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All-wavelength Extended Groth Strip International Survey (AEGIS)
All-wavelength Extended Groth Strip International Survey (AEGIS)


*Region:Extended Groth Strip (EGS: Ra=14h17m, DEc= 52d�30m�)
*Region:[[Extended Groth Strip]] (EGS: Ra=14h17m, DEc= 52d30m)
:a Hubble Space Telescope (HST) survey consisting of 28 Wide-
:a Hubble Space Telescope (HST) survey consisting of 28 Wide-Field Planetary Camera 2 (WFPC2) pointings carried out in 1994 by the WFPC team;
⚫
:low extinction, low Galactic/zodiacal infrared emission, and good schedulability by space-based observatories
Field Planetary Camera 2 (WFPC2) pointings carried out in 1994
by the WFPC team
⚫
:low extinction, low Galactic/zodiacal infrared emission, and good
schedulability by space-based observatories


* comparsion with other deep fields
* comparsion with other deep fields
:2x (for HST) to 4x (for Spitzer and Chandra) larger than the combined [[GOODS]] fields
:2x (for HST) to 4x (for Spitzer and Chandra) larger than the combined [[GOODS]] fields
:The [[GEMS]] field covers a similar area to similar depths but was studied by the COMBO-
:The [[GEMS]] field covers a similar area to similar depths but was studied by the [[COMBO-17]] photometric redshift survey rather than a spectroscopic survey.
⚫
::the GEMS F850LP imaging is too shallow to study subcomponent colors for most galaxies.
17 photometric redshift survey rather than a spectroscopic survey.
::the GEMS F850LP imaging is too shallow to
⚫
study subcomponent colors for most galaxies.
::Most AEGIS data sets cover ∼0.5–1 deg2, smaller than the 2 deg2 [[COSMOS]] field, but AEGIS is deeper
::Most AEGIS data sets cover ∼0.5–1 deg2, smaller than the 2 deg2 [[COSMOS]] field, but AEGIS is deeper
::AEGIS is that deep HST/ACS imaging is available in two bands (F606W�F814W), in contrast to only F814W for the
::AEGIS is that deep HST/ACS imaging is available in two bands (F606W+F814W), in contrast to only F814W for the COSMOS field;

COSMOS field;
* Data Set
:Chandra/ACIS
:GALEX
:CFHT/MegaCam
:CFHT/CFH12K
:HST/ACS(WFC)
:HST/NICMOS(NIC3)
:Palomar/WIRC
:Spitzer/IRAC
:Spitzer/MIPS
:VLA
:Keck/DEIMOS([[DEEP2]]/Spectra)

2016年1月12日 (二) 13:20的最新版本

All-wavelength Extended Groth Strip International Survey (AEGIS)

a Hubble Space Telescope (HST) survey consisting of 28 Wide-Field Planetary Camera 2 (WFPC2) pointings carried out in 1994 by the WFPC team;
low extinction, low Galactic/zodiacal infrared emission, and good schedulability by space-based observatories
  • comparsion with other deep fields
2x (for HST) to 4x (for Spitzer and Chandra) larger than the combined GOODS fields
The GEMS field covers a similar area to similar depths but was studied by the COMBO-17 photometric redshift survey rather than a spectroscopic survey.
the GEMS F850LP imaging is too shallow to study subcomponent colors for most galaxies.
Most AEGIS data sets cover ∼0.5–1 deg2, smaller than the 2 deg2 COSMOS field, but AEGIS is deeper
AEGIS is that deep HST/ACS imaging is available in two bands (F606W+F814W), in contrast to only F814W for the COSMOS field;
  • Data Set
Chandra/ACIS
GALEX
CFHT/MegaCam
CFHT/CFH12K
HST/ACS(WFC)
HST/NICMOS(NIC3)
Palomar/WIRC
Spitzer/IRAC
Spitzer/MIPS
VLA
Keck/DEIMOS(DEEP2/Spectra)
取自“http://202.127.29.3/~shen/wiki/index.php?title=AEGIS&oldid=1967”