OPTICAL IDENTIFICATION OF CEPHEIDS IN 19 HOST GALAXIES OF TYPE Ia SUPERNOVAE AND NGC 4258 WITH THE HUBBLE SPACE TELESCOPE

被引:41
作者
Hoffmann, Samantha L. [1 ]
Macri, Lucas M. [1 ]
Riess, Adam G. [2 ,3 ]
Yuan, Wenlong [1 ]
Casertano, Stefano [3 ]
Foley, Ryan J. [4 ,5 ,6 ,9 ]
Filippenko, Alexei V. [7 ]
Tucker, Brad E. [7 ,8 ]
Chornock, Ryan
Silverman, Jeffrey M. [10 ]
Welch, Douglas L. [11 ]
Goobar, Ariel [12 ]
Amanullah, Rahman [12 ]
机构
[1] Texas A&M Univ, George P & Cynthia W Mitchell Inst Fundamental Ph, Dept Phys & Astron, College Stn, TX 77843 USA
[2] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[3] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[4] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
[5] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA
[6] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA
[7] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[8] Australian Natl Univ, Mt Stromlo Observ, Res Sch Astron & Astrophys, Weston, ACT, Australia
[9] Ohio Univ, Dept Phys & Astron, Astrophys Inst, Athens, OH 45701 USA
[10] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA
[11] McMaster Univ, Dept Phys & Astron, Hamilton, ON, Canada
[12] Stockholm Univ, Phys Dept, Oskar Klein Ctr, SE-10691 Stockholm, Sweden
基金
美国国家科学基金会;
关键词
distance scale; galaxies: distances and redshifts; cosmology: observations; stars: variables: Cepheids; LARGE-MAGELLANIC-CLOUD; PERIOD-LUMINOSITY RELATION; FIELD CAMERA 3; EXTRAGALACTIC DISTANCE SCALE; METALLICITY DEPENDENCE; KEY PROJECT; GEOMETRIC DISTANCE; CLASSICAL CEPHEIDS; GALACTIC CEPHEIDS; SPIRAL GALAXIES;
D O I
10.3847/0004-637X/830/1/10
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results of an optical search conducted as part of the SH0ES project (Supernovae and H-0 for the Equation of State of dark energy) for Cepheid variable stars using the Hubble Space Telescope (HST) in 19 hosts of Type Ia supernovae (SNe Ia) and the maser-host galaxy NGC 4258. The targets include nine newly imaged SN. Ia hosts using a novel strategy based on a long-pass filter that minimizes the number of HST orbits required to detect and accurately determine Cepheid properties. We carried out a homogeneous reduction and analysis of all observations, including new universal variability searches in all SN. Ia hosts, which yielded a total of 2200 variables with well-defined selection criteria, the largest such sample identified outside the Local Group. These objects are used in a companion paper to determine the local value of H-0 with a total uncertainty of 2.4%.
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页数:15
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