“SWIRE”的版本间差异
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（以“SWIRE(The Spitzer Wide-area InfraRed Extragalactic survey) * 50 sq deg * 波段 #IRAC Channel Image Sensitivity DR2 Catalog 95% Completenes 3.6 µm 3.7 µJy 1...”为内容创建页面） |
无编辑摘要 |
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* 50 sq deg |
* 50 sq deg |
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* 波段 |
* 波段 |
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#IRAC |
#IRAC |
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Channel Image Sensitivity DR2 Catalog 95% Completenes |
Channel Image Sensitivity DR2 Catalog 95% Completenes |
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70 µm 18 mJy 15.5 mJy (flux limits) |
70 µm 18 mJy 15.5 mJy (flux limits) |
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160 µm 150 mJy 90 mJy (flux limits) |
160 µm 150 mJy 90 mJy (flux limits) |
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*天区（一共4个） |
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#The XMM Large-Scale Structure Survey XMM-LSS and the NOAO Deep Wide-Field Survey NOAO DWS (South) |
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#The European Large-Area ISO Survey (ELAIS) - ELAIS N1, N2, and S1. |
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#The Chandra Deep South Survey Field. |
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#The well-studied Lockman Hole. |
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2013年3月21日 (四) 01:58的版本
SWIRE(The Spitzer Wide-area InfraRed Extragalactic survey)
- 50 sq deg
- 波段
- IRAC
Channel Image Sensitivity DR2 Catalog 95% Completenes 3.6 µm 3.7 µJy 14 µJy 4.5 µm 5.4 µJy 15 µJy 5.8 µm 48 µJy 2 µJy 8.0 µm 37.8 µJy 56 µJy
- MIPS
Channel Image Sensitivity DR2 Catalog Limits 24 µm 230 µJy 280 µJy (90% completeness) 70 µm 18 mJy 15.5 mJy (flux limits) 160 µm 150 mJy 90 mJy (flux limits)
- 天区（一共4个）
- The XMM Large-Scale Structure Survey XMM-LSS and the NOAO Deep Wide-Field Survey NOAO DWS (South)
- The European Large-Area ISO Survey (ELAIS) - ELAIS N1, N2, and S1.
- The Chandra Deep South Survey Field.
- The well-studied Lockman Hole.