Numerical color-magnitude diagram analysis of sloan digital sky survey data and application to the new milky way satellites

被引:40
作者
De Jong, J. T. A. [1 ]
Rix, H. -W. [1 ]
Martin, N. F. [1 ]
Zucker, D. B. [2 ]
Dolphin, A. E. [3 ]
Bell, E. F. [1 ]
Belokurov, V. [2 ]
Evans, N. W. [2 ]
机构
[1] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[2] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[3] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
基金
英国科学技术设施理事会;
关键词
galaxies : dwarf; galaxies : stellar content; methods : numerical; methods : statistical; surveys;
D O I
10.1088/0004-6256/135/4/1361
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have tested the application to Sloan Digital Sky Survey (SDSS) data of the software package MATCH, which fits color-magnitude diagrams (CMDs) to estimate stellar population parameters and distances. These tests on a set of six globular clusters show that these techniques recover their known properties. New ways of using the CMD-fitting software enable us to deal with an extended distribution of stars along the line-of-sight, to constrain the overall properties of sparsely populated objects, and to detect the presence of stellar overdensities in wide-area surveys. We then also apply MATCH to CMDs for 12 recently discovered Milky Way satellites to derive in a uniform fashion their distances, ages, and metallicities. While the majority of them appear consistent with a single stellar population, CVn I, UMa II, and Leo T exhibit (from SDSS data alone) a more complex history with multiple epochs of star formation.
引用
收藏
页码:1361 / 1383
页数:23
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