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The IRAS PSC/FSC Combined Catalogue

机译:IRAS PSC / FSC组合目录

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Optical identifications of a few thousands of IRAS sources showed that IRAS Point Source and IRAS Faint Source catalogues (PSC and FSC, respectively) contain many quasars and active galactic nuclei, late-type stars, planetary nebulae, variables, etc. To increase the efficiency of using IRAS PSC and FSC, which contain a lot of common sources, one needs a joint catalogue of all IRAS point sources with improved data based on both catalogues. However, cross-correlation of the catalogues is not so easy, as the association of many sources is relative, and not always it is obvious, whose source from one catalogue corresponds to the other one in the second catalogue. This problem exists in case of using standard cross-correlation tools like VizieR. Therefore, we have created a tool for cross-matching astronomical catalogues and we have applied it to IRAS PSC and FSC. Using this tool we have carried out identifications with a search radius corresponding to 3 σ of errors for each source individually rather than a standard radius for all sources. As a result, we obtained 73,770 associations. We showed that in case of cross-correlation of these catalogues by VizieR, we had to take 161.95 arcseconds radius not to lose any association; however, in this case a lot of false associations appear for many sources. In addition, we have made cross-correlations with AKARIIRC, AKARI-FIS and WISE catalogues. As a result we created a catalogue with high positional accuracy and with 17 photometric measurements from 1.25 to 160 μm range, providing a detailed catalogue for IRAS point sources.
机译:对数千个IRAS源的光学识别表明,IRAS点源和IRAS微弱源目录(分别为PSC和FSC)包含许多类星体和活动星系核,后型恒星,行星状星云,变量等。提高效率在使用IRAS PSC和FSC(包含许多常见资源)的过程中,需要将所有IRAS点源的联合目录与基于这两个目录的数据进行改进。但是,目录的互相关不是那么容易,因为许多来源的关联是相对的,而且并非总是很明显,后者来自一个目录的来源对应于第二个目录中的另一个。在使用标准互相关工具(例如VizieR)的情况下会出现此问题。因此,我们创建了一个用于交叉匹配天文目录的工具,并将其应用于IRAS PSC和FSC。使用该工具,我们进行了识别,其搜索半径分别对应于每个辐射源的3σ误差,而不是所有辐射源的标准半径。结果,我们获得了73,770个关联。我们证明了在VizieR对这些目录进行互相关的情况下,我们必须花费161.95 arcseconds半径才能失去任何关联。但是,在这种情况下,许多来源会出现许多错误的关联。此外,我们还与AKARIIRC,AKARI-FIS和WISE目录进行了互相关。结果,我们创建了一个目录,该目录具有很高的位置精度,并且具有1.25至160μm范围内的17个光度测量值,为IRAS点源提供了详细的目录。

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