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HeCS-red: Dense Hectospec Surveys of redMaPPer-selected Clusters
DC Field | Value | Language |
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dc.contributor.author | Rines, Kenneth J. | - |
dc.contributor.author | Geller, Margaret J. | - |
dc.contributor.author | Diaferio, Antonaldo | - |
dc.contributor.author | Hwang, Ho Seong | - |
dc.contributor.author | Sohn, Jubee | - |
dc.date.accessioned | 2024-05-03T02:27:10Z | - |
dc.date.available | 2024-05-03T02:27:10Z | - |
dc.date.created | 2024-05-03 | - |
dc.date.created | 2024-05-03 | - |
dc.date.issued | 2018-08 | - |
dc.identifier.citation | ASTROPHYSICAL JOURNAL, Vol.862 No.2 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | https://hdl.handle.net/10371/200752 | - |
dc.description.abstract | We use dense redshift surveys to explore the properties of galaxy clusters selected from the redMaPPer catalog. Our new survey, Hectospec Cluster Survey of red-sequence-selected clusters (HeCS-red), includes 10,589 new or remeasured redshifts from MMT/Hectospec observations of 27 redMaPPer clusters at redshifts z = 0.08-0.25 with large estimated richnesses (richness estimate lambda > 64). Our spectra confirm that each candidate cluster corresponds to a large overdensity in redshift space. The redMaPPer photometric redshifts have a slight bias toward higher redshifts. We measure the relation between velocity dispersion sigma(p) and lambda The relation shows intrinsic scatter of 24% (and a range of 2x) in velocity dispersion at fixed richness. We extend our analysis to HeCS-red-ext, a sample that includes several clusters selected by X-ray flux or Sunyaev-Zeldovich signal. The heterogeneous sample of 121 clusters in HeCS-red-ext shows similar intrinsic scatter in the sigma(p)-lambda relation as the HeCS-red sample, but the range of sp at fixed richness increases to 3x. We evaluate the membership probability estimates P-mem for individual galaxies provided by redMaPPer. The spectroscopic membership fraction is larger than P-mem for 0.05 <= P-mem <= 0.7; conversely, the spectroscopic membership fraction is smaller than P-mem at P-mem >= 0.8. We compare spectroscopic richness estimates with redMaPPer richness estimates and find good agreement on average, but a range of a factor of two in spectroscopic richness at fixed redMaPPer richness. Overall, within the high-richness and low-redshift cut of our sample, spectroscopically estimated parameters such as velocity dispersion correlate well with photometric richness estimates, although the relations contain substantial scatter. | - |
dc.language | 영어 | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.title | HeCS-red: Dense Hectospec Surveys of redMaPPer-selected Clusters | - |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/aacd49 | - |
dc.citation.journaltitle | ASTROPHYSICAL JOURNAL | - |
dc.identifier.wosid | 000440726900010 | - |
dc.identifier.scopusid | 2-s2.0-85051478850 | - |
dc.citation.number | 2 | - |
dc.citation.volume | 862 | - |
dc.description.isOpenAccess | Y | - |
dc.contributor.affiliatedAuthor | Sohn, Jubee | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.subject.keywordPlus | DIGITAL SKY SURVEY | - |
dc.subject.keywordPlus | 1ST SPECTROSCOPIC DATA | - |
dc.subject.keywordPlus | GALAXY CLUSTERS | - |
dc.subject.keywordPlus | DATA RELEASE | - |
dc.subject.keywordPlus | MASS PROFILES | - |
dc.subject.keywordPlus | COSMOLOGICAL CONSTRAINTS | - |
dc.subject.keywordPlus | RICHNESS RELATION | - |
dc.subject.keywordPlus | INFALL REGIONS | - |
dc.subject.keywordPlus | REDSHIFTS | - |
dc.subject.keywordPlus | VELOCITY | - |
dc.subject.keywordAuthor | cosmology: observations | - |
dc.subject.keywordAuthor | galaxies: clusters: general | - |
dc.subject.keywordAuthor | galaxies: distances and redshifts | - |
dc.subject.keywordAuthor | galaxies: kinematics and dynamics | - |
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