Cosmicflows-4: The Catalog of ∼10,000 Tully-Fisher Distances

被引:50
|
作者
Kourkchi, Ehsan [1 ]
Tully, R. Brent [1 ]
Eftekharzadeh, Sarah [2 ]
Llop, Jordan [3 ]
Courtois, Helene M. [4 ]
Guinet, Daniel [4 ]
Dupuy, Alexandra [4 ]
Neill, James D. [5 ]
Seibert, Mark [6 ]
Andrews, Michael [3 ]
Chuang, Juana [3 ]
Danesh, Arash [7 ]
Gonzalez, Randy [3 ]
Holthaus, Alexandria [3 ]
Mokelke, Amber [3 ]
Schoen, Devin [3 ]
Urasaki, Chase [3 ]
机构
[1] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[2] Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
[3] Univ Hawaii, Dept Phys & Astron, 2505 Correa Rd, Honolulu, HI 96822 USA
[4] Univ Lyon, UCB Lyon 1, CNRS, IUF,IN2P3,IP2I Lyon,UMR5822, F-69622 Villeurbanne, France
[5] CALTECH, 1200 East Calif Blvd,MC 278-17, Pasadena, CA 91125 USA
[6] Carnegie Inst Sci, Observ, 813 Santa Barbara St, Pasadena, CA 91101 USA
[7] Univ Zanjan, Dept Phys, Univ Blvd, Zanjan 4537138791, Iran
来源
ASTROPHYSICAL JOURNAL | 2020年 / 902卷 / 02期
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
Galaxy distances; Spiral galaxies; Galaxy photometry; Hubble constant; H I line emission; Large-scale structure of the universe; Inclination; Sky surveys; Catalogs; Distance measure; Random Forests; 6DF GALAXY SURVEY; FIELD;
D O I
10.3847/1538-4357/abb66b
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the distances of 9792 spiral galaxies lying within 15,000 km s(-1) using the relation between luminosity and rotation rate of spiral galaxies. The sample is dominantly, but not exclusively, drawn from galaxies detected in the course of the ALFALFA H i survey with the Arecibo Telescope. Relations between H i line widths and luminosity are calibrated at SDSS u, g, r, i, z bands and WISE W1 and W2 bands. By exploiting secondary parameters, particularly color indices, we address discrepancies between measured distances at different wave bands with unprecedented detail. We provide a catalog that includes reduced kinematic, photometric, and inclination parameters. We also describe a machine-learning algorithm, based on the random forest technique, that predicts the dust attenuation in spirals lacking infrared photometry. We determine a Hubble Constant value of H-0 = 75.1 0.2(stat.), with potential systematics up to 3 km s(-1) Mpc(-1).
引用
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页数:36
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