The Galaxy Stellar Mass Function at 3.5 Greater Than or Equal to z Greater Than or Equal to 7.5 in the CANDLES/UDS, GOODS-South, and HUDF Fields
The Galaxy Stellar Mass Function at 3.5 Greater Than or Equal to z Greater Than or Equal to 7.5 in the CANDLES/UDS, GOODS-South, and HUDF Fields
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CANDLES/UDS、GOODS-South 和 HUDF 场中 3.5 大于或等于 z 大于或等于 7.5 时的星系恒星质量函数
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发表时间：
2014
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影响因子：
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通讯作者：
E. Vanzella
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作者：
A. Grazian;A. Fontana;P. Santini;J. Dunlop;H. Ferguson;M. Castellano;R. Amorin;M. Ashby;G. Barro;P. Behroozi;K. Boutsia;K. Caputi;R. Chary;A. Dekel;M. Dickinson;S. Faber;G. Fazio;S. Finkelstein;A. Galametz;E. Giallongo;M. Giavalisco;N. Grogin;Yicheng Guo;D. Kocevski;A. Koekemoer;D. Koo;Kyoung;Yu Lu;E. Merlin;B. Mobasher;M. Nonino;C. Papovich;D. Paris;L. Pentericci;N. Reddy;A. Renzini;B. Salmon;M. Salvato;V. Sommariva;Mimi Song;E. Vanzella
高z处的星系恒星质量函数（GSMF）提供了有关年轻宇宙中恒星形成历史和质量组装的关键信息。我们的目标是利用 HST、斯皮策和 VLT 在 CANDELS-UDS、GOODS-South 和 HUDF 场中提供的深光学/NIR/MIR 成像的独特组合来确定红移范围 3.5 4 上的 GSMF。这些结果证实了 CANDELS+HUDF、HUGS 和 SEDS 巡天在发现和研究高红移中/低质量星系方面的独特协同作用。
The galaxy stellar mass function (GSMF) at high-z provides key information on star-formation history and mass assembly in the young Universe. We aimed to use the unique combination of deep optical/NIR/MIR imaging provided by HST, Spitzer and the VLT in the CANDELS-UDS, GOODS-South, and HUDF fields to determine the GSMF over the redshift range 3.5 4. These results confirm the unique synergy of the CANDELS+HUDF, HUGS, and SEDS surveys for the discovery and study of moderate/low-mass galaxies at high redshifts.