“Multi-wavelength”的版本间差异
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==光学，近红外== |
==光学，近红外== |
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参见[[星系巡天]] |
参见[[星系巡天]] |
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===Ha窄带=== |
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*近邻星系的100Mpc以内的数据见[https://arxiv.org/abs/1710.05016] |
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==红外== |
==红外== |
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*[[Spitzer]] |
*[[Spitzer]] |
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===[[Herschel]]=== |
===[[Herschel]]=== |
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*Herschel reference survey (HRS) |
*[[Herschel reference survey (HRS)]] |
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:323 K-band(Ks<12) selected galaxies from 100 to 500 mu, volume limited (between 15 and 25 Mpc) |
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*Herscchel [[Stripe 82]] survey |
*Herscchel [[Stripe 82]] survey |
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:79 deg^2 with SPIRE at 250,350,500 mu |
:79 deg^2 with SPIRE at 250,350,500 mu |
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2017年10月16日 (一) 13:17的最新版本
高能
- Swift/BAT (burst alert telescope) AGN
- 313 AGN
- XBOOTES Chandra
- MAXI，Monitor of All sky X-ray Image，装在空间站上
紫外
- SWIFT UVOT
- 30 cm telescope with a 17× 17 square arcminute field of view that provides ultraviolet and optical coverage (1600–8000A)
光学，近红外
参见星系巡天
Ha窄带
- 近邻星系的100Mpc以内的数据见[1]
红外
- WISE
- IRAS
- 30cm口径，all sky survey at 12, 25, 60 and 100 µm.
Herschel
- Herscchel Stripe 82 survey
- 79 deg^2 with SPIRE at 250,350,500 mu
- KINGFISH
- HELP
- Herschel Extra-galactic Legacy Project (Vaccari (2016), Oliver et al. 2016, in prep.) aims to collate and homogenize observations from many astronomical observatories to provide an integrated data set covering a wide range of wavelengths from the radio to the UV.
- data from the extra-surveys covering over 1300 deg2
- H-ATLAS
- Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS)
- largest-area submillimetre (submm) survey conducted with the Herschel Space Observatory
- imaging around 600 deg2 at 100 and 160µm with PACS and 250, 350 and 500µm with SPIRE ,
- Data release 1(DR1) covers 161 deg2 in three equatorial fields at RA of approximately 9h, 12h and 14.5h (GAMA9, GAMA12, GAMA15),
- DR1 paper [2]
射电
- 850mu的源，JCMT的分辨率只能到15arcsec，confuse limit大概在2mJy。80%的SMG的流量小于2mJy
- 强引力透镜？ALMA的深场（视场小），颜色选(z − K), (K−[3.6]) and ([3.6]-[4.5]),[[3]]
波段
- L 波段 ~ 20cm
- S 波段 ~ 10cm
- C 波段 ~ 6cm
- X 波段 ~ 3cm
- Ku 波段 ~2cm
- K 波段 ~1cm
巡天
专题
HI巡天
CO
- COLD GASS
- CO legacy Database for GASS
- 3666 galaxies randomly from GASS to form COLD GASS
- deep CO(1-0) imaging with IRAM