“Multi-wavelength”的版本间差异

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*[[ALMA]]
*[[ALMA]]
*[[SMG]]亚毫米波源[[SCUBA]] [[SCUBA-2]]
*[[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
: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]]
: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]]



2016年9月5日 (一) 05:46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

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

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]


79 deg^2 with SPIRE at 250,350,500 mu
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]]



巡天

radio survey