View : 14 Download: 3

Photometric redshift requirements for lens galaxies in galaxy-galaxy lensing analyses

Title
Photometric redshift requirements for lens galaxies in galaxy-galaxy lensing analyses
Authors
Nakajima R.Mandelbaum R.Seljak U.Cohn J.D.Reyes R.Cool R.
Ewha Authors
Uros Seljak
Issue Date
2012
Journal Title
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711JCR Link
Citation
vol. 420, no. 4, pp. 3240 - 3263
Indexed
SCI; SCIE; SCOPUS WOS scopus
Abstract
Weak gravitational lensing is a valuable probe of galaxy formation and cosmology. Here we quantify the effects of using photometric redshifts (photo-z) in galaxy-galaxy lensing, for both sources and lenses, both for the immediate goal of using galaxies with photo-z as lenses in the Sloan Digital Sky Survey (SDSS) and as a demonstration of methodology for large, upcoming weak lensing surveys that will by necessity be dominated by lens samples with photo-z. We calculate the bias in the lensing mass calibration as well as consequences for absolute magnitude (i.e. k-corrections) and stellar mass estimates for a large sample of SDSS Data Release 8 (DR8) galaxies. The redshifts are obtained with the template-based photo-z code zebra on the SDSS DR8 ugriz photometry. We assemble and characterize the calibration samples (~9000 spectroscopic redshifts from four surveys) to obtain photometric redshift errors and lensing biases corresponding to our full SDSS DR8 lens and source catalogues. Our tests of the calibration sample also highlight the impact of observing conditions in the imaging survey when the spectroscopic calibration covers a small fraction of its footprint; atypical imaging conditions in calibration fields can lead to incorrect conclusions regarding the photo-z of the full survey. For the SDSS DR8 catalogue, we find σ Δz/(1+z)= 0.096 and 0.113 for the lens and source catalogues, with flux limits of r= 21 and 21.8, respectively. The photo-z bias and scatter is a function of photo-z and template types, which we exploit to apply photo-z quality cuts. By using photo-z rather than spectroscopy for lenses, dim blue galaxies and L * galaxies up to z~ 0.4 can be used as lenses, thus expanding into unexplored areas of parameter space. We also explore the systematic uncertainty in the lensing signal calibration when using source photo-z, and both lens and source photo-z; given the size of existing training samples, we can constrain the lensing signal calibration (and therefore the normalization of the surface mass density) to within 2 and 4per cent, respectively. © 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS.
DOI
10.1111/j.1365-2966.2011.20249.x
Appears in Collections:
자연과학대학 > 물리학전공 > Journal papers
Files in This Item:
Photometric redshift requirements for lens galaxies in galaxy-galaxy lensing analyses.pdf(6.85 MB)Download
Export
RIS (EndNote)
XLS (Excel)
XML


qrcode

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

BROWSE