“DESI”的版本间差异

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* BASS[http://batc.bao.ac.cn/BASS/doku.php] lead by Zhouxu
* BASS[http://batc.bao.ac.cn/BASS/doku.php] lead by Zhouxu
* DECaLS
* DECaLS

*
==光谱巡天==
* 5 000 spectra simultaneously
* wavelength range 360 to 980 nm *
* spectral resolution of R = between 2000 and 5 500,
* fi�ve-year survey starting in 2020,
* measuring redshifts over a solid angle of 14 000 deg2
* More than 30 million spectroscopic targets will be selected for four different tracer samples
:* (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
* r<19.5 (800 galaxies/deg^2)
* 19.5 < r < 20 (a secondary sample, 600 galaxies/deg^2)

2020年10月25日 (日) 14:11的版本

http://desi.lbl.gov/

图像

  • BASS[1] lead by Zhouxu
  • DECaLS

光谱巡天

  • 5 000 spectra simultaneously
  • wavelength range 360 to 980 nm *
  • spectral resolution of R = between 2000 and 5 500,
  • fi�ve-year survey starting in 2020,
  • measuring redshifts over a solid angle of 14 000 deg2
  • More than 30 million spectroscopic targets will be selected for four different tracer samples
  • (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
  • r<19.5 (800 galaxies/deg^2)
  • 19.5 < r < 20 (a secondary sample, 600 galaxies/deg^2)