查看“Multi-wavelength”的源代码

*[[黑体谱]]

*[[cooling rate]]

==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==
*[[GALEX]]

*[[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]]

==红外==

*[[WISE]]
*IRAS
:30cm口径，all sky survey at 12, 25, 60 and 100 µm. 
*[[AKARI]]
*[[Spitzer]]
===[[Herschel]]===
*Herschel reference survey (HRS)
:323 K-band(Ks<12) selected galaxies from 100 to 500 mu, volume limited (between 15 and 25 Mpc)
*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 [http://arxiv.org/abs/1606.09254]

==射电==

*[[JCMT]]
*[[ALMA]]
*[[SMG]]亚毫米波源[[SCUBA]] [[SCUBA-2]]
: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]),[[http://arxiv.org/abs/1609.00388]]

===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===


[[文件:Radio survey.PNG|缩略图|radio survey]]
*[[TGSS]]
*[[NVSS]]
*[[FIRST]]
*[[WENSS]]
*VLSS:Very Large Array (VLA) Low-frequency Sky Survey (VLSS) data.

===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