J/ApJ/896/3 Cosmicflows-4: Tully-Fisher relation calibrations (Kourkchi+, 2020)
Cosmicflows-4: The calibration of optical and infrared Tully-Fisher relations.
Kourkchi E., Tully R.B., Anand G.S., Courtois H.M., Dupuy A., Neill J.D.,
Rizzi L., Seibert M.
<Astrophys. J., 896, 3 (2020)>
=2020ApJ...896....3K 2020ApJ...896....3K
ADC_Keywords: Galaxies, photometry; H I data; Clusters, galaxy; Photometry, SDSS
Keywords: Distance measure ; Galaxy distances ; Galaxy photometry ;
H I line emission ; Spiral galaxies ; Inclination ; Galaxy structure ;
Large-scale structure of the universe
Abstract:
This study is a part of the Cosmicflows-4 project with the aim of
measuring the distances of more than ∼10000 spiral galaxies in the
local universe up to ∼15000km/s. New HI line width information has
come primarily from the Arecibo Legacy Fast ALFA Survey. Photometry of
our sample galaxies has been carried out in optical (SDSS u, g, r, i,
and z) and infrared (WISE W1 and W2) bands. Inclinations have been
determined using an online graphical interface accessible to a
collaboration of citizen scientists. Galaxy distances are measured
based on the correlation between the rotation rate of spirals and
their absolute luminosity, known as the Tully-Fisher relation (TFR).
In this study, we present the calibration of the TFR using a subsample
of ∼600 spirals located in 20 galaxy clusters. Correlations among such
observables as color, surface brightness, and relative HI content are
explored in an attempt to reduce the scatter about the TFR with the
goal of obtaining more accurate distances. A preliminary determination
of the Hubble constant from the distances and velocities of the
calibrator clusters is H0=76.0±1.1(stat.)±2.3(sys.)km/s/Mpc.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 336 735 Galaxy data catalog
clusters.dat 101 20 The parameters of the fitted "inverse" TFRs for
individual clusters in the W1 band (see Figure 4)
and in the i Band (see Figure 3)
table10.dat 95 318 Cluster distances and H0 data
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See also:
VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)
VII/238 : HYPERLEDA. II. Homogenized HI data (Paturel+, 2003)
VIII/77 : HI spectral properties of galaxies (Springob+, 2005)
II/328 : AllWISE Data Release (Cutri+ 2013)
V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)
J/AJ/112/2471 : The Ursa Major cluster. I. (Tully+ 1996)
J/ApJ/533/744 : Calibration of the Tully-Fischer relation (Tully+, 2000)
J/ApJS/172/599 : SFI++ II. A new I-band Tully-Fisher cat. (Springob+, 2007)
J/ApJ/676/184 : Peculiar motion away from the Local Void (Tully+, 2008)
J/AJ/138/1938 : EDD: All Digital HI profile catalog (Courtois+, 2009)
J/AJ/138/332 : LEDA CMD/tip of the red giant branch (Jacobs+, 2009)
J/MNRAS/414/2005 : Cosmic flows observations (Courtois+, 2011)
J/AJ/142/170 : ALFALFA survey: α.40 HI source cat. (Haynes+, 2011)
