RCSLenS: the Red Cluster Sequence Lensing Survey

We present the Red-sequence Cluster Lensing Survey (RCSLenS), an application of the methods developed for the Canada France Hawaii Telescope Lensing Survey (CFHTLenS) to the ~785deg$^2$, multi-band imaging data of the Red-sequence Cluster Survey 2 (RCS2). This project represents the largest public,...

Celý popis

Podrobná bibliografie
Hlavní autoři: Hildebrandt, H, Choi, A, Heymans, C, Blake, C, Erben, T, Miller, L, Nakajima, R, van Waerbeke, L, Viola, M, Buddendiek, A, Harnois-Déraps, J, Hojjati, A, Joachimi, B, Joudaki, S, Kitching, T, Wolf, C, Gwyn, S, Johnson, N, Kuijken, K, Sheikhbahaee, Z, Tudorica, A, Yee, H
Médium: Journal article
Vydáno: Oxford University Press 2016
_version_ 1826270220380012544
author Hildebrandt, H
Choi, A
Heymans, C
Blake, C
Erben, T
Miller, L
Nakajima, R
van Waerbeke, L
Viola, M
Buddendiek, A
Harnois-Déraps, J
Hojjati, A
Joachimi, B
Joudaki, S
Kitching, T
Wolf, C
Gwyn, S
Johnson, N
Kuijken, K
Sheikhbahaee, Z
Tudorica, A
Yee, H
author_facet Hildebrandt, H
Choi, A
Heymans, C
Blake, C
Erben, T
Miller, L
Nakajima, R
van Waerbeke, L
Viola, M
Buddendiek, A
Harnois-Déraps, J
Hojjati, A
Joachimi, B
Joudaki, S
Kitching, T
Wolf, C
Gwyn, S
Johnson, N
Kuijken, K
Sheikhbahaee, Z
Tudorica, A
Yee, H
author_sort Hildebrandt, H
collection OXFORD
description We present the Red-sequence Cluster Lensing Survey (RCSLenS), an application of the methods developed for the Canada France Hawaii Telescope Lensing Survey (CFHTLenS) to the ~785deg$^2$, multi-band imaging data of the Red-sequence Cluster Survey 2 (RCS2). This project represents the largest public, sub-arcsecond seeing, multi-band survey to date that is suited for weak gravitational lensing measurements. With a careful assessment of systematic errors in shape measurements and photometric redshifts we extend the use of this data set to allow cross-correlation analyses between weak lensing observables and other data sets. We describe the imaging data, the data reduction, masking, multi-colour photometry, photometric redshifts, shape measurements, tests for systematic errors, and a blinding scheme to allow for more objective measurements. In total we analyse 761 pointings with r-band coverage, which constitutes our lensing sample. Residual large-scale B-mode systematics prevent the use of this shear catalogue for cosmic shear science. The effective number density of lensing sources over an unmasked area of 571.7deg$^2$ and down to a magnitude limit of r~24.5 is 8.1 galaxies per arcmin$^2$ (weighted: 5.5 arcmin$^{-2}$) distributed over 14 patches on the sky. Photometric redshifts based on 4-band griz data are available for 513 pointings covering an unmasked area of 383.5 deg$^2$ We present weak lensing mass reconstructions of some example clusters as well as the full survey representing the largest areas that have been mapped in this way. All our data products are publicly available through CADC at http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/en/community/rcslens/query.html in a format very similar to the CFHTLenS data release.
first_indexed 2024-03-06T21:37:27Z
format Journal article
id oxford-uuid:46c01860-cc07-485a-aa6b-e5c1df49a3ce
institution University of Oxford
last_indexed 2024-03-06T21:37:27Z
publishDate 2016
publisher Oxford University Press
record_format dspace
