“SWIRE”的版本间差异
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无编辑摘要 |
无编辑摘要 |
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第4行: | 第4行: | ||
* 波段 |
* 波段 |
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:*IRAC |
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Channel Image Sensitivity DR2 Catalog 95% Completenes |
Channel Image Sensitivity DR2 Catalog 95% Completenes |
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3.6 µm 3.7 µJy 14 µJy |
3.6 µm 3.7 µJy 14 µJy |
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第10行: | 第10行: | ||
5.8 µm 48 µJy 2 µJy |
5.8 µm 48 µJy 2 µJy |
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8.0 µm 37.8 µJy 56 µJy |
8.0 µm 37.8 µJy 56 µJy |
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:*MIPS |
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Channel Image Sensitivity DR2 Catalog Limits |
Channel Image Sensitivity DR2 Catalog Limits |
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24 µm 230 µJy 280 µJy (90% completeness) |
24 µm 230 µJy 280 µJy (90% completeness) |
2013年3月21日 (四) 01:58的最新版本
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.