Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field
<p style="text-align:justify;">We present properties of moderately massive clusters of galaxies detected by the newly developed Hyper Suprime-Cam on the Subaru telescope using weak gravitational lensing. Eight peaks exceeding a signal-to-noise ratio (S/N) of 4.5 are identified on th...
| Main Authors: | , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Journal article |
| Language: | English |
| Published: |
IOP Publishing
2015
|
| _version_ | 1826307891898875904 |
|---|---|
| author | Miyazaki, S Oguri, M Hamana, T Tanaka, M Miller, L Utsumi, Y Komiyama, Y Furusawa, H Sakurai, J Kawanomoto, S Nakata, F Uraguchi, F Koike, M Tomono, D Lupton, R Gunn, J Karoji, H Aihara, H Murayama, H Takada, M |
| author_facet | Miyazaki, S Oguri, M Hamana, T Tanaka, M Miller, L Utsumi, Y Komiyama, Y Furusawa, H Sakurai, J Kawanomoto, S Nakata, F Uraguchi, F Koike, M Tomono, D Lupton, R Gunn, J Karoji, H Aihara, H Murayama, H Takada, M |
| author_sort | Miyazaki, S |
| collection | OXFORD |
| description | <p style="text-align:justify;">We present properties of moderately massive clusters of galaxies detected by the newly developed Hyper Suprime-Cam on the Subaru telescope using weak gravitational lensing. Eight peaks exceeding a signal-to-noise ratio (S/N) of 4.5 are identified on the convergence S/N map of a 2.3 deg2 field observed during the early commissioning phase of the camera. Multi-color photometric data are used to generate optically selected clusters using the Cluster finding algorithm based on the Multiband Identification of Red-sequence galaxies algorithm. The optical cluster positions were correlated with the peak positions from the convergence map. All eight significant peaks have optical counterparts. The velocity dispersion of clusters is evaluated by adopting the Singular Isothemal Sphere fit to the tangential shear profiles, yielding virial mass estimates, ${M}_{{500}_{c}}$, of the clusters which range from 2.7 × 1013 to 4.4 × 10 ${}^{14}\ {M}_{\odot }$. The number of peaks is considerably larger than the average number expected from ΛCDM cosmology but this is not extremely unlikely if one takes the large sample variance in the small field into account. We could, however, safely argue that the peak count strongly favors the recent Planck result suggesting a high ${\sigma }_{8}$ value of 0.83. The ratio of stellar mass to the dark matter halo mass shows a clear decline as the halo mass increases. If the gas mass fraction, fg, in halos is universal, as has been suggested in the literature, the observed baryon mass in stars and gas shows a possible deficit compared with the total baryon density estimated from the baryon oscillation peaks in anisotropy of the cosmic microwave background.</p> |
| first_indexed | 2024-03-07T07:09:49Z |
| format | Journal article |
| id | oxford-uuid:d1aa0927-8a42-4946-9d26-220e43c4985d |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T07:09:49Z |
| publishDate | 2015 |
| publisher | IOP Publishing |
| record_format | dspace |
| spelling | oxford-uuid:d1aa0927-8a42-4946-9d26-220e43c4985d2022-06-15T09:57:04ZProperties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 fieldJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:d1aa0927-8a42-4946-9d26-220e43c4985dEnglishSymplectic Elements at OxfordIOP Publishing2015Miyazaki, SOguri, MHamana, TTanaka, MMiller, LUtsumi, YKomiyama, YFurusawa, HSakurai, JKawanomoto, SNakata, FUraguchi, FKoike, MTomono, DLupton, RGunn, JKaroji, HAihara, HMurayama, HTakada, M <p style="text-align:justify;">We present properties of moderately massive clusters of galaxies detected by the newly developed Hyper Suprime-Cam on the Subaru telescope using weak gravitational lensing. Eight peaks exceeding a signal-to-noise ratio (S/N) of 4.5 are identified on the convergence S/N map of a 2.3 deg2 field observed during the early commissioning phase of the camera. Multi-color photometric data are used to generate optically selected clusters using the Cluster finding algorithm based on the Multiband Identification of Red-sequence galaxies algorithm. The optical cluster positions were correlated with the peak positions from the convergence map. All eight significant peaks have optical counterparts. The velocity dispersion of clusters is evaluated by adopting the Singular Isothemal Sphere fit to the tangential shear profiles, yielding virial mass estimates, ${M}_{{500}_{c}}$, of the clusters which range from 2.7 × 1013 to 4.4 × 10 ${}^{14}\ {M}_{\odot }$. The number of peaks is considerably larger than the average number expected from ΛCDM cosmology but this is not extremely unlikely if one takes the large sample variance in the small field into account. We could, however, safely argue that the peak count strongly favors the recent Planck result suggesting a high ${\sigma }_{8}$ value of 0.83. The ratio of stellar mass to the dark matter halo mass shows a clear decline as the halo mass increases. If the gas mass fraction, fg, in halos is universal, as has been suggested in the literature, the observed baryon mass in stars and gas shows a possible deficit compared with the total baryon density estimated from the baryon oscillation peaks in anisotropy of the cosmic microwave background.</p> |
| spellingShingle | Miyazaki, S Oguri, M Hamana, T Tanaka, M Miller, L Utsumi, Y Komiyama, Y Furusawa, H Sakurai, J Kawanomoto, S Nakata, F Uraguchi, F Koike, M Tomono, D Lupton, R Gunn, J Karoji, H Aihara, H Murayama, H Takada, M Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field |
| title | Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field |
| title_full | Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field |
| title_fullStr | Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field |
| title_full_unstemmed | Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field |
| title_short | Properties of weak lensing clusters detected on hyper suprime-cam's 2.3 deg2 field |
| title_sort | properties of weak lensing clusters detected on hyper suprime cam s 2 3 deg2 field |
| work_keys_str_mv | AT miyazakis propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT ogurim propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT hamanat propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT tanakam propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT millerl propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT utsumiy propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT komiyamay propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT furusawah propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT sakuraij propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT kawanomotos propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT nakataf propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT uraguchif propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT koikem propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT tomonod propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT luptonr propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT gunnj propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT karojih propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT aiharah propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT murayamah propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field AT takadam propertiesofweaklensingclustersdetectedonhypersuprimecams23deg2field |