The Stellar Abundances and Galactic Evolution Survey (SAGES). I. General Description and the First Data Release (DR1)

被引：17

作者：

Fan, Zhou ^{[1
]}

Zhao, Gang ^{[1
,2
]}

Wang, Wei ^{[1
]}

Zheng, Jie ^{[1
]}

Zhao, Jingkun ^{[1
]}

Li, Chun ^{[1
]}

Chen, Yuqin ^{[1
]}

Yuan, Haibo ^{[3
]}

Li, Haining ^{[1
]}

Tan, Kefeng ^{[1
]}

Song, Yihan ^{[1
]}

Zuo, Fang ^{[1
]}

Huang, Yang ^{[1
,2
]}

Luo, Ali ^{[1
]}

Esamdin, Ali ^{[4
]}

Ma, Lu ^{[4
]}

Li, Bin ^{[5
,6
]}

Song, Nan ^{[7
]}

Grupp, Frank ^{[8
]}

Zhao, Haibin ^{[5
,6
]}

Ehgamberdiev, Shuhrat A. ^{[9
,10
]}

Burkhonov, Otabek A. ^{[9
]}

Feng, Guojie ^{[4
]}

Bai, Chunhai ^{[4
]}

Zhang, Xuan ^{[4
]}

Niu, Hubiao ^{[4
]}

Khodjaev, Alisher S. ^{[9
]}

Khafizov, Bakhodir M. ^{[9
]}

Asfandiyarov, Ildar M. ^{[9
]}

Shaymanov, Asadulla M. ^{[9
]}

Karimov, Rivkat G. ^{[9
]}

Yuldashev, Qudratillo ^{[9
]}

Lu, Hao ^{[5
]}

Zhaori, Getu ^{[5
]}

Hong, Renquan ^{[5
]}

Hu, Longfei ^{[5
]}

Liu, Yujuan ^{[1
]}

Xu, Zhijian ^{[5
,11
]}

机构：

[1] Chinese Acad Sci, CAS Key Lab Opt Astron, Natl Astron Observ, Beijing 100101, Peoples R China

[2] Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China

[3] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China

[4] Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China

[5] Chinese Acad Sci, Key Lab Planetary Sci, Purple Mt Observ, Nanjing 210023, Peoples R China

[6] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China

[7] China Sci & Technol Museum, Beijing 100101, Peoples R China

[8] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[9] Uzbek Acad Sci, Ulugh Beg Astron Inst, Astron Skaya Str 33, Tashkent, Uzbekistan

[10] Natl Univ Uzbekistan, Tashkent, Uzbekistan

[11] China Three Gorges Univ, Yichang 443002, Peoples R China

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2023年 / 268卷 / 01期

基金：

中国国家自然科学基金;

关键词：

DIGITAL SKY SURVEY; DARK-MATTER HALOES; PHOTOMETRIC CALIBRATION; COLOR REGRESSION; METALLICITY DISTRIBUTION; EXTINCTION COEFFICIENTS; WHITE-DWARFS; DUSTY VEIL; NIGHT-SKY; STARS;

D O I：

10.3847/1538-4365/ace04a

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Stellar Abundances and Galactic Evolution Survey (SAGES) of the northern sky is a specifically designed multiband photometric survey aiming to provide reliable stellar parameters with accuracy comparable to those from low-resolution optical spectra. It was carried out with the 2.3 m Bok telescope of Steward Observatory and three other telescopes. The observations in the u ( s ) and v ( s ) passband produced over 36,092 frames of images in total, covering a sky area of & SIM;9960 deg(2). The median survey completenesses of all observing fields for the two bands are u (s) = 20.4 mag and v ( s ) = 20.3 mag, respectively, while the limiting magnitudes with signal-to-noise ratio of 100 are u ( s ) & SIM; 17 mag and v ( s ) & SIM; 18 mag, correspondingly. We combined our catalog with the data release 1 (DR1) of the first Panoramic Survey Telescope And Rapid Response System (Pan-STARRS, PS1) catalog, and obtained a total of 48,553,987 sources that have at least one photometric measurement in each of the SAGES u ( s ) and v ( s ) and PS1 grizy passbands. This is the DR1 of SAGES, released in this paper. We compared our gri point-source photometry with those of PS1 and found an rms scatter of & SIM;2% difference between PS1 and SAGES for the same band. We estimated an internal photometric precision of SAGES to be of the order of & SIM;1%. Astrometric precision is better than 0.& DPRIME;2 based on comparison with DR1 of the Gaia mission. In this paper, we also describe the final end-user database, and provide some science applications.

引用

页数：18

共 38 条

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