“AEGIS”的版本间差异
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（以“All-wavelength Extended Groth Strip International Survey (AEGIS) *Region:Extended Groth Strip (EGS: Ra=14h17m, DEc= 52d�30m�) :a Hubble Space Telescope (HST) s...”为内容创建页面） |
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All-wavelength Extended Groth Strip International Survey (AEGIS) |
All-wavelength Extended Groth Strip International Survey (AEGIS) |
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*Region:Extended Groth Strip (EGS: Ra=14h17m, DEc= |
*Region:Extended Groth Strip (EGS: Ra=14h17m, DEc= 52d30m) |
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:a Hubble Space Telescope (HST) survey consisting of 28 Wide- |
:a Hubble Space Telescope (HST) survey consisting of 28 Wide- |
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Field Planetary Camera 2 (WFPC2) pointings carried out in 1994 |
Field Planetary Camera 2 (WFPC2) pointings carried out in 1994 |
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* comparsion with other deep fields |
* comparsion with other deep fields |
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: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 |
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: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. |
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17 photometric redshift survey rather than a spectroscopic survey. |
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::the GEMS F850LP imaging is too shallow to |
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::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 |
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::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; |
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COSMOS field; |
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* Data Set |
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:Chandra/ACIS |
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:GALEX |
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:CFHT/MegaCam |
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:CFHT/CFH12K |
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:HST/ACS(WFC) |
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:HST/NICMOS(NIC3) |
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:Palomar/WIRC |
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:Spitzer/IRAC |
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:Spitzer/MIPS |
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:VLA |
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:Keck/DEIMOS([[DEEP2]]/Spectra) |
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2013年3月21日 (四) 08:34的版本
All-wavelength Extended Groth Strip International Survey (AEGIS)
- Region:Extended Groth Strip (EGS: Ra=14h17m, DEc= 52d30m)
- 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)