Calibrating photometric redshift measurements with the Multi-channel Imager (MCI) of the China Space Station Telescope (CSST)
Ye Cao, Yan Gong, Zhen-Ya Zheng, and Chun Xu

TL;DR
This paper evaluates the filter design of the CSST's Multi-channel Imager for accurate photometric redshift measurements, demonstrating its effectiveness in meeting scientific goals through mock data analysis.
Contribution
It assesses the MCI filter design's capability to produce precise photo-z estimates, confirming its suitability for the CSST survey.
Findings
MCI filters achieve photo-z accuracy of sigma_z~0.017
Outlier fraction is approximately 2.2% with current filters
Filters can improve main survey photo-z accuracy to sigma_z~0.015
Abstract
The China Space Station Telescope (CSST) photometric survey aims to perform a high spatial resolution (~0.15'') photometric imaging for the targets that cover a large sky area (~17,500 deg^2) and wide wavelength range (from NUV to NIR). It expects to explore the properties of dark matter, dark energy, and other important cosmological and astronomical areas. In this work, we evaluate whether the filter design of the Multi-channel Imager (MCI), one of the five instruments of the CSST, can provide accurate photometric redshift (photo-z) measurements with its nine medium-band filters to meet the relevant scientific objectives. We generate the mock data based on the COSMOS photometric redshift catalog with astrophysical and instrumental effects. The application of upper limit information of low signal-to-noise ratio (SNR) data is adopted in the estimation of photo-z. We investigate the…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · CCD and CMOS Imaging Sensors
