Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
urumqi [2017/12/05 15:08]
Déborah Paradis
urumqi [2023/04/11 15:33] (current)
Déborah Paradis
Line 1: Line 1:
 ====== Urumqi 6 cm Radio continuum and Polarization ====== ====== Urumqi 6 cm Radio continuum and Polarization ======
  
 +The Sino-German 6 cm surveys of the Galactic Plane (10°<​l<​230° and |b|<5°) were made using the Urumqi 25-m telescope, at an angular resolution of 9.5'​. ​
 +Units of the Healpix maps are ''​micro KTB''​.\\
 +
 +Healpix maps made by D. Paradis.
  
 === References=== === References===
 +  * 'A Sino-German λ6 cm polarization survey of the Galactic plane. I. Survey strategy and results for the first survey region'​ by Sun, X. H. et al. 2007, A&A, 463, 993 http://​adsabs.harvard.edu/​abs/​2007A%26A...463..993S
   * 'A Sino-German λ6 cm polarization survey of the Galactic plane. II. The region from 129° to 230° longitude'​ by Gao, X. Y. et al, 2010, A&A, 515, 64 http://​adsabs.harvard.edu/​abs/​2010A%26A...515A..64G   * 'A Sino-German λ6 cm polarization survey of the Galactic plane. II. The region from 129° to 230° longitude'​ by Gao, X. Y. et al, 2010, A&A, 515, 64 http://​adsabs.harvard.edu/​abs/​2010A%26A...515A..64G
   * 'A Sino-German λ6 cm polarization survey of the Galactic plane. III. The region from 10° to 60° longitude'​ by Sun, X. H. et al, 2011, A&A, 527, 74 http://​adsabs.harvard.edu/​abs/​2011A%26A...527A..74S   * 'A Sino-German λ6 cm polarization survey of the Galactic plane. III. The region from 10° to 60° longitude'​ by Sun, X. H. et al, 2011, A&A, 527, 74 http://​adsabs.harvard.edu/​abs/​2011A%26A...527A..74S
Line 44: Line 49:
 </​html>​ </​html>​
  
- +^  __**Urumqi Intensity**__  ^  __**Urumqi POLU**__ ​ ^  __**Urumqi POLQ**__ ​ ^ 
-^  __**Urumqi Intensity*__ ​ ^  __**Urumqi POLU**__ ​ ^  __**Urumqi POLQ**__ ​ ^|  <​html>​+|  <​html>​
 <div id="​aladin-lite-div-urumqi"​ class="​aladin-lite-container200"></​div>​ <div id="​aladin-lite-div-urumqi"​ class="​aladin-lite-container200"></​div>​
 </​html> ​ |  <​html>​ </​html> ​ |  <​html>​
Line 76: Line 81:
     aladin_02.getBaseImageLayer().getColorMap().update('​rainbow'​);​     aladin_02.getBaseImageLayer().getColorMap().update('​rainbow'​);​
     ​     ​
-        var aladin_03 = A.aladin('#​aladin-lite-div-urumqipolu', {zoom:​170});​+        var aladin_03 = A.aladin('#​aladin-lite-div-urumqipolq', {zoom:​170});​
     aladin_03.setFrame('​Galactic'​);​     aladin_03.setFrame('​Galactic'​);​
     aladin_03.gotoPosition(60,​ 0);     aladin_03.gotoPosition(60,​ 0);
Line 89: Line 94:
 </​script>​ </​script>​
 </​html>​ </​html>​
 +
 +===HiPS ===
 +
 +URUMQI intensity HiPS are available in Aladin Collections/​Image
 +
 +For All URUMQI HiPS, enter the following URLs in Aladin ("​Files"​ then "Use directly a URL"):
 +http://​cade.irap.omp.eu/​documents/​Ancillary/​4Aladin/​URUMQI_I
 +http://​cade.irap.omp.eu/​documents/​Ancillary/​4Aladin/​URUMQI_POLU ​
 +http://​cade.irap.omp.eu/​documents/​Ancillary/​4Aladin/​URUMQI_POLQ
 +
 +===Original WCS Data ===
 +http://​www3.mpifr-bonn.mpg.de/​survey.html