J/ApJ/743/76 : Spitzer photometry of LMC Cepheids (Scowcroft+, 2011)
J/ApJS/199/26 : The 2MASS Redshift Survey (2MRS) (Huchra+, 2012)
J/ApJ/759/146 : Spitzer/IRAC phot. for 37 Galactic Cepheids (Monson+, 2012)
J/AcA/62/247 : LMC phot. maps from OGLE-III shallow survey (Ulaczyk+, 2012)
J/ApJ/765/94 : Calibration of the MIR Tully-Fisher relation (Sorce+, 2013)
J/AJ/146/86 : Cosmicflows-2 catalog (Tully+, 2013)
J/ApJ/792/129 : WISE W1/W2 Tully-Fisher relation calibrators (Neill+, 2014)
J/MNRAS/445/2677 : Peculiar velocities in 6dFGS (Springob+, 2014)
J/AJ/149/171 : 2MASS galaxy group catalog (Tully, 2015)
J/AJ/151/88 : LMC NIR Synoptic Survey. II. (Bhardwaj+, 2016)
J/ApJ/816/L14 : Tully-Fisher relation in disk gal. from SPARC (Lelli+, 2016)
J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)
J/AJ/152/50 : Cosmicflows-3 catalog (CF3) (Tully+, 2016)
J/ApJ/843/16 : Galaxy groups within 3500km/s (Kourkchi+, 2017)
J/ApJ/861/49 : ALFALFA extragalactic HI source catalog (Haynes+, 2018)
J/ApJ/884/82 : SDSS, WISE & HI data of local spiral gal. (Kourkchi+, 2019)
J/ApJ/876/85 : HST observations for LMC Cepheids (Riess+, 2019)
J/ApJ/886/61 : OGLE-III, MCPS and HST VI obs. of LMC & SMC (Yuan+, 2019)
J/A+A/646/A113 : Towards Cosmicflows-4 HI data catalog (Dupuy+, 2021)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 7 I7 --- PGC [218/5808041] Principal Galaxies Catalog ID
9- 31 A23 --- Name Common identifier
33- 34 I2 deg Inc [45/90] Measured inclination
36- 37 I2 deg e_Inc [1/18] Uncertainty in Inc
39- 41 I3 km/s Wmx [50/909] Adjusted HI line width (1)
43- 44 I2 km/s e_Wmx [5/56] Uncertainty in Wmx
46- 50 F5.3 [km/s] logWmxi [1.74/3] Log of inclination corrected Wmx (1)
52- 56 F5.3 [km/s] e_logWmxi [0.004/0.15] Uncertainty in logWmxi
58- 63 F6.3 mag m21 [9.14/38.34] HI 21cm magnitude (2)
65- 69 F5.3 mag e_m21 [0/0.3] Uncertainty in m21
71- 75 F5.2 mag umag [9/19.7]?=0 Apparent u band AB magnitude (3)
77- 81 F5.2 mag gmag [7.5/18.5]?=0 Apparent g band AB magnitude (3)
83- 87 F5.2 mag rmag [6.6/18.4]?=0 Apparent r band AB magnitude (3)
89- 93 F5.2 mag imag [6.2/18.6]?=0 Apparent i band AB magnitude (3)
95- 99 F5.2 mag zmag [6.9/18.4]?=0 Apparent z band AB magnitude (3)
101- 105 F5.2 mag W1mag [5.6/18]?=0 WISE 3.26um band apparent AB
magnitude (3)
107- 111 F5.2 mag W2mag [6.4/18.5]?=0 WISE 4.62um band apparent AB
magnitude (3)
113- 116 F4.2 --- (b/a)s [0.1/0.9]?=0 Axial ratio from SDSS image (4)
118- 121 F4.2 --- (b/a)W [0.1/0.97]?=0 Axial ratio from WISE image (4)
123- 126 F4.2 arcmin Reu [0.07/4.7]?=0 Half light semi-major axis in
u band
128- 131 F4.2 arcmin Reg [0.07/4]?=0 Half light semi-major axis in g
band
133- 137 F5.2 arcmin Rer [-0.02/3.6]?=0 Half light semi-major axis in
r band
139- 142 F4.2 arcmin Rei [0.07/3.4]?=0 Half light semi-major axis in
i band
144- 147 F4.2 arcmin Rez [0.07/3.2]?=0 Half light semi-major axis in
z band
149- 153 F5.2 arcmin ReW1 [0.1/12.4]?=0 Half light semi-major axis in
