“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]]
[[SDSS]]
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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]]


[[VIKING]]ongoing
[[GASS]]


[[KIDS]]
[[MGC]]


[[HATLAS]]
[[VIKING]]

[[KIDS]]


[[UKIDSS]]
[[UKIDSS]]
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[[SERVS]]
[[SERVS]]


[[THINGS]]
[[SkyMapper]]


[[VIDEO]]
[[VIDEO]]


[[WISE]]
[[J-PLUS]]


[[SCUSS]]
[[SCUSS]]

[[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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[[LEGA-C]]
[[LEGA-C]]

[[VANDELS]]



===大望远镜===
*PFS
*CFHT MSE
:10m


==IFS==
==IFS==
*[[CALIFA]]
*[[CALIFA]]
*[[CHILI]]
*[[CHILI]]
*[[ATLAS3D]]
*[[MaNGA]]: 同时17个源
*[[MaNGA]]: 同时17个源
*[[SAMI]]: 同时观测12个源
*[[SAMI]]: 同时观测12个源
*[[MASSIVE]] galaxy survey [Ma et al. 2014]
*[[MASSIVE]] galaxy survey [Ma et al. 2014]
:MASSIVE is a volume-limited sample of the 116 most massive early-type galaxies within 108 Mpc(Mk<-25.3).
:IFS (107"x107") taken with the Mitchell Spectrograph on the 2.7m Harlan J. Smith telescope at the McDonald Observatory (Green et al. 2013)



*[[S7]]


===VLT上的两个IFS终端===
===VLT上的两个IFS终端===
*MUSE
*MUSE
:a giant IFS on VLT wth 1 arcmin FoV, 0.2" spaxel
:*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
*KMOS
:The K-band Multi Object Spectrograph (KMOS). IFS in the near-infrared bands for 24 targets simultaneously.
: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==
==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