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Cited by 846

The DOI matches its Crossref record; 39 of the 39 references it cites were found in a registry or an index.

Four new observational H(z) data from luminous red galaxies in the Sloan Digital Sky Survey data release seven

Open access
Zhang, Cong, Zhang, Han, Yuan, Shuo, Liu, Siqi, Zhang, Tong-Jie, Sun, Yan-Chun·2014·Research in Astronomy and Astrophysics
DOI 10.1088/1674-4527/14/10/002
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Abstract

By adopting the differential age method, we select 17 832 luminous red galaxies from the Sloan Digital Sky Survey Data Release Seven covering redshift 0 < z < 0.4 to measure the Hubble parameter. Using the full spectrum fitting package UlySS, these spectra are reduced with single stellar population models and optimal age information from our selected sample is derived. With the decreasing age-redshift relation, four new observational H ( z ) data (OHD) points are obtained, which are H ( z ) = 69.0 ± 19.6 km s −1 Mpc −1 at z = 0.07, H ( z ) = 68.6 ± 26.2km s −1 Mpc −1 at z = 0.12, H ( z ) = 72.9 ± 29.6 km s −1 Mpc −1 at z = 0.2 and H ( z )=88.8 ± 36.6 km s −1 Mpc −1 at z = 0.28, respectively. Combined with 21 other available OHD data points, the performance of the constraint on both flat and non-flat ΛCDM models is presented.

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Metadata

Authors
Zhang, C., Zhang, H., Yuan, S., Liu, S., Zhang, T.-J., & Sun, Y.-C.
Venue
Research in Astronomy and Astrophysics
Publisher
IOP Publishing
Published
2014-09-26
Volume
14
Issue
10
Pages
1221-1233
ISSN
1674-4527 (ISSN-L)
DOI
10.1088/1674-4527/14/10/002
OpenAlex
W2056583201
Cited by
846
References
39
FWCI
15.10
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Four new observational H(z) data from luminous red galaxies in the Sloan Digital Sky Survey data release seven. https://app.cochat.ai/papers/10.1088/1674-4527/14/10/002
The paper
Zhang, C., Zhang, H., Yuan, S., Liu, S., Zhang, T.-J., & Sun, Y.-C. (2014). Four new observational H(z) data from luminous red galaxies in the Sloan Digital Sky Survey data release seven. Research in Astronomy and Astrophysics. https://doi.org/10.1088/1674-4527/14/10/002

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