“星系巡天”的版本间差异

来自Shiyin's note
跳到导航 跳到搜索
第62行: 第62行:


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

[[VANDELS]]


===大望远镜===
===大望远镜===

2018年3月21日 (三) 09:03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

VANDELS

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).
  • 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.

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