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arXiv 1003.3790astro-ph.CO
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AKARI FU-HYU星系演化计划:来自GOODS-N场的第一个结果

The AKARI FU-HYU galaxy evolution program: First results from the GOODS-N field

C. P. Pearson, S. Serjeant, M. Negrello, T. Takagi, W. -S. Jeong, H. Matsuhara, T. Wada, S. Oyabu, H. M. Lee, M. S. Im

摘要:

AKARI FU-HYU任务计划对几个研究得很好的斯皮策场进行了中红外成像,优先选择已经富含多波长数据的场,从无线电到X射线波长,填充在斯皮策IRAC和MIPS波段之间的波长沙漠中。我们提出了GOODS-N场中FU-HYU调查的初步结果。我们利用GOODS-N场中最高的多波长覆盖率,N场产生从红外到紫外波长的多波长目录,包含超过4393个源,包括光度红移。使用FU-HYU目录,我们提出了彩色图,通过我们的观测波段映射PAH功能的通道。我们发现,AKARI(IRC-L18 W 18微米波段)和斯皮策(MIPS 24 24微米波段)的较长中红外波段提供了对源的总MIR发射的准确测量,因此它们可能的总中红外光度。我们还发现,将AKARI IRC-S11 11微米波段的颜色产生双峰分布,其中在11微米处的过量优先选择中等红移的恒星形成星系。这些强大的颜色颜色诊断进一步用作工具,以提取异常的颜色人口,特别是人口的硅酸盐断裂星系的GOODS-N领域显示,尘埃星爆可以选择特定的红移范围(z=1.2 - 1.6)的中红外辍学技术。FU-HYU星表将以电子方式提供给天文学界。

英文摘要:

The AKARI FU-HYU mission program carried out mid-infrared imaging of several well studied Spitzer fields preferentially selecting fields already rich in multi-wavelength data from radio to X-ray wavelengths filling in the wavelength desert between the Spitzer IRAC and MIPS bands.We present the initial results for the FU-HYU survey in the GOODS-N field.We utilize the supreme multiwavelength coverage in the GOODS-N field to produce a multiwavelength catalogue from infrared to ultraviolet wavelengths, containing more than 4393 sources, including photometric redshifts. Using the FU-HYU catalogue we present colour-colour diagrams that map the passage of PAH features through our observation bands. We find that the longer mid-infrared bands from AKARI (IRC-L18W 18 micron band) and Spitzer (MIPS24 24 micron band) provide an accurate measure of the total MIR emission of the sources and therefore their probable total mid-infrared luminosity. We also find that colours incorporating the AKARI IRC-S11 11 micron band produce a bimodal distribution where an excess at 11 microns preferentially selects moderate redshift star-forming galaxies. These powerful colour-colour diagnostics are further used as tools to extract anomalous colour populations, in particular a population of Silicate Break galaxies from the GOODS-N field showing that dusty starbursts can be selected of specific redshift ranges (z=1.2 - 1.6) by mid-infrared drop-out techniques. The FU-HYU catalogue will be made publically available to the astronomical community.

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