SXDF-ALMA 1.5 arcmin^2 deep survey. A compact dusty star-forming galaxy at z=2.5

Autor: Itziar Aretxaga, Hideki Umehata, Kouichiro Nakanishi, Bunyo Hatsukade, Stijn Wuyts, Masao Hayashi, Wei-Hao Wang, Yoichi Tamura, Soh Ikarashi, Yusei Koyama, Takuma Izumi, Yuki Yamaguchi, Rob Ivison, Kotaro Kohno, Tadayuki Kodama, Stefano Berta, James Dunlop, Karina Caputi, Yuichi Matsuda, Wiphu Rujopakarn, Min S. Yun, Grant W. Wilson, David H. Hughes, Dieter Lutz, Ryu Makiya, Ken-ichi Tadaki
Přispěvatelé: Astronomy, Kapteyn Astronomical Institute
Rok vydání: 2015
Předmět:
Zdroj: Astrophysical Journal Letters, 811(1). IOP PUBLISHING LTD
Tadaki, K, Kohno, K, Kodama, T, Ikarashi, S, Aretxaga, I, Berta, S, Caputi, K I, Dunlop, J S, Hatsukade, B, Hayashi, M, Hughes, D H, Ivison, R, Izumi, T, Koyama, Y, Lutz, D, Makiya, R, Matsuda, Y, Nakanishi, K, Rujopakarn, W, Tamura, Y, Umehata, H, Wilson, G W, Wuyts, S, Yamaguchi, Y & Yun, M S 2015, ' SXDF-ALMA 1.5 arcmin$^2$ Deep Survey: A Compact Dusty Star-forming Galaxy at z = 2.5 ', Astrophysical Journal Letters, vol. 811, L3 . https://doi.org/10.1088/2041-8205/811/1/L3
ISSN: 2041-8205
DOI: 10.48550/arxiv.1508.05950
Popis: We present first results from the SXDF-ALMA 1.5 arcmin^2 deep survey at 1.1 mm using Atacama Large Millimeter Array (ALMA). The map reaches a 1sigma depth of 55 uJy/beam and covers 12 Halpha-selected star-forming galaxies at z = 2.19 or z=2.53. We have detected continuum emission from three of our Halpha-selected sample, including one compact star-forming galaxy with high stellar surface density, NB2315-07. They are all red in the rest-frame optical and have stellar masses of log (M*/Msun)>10.9 whereas the other blue, main-sequence galaxies with log(M*/Msun)=10.0-10.8 are exceedingly faint
6 pages, 4 figures, 1 table, accepted for publication in ApJL
Databáze: OpenAIRE