Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data

We present new spectroscopic data for 532 early-type galaxies, predominantly Abell cluster members with cz < 12 000 km s-1. We tabulate 919 individual measurements, from six observing runs, for recession velocity, cz, central velocity dispersion, σ, and magnesium line-strength indices, Mg2 an...

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मुख्य लेखकों: Smith, R, Lucey, JR, Hudson, M, Schlegel, D, Davies, R
स्वरूप: Journal article
भाषा:English
प्रकाशित: 2000
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author Smith, R
Lucey, JR
Hudson, M
Schlegel, D
Davies, R
author_facet Smith, R
Lucey, JR
Hudson, M
Schlegel, D
Davies, R
author_sort Smith, R
collection OXFORD
description We present new spectroscopic data for 532 early-type galaxies, predominantly Abell cluster members with cz < 12 000 km s-1. We tabulate 919 individual measurements, from six observing runs, for recession velocity, cz, central velocity dispersion, σ, and magnesium line-strength indices, Mg2 and Mgb. The median estimated error, per measurement, in σ is 5 per cent. The Mg2 line-strength data have median errors of 0.009 mag. The observed scatter between repeat measurements is largely accounted for by photon-counting errors. These data will be employed in forthcoming papers, where they will form part of a merged and standardized catalogue of Fundamental Plane data for use in cluster distance estimates and peculiar velocity analyses.
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spelling oxford-uuid:79806b15-25d4-48bb-b545-4211e67e49722022-03-26T20:37:51ZStreaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic dataJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:79806b15-25d4-48bb-b545-4211e67e4972EnglishSymplectic Elements at Oxford2000Smith, RLucey, JRHudson, MSchlegel, DDavies, RWe present new spectroscopic data for 532 early-type galaxies, predominantly Abell cluster members with cz < 12 000 km s-1. We tabulate 919 individual measurements, from six observing runs, for recession velocity, cz, central velocity dispersion, σ, and magnesium line-strength indices, Mg2 and Mgb. The median estimated error, per measurement, in σ is 5 per cent. The Mg2 line-strength data have median errors of 0.009 mag. The observed scatter between repeat measurements is largely accounted for by photon-counting errors. These data will be employed in forthcoming papers, where they will form part of a merged and standardized catalogue of Fundamental Plane data for use in cluster distance estimates and peculiar velocity analyses.
spellingShingle Smith, R
Lucey, JR
Hudson, M
Schlegel, D
Davies, R
Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data
title Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data
title_full Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data
title_fullStr Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data
title_full_unstemmed Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data
title_short Streaming motions of galaxy clusters within 12 000 km s(-1) - I. New spectroscopic data
title_sort streaming motions of galaxy clusters within 12 000 km s 1 i new spectroscopic data
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AT luceyjr streamingmotionsofgalaxyclusterswithin12000kms1inewspectroscopicdata
AT hudsonm streamingmotionsofgalaxyclusterswithin12000kms1inewspectroscopicdata
AT schlegeld streamingmotionsofgalaxyclusterswithin12000kms1inewspectroscopicdata
AT daviesr streamingmotionsofgalaxyclusterswithin12000kms1inewspectroscopicdata