Cosmological weak lensing with the HST GEMS survey
We present our cosmic shear analysis of GEMS, one of the largest wide-field surveys ever undertaken by the Hubble Space Telescope. Imaged with the Advanced Camera for Surveys (ACS), GEMS spans 795 square arcmin in the Chandra Deep Field South. We detect weak lensing by large-scale structure in high...
| Main Authors: | , , , , , , , , , , , , , , , , , , |
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| Format: | Journal article |
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2005
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| _version_ | 1826262884833820672 |
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| author | Heymans, C Brown, M Barden, M Caldwell, J Jahnke, K Peng, C Rix, H Taylor, A Beckwith, S Bell, E Borch, A Haeussler, B Jogee, S McIntosh, D Meisenheimer, K Sanchez, S Somerville, R Wisotzki, L Wolf, C |
| author_facet | Heymans, C Brown, M Barden, M Caldwell, J Jahnke, K Peng, C Rix, H Taylor, A Beckwith, S Bell, E Borch, A Haeussler, B Jogee, S McIntosh, D Meisenheimer, K Sanchez, S Somerville, R Wisotzki, L Wolf, C |
| author_sort | Heymans, C |
| collection | OXFORD |
| description | We present our cosmic shear analysis of GEMS, one of the largest wide-field surveys ever undertaken by the Hubble Space Telescope. Imaged with the Advanced Camera for Surveys (ACS), GEMS spans 795 square arcmin in the Chandra Deep Field South. We detect weak lensing by large-scale structure in high resolution F606W GEMS data from ~60 resolved galaxies per square arcminute. We measure the two-point shear correlation function, the top-hat shear variance and the shear power spectrum, performing an E/B mode decomposition for each statistic. We show that we are not limited by systematic errors and use our results to place joint constraints on the matter density parameter Omega_m and the amplitude of the matter power spectrum sigma_8. We find sigma_8(Omega_m/0.3)^{0.65}=0.68 +/- 0.13 where the 1sigma error includes both our uncertainty on the median redshift of the survey and sampling variance. Removing image and point spread function (PSF) distortions are crucial to all weak lensing analyses. We therefore include a thorough discussion on the degree of ACS PSF distortion and anisotropy which we characterise directly from GEMS data. Consecutively imaged over 20 days, GEMS data also allows us to investigate PSF instability over time. We find that, even in the relatively short GEMS observing period, the ACS PSF ellipticity varies at the level of a few percent which we account for with a semi-time dependent PSF model. Our correction for the temporal and spatial variability of the PSF is shown to be successful through a series of diagnostic tests. |
| first_indexed | 2024-03-06T19:42:53Z |
| format | Journal article |
| id | oxford-uuid:214356a7-d360-4d4b-95f2-62b6668d6d12 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T19:42:53Z |
| publishDate | 2005 |
| record_format | dspace |
| spelling | oxford-uuid:214356a7-d360-4d4b-95f2-62b6668d6d122022-03-26T11:32:26ZCosmological weak lensing with the HST GEMS surveyJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:214356a7-d360-4d4b-95f2-62b6668d6d12Symplectic Elements at Oxford2005Heymans, CBrown, MBarden, MCaldwell, JJahnke, KPeng, CRix, HTaylor, ABeckwith, SBell, EBorch, AHaeussler, BJogee, SMcIntosh, DMeisenheimer, KSanchez, SSomerville, RWisotzki, LWolf, CWe present our cosmic shear analysis of GEMS, one of the largest wide-field surveys ever undertaken by the Hubble Space Telescope. Imaged with the Advanced Camera for Surveys (ACS), GEMS spans 795 square arcmin in the Chandra Deep Field South. We detect weak lensing by large-scale structure in high resolution F606W GEMS data from ~60 resolved galaxies per square arcminute. We measure the two-point shear correlation function, the top-hat shear variance and the shear power spectrum, performing an E/B mode decomposition for each statistic. We show that we are not limited by systematic errors and use our results to place joint constraints on the matter density parameter Omega_m and the amplitude of the matter power spectrum sigma_8. We find sigma_8(Omega_m/0.3)^{0.65}=0.68 +/- 0.13 where the 1sigma error includes both our uncertainty on the median redshift of the survey and sampling variance. Removing image and point spread function (PSF) distortions are crucial to all weak lensing analyses. We therefore include a thorough discussion on the degree of ACS PSF distortion and anisotropy which we characterise directly from GEMS data. Consecutively imaged over 20 days, GEMS data also allows us to investigate PSF instability over time. We find that, even in the relatively short GEMS observing period, the ACS PSF ellipticity varies at the level of a few percent which we account for with a semi-time dependent PSF model. Our correction for the temporal and spatial variability of the PSF is shown to be successful through a series of diagnostic tests. |
| spellingShingle | Heymans, C Brown, M Barden, M Caldwell, J Jahnke, K Peng, C Rix, H Taylor, A Beckwith, S Bell, E Borch, A Haeussler, B Jogee, S McIntosh, D Meisenheimer, K Sanchez, S Somerville, R Wisotzki, L Wolf, C Cosmological weak lensing with the HST GEMS survey |
| title | Cosmological weak lensing with the HST GEMS survey |
| title_full | Cosmological weak lensing with the HST GEMS survey |
| title_fullStr | Cosmological weak lensing with the HST GEMS survey |
| title_full_unstemmed | Cosmological weak lensing with the HST GEMS survey |
| title_short | Cosmological weak lensing with the HST GEMS survey |
| title_sort | cosmological weak lensing with the hst gems survey |
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