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

Hoffmann, Samantha L. (author)
Macri, Lucas M. (author)
Riess, Adam G. (author)
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Yuan, Wenlong (author)
Casertano, Stefano (author)
Foley, Ryan J. (author)
Filippenko, Alexei V. (author)
Tucker, Brad E. (author)
Chornock, Ryan (author)
Silverman, Jeffrey M. (author)
Welch, Douglas L. (author)
Goobar, Ariel (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Amanullah, Rahman (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
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 (creator_code:org_t)
2016
2016
English.
In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 830:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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%.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

distance scale
galaxies: distances and redshifts
cosmology: observations
stars: variables: Cepheids

Publication and Content Type

ref (subject category)
art (subject category)

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