“Multi-wavelength”的版本间差异

来自Shiyin's note
跳到导航 跳到搜索
 
(未显示同一用户的6个中间版本)
第17行: 第17行:
==光学,近红外==
==光学,近红外==
参见[[星系巡天]]
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26行: 第29行:
*[[Spitzer]]
*[[Spitzer]]
===[[Herschel]]===
===[[Herschel]]===
*Herschel reference survey (HRS)
*[[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
*Herscchel [[Stripe 82]] survey
:79 deg^2 with SPIRE at 250,350,500 mu
:79 deg^2 with SPIRE at 250,350,500 mu
第42行: 第45行:


==射电==
==射电==
*[[SKA]]
*[[JCMT]]
*[[JCMT]]
*[[ALMA]]
*[[ALMA]]
第47行: 第51行:
: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]]

===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===
===巡天===


[[文件:Radio survey.PNG|缩略图|radio survey]]
[[文件:Radio survey.PNG|缩略图|radio survey]]
*[[TGSS]]
*[[TGSS]]
第56行: 第71行:
*VLSS:Very Large Array (VLA) Low-frequency Sky Survey (VLSS) data.
*VLSS:Very Large Array (VLA) Low-frequency Sky Survey (VLSS) data.


*'''专题:[[HI巡天]]'''
===专题===
===CO===
====[[HI巡天]]====

====CO====
*COLD GASS
*COLD GASS
:CO legacy Database for [[GASS]]
:CO legacy Database for [[GASS]]

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