“星系巡天”的版本间差异

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'''这里主要是光学的,其它波段参考[[Multi-wavelength]]'''
==综合==
==综合==
[[SDSS IV|AS3]]
[[SDSS]]
*[[eBOSS]]
*[[ManGA]]


[[BigBOSS]]
[[SDSS IV]]


==测光巡天==
==测光巡天==
[[AEGIS]]:2007
[[AEGIS]]:2007


[[COSMOS]]:2008
[[AGES]]


[[VIKING]]ongoing
[[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]]

[[SkyMapper]]

[[VIDEO]]

[[J-PLUS]]

[[SCUSS]]

[[巡天仿真]]


==红移巡天==
==红移巡天==
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[[VIPERS]]
[[VIPERS]]

[[SHELS]]

[[GAMA]]


[[DEEP2]]
[[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)
===[[JWST]]上的NIRspec===
*NIRSpec is equipped with an integral field unit optimized for the spectroscopic study of complex extended objects. It will provide 900 spectra per exposure over a field of view of 3 x 3 arcminutes.(0.6-5mu)

==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==
==星系团==

2024年6月18日 (二) 02:18的最新版本

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

Survey_comparison

DES

HSC-SSP

GASS

MGC

VIKING

KIDS

UKIDSS

Pan-STAR

SERVS

SkyMapper

VIDEO

J-PLUS

SCUSS

巡天仿真

红移巡天

WiggleZ

VIPERS

SHELS

GAMA

DEEP2

VVDS

VUDS

LEGA-C

VANDELS


大望远镜

  • PFS
  • CFHT MSE
10m

IFS

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)

JWST上的NIRspec

  • NIRSpec is equipped with an integral field unit optimized for the spectroscopic study of complex extended objects. It will provide 900 spectra per exposure over a field of view of 3 x 3 arcminutes.(0.6-5mu)

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