spelling oxford-uuid:46c01860-cc07-485a-aa6b-e5c1df49a3ce2022-03-26T15:15:37ZRCSLenS: the Red Cluster Sequence Lensing SurveyJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:46c01860-cc07-485a-aa6b-e5c1df49a3ceSymplectic Elements at OxfordOxford University Press2016Hildebrandt, HChoi, AHeymans, CBlake, CErben, TMiller, LNakajima, Rvan Waerbeke, LViola, MBuddendiek, AHarnois-Déraps, JHojjati, AJoachimi, BJoudaki, SKitching, TWolf, CGwyn, SJohnson, NKuijken, KSheikhbahaee, ZTudorica, AYee, HWe present the Red-sequence Cluster Lensing Survey (RCSLenS), an application of the methods developed for the Canada France Hawaii Telescope Lensing Survey (CFHTLenS) to the ~785deg$^2$, multi-band imaging data of the Red-sequence Cluster Survey 2 (RCS2). This project represents the largest public, sub-arcsecond seeing, multi-band survey to date that is suited for weak gravitational lensing measurements. With a careful assessment of systematic errors in shape measurements and photometric redshifts we extend the use of this data set to allow cross-correlation analyses between weak lensing observables and other data sets. We describe the imaging data, the data reduction, masking, multi-colour photometry, photometric redshifts, shape measurements, tests for systematic errors, and a blinding scheme to allow for more objective measurements. In total we analyse 761 pointings with r-band coverage, which constitutes our lensing sample. Residual large-scale B-mode systematics prevent the use of this shear catalogue for cosmic shear science. The effective number density of lensing sources over an unmasked area of 571.7deg$^2$ and down to a magnitude limit of r~24.5 is 8.1 galaxies per arcmin$^2$ (weighted: 5.5 arcmin$^{-2}$) distributed over 14 patches on the sky. Photometric redshifts based on 4-band griz data are available for 513 pointings covering an unmasked area of 383.5 deg$^2$ We present weak lensing mass reconstructions of some example clusters as well as the full survey representing the largest areas that have been mapped in this way. All our data products are publicly available through CADC at http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/en/community/rcslens/query.html in a format very similar to the CFHTLenS data release.
spellingShingle Hildebrandt, H
Choi, A
Heymans, C
Blake, C
Erben, T
Miller, L
Nakajima, R
van Waerbeke, L
Viola, M
Buddendiek, A
Harnois-Déraps, J
Hojjati, A
Joachimi, B
Joudaki, S
Kitching, T
Wolf, C
Gwyn, S
Johnson, N
Kuijken, K
Sheikhbahaee, Z
Tudorica, A
Yee, H
RCSLenS: the Red Cluster Sequence Lensing Survey
title RCSLenS: the Red Cluster Sequence Lensing Survey
title_full RCSLenS: the Red Cluster Sequence Lensing Survey
title_fullStr RCSLenS: the Red Cluster Sequence Lensing Survey
title_full_unstemmed RCSLenS: the Red Cluster Sequence Lensing Survey
title_short RCSLenS: the Red Cluster Sequence Lensing Survey
title_sort rcslens the red cluster sequence lensing survey
work_keys_str_mv AT hildebrandth rcslenstheredclustersequencelensingsurvey
AT choia rcslenstheredclustersequencelensingsurvey
AT heymansc rcslenstheredclustersequencelensingsurvey
AT blakec rcslenstheredclustersequencelensingsurvey
AT erbent rcslenstheredclustersequencelensingsurvey
AT millerl rcslenstheredclustersequencelensingsurvey
AT nakajimar rcslenstheredclustersequencelensingsurvey
AT vanwaerbekel rcslenstheredclustersequencelensingsurvey
AT violam rcslenstheredclustersequencelensingsurvey
AT buddendieka rcslenstheredclustersequencelensingsurvey
AT harnoisderapsj rcslenstheredclustersequencelensingsurvey
AT hojjatia rcslenstheredclustersequencelensingsurvey
AT joachimib rcslenstheredclustersequencelensingsurvey
AT joudakis rcslenstheredclustersequencelensingsurvey
AT kitchingt rcslenstheredclustersequencelensingsurvey
AT wolfc rcslenstheredclustersequencelensingsurvey
AT gwyns rcslenstheredclustersequencelensingsurvey
AT johnsonn rcslenstheredclustersequencelensingsurvey
AT kuijkenk rcslenstheredclustersequencelensingsurvey
AT sheikhbahaeez rcslenstheredclustersequencelensingsurvey
AT tudoricaa rcslenstheredclustersequencelensingsurvey
AT yeeh rcslenstheredclustersequencelensingsurvey