J/AJ/113/22 Tully-Fisher Relation. I. (Giovanelli+ 1997)
The I Band Tully-Fisher Relation for Cluster Galaxies: Data Presentation
Giovanelli R., Haynes M.P., Herter T., Vogt N.P., Wegner G.,
Salzer J.J., Da Costa L.N., Freudling W.
<Astron. J. 113, 22 (1997)>
=1997AJ....113...22G 1997AJ....113...22G (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Photometry ; Morphology ; Radial velocities
Abstract:
Observational parameters which can be used for redshift-independent
distance determination using the Tully-Fisher (TF) technique are given
for 782 spiral galaxies in the fields of 24 clusters or groups. I band
photometry for the full sample was either obtained by us or compiled
from published literature. Rotational velocities are derived either
from 21 cm spectra or optical emission line long-slit spectra, and
converted to a homogeneous scale. In addition to presenting the data,
a discussion of the various sources of error on TF parameters is
introduced, and the criteria for the assignment of membership to each
cluster are given.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table2 128 782 Galaxy parameters, by cluster
table2.tex 140 1328 AASTeX version of table2
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Byte-by-byte Description of file: table2
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Bytes Format Units Label Explanations
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1- 16 A16 --- Cluster Cluster name
18- 23 A6 --- Name1 *First identification name
25- 32 A8 --- Name2 *Second identification name
35- 36 I2 h RAh Right ascension, 1950.0
37- 38 I2 min RAm Right ascension, 1950.0
39- 42 F4.1 s RAs Right ascension, 1950.0
44 A1 --- DE- Sign of declination
45- 46 I2 deg DEd Declination, 1950.0
47- 48 I2 arcmin DEm Declination, 1950.0
49- 50 I2 arcsec DEs Declination, 1950.0
52- 54 A3 --- T *Hubble morphological type
56- 60 I5 km/s Vcmb Radial velocity in the Cosmic Microwave
Background (CMB) reference frame
62- 65 F4.1 deg Theta Angular distance from center of cluster
68- 69 A2 --- Mem *Membership code
71- 73 I3 km/s W ? Measured velocity width
75- 77 I3 km/s W1 ? Velocity width, corrected except for
inclination
79- 81 I3 km/s Wcor ? Velocity width, converted to edge-on
83- 85 I3 deg Inc Adopted inclination of plane of disk
88- 92 F5.3 --- log(Wcor) ? Log10 of Wcor
94- 96 I3 10-3 e_log(Wcor) *? Estimated uncertainty in log(Wcor)
99-103 F5.2 mag Imag *Measured and extrapolated I band mag.
105-109 F5.2 mag Icor *Corrected apparent magnitude
112-117 F6.2 mag Mcor *? Corrected absolute magnitude
119-120 I2 0.01mag e_Mcor *? Uncertainty of Mcor
122 A1 --- u_Mcor Uncertainty flag on Mcor
124 A1 --- Ref1 *Reference code for photometry
126 A1 --- Ref2 *Reference code for velocity width
128 A1 --- Note *[*] Indicates notes in printed paper
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Note to Name1:
If the galaxy is listed in the UGC catalog, the UGC number is
listed first; if not, the first listing corresponds to the
author's internal coding number.
Note to Name2:
The second name is added with the following priority scheme:
NGC or IC number; CGCG number in the form "field-number"; for
southern galaxies, if and NGC or IC number is not available
the ESO/Uppsala catalog name is given.
Note to T:
Morphological type code in the RC3 scheme, where 1 corresponds to
Sa, 3 to Sb, 5 to Sc, etc. If the code is followed by a B, the
galaxy disk has an identifiable bar.
Note to Mem:
c - galaxy is considered a bona fide cluster member
g - galaxy is sufficiently removed from the cluster center that
cluster membership cannot be safely assigned; the galaxy is,
however, in the periphery of the cluster, at roughly the same
redshift and it is a nearby supercluster member
f - foreground galaxy
b - background galaxy
Note to e_log(Wcor):
The uncertainty takes into account both measurement errors and
uncertainties arising from the corrections. The value (11), for
example is equivalent to ± 0.011.
Note to Imag:
Measure I band magnitude, extrapolated to infinity assuming that
the surface brightness profile of the disk is well described by
an exponential function; this value is sometimes adopted as an
average of two or more measurements, as footnoted.
Note to Icor:
Apparent magnitude, to which k-term, galactic, and internal
extinction corrections were applied.
Note to Mcor:
Absolute magnitude, computed assuming that the galaxy is at the
distance indicated either by the cluster redshift, if the galaxy
is a member, or by the galaxy redshift if not.
Note to e_Mcor:
The uncertainty on the magnitude is the sum in quadrature of the
measurement errors and the estimate of the uncertainty in the
corrections applied to the measured parameter. The error estimate
does not include the uncertainty on the value of the distance.
Note to Ref1:
A letter code identifies the source for the photometry:
a - Authors' photometric observations
b - Bernstein et al. 1994AJ....107..1962B, restricted to Coma
h - Han & Mould 1992ApJ...396..453H 1992ApJ...396..453H
m - Mathewson, Ford, & Buchhorn 1992ApJS...81. 413M
p - Pierce & Tully 1988ApJ...330..579P 1988ApJ...330..579P, restricted to Ursa Major
s - Bureau et al. 1996ApJ...463...60B 1996ApJ...463...60B, restricted to Fornax
x - Combination of different sources as noted
Note to Ref2:
A numerical code identifies the source of velocity width:
0 - Author's 21 cm measurements
1 - Author's optical spectroscopy
2 - Averages of several measurements, see notes
3 - 21 cm observations of Gavazzi 1987ApJ...320...96G 1987ApJ...320...96G and Scodeggio
& Gavazzi 1993ApJ...409..110S 1993ApJ...409..110S
4 - 21 cm observations of Bothun et al. 1985ApJS...57..423B 1985ApJS...57..423B, and
Aaronson et al. 1989ApJ...338..654A 1989ApJ...338..654A, cross-identified with the
compilation of Bottinelli et al. 1990A&AS...82..391B 1990A&AS...82..391B
5 - 21 cm measurements of Mathewson, Ford, & Buchhorn
1992ApJS...81. 413M
6 - Optical spectroscopy of Mathewson, Ford, & Buchhorn
1992ApJS...81. 413M
7 - 21 cm measurements of Pierce & Tully 1988ApJ...330..579P 1988ApJ...330..579P
8 - 21 cm observations of Fontanelli 1984A&A...138...85F 1984A&A...138...85F;
Lewis 1985ApJS...59. 161L; and Schneider et al. 1991ApJS...72.2455S 1991ApJS...72.2455S
9 - 21 cm observations of Bureau et al. 1996ApJ...463...60B 1996ApJ...463...60B
Note to Note:
If an asterisk appears in this column a note for this galaxy is given
in the printed paper.
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Origin: AAS CD-ROM series, Volume 7, 1996 Lee Brotzman [ADS] 06-Nov-1996
(End) Patricia Bauer [CDS] 11-Feb-1997