“Multi-wavelength”的版本间差异
跳到导航
跳到搜索
(→光学,近红外) |
|||
(未显示同一用户的28个中间版本) | |||
第6行: | 第6行: | ||
*Swift/BAT (burst alert telescope) AGN |
*Swift/BAT (burst alert telescope) AGN |
||
:313 AGN |
:313 AGN |
||
*XBOOTES [[Chandra]] |
|||
*MAXI,Monitor of All sky X-ray Image,装在空间站上 |
|||
==紫外== |
==紫外== |
||
[[GALEX]] |
*[[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== |
==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20行: | 第29行: | ||
*[[Spitzer]] |
*[[Spitzer]] |
||
===[[Herschel]]=== |
===[[Herschel]]=== |
||
*Herschel reference survey (HRS) |
*[[Herschel reference survey (HRS)]] |
||
:323 K-band 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== |
==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
- 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[1]
红外
- WISE
- IRAS
- 30cm口径,all sky survey at 12, 25, 60 and 100 µm.
Herschel
- 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]]
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
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