THE SLOAN DIGITAL SKY SURVEY CO-ADD: CROSS-CORRELATION WEAK LENSING AND TOMOGRAPHY OF GALAXY CLUSTERS
The shapes of distant galaxies are sheared by intervening galaxy clusters. We examine this effect in Stripe 82, a 275 deg super(2) region observed multiple times in the Sloan Digital Sky Survey (SDSS) and co-added to achieve greater depth. We obtain a mass-richness calibration that is similar to oth...
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| Veröffentlicht in: | The Astrophysical journal 2012-04, Vol.748 (2), p.1-8, Article 128 |
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| creator | SIMET, Melanie KUBO, Jeffrey M DODELSON, Scott ANNIS, James T JIANGANG HAO JOHNSTON, David HUAN LIN REIS, Ribamar R. R SOARES-SANTOS, Marcelle SEO, Hee-Jong |
| description | The shapes of distant galaxies are sheared by intervening galaxy clusters. We examine this effect in Stripe 82, a 275 deg super(2) region observed multiple times in the Sloan Digital Sky Survey (SDSS) and co-added to achieve greater depth. We obtain a mass-richness calibration that is similar to other SDSS analyses, demonstrating that the co-addition process did not adversely affect the lensing signal. We also propose a new parameterization of the effect of tomography on the cluster lensing signal which does not require binning in redshift, and we show that using this parameterization we can detect tomography for stacked clusters at varying redshifts. Finally, due to the sensitivity of the tomographic detection to accurately marginalize over the effect of the cluster mass, we show that tomography at low redshift (where dependence on exact cosmological models is weak) can be used to constrain mass profiles in clusters. |
| doi_str_mv | 10.1088/0004-637X/748/2/128 |
| format | Article |
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| subjects | Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CALIBRATION Clusters COSMOLOGICAL MODELS Cosmology Earth, ocean, space Exact sciences and technology Galactic clusters GALAXIES GALAXY CLUSTERS MASS Parametrization RED SHIFT Signal processing Sky surveys (astronomy) TOMOGRAPHY |
| title | THE SLOAN DIGITAL SKY SURVEY CO-ADD: CROSS-CORRELATION WEAK LENSING AND TOMOGRAPHY OF GALAXY CLUSTERS |
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