxy is part of the cluster Abell 496 and its t is taken from
Chilingarian et al. (2008, Cat. J/A+A/486/85)
6 = from Weisz et al. (2014) for t or
from McConnachie (2012, Cat. J/AJ/144/4) for [Z/H]
7 = galaxy is part of the Virgo Cluster and its t is taken from
Toloba et al. (2014ApJS..215...17T 2014ApJS..215...17T)
8 = galaxy is part of the Virgo Cluster and its t is taken from
Guerou et al. (2015ApJ...804...70G 2015ApJ...804...70G)
1010 = if (g-r), (g-i) and LV of the galaxy are available, but t is unknown
for it. In this case, its t is assumed to be equal to the mean t of
galaxies with similar LV, as listed in table 14. Its [Z/H] is then
estimated using Eq. (15) with the appropriate entries in table 12.
1020 = if (B-V) and LV of the galaxy are available, but its (g-r), (g-i) and
t are unknown. In this case, its t is assumed to be equal to the mean
t of galaxies with similar LV, as listed in table 14.
Its [Z/H] is then estimated on this basis, using Eq. (18) with
the appropriate entries in table (13)
Note (3): References for logMs as follows:
0 = no data available
1 = galaxy is a member of the Local Group and its estimate for Ms is taken
from table 1 in Misgeld & Hilker (2011, Cat. J/MNRAS/414/3699)
1000 = if only LV of the galaxy is available, while its (g-r), (g-i), (B-V)
and t are unknown. In this case, its (g-r), (g-i) and age is assumed to
be equal to the mean (g-r), (g-i) and t of galaxies with similar LV,
as listed in table 14. Its Ms is then estimated on this basis, using
Eq. (18) with the appropriate entries in table 13.
1010 = (g-r), (g-i) and LV of the galaxy are available, but t is unknown for
it. In this case, t is assumed to be equal to the mean age of galaxies
with similar LV, as listed in table 14. Ms is then estimated for it on
this basis, using Eq. (18) with the appropriate entries in table 13.
1011 = if (g-r), (g-i), LV and an individual estimate for t are available for
the galaxy. Ms is then estimated for it on this basis, using Eq. (18)
with the appropriate entries in table 13.
1020 = (B-V) and LV of the galaxy are available, but its (g-r), (g-i) and t are
unknown. In this case, its age is assumed to be equal to the mean age
of galaxies with similar LV, as listed in table 14. Its Ms is then
estimated on this basis, using Eq. (18) with the appropriate entries
in table 13.
1021 = if (B-V), LV and an individual estimate for t are available for the
galaxy, but its (g-r) and (g-i) are unknown. Its Ms is then estimated
on this basis, using Eq. (18) with the appropriate entries in table 13.
--------------------------------------------------------------------------------
Global notes:
Note (G1): all values are corrected for extinction and redshift.
Note (G2): References for UBVI bands as follows:
For U magnitude:
0 = no data available
1 = HyperLeda
2 = Eisenhardt et al. (2007, Cat. J/ApJS/169/225)
For B magnitude:
0 = no data available
1 = HyperLeda
2 = Eisenhardt et al. (2007, Cat. J/ApJS/169/225)
3 = Karick et al. (2003, Cat. J/MNRAS/344/188)
4 = member of the Local Group whose value for Bmag comes from the catalogue
by Karachentsev et al. (2013, Cat. J/AJ/145/101)
5 = Koleva et al. (2011MNRAS.417.1643K 2011MNRAS.417.1643K)
For V magnitude:
0 = no data available
1 = HyperLeda
2 = Toloba et al. (2012A&A...548A..78T 2012A&A...548A..78T)
3 = Geha et al. (2003AJ....126.1794G 2003AJ....126.1794G)
4 = Eisenhardt et al. (2007, Cat. J/ApJS/169/225)
5 = Karick et al. (2003, Cat. J/MNRAS/344/188)
6 = Mieske et al. (2007, Cat. J/A+A/463/503)
7 = galaxy is a member of the Local Group, whose value for Vmag comes from
the catalogue by McConnachie (2012, Cat. J/AJ/144/4)
8 = the galaxy is a member of the Virgo Cluster whose value for Vmag comes
from Lieder et al. (2012, Cat. J/A+A/538/A69)
9 = galaxy is a member of the Hydra Cluster whose extinction-corrected value
for Vmag comes from Misgeld et al. (2008, Cat J/A+A/486/607)
10 = the galaxy is a member of the Centaurus Cluster, whose
extinction-corrected value for Vmag comes from
Misgeld et al. (2009, Cat. J/A+A/496/683)
For I magnitude:
0 = no data available
2 = Eisenhardt et al. (2007, Cat. J/ApJS/169/225)
3 = Karick et al. (2003, Cat. J/MNRAS/344/188)
4 = Mieske et al. (2007, Cat. J/A+A/463/503)
5 = member of the Virgo Cluster, whose value for Imag is taken from
Lieder et al. (2012, Cat. J/A+A/538/A69)
6 = galaxy is a member of the Hydra Cluster, whose value for Imag is
calculated from the extinction-corrected Vmag and (V-I)-colours in
Misgeld et al. (2008, Cat J/A+A/486/607)
7 = galaxy is a member of the Centaurus Cluster whose value for Imag is
calculated from the extinction-corrected Vmag and the (V-I)-colours
in Misgeld et al. (2009, Cat. J/A+A/496/683)
10NN = calculated from luminosities estimated with Eq. (4), using
the distances in Table2 and the absolute magnitude of the Sun in Table3,
For apparent magnitudes in the standard system that have been estimated
from SDSS-luminosities with Eqs. (4) and (5).
NN specifies the luminosities in the SDSS-system that entered the
estimate. In this context, u = 1, g = 2, r = 3, i = 4 and z = 5.
If only a single passband was used, the other digit is set to '0'.
The numbers indicating how magnitudes in the SDSS system were calculated
from the standard system follow the same principle. However, in this
context, U = 1, B = 2, V = 3 and I = 4.
Note (G3): References for SDSS bands as follows:
0 = no data
1 = tenth data release of the SDSS
2 = galaxy is a member of the galaxy cluster Abell 496 from
Chilingarian et al. (2008, Cat. J/A+A/486/85)
10NN = calculated from the U-band luminosities estimated with Eq. (4), using
the distances in Table2 and the absolute magnitude of the Sun in Table3,
For apparent magnitudes in the standard system that have been estimated
from SDSS-luminosities with Eqs. (4) and (5).
NN specifies the luminosities in the SDSS-system that entered the
estimate. In this context, u = 1, g = 2, r = 3, i = 4 and z = 5.
If only a single passband was used, the other digit is set to '0'.
The numbers indicating how magnitudes in the SDSS system were calculated
from the standard system follow the same principle. However, in this
context, U = 1, B = 2, V = 3 and I = 4.
--------------------------------------------------------------------------------
Acknowledgements:
Joerg Dabringhausen, joerg(at)astro-udec.cl
Michael Fellhauer, mfellhauer(at)astro-udec.cl
(End) Joerg Dabringhausen [Univ. Concepcion], Patricia Vannier [CDS] 14-Jun-2016