“Multi-wavelength”的版本间差异
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==射电== |
==射电== |
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*[[JCMT]] |
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*[[ALMA]] |
*[[ALMA]] |
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*[[SMG]]亚毫米波源[[SCUBA]] [[SCUBA-2]] |
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: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 |
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: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]),[[http://arxiv.org/abs/1609.00388]] |
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===巡天=== |
===巡天=== |
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*[[HI巡天]] |
*[[HI巡天]] |
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2016年9月5日 (一) 05:45的版本
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
红外
- WISE
- IRAS
- 30cm口径，all sky survey at 12, 25, 60 and 100 µm.
Herschel
- Herschel reference survey (HRS)
- 323 K-band(Ks<12) selected galaxies from 100 to 500 mu, volume limited (between 15 and 25 Mpc)
- 星系的气（HI+H2）尘比对环境的依赖性很弱（从isolated 到 virgo cluster）,团星系同样的气体，尘埃略多[1]
- 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]]
