Differences

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

Link to this comparison view

Next revision
Previous revision
sgps [2016/07/26 13:19]
127.0.0.1 external edit
sgps [2023/04/11 15:30] (current)
Déborah Paradis
Line 1: Line 1:
 ====== Southern Galactic Plane Survey (SGPS) ====== ====== Southern Galactic Plane Survey (SGPS) ======
 +
 +/*
 +AH 27/8/2018
 +Do our maps cover the SGPS 2 region for HI? The ATNF SGPS server seems to be out of action
 +*/
  
 The //Southern Galactic Plane Survey// (SGPS) provides ''​21-cm''​ line emission The //Southern Galactic Plane Survey// (SGPS) provides ''​21-cm''​ line emission
 from neutral atomic hydrogen and continuum data of the Southern Milky Way from neutral atomic hydrogen and continuum data of the Southern Milky Way
-obtained with the //Australia Telescope Compact Array// and //​Parkes ​Radiotelescopes//.+obtained with the //Australia Telescope Compact Array// and //​Parkes ​Radiotelescope//.
  
 SGPS HI data cover galactic longitudes ''​l=253 deg''​ to ''​l=358 deg''​ (SGPS I) SGPS HI data cover galactic longitudes ''​l=253 deg''​ to ''​l=358 deg''​ (SGPS I)
Line 10: Line 15:
 The SGPS continuum survey is available for longitudes ''​l=253 deg''​ to ''​l=358 deg''​. The SGPS continuum survey is available for longitudes ''​l=253 deg''​ to ''​l=358 deg''​.
 The resolution of the data is ''​2.2'''​ (SGPS I) and ''​3.3'''​ (SGPS II). The resolution of the data is ''​2.2'''​ (SGPS I) and ''​3.3'''​ (SGPS II).
-HI data are in ''​K m/​s''​ and continuum data are in ''​Jy/​beam''​.+HI data are in ''​K m/​s''​ and continuum data are in ''​Jy/​beam''​.\\
  
-Data in the WCS format can be downloaded here: http://www.atnf.csiro.au/​research/​HI/​sgps/​queryForm.html+Healpix maps made by DParadis.
  
-References: +===References=== 
-    * http://​adsabs.harvard.edu/​abs/​2005ApJS..158..178M +    * 'The Southern Galactic Plane Survey: H I Observations and Analysis'​ by McCLure-Griffiths et al, 2006, ApJS, 158, 178 http://​adsabs.harvard.edu/​abs/​2005ApJS..158..178M 
-    * http://​adsabs.harvard.edu/​abs/​2006ApJS..167..230H+    * 'The Southern Galactic Plane Survey: Polarized Radio Continuum Observations and Analysis'​ by Haverkorn et al, 2006, ApJS, 167, 230 http://​adsabs.harvard.edu/​abs/​2006ApJS..167..230H
  
  
Line 22: Line 27:
 |  <​html><​div id="​aladin-lite-div-sgps"​ class="​aladin-lite-container"></​div></​html> ​ |  <​html><​div id="​aladin-lite-div-sgpscont"​ class="​aladin-lite-container"></​div></​html> ​ | |  <​html><​div id="​aladin-lite-div-sgps"​ class="​aladin-lite-container"></​div></​html> ​ |  <​html><​div id="​aladin-lite-div-sgpscont"​ class="​aladin-lite-container"></​div></​html> ​ |
  
 +===Maps===
 +* Atomic Hydrogen (Continuum subtracted): ​
  
- +Partial Healpix: [[http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_II/​SGPS_II_1_4096_partial.fits|SGPS_II_1_4096_partial.fits]]<​html>​
-===== Atomic Hydrogen (Continuum subtracted) ===== +
- +
-**Map:** [[http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_II/​SGPS_II_1_4096.fits|SGPS_II_1_4096.fits]] +
-<​html>​+
 <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(sgps)">​Aladin</​button>​ <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(sgps)">​Aladin</​button>​
 </​html>​ </​html>​
  
 +Full sky: [[http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_II/​SGPS_II_1_4096.fits|SGPS_II_1_4096.fits]]
  
-===== Radio Continuum ​=====+  * Radio Continuum:  ​
  
-**Map:** [[http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_CONT/​SGPS_CONT_1_4096.fits|SGPS_CONT_1_4096.fits]] +Partial Healpix: [[http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_CONT/​SGPS_CONT_1_4096_partial.fits|SGPS_CONT_1_4096_partial.fits]]<​html>​
-<​html>​+
 <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(sgpscont)">​Aladin</​button>​ <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(sgpscont)">​Aladin</​button>​
 </​html>​ </​html>​
  
- +Full sky: [[http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_CONT/​SGPS_CONT_1_4096.fits|SGPS_CONT_1_4096.fits]]
 <​html>​ <​html>​
 <script src="​lib/​scripts/​aladin-btns.js"></​script>​ <script src="​lib/​scripts/​aladin-btns.js"></​script>​
Line 47: Line 49:
 var sgps = function(connection) { var sgps = function(connection) {
       var msg = new samp.Message("​image.load.fits",​       var msg = new samp.Message("​image.load.fits",​
-      {"​url":​ "​http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_II/​SGPS_II_1_4096.fits","​name":"​SGPS"​} );+      {"​url":​ "​http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_II/​SGPS_II_1_4096_partial.fits","​name":"​SGPS"​} );
       connection.notifyAll([msg]);​       connection.notifyAll([msg]);​
 }; };
 var sgpscont = function(connection) { var sgpscont = function(connection) {
     var msg = new samp.Message("​image.load.fits",​     var msg = new samp.Message("​image.load.fits",​
-    {"​url":​ "​http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_CONT/​SGPS_CONT_1_4096.fits","​name":"​SGPS continuum"​} );+    {"​url":​ "​http://​cade.irap.omp.eu/​documents/​Ancillary/​SGPS_CONT/​SGPS_CONT_1_4096_partial.fits","​name":"​SGPS continuum"​} );
     connection.notifyAll([msg]);​     connection.notifyAll([msg]);​
 }; };
Line 81: Line 83:
 </​html>​ </​html>​
  
 +=== HiPS=== ​
 +
 +HiPS of the SGPS integrated intensity ​ are available in Aladin Collections/​Image
 +
 +For the SGPS Continuum HiPS,  enter the following URLs in Aladin ("​Files"​ then "Use directly a URL"):
  
 +http://​cade.irap.omp.eu/​documents/​Ancillary/​4Aladin/​SGPS_CONT \\
  
 +===Original WCS Data===
 +https://​www.atnf.csiro.au/​research/​HI/​sgps/​fits_files.html