论文标题

Scuba-2 Cosmos场中最明亮的亚毫米源的ALMA调查

An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2 COSMOS field

论文作者

Simpson, J. M., Smail, Ian, Dudzeviciute, U., Matsuda, Y., Hsieh, B. -C., Wang, W. -H., Swinbank, A. M., Stach, S. M., An, Fang Xia, Birkin, J. E., Ao, Y., Bunker, A. J., Chapman, S. C., Chen, Chian-Chou, Coppin, K. E. K., Ikarashi, S., Ivison, R. J., Mitsuhashi, I., Saito, T., Umehata, H., Wang, R., Zhao, Y.

论文摘要

我们介绍了S2COSMOS调查中的cosmos领域的Scuba -2图中〜180个最亮的来源的ALMA研究,作为AS2COSMOS的试点研究,这是对该领域〜1,000个来源的全面调查。在这个飞行员中,我们在宇宙中获得了最明亮的182个亚毫米源(S_850UM = 6.2MJY)的基本完整样品的870-UM连续图。我们的ALMA地图检测260个亚毫米级星系(SMG),跨度范围为S_870UM = 0.7-19.2MMJY。我们在34 +/- 2%的亚米特源中检测到了一个以上的SMG对应物,而Scuba-2来源比S_850UM更明亮的Scuba-2来源增加到53 +/- 8%。我们估计,这些SMG-SMG对中约有三分之一在物理上是相关的(更明亮的次级SMG的速率较高,S_870UM> 3MJY),并以偶然的[CII] 157.74UM线发射的偶然性检测到两个SMGS,AS2COS0001.1.1.1.1.1.1.1.1&dish AT Z =; dish AT Z = ac.10001.2 at ic in ac.157.74UM线发射。使用我们的源目录,我们在S_870UM> 6.2MJY构建了干涉测定法870UM数量。我们使用该领域的广泛档案数据来构建每个AS2COSMOS SMG的多波长光谱分布,然后用Magphys对此发射进行建模,以估算其光度红移。我们发现S_870UM> 6.2MJY AS2COSMOS样品Z = 2.87 +/- 0.08的中位光度降轴,并有清晰的证据表明,中位红移的中位数增加了870-UM磁通密度,表明870UM LuminInosisy函数的亮端具有强烈的强劲演化。

We present an ALMA study of the ~180 brightest sources in the SCUBA-2 map of the COSMOS field from the S2COSMOS survey, as a pilot study for AS2COSMOS - a full survey of the ~1,000 sources in this field. In this pilot we have obtained 870-um continuum maps of an essentially complete sample of the brightest 182 sub-millimetre sources (S_850um=6.2mJy) in COSMOS. Our ALMA maps detect 260 sub-millimetre galaxies (SMGs) spanning a range in flux density of S_870um=0.7-19.2mJy. We detect more than one SMG counterpart in 34+/-2 per cent of sub-millimetre sources, increasing to 53+/-8 per cent for SCUBA-2 sources brighter than S_850um>12mJy. We estimate that approximately one-third of these SMG-SMG pairs are physically associated (with a higher rate for the brighter secondary SMGs, S_870um>3mJy), and illustrate this with the serendipitous detection of bright [CII] 157.74um line emission in two SMGs, AS2COS0001.1 & 0001.2 at z=4.63, associated with the highest significance single-dish source. Using our source catalogue we construct the interferometric 870um number counts at S_870um>6.2mJy. We use the extensive archival data of this field to construct the multiwavelength spectral energy distribution of each AS2COSMOS SMG, and subsequently model this emission with MAGPHYS to estimate their photometric redshifts. We find a median photometric redshift for the S_870um>6.2mJy AS2COSMOS sample of z=2.87+/-0.08, and clear evidence for an increase in the median redshift with 870-um flux density suggesting strong evolution in the bright-end of the 870um luminosity function.

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