Emulating galaxy clustering and galaxy–galaxy lensing into the deeply non-linear regime: methodology, information, and forecasts-Reference-Cited by-同舟云学术

Emulating galaxy clustering and galaxy–galaxy lensing into the deeply non-linear regime: methodology, information, and forecasts

Published:2018-08-25 Issue:1 Volume:484 Page:989-1006
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Wibking Benjamin D¹^ORCID,Salcedo Andrés N¹,Weinberg David H¹,Garrison Lehman H²,Ferrer Douglas²,Tinker Jeremy³,Eisenstein Daniel²,Metchnik Marc⁴,Pinto Philip⁴

Affiliation:

1. Department of Astronomy and Center for Cosmology and AstroParticle Physics, Ohio State University, 140 W 18th Ave, Columbus, OH, USA 43210

2. Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS-10, Cambridge, MA 02138, USA

3. Center for Cosmology and Particle Physics, New York University, 4 Washington Place, New York, NY 10003, USA

4. Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85121, USA

Funder

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/1/989/27578378/sty2258.pdf

Reference78 articles.

1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

2. Algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering

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4. The nature of galaxy bias and clustering

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