WISE 3.26 micron band
155- 158 F4.2 arcmin ReW2 [0.1/9.7]?=0 Half light semi-major axis in
WISE 4.62 micron band
160- 172 A13 --- Cl Host cluster identifier (5)
180 A1 --- f_Cl [*] * = "anomalous" galaxy (strongly deviant)
182- 186 F5.2 mag ucmag [8.6/19.4]?=0 Corrected u band AB mag (6)
188- 192 F5.2 mag gcmag [7.2/18.3]?=0 Corrected g band AB mag (6)
194- 198 F5.2 mag rcmag [6.4/18.4]?=0 Corrected r band AB mag (6)
200- 204 F5.2 mag icmag [6/18.6]?=0 Corrected i band AB mag (6)
206- 210 F5.2 mag zcmag [6.9/18.4]?=0 Corrected z band AB mag (6)
212- 216 F5.2 mag W1cmag [5.6/18]?=0 Corrected WISE 3.26 micron band
AB magnitude (6)
218- 222 F5.2 mag W2cmag [6.4/18.6]?=0 Corrected WISE 4.62 micron
band AB magnitude (6)
224- 227 F4.2 mag Au [0/1.8] U band dust attenuation
correction
229- 232 F4.2 mag e_Au [0/2.4] Uncertainty in Au
234- 237 F4.2 mag Ag [0/1.4] G band dust attenuation
correction
239- 242 F4.2 mag e_Ag [0/2.4] Uncertainty in Ag
244- 247 F4.2 mag Ar [0/1.2] R band dust attenuation
correction
249- 252 F4.2 mag e_Ar [0/2.3] Uncertainty in Ar
254- 257 F4.2 mag Ai [0/1] I band dust attenuation
correction
259- 262 F4.2 mag e_Ai [0/2.3] Uncertainty in Ai
264- 267 F4.2 mag Az [0/0.8] Z band dust attenuation
correction
269- 272 F4.2 mag e_Az [0/2.2] Uncertainty in Az
274- 278 F5.2 mag AW1 [-1.1/0.5] WISE 3.26um band dust attenuation
correction
280- 283 F4.2 mag e_AW1 [0.01/0.33]?=0 Uncertainty in AW1
285- 289 F5.2 mag AW2 [-1.1/0.4]?=0 WISE 4.62um band dust
attenuation correction
291- 294 F4.2 mag e_AW2 [0.01/0.33]?=0 Uncertainty in AW2
296- 300 F5.2 mag u*mag [-1/18.52]?=0 Dust corrected u band AB
magnitude (7)
302- 306 F5.2 mag g*mag [7/17.8]?=0 Dust corrected g band AB
magnitude (7)
308- 312 F5.2 mag r*mag [6.4/17.8]?=0 Dust corrected r band AB
magnitude (7)
314- 318 F5.2 mag i*mag [6/18.1]?=0 Dust corrected i band AB
magnitude (7)
320- 324 F5.2 mag z*mag [6.9/18]?=0 Dust corrected z band AB
magnitude (7)
326- 330 F5.2 mag W1*mag [5.6/18.19]?=0 Dust corrected WISE 3.26
micron band AB magnitude (7)
332- 336 F5.2 mag W2*mag [6.4/18.8]?=0 Dust corrected WISE 4.62
micron band AB magnitude (7)
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Note (1): Observed linewidths at 50% average HI flux are corrected for spectral
resolution and redshift and further adjusted to approximate twice
(projected) maximum rotation, Wmx. The parameter de-projected to
edge-on orientation is Wmxi=Wmx/sin(Inc).
Note (2): Calculated from the HI flux, FHI, using m21=-2.5log(FHI)+17.4.
Note (3): Total raw magnitudes. The uncertainty on the measured u-band
magnitudes are ∼0.1mag. The uncertainties on all other measured
magnitudes are not worse than 0.05 mag, which is conservatively
adopted for the purpose of error propagation in this study.
Note (4): Where a and b are the semi-major and semi-minor axes of
the elliptical aperture, respectively.
Note (5): With the 94 zero point calibrators identified as "ZP calibrator".
