“星系巡天”的版本间差异

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===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).
*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.

2017年10月12日 (四) 12:54的版本

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

CFHTLS

COSMOS:2008

Survey_comparison

DES

DESI

GASS

MGC

VIKINGongoing

KIDS

UKIDSS

Pan-STAR

SERVS

VIDEO

SCUSS

HSC-SSP

红移巡天

WiggleZ

VIPERS

SHELS

BOSS

GAMA

DEEP2

VVDS

VUDS

LEGA-C

大望远镜

  • PFS
  • CFHT MSE
10m

IFS

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)

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).

  • KMOS
The K-band Multi Object Spectrograph (KMOS). IFS in the near-infrared bands for 24 targets simultaneously.

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