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
effelsberg [2016/12/07 15:53]
Déborah Paradis
effelsberg [2023/04/11 15:22] (current)
Déborah Paradis
Line 1: Line 1:
 ====== EFFELSBERG 1408/2695 MHz Radio continuum and Polarization ====== ====== EFFELSBERG 1408/2695 MHz Radio continuum and Polarization ======
 +
 +/* 
 +AH 27/8/18: should we separate this into several pages -- by wavelength and by polarisation? ​
 +*/
  
 **__Radio continuum__** **__Radio continuum__**
  
 These surveys of continuum radiation at 1408 MHz (21cm) and 2695 MHz (11cm) were made with the Effelsberg 100-m telescope, with an angular resolution of 9.4' (21cm) and 4.3' (11cm).  ​ These surveys of continuum radiation at 1408 MHz (21cm) and 2695 MHz (11cm) were made with the Effelsberg 100-m telescope, with an angular resolution of 9.4' (21cm) and 4.3' (11cm).  ​
 +Units of the Healpix maps are ''​mKTB''​.
  
 Both surveys cover the Galactic plane between : \\ Both surveys cover the Galactic plane between : \\
Line 14: Line 19:
 - a field of 20°x11.2° centered on l=200°, b=9.4° \\ - a field of 20°x11.2° centered on l=200°, b=9.4° \\
  
 +Healpix maps made by D. Paradis
  
-References for the 11cm survey: \\ +===References for the 11cm survey ​=== 
-- http://​adsabs.harvard.edu/​abs/​1984A%26AS...58..197R \\ +  * 'A radio continuum survey of the Galactic Plane at 11 CM wavelength. I The area L = 357.4 to 76 deg, B = -1.5 to +1.5 deg' by Reich et al, 1984, A&AS, 58, 197 http://​adsabs.harvard.edu/​abs/​1984A%26AS...58..197R \\ 
-- http://​adsabs.harvard.edu/​abs/​1990A%26AS...85..633R \\ +  * 'A radio continuum survey of the Galactic Plane at 11 CM wavelength. II The area L = 358-76 deg, B = -5 to 5 deg. ' by Reich et al, 1990, A&AS, 85, 633 http://​adsabs.harvard.edu/​abs/​1990A%26AS...85..633R \\ 
-- http://​adsabs.harvard.edu/​abs/​1990A%26AS...85..691F \\+  * 'A Radio Continuum Survey of the Galactic Plane at 11-CENTIMETER Wavelength - Part Three - the Area 76DEG < L< 240DEG'​ by Furts et al, 1990, A&AS, 85, 691 http://​adsabs.harvard.edu/​abs/​1990A%26AS...85..691F \\
  
-References for the 21cm survey: \\ +===References for the 21cm survey ​=== 
-http://​adsabs.harvard.edu/​abs/​1990A%26AS...83..539R \\ +  * 'The Effelsberg 21 CM radio continuum survey of the Galactic plane between L = 357 deg and L = 95.5 deg' by Reich et al, 1990, A&AS, 83, 539 http://​adsabs.harvard.edu/​abs/​1990A%26AS...83..539R \\ 
-http://​adsabs.harvard.edu/​abs/​1997A%26AS..126..413R \\+  * 'The Effelsberg 21 CM radio continuum survey of the Galactic plane between L = 95.5 deg and L = 240 deg.' by Reich et al, 1997, 126, 413 http://​adsabs.harvard.edu/​abs/​1997A%26AS..126..413R \\
  
-Reference for the EMLS 21cm surveyhttp://​adsabs.harvard.edu/​abs/​1999A%26AS..138...31U +===Reference for the EMLS 21cm survey ​=== 
- +  * 'A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes. II. First section'​ by Uyaniker et al, 1999, A&AS, 138, 31 http://​adsabs.harvard.edu/​abs/​1999A%26AS..138...31U
- +
-Data in the WCS format can be downloaded here:  +
-http://​www3.mpifr-bonn.mpg.de/​survey.html+
  
 ^  __**Effelsberg 11cm**__ ​ ^  __**Effelsberg 11cm (Background)**__ ​ ^ ^  __**Effelsberg 11cm**__ ​ ^  __**Effelsberg 11cm (Background)**__ ​ ^
Line 67: Line 70:
 </​html>​ </​html>​
  