Note (6): Corrected for Milky Way obscuration, redshift k-correction, and
aperture effects, but not the inclination dependent dust attenuation,
based on the corresponding raw magnitude,
mc=mtotal-Ab-Ak-Aa.
Note (7): Correcting for the effect of global dust obscuration,
m*=mtotal-Ab-Ak-Aa-Ai.
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Byte-by-byte Description of file: clusters.dat
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Bytes Format Units Label Explanations
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1- 13 A13 --- Cl Cluster name
15- 18 A4 --- Code Cluster code
20- 21 I2 --- NgalW1 [11/75] Number of galaxies incorporated in the
ITFR fit, W1 band
23- 28 F6.2 --- SlopeW1 [-10.5/-7.8] Slope of the individually fitted
ITFR in W1 band
30- 33 F4.2 --- e_SlopeW1 [0.4/1.4] SlopeW1
35- 39 F5.2 --- ZPW1 [10.5/15.7] Zero-point of the individually
fitted ITFR in W1 band
41- 44 F4.2 --- e_ZPW1 [0.06/0.3] ZP uncertainty
46- 50 F5.2 --- ZP0W1 [10.4/15.7] Zero-point from the linear
regression with the fixed ITFR universal slope
52- 55 F4.2 --- e_ZP0W1 [0.06/0.2] ZP0 uncertainty
57- 60 F4.2 --- rmsW1 [0.3/1] The rms of galaxy deviations from the
universal lines along the magnitude axis
62- 63 I2 --- Ngali [11/79]? Number of galaxies incorporated in the
ITFR fit, i band
65- 69 F5.2 --- Slopei [-9.4/-7.2]? Slope of the individually fitted
ITFR in i-band
71- 74 F4.2 --- e_Slopei [0.4/1.3]? Slope uncertainty
76- 80 F5.2 --- ZPi [10.13/15.1]? Zero-point of the individually
fitted ITFR in i-band
82- 85 F4.2 --- e_ZPi [0.06/0.3]? ZP uncertainty
87- 91 F5.2 --- ZP0i [10/15.1]? Zero-point from the linear regression
with the fixed ITFR universal slope in i-band
93- 96 F4.2 --- e_ZP0i [0.06/0.2]? ZP0 uncertainty
98-101 F4.2 --- rmsi [0.3/0.7]? The rms of galaxy deviations from the
universal lines along the magnitude axis
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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- 13 A13 --- Cl Host cluster identifier
14 A1 --- f_Cl h: Abell 2151 = Hercules
16- 20 I5 km/s Vmod [1141/11353] Velocity adjusted for
cosmological curvature
22- 24 I3 km/s e_Vmod [13/121] Uncertainty in Vmod
26- 27 A2 --- Band Tully-Fisher Relation band (ugriz or W1, W2)
29- 39 A11 --- Model Tully-Fisher Relation model
41- 42 I2 --- Ngal [11/79] Number of galaxies
44- 48 F5.2 mag DMo [30.79/36.1] Raw distance modulus using Model
50- 55 F6.3 mag Bias [-0.06/0.09] Cutoff magnitude bias
57- 60 F4.2 mag DelDM [0.04/0.2]? Distance modulus additional
adjustment
62- 66 F5.2 mag DMc [30.79/36.1] Adjusted distance modulus (1)
68- 71 F4.2 mag e_DMc [0.06/0.16] Uncertainty in DMc
73- 78 F6.2 Mpc Dist [14.39/162.4] Cluster distance
80- 83 F4.2 Mpc e_Dist [0.5/6.8] Uncertainty in Dist
85- 90 F6.2 km/s/Mpc Vmod/D [58.2/109.5] Hubble parameter
92- 95 F4.2 km/s/Mpc e_Vmod/D [1.9/7.3] Uncertainty in Vmod/D
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Note (1): Where DMc = DMo + Bias + DelDM.
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History:
From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 22-Sep-2021