查看“DESI”的源代码

http://desi.lbl.gov/
==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)

==Data Release==
* Petal： A wedge of 1/10 of the DESI focal plane, containing 500 positioners/fibers going to a single spectrograph. The petal number is the same as the spectrograph number to which it is attached.
* Rosette: One of 20 non-overlapping subfields that compose the total observation field of the One-Percent Survey (sv3). Each rosette was observed at least 12 times during the One-Percent Survey to ensure high a fiber assignment completeness of at least 85% for ELGs and over 94% for the other tracers (BGS, LRGs, and QSOs).
* In DESI, spectroscopic productions are alphabetically named after mountains or mountain ranges. (Fuji,Iron)