“Multi-wavelength”的版本间差异

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==黑体谱==
*[[黑体谱]]
*温度和波长(频率)的关系,维恩位移定理
:<math>\lambda_{peak}\approx\frac{2.9cm K}{T} </math>
:<math>\mu_{peak}\approx58.8GHzK^{-1}T</math>


*[[cooling rate]]
*能量-波长(频率)-温度的关系

:<math> 1eV\approx1.6\times 10^{-19}J\\
==高能==
h\approx6.63\times10^{-33}JHz </math>
*Swift/BAT (burst alert telescope) AGN
:<math> \mu(1eV)\approx 4\times10^{5}GHz\\
:313 AGN
\lambda(1eV)\approx 1.24um\\
*XBOOTES [[Chandra]]
T(1ev)\approx 4100K</math>
*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]]

===Ha窄带===
*近邻星系的100Mpc以内的数据见[https://arxiv.org/abs/1710.05016]


==红外==
==红外==
第18行: 第28行:
*[[AKARI]]
*[[AKARI]]
*[[Spitzer]]
*[[Spitzer]]
*[[Herschel]]
===[[Herschel]]===
*[[Herschel reference survey (HRS)]]

*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==
*[[SKA]]
*[[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

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

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

30cm口径,all sky survey at 12, 25, 60 and 100 µm.

Herschel

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]]

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

radio survey

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