论文标题

来自盖亚和明智数据的候选人双重和镜头的类星体目录

A catalog of candidate double and lensed quasars from Gaia and WISE data

论文作者

Makarov, Valeri V., Secrest, Nathan J.

论文摘要

在Gaia EDR3中使用紧密分离的多个或双源以及光度法和星体元数据之间的强相关性,我们生成了一个由3140个系统组成的候选候选者double和乘以成型的镜头的类星体和AGN。它包括两个部分重叠的零件,一个带有扰动数据的远处(大于1个大于1)的源样本,以及Gaia以小于$ 2 \ arcsec $的分离为单独的组件。对于第一部分(大约是已发布目录的三分之一),我们使用来自GAIA EDR3的独立光度法和星体数据,通过多个机器学习预测和分类方法合成了6.17亿个红移,并以准确的光谱型和Astretric数据与SDSS的准确光谱红移一起训练。使用这些合成红移,我们估计在目录的这一部分中,光谱红移低于1的闯入者的速率为4.9%。未解决的候选候选二重AGN和类星体被选为少量bp/rp多余因子(PHOT_BP_RP_EXCESS_FACTOR)的来源,这对源范围很敏感,从而将我们的搜索限制为高降低的Quasars。在目录的第二部分中,对测量的视差和近邻统计的其他过滤器可用于减少剩余恒星污染物的传播。估计的阳性率(双重或多个来源)为98 \%,估计的双重(物理相关类星体)大于54 \%。更详细地讨论了几十个偶然发现的感兴趣的对象,包括已知的和新的镜头图像,行星星云和奇特形态的年轻红外恒星,以及在SDS中具有灾难性红移误差的类星体。

Making use of strong correlations between closely separated multiple or double sources and photometric and astrometric metadata in Gaia EDR3, we generate a catalog of candidate double and multiply imaged lensed quasars and AGNs, comprising 3140 systems. It includes two partially overlapping parts, a sample of distant (redshifts mostly greater than 1) sources with perturbed data, and systems resolved into separate components by Gaia at separations less than $2\arcsec$. For the first part, which is roughly one third of the published catalog, we synthesized 0.617 million redshifts by multiple machine learning prediction and classification methods, using independent photometric and astrometric data from Gaia EDR3 and WISE with accurate spectroscopic redshifts from SDSS as a training set. Using these synthetic redshifts, we estimate a rate of 4.9\% of interlopers with spectroscopic redshift below 1 in this part of the catalog. Unresolved candidate double and dual AGNs and quasars are selected as sources with marginally high BP/RP excess factor (phot_bp_rp_excess_factor), which is sensitive to source extent, limiting our search to high-redshift quasars. For the second part of the catalog, additional filters on measured parallax and near-neighbor statistics are applied to diminish the propagation of remaining stellar contaminants. The estimated rate of positives (double or multiple sources) is 98\%, and the estimated rate of dual (physically related quasars) is greater than 54\%. A few dozen serendipitously found objects of interest are discussed in more detail, including known and new lensed images, planetary nebulae and young infrared stars of peculiar morphology, and quasars with catastrophic redshift errors in SDSS.

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