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SRGz: Classification of eROSITA Point X-ray Sources in the 1 $${\%}$$ DESI Region and Calibration of Photometric Redshifts*
Astronomy Letters ( IF 0.9 ) Pub Date : 2023-11-01 , DOI: 10.1134/s1063773723110129
A. V. Meshcheryakov , G. A. Khorunzhev , S. A. Voskresenskaya , P. S. Medvedev , M. R. Gilfanov , R. A. Sunyaev

Abstract

We consider the population of point X-ray sources from the two-year SRG/eROSITA survey in the 1 \(\%\) DESI spectroscopic survey region in the eastern Galactic hemisphere (eROSITA–1 \(\%\) DESI–East). The data under consideration combine a large survey area (compared to the medium-format Stripe82X and XMM-XXL X-ray surveys) and a record high completeness of spectroscopy for the optical counterparts of X-ray sources. We compare the results of the photometric (SRGz) and spectroscopic/astrometric (DESI EDR, SDSS, HELP, GAIA) measurements of the classes and redshifts of objects in three X-ray-flux-limited eROSITA–1 \(\%\) DESI–East samples: \(F_{X,0.5-2}\geqslant 4\times 10^{-14}\) erg s \({}^{-1}\) cm \({}^{-2}\) (bright), \(F_{X,0.5-2}=(1.5{-}4)\times 10^{-14}\) erg s \({}^{-1}\) cm \({}^{-2}\) (medium), and \(F_{X,0.5-2}=(0.6{-}1.5)\times 10^{-14}\) erg s \({}^{-1}\) cm \({}^{-2}\) (faint) with a total area of 91.4, 91.4, and 16.62 deg \({}^{2}\) , respectively. We propose a new method of postprocessing the probabilistic photo-z predictions based on a two-temperature correction of the probability density function \(PDF(z)\) . This approach allows the calibration of the probabilistic predictions and confidence intervals of the photometric redshifts for eROSITA X-ray sources obtained by SRGz to be improved significantly.



中文翻译:

SRGz:1 $${\%}$$ DESI 区域中 eROSITA 点 X 射线源的分类和光度红移校准*

摘要

我们考虑了东银河半球1 \(\%\) DESI 光谱巡天区域 (eROSITA–1 \(\%\) DESI–East两年 SRG/eROSITA 巡天的点 X 射线源数量)。正在考虑的数据结合了大调查区域(与中格式 Stripe82X 和 XMM-XXL X 射线调查相比)和 X 射线源光学对应物的光谱学的高完整性。我们比较了三个 X 射线通量限制 eROSITA–1 \(\%\)中物体的类别和红移的光度 (SRGz) 和光谱/天体测量 (DESI EDR、SDSS、HELP、GAIA) 测量结果DESI–East 样本:\(F_{X,0.5-2}\geqslant 4\times 10^{-14}\) erg s \({}^{-1}\) cm \({}^{-2 }\)(亮),\(F_{X,0.5-2}=(1.5{-}4)\times 10^{-14}\) erg s \({}^{-1}\) cm \ ({}^{-2}\)(中),且\(F_{X,0.5-2}=(0.6{-}1.5)\times 10^{-14}\) erg s \({}^ {-1}\) cm \({}^{-2}\)(微弱),总面积分别为 91.4、91.4 和 16.62 deg \({}^{2}\)我们提出了一种基于概率密度函数\(PDF(z)\)的两个温度校正来后处理概率 photo-z 预测的新方法。这种方法可以显着改善 SRGz 获得的 eROSITA X 射线源光度红移的概率预测和置信区间的校准。

更新日期:2023-11-01
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