-- Galactic plane + Medium latitude surveys 21cm (only source component): [[http://​cade.irap.omp.eu/​documents/​Ancillary/​EFFELSBERG/​EFFELSBERG+EMLS_21cm_1_1024.fits|EFFELSBERG+EMLS_21cm_1_1024.fits]]+- Galactic plane + Medium latitude surveys 21cm (only source component): [[http://​cade.irap.omp.eu/​documents/​Ancillary/​EFFELSBERG/​EFFELSBERG_EMLS_21cm_1_1024.fits|EFFELSBERG_EMLS_21cm_1_1024.fits]]
 <​html>​ <​html>​
 <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(effemls21)">​Aladin</​button>​ <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(effemls21)">​Aladin</​button>​
 </​html>​ </​html>​
  
-- Galactic plane + Medium latitude surveys 21cm (background component): [[http://​cade.irap.omp.eu/​documents/​Ancillary/​EFFELSBERG/​EFFELSBERG+EMLS_21cm_back_1_1024.fits|EFFELSBERG+EMLS_21cm_back_1_1024.fits]]+- Galactic plane + Medium latitude surveys 21cm (background component): [[http://​cade.irap.omp.eu/​documents/​Ancillary/​EFFELSBERG/​EFFELSBERG_EMLS_21cm_back_1_1024.fits|EFFELSBERG_EMLS_21cm_back_1_1024.fits]]
 <​html>​ <​html>​
 <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(effemls21back)">​Aladin</​button>​ <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(effemls21back)">​Aladin</​button>​
 </​html>​ </​html>​
  
 +===Original WCS Data ===
 +http://​www3.mpifr-bonn.mpg.de/​survey.html
  
 <​html>​ <​html>​
Line 106: Line 111:
 var effemls21 = function(connection) { var effemls21 = 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/​EFFELSBERG/​EFFELSBERG+EMLS_21cm_1_1024.fits","​name":"​EFFELSBERG+EMLS ​21cm"} );+    {"​url":​ "​http://​cade.irap.omp.eu/​documents/​Ancillary/​EFFELSBERG/​EFFELSBERG_EMLS_21cm_1_1024.fits","​name":"​EFFELSBERG_EMLS ​21cm"} );
     connection.notifyAll([msg]);​     connection.notifyAll([msg]);​
 }; };
 var effemls21back = function(connection) { var effemls21back = 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/​EFFELSBERG/​EFFELSBERG+EMLS_21cm_back_1_1024.fits","​name":"​EFFELSBERG+EMLS ​21cm background"​} );+    {"​url":​ "​http://​cade.irap.omp.eu/​documents/​Ancillary/​EFFELSBERG/​EFFELSBERG_EMLS_21cm_back_1_1024.fits","​name":"​EFFELSBERG_EMLS ​21cm background"​} );
     connection.notifyAll([msg]);​     connection.notifyAll([msg]);​
 }; };
Line 171: Line 176:
 **__Polarization__** **__Polarization__**
  
-References for the 11cm Stokes Q and U emission components: \\ +===References for the 11cm Stokes Q and U emission components ​=== 
-http://​adsabs.harvard.edu/​abs/​1999A%26A...350..447D \\ +  * '​Polarimetric structure in the first Galactic quadrant from the 2.695 GHz Effelsberg survey'​ by Duncan et al, 1999, A&A, 350, 447 http://​adsabs.harvard.edu/​abs/​1999A%26A...350..447D \\ 
-- http://​adsabs.harvard.edu/​abs/​1987A%26AS...69..451J \\+  * 'A survey of linear polarization along the Galactic plane The area L = 4.9 to 76 deg, B = -1.5 to 1.5 deg' by Junkes et al, 1987, A&AS, 69, 451 http://​adsabs.harvard.edu/​abs/​1987A%26AS...69..451J \\
  
-Reference for the 21cm Stokes Q and U emission components: \\ +===Reference for the 21cm Stokes Q and U emission components ​=== 
-http://​adsabs.harvard.edu/​abs/​1999A%26AS..138...31U \\+  * 'A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes. II. First section'​ by Uyaniker et al, 1999, 138, 31 http://​adsabs.harvard.edu/​abs/​1999A%26AS..138...31U \\
  
 ^  __**Effelsberg 11cm POLU**__ ​ ^  __**Effelsberg 11cm POLQ**__ ​ ^ ^  __**Effelsberg 11cm POLU**__ ​ ^  __**Effelsberg 11cm POLQ**__ ​ ^
Line 281: Line 286:
 <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(eff21polq)">​Aladin</​button>​ <button class="​aladin-btn"​ type="​button"​ onclick="​connector.runWithConnection(eff21polq)">​Aladin</​button>​
 </​html>​ </​html>​
 +
 +=== HiPS=== ​
 +
 +EFFELSBERG HiPS are available in Aladin Collections/​Image
 +
 +
 +===Original WCS Data ===
 +http://​www3.mpifr-bonn.mpg.de/​survey.html