“DESI”的版本间差异
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无编辑摘要 |
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(未显示同一用户的6个中间版本) | |||
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http://desi.lbl.gov/ |
http://desi.lbl.gov/ |
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==辅助数据== |
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*https://github.com/EigenHermit/get_stamp_desi_ls/ 在DESI里面切大图的程序,输入RA,DEC和boxsize从DESI的图像数据库里面切出fits file |
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*previously [[BigBOSS]] |
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* The Beijing-Arizona Sky Survey (BASS) |
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* The DECam Legacy Survey (DECaLS) |
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* The Mayall z-band Legacy Survey (MzLS) |
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* BASS[http://batc.bao.ac.cn/BASS/doku.php] lead by Zhouxu |
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* https://www.legacysurvey.org/ |
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* DECaLS |
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* 14000平方度,g,r,z及WISE的四个波段 |
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==光谱巡天== |
==光谱巡天== |
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* * 5000根光纤 |
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* 5 000 spectra simultaneously |
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* wavelength range 360 to 980 nm |
* wavelength range 360 to 980 nm |
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* spectral resolution of R = between 2000 and |
* spectral resolution of R = between 2000 and 5500 |
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* 天区覆盖:14000 deg2,总样本 30 million spectroscopic target |
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* fi�ve-year survey starting in 2020, |
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* 四个子样本 |
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* measuring redshifts over a solid angle of 14 000 deg2 |
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* More than 30 million spectroscopic targets will be selected for four different tracer samples |
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:* (i) luminous red galaxies (LRGs) in the redshift range z = 0.3 to z = 1 |
:* (i) luminous red galaxies (LRGs) in the redshift range z = 0.3 to z = 1 |
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:* (ii) emission line galaxies (ELGs) to z = 1.7 |
:* (ii) emission line galaxies (ELGs) to z = 1.7 |
2023年7月8日 (六) 04:09的最新版本
辅助数据
- https://github.com/EigenHermit/get_stamp_desi_ls/ 在DESI里面切大图的程序,输入RA,DEC和boxsize从DESI的图像数据库里面切出fits file
图像巡天
- The Beijing-Arizona Sky Survey (BASS)
- The DECam Legacy Survey (DECaLS)
- The Mayall z-band Legacy Survey (MzLS)
- https://www.legacysurvey.org/
- 14000平方度,g,r,z及WISE的四个波段
光谱巡天
- * 5000根光纤
- wavelength range 360 to 980 nm
- spectral resolution of R = between 2000 and 5500
- 天区覆盖:14000 deg2,总样本 30 million spectroscopic target
- 四个子样本
- (i) luminous red galaxies (LRGs) in the redshift range z = 0.3 to z = 1
- (ii) emission line galaxies (ELGs) to z = 1.7
- (iii) quasars to higher redshifts (2.1 < z < 3.5)
- (iv) a magnitude-limited Bright Galaxy Survey out to z~0.6 with a median redshift of z~0.2
BGS
- 在bright observing time进行
- a flux limited sample of around 10 million galaxies
- r<19.5 (800 galaxies/deg^2)
- 19.5 < r < 20 (a secondary sample, 600 galaxies/deg^2)