“星系巡天”的版本间差异

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(未显示同一用户的12个中间版本)
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[[CANDLES]]
[[CANDLES]]

[[CLAUDS]]


[[CFHTLS]]
[[CFHTLS]]


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


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


[[DESI]]
[[HSC-SSP]]


[[GASS]]
[[GASS]]
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[[MGC]]
[[MGC]]


[[VIKING]]ongoing
[[VIKING]]


[[KIDS]]
[[KIDS]]
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[[SERVS]]
[[SERVS]]

[[SkyMapper]]


[[VIDEO]]
[[VIDEO]]
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[[SCUSS]]
[[SCUSS]]


[[HSC-SSP]]
[[巡天仿真]]


==红移巡天==
==红移巡天==
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[[SHELS]]
[[SHELS]]

[[BOSS]]


[[GAMA]]
[[GAMA]]
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[[VANDELS]]
[[VANDELS]]



[[SHELS]]


===大望远镜===
===大望远镜===
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:14x14 spectra with ~1000 Nyquist-sampled spectral resolution elements for each of the 24 independent sub-fields.
: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)
: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==
==Keck上的终端==

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