The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15

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The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 is …
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scholarly articleQ13442814

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P819ADS bibcode2015MNRAS.449..835R
P818arXiv ID1409.3242
P356DOI10.1093/MNRAS/STV154
P724Internet Archive IDarxiv-1409.3242

P50authorCullan HowlettQ57076642
Ashley J. RossQ57514397
Lado SamushiaQ63230371
Will PercivalQ63230628
P2093author name stringAngela Burden
Marc Manera
P2860cites workPlanck 2013 results. I. Overview of products and scientific resultsQ15217920
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On the Robustness of the Acoustic Scale in the Low‐Redshift Clustering of MatterQ57630842
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The clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: including covariance matrix errorsQ58262216
The clustering of galaxies in the SDSS-III DR10 Baryon Oscillation Spectroscopic Survey: no detectable colour dependence of distance scale or growth rate measurementsQ58262230
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P433issue1
P407language of work or nameEnglishQ1860
P1104number of pages13
P304page(s)835–847
P577publication date2015-03-19
P1433published inMonthly Notices of the Royal Astronomical SocietyQ1536490
P1476titleThe clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15
P478volume449

Reverse relations

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Q59237360Dark radiation and inflationary freedom after Planck 2015
Q58262095Dynamical dark energy in light of the latest observations
Q53802676From Planck Data to Planck Era: Observational Tests of Holographic Cosmology.
Q47139211Is exponential gravity a viable description for the whole cosmological history?
Q59780545Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters
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