“COSMOS”的版本间差异
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无编辑摘要 |
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| （未显示2个用户的11个中间版本） | |||
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=Field= |
=Field= |
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*2 square degree |
*2 square degree, 最大的深场 |
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*equatorial, for easy access to telescopes in both hemispheres |
*equatorial, for easy access to telescopes in both hemispheres |
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RA (J2000) = 10:00:28.6 |
RA (J2000) = 10:00:28.6 |
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DEC (J2000) = +02:12:21.0 |
DEC (J2000) = +02:12:21.0 |
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=Photometry= |
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=iamged by= |
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* HST ACS (IAB > 27 mag ) |
* HST ACS (IAB > 27 mag ) |
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* WFC3 NIR |
* WFC3 NIR |
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* UltraVISTA (YJHKs,Halpha(z=0.8_ |
* [[UltraVISTA]] (YJHKs,Halpha(z=0.8_ |
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* XMM-Newton |
* XMM-Newton |
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* Chandra |
* Chandra |
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* CFHT |
* CFHT |
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* Subaru |
* Subaru |
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* Spitzer |
* [[Spitzer]] |
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* Hersechel (sub-millimeter) |
* Hersechel (sub-millimeter) |
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* AzTEC, MAMBO (millimeter) |
* AzTEC, MAMBO (millimeter) |
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* VLA (radio) |
* VLA (radio) |
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* CANDELS |
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* A3cosmos（ALMA）：有星表数据释放 |
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* COSMOS-web：JWST 0.6deg |
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==COSMOS/SMUVS== |
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*The Spitzer Matching survey of the Ultra-VISTA ultra-deep stripes (SMUVS, Ashby et al. 2018) is an Exploration Science Program which collected infrared |
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imaging with Spitzer's data (Werner et al. 2004) with the Infrared Array Camera (IRAC, Fazio et al. 2004) at 3.6 and 4.5 um over 0.66 deg2 of the COSMOS �field. |
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*The region covered by SMUVS corresponds to the part of the COSMOS fi�eld with deepest near-IR data from the UltraVISTA program (McCracken et al. 2012) and optical Subaru data (Taniguchi et al. 2007). |
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*The SMUVS data has an average integration time of 25 h/pointing and reaches 80% completeness at 25.5 mag, both in the 3.6 and 4.5 um �lfilters (Deshmukh et al. 2018). |
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=Spectra= |
=Spectra= |
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*zCOSMOS |
*zCOSMOS |
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:*VLT using the [[VIMOS]] spectrograph |
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:#25,000 galaxies at 0.3 < z < 1.0 with IAB < 22.5 |
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:#12,500 star-forming galaxies color selected for 1.4 < z < 2.5 |
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=样本= |
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*grism spectroscopy |
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*X-ray group sample |
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红移在0.2-12， 276 extended source identified from co-added XMM-Newton images |
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*COSMOS2015 released |
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:photometric redshifts and stellar masses for more than half a million objects o |
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:$YJHK_{\rm s}$ images from the UltraVISTA-DR2 survey, $Y$-band from Subaru/Hyper-Suprime-Cam and infrared data from the Spitzer Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program |
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2024年6月20日 (四) 07:19的最新版本
COSMOS( Cosmic Evolution Survey )
Field
- 2 square degree, 最大的深场
- equatorial, for easy access to telescopes in both hemispheres
RA (J2000) = 10:00:28.6 DEC (J2000) = +02:12:21.0
Photometry
- HST ACS (IAB > 27 mag )
- WFC3 NIR
- UltraVISTA (YJHKs,Halpha(z=0.8_
- XMM-Newton
- Chandra
- GALEX
- CFHT
- Subaru
- Spitzer
- Hersechel (sub-millimeter)
- AzTEC, MAMBO (millimeter)
- VLA (radio)
- CANDELS
- A3cosmos（ALMA）：有星表数据释放
- COSMOS-web：JWST 0.6deg
COSMOS/SMUVS
- The Spitzer Matching survey of the Ultra-VISTA ultra-deep stripes (SMUVS, Ashby et al. 2018) is an Exploration Science Program which collected infrared
imaging with Spitzer's data (Werner et al. 2004) with the Infrared Array Camera (IRAC, Fazio et al. 2004) at 3.6 and 4.5 um over 0.66 deg2 of the COSMOS �field.
- The region covered by SMUVS corresponds to the part of the COSMOS fi�eld with deepest near-IR data from the UltraVISTA program (McCracken et al. 2012) and optical Subaru data (Taniguchi et al. 2007).
- The SMUVS data has an average integration time of 25 h/pointing and reaches 80% completeness at 25.5 mag, both in the 3.6 and 4.5 um �lfilters (Deshmukh et al. 2018).
Spectra
- zCOSMOS
- VLT using the VIMOS spectrograph
- 25,000 galaxies at 0.3 < z < 1.0 with IAB < 22.5
- 12,500 star-forming galaxies color selected for 1.4 < z < 2.5
样本
- X-ray group sample
红移在0.2-12， 276 extended source identified from co-added XMM-Newton images
- COSMOS2015 released
- photometric redshifts and stellar masses for more than half a million objects o
- $YJHK_{\rm s}$ images from the UltraVISTA-DR2 survey, $Y$-band from Subaru/Hyper-Suprime-Cam and infrared data from the Spitzer Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program