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首页> 外文期刊>The Astrophysical Journal. Supplement Series >The Spitzer mid-infrared active galactic nucleus survey. I. Optical and near-infrared spectroscopy of obscured candidates and normal active galactic nuclei selected in the mid-infrared
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The Spitzer mid-infrared active galactic nucleus survey. I. Optical and near-infrared spectroscopy of obscured candidates and normal active galactic nuclei selected in the mid-infrared

机译:Spitzer中红外主动银河核调查。 I.中红外中隐蔽的候选物和正常活动的银河核的光学和近红外光谱

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摘要

We present the results of a program of optical and near-infrared spectroscopic follow-up of candidate active galactic nuclei (AGNs) selected in the mid-infrared. This survey selects both normal and obscured AGNs closely matched in luminosity across a wide range, from Seyfert galaxies with bolometric luminosities L bol ~ 10~(10) L to highly luminous quasars (L bol ~ 10~(14) L), all with redshifts ranging from 0 to 4.3. Samples of candidate AGNs were selected with mid-infrared color cuts at several different 24 μm flux density limits to ensure a range of luminosities at a given redshift. The survey consists of 786 candidate AGNs and quasars, of which 672 have spectroscopic redshifts and classifications. Of these, 137 (20%) are type 1 AGNs with blue continua, 294 (44%) are type 2 objects with extinctions AV ? 5 toward their AGNs, 96 (14%) are AGNs with lower extinctions (AV ~ 1), and 145 (22%) have redshifts, but no clear signs of AGN activity in their spectra. Of the survey objects 50% have L bol > 10~(12) L, in the quasar regime. We present composite spectra for type 2 quasars and objects with no signs of AGN activity in their spectra. We also discuss the mid-infrared - emission-line luminosity correlation and present the results of cross correlations with serendipitous X-ray and radio sources. The results show that: (1) obscured objects dominate the overall AGN population, (2) mid-infrared selected AGN candidates exist which lack AGN signatures in their optical spectra but have AGN-like X-ray or radio counterparts, and (3) X-ray and optical classifications of obscured and unobscured AGNs often differ.
机译:我们介绍了在中红外中选择的候选活动银河核(AGNs)的光学和近红外光谱跟踪程序的结果。这项调查选择了在广泛的亮度范围内紧密匹配的正常AGN和模糊AGN,从具有辐射强度L bol〜10〜(10)L的塞弗特星系到高度发光的类星体(L bol〜10〜(14)L),都具有红移范围从0到4.3。选择候选AGN的样品,并在几种不同的24μm通量密度极限下进行中红外色彩切割,以确保在给定的红移范围内具有一定的发光度。该调查由786个候选AGN和类星体组成,其中672个具有光谱红移和分类。其中137个(20%)是具有蓝色连续性的1型AGN,294个(44%)是具有消光AV 2的2型物体。朝向其AGN的有5个,有96个(14%)具有较低消光(AV〜1)的AGN,有145个(22%)具有红移,但在光谱中没有明显的AGN活性迹象。在类星体中,调查对象中有50%的L bol> 10〜(12)L。我们介绍了类型2类星体和对象在其频谱中没有AGN活动迹象的复合频谱。我们还将讨论中红外-发射线的光度相关性,并介绍与偶然X射线和无线电源的互相关结果。结果表明:(1)被遮挡的物体在整个AGN人群中占主导地位;(2)存在中红外选择的AGN候选物,它们在光谱中没有AGN签名,但具有类似AGN的X射线或射电对应物;(3)遮盖和未遮盖的AGN的X射线和光学分类通常不同。

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