查看“星系巡天”的源代码

'''这里主要是光学的，其它波段参考[[Multi-wavelength]]'''
==综合==
[[SDSS]]

[[SDSS IV]]

==测光巡天==
[[AEGIS]]:2007

[[AGES]]

[[ALHAMBRA]]

[[CANDLES]]

[[CLAUDS]]

[[CFHTLS]]

[[COSMOS]]

[[文件:Survey comparison.png|缩略图|Survey_comparison]]

[[DES]]

[[HSC-SSP]]

[[GASS]]

[[MGC]]

[[VIKING]]

[[KIDS]]

[[UKIDSS]]

[[Pan-STAR]]

[[SERVS]]

[[VIDEO]]

[[J-PLUS]]

[[SCUSS]]

==红移巡天==
[[WiggleZ]]

[[VIPERS]]

[[SHELS]]

[[GAMA]]

[[DEEP2]]

[[VVDS]]

[[VUDS]]

[[LEGA-C]]

[[VANDELS]]



===大望远镜===
*PFS
*CFHT MSE
:10m

==IFS==
*[[CALIFA]]
*[[CHILI]]
*[[ATLAS3D]]
*[[MaNGA]]: 同时17个源
*[[SAMI]]: 同时观测12个源
*[[MASSIVE]] galaxy survey [Ma et al. 2014]

*[[S7]]

===VLT上的两个IFS终端===
*MUSE
:*a giant IFS on VLT wth 1 arcmin FoV, 0.2" spaxel, wide simultaneous wavelength coverage (4650 − 9300Å), relatively high spectral resolution (R ∼ 3000), and high throughput (35% end-to-end).
:*The concept of MUSE foresees the splitting of the adaptive optics corrected field of view in 24 sub-fields. Each of these sub-fields is fed into a spectrograph (called Integral Field Unit, IFU). An image slicer in front of each IFU serves as entrance slit, thus producing a spatially resolved spectrum of the full sub-field.
*KMOS
:The K-band Multi Object Spectrograph (KMOS). IFS in the near-infrared bands for 24 targets simultaneously.
:14x14 spectra with ~1000 Nyquist-sampled spectral resolution elements for each of the 24 independent sub-fields. 
:Each IFU has a square field of view of 2.8 x 2.8 arcsec;ensures uniform spatial sampling of 0.2 x 0.2 arcsec whilst maintaining Nyquist sampling (~2 pixel)

==Keck上的终端==
*MOSFIRE
:Multi-Object Spectrometer for Infra-Red Exploration

===100%filling IFUs===
:SAURON:33"x4"
:WiFeS:38"x25"

==星系团==
[[ICBS]]

[[SpARCS]]

[[GCLASS]]