✎ CHIMPS [CADE]

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====== CHIMPS ======

The CO Heterodyne Inner Milky Way Plane Survey (CHIMPS) mapped the 13CO(3-2) and C18O(3-2) emission in the inner Galactic plane with the James Clerk Maxwell Telescope (JCMT). 

CHIMPS mapped the longitude range l = (28°,46°) and latitude range |b| ≤ 0.5°, across the radial velocity range VLSR = (-75, +150) km/s. The 12CO(3-2) emission across the same region was mapped by the [[COHRS|COHRS]] survey.

The original angular resolution of CHIMPS is 15 arcseconds and the velocity resolution is 0.5 km/s. The typical rms sensitivity per channel of the CHIMPS data cubes is σ(T) ~ 0.5K .

CADE currently delivers 13CO(3-2) and C18O(3-2) integrated intensity and peak brightness maps of the full CHIMPS region using the survey's public data release. /*To facilitate processing, the input WCS FITS data cubes were convolved to 33 arcseconds prior to the generation of the HEALpix moment maps delivered by CADE. */

The units of the Healpix maps are K.km/s.

Healpix maps made by D. Paradis. 

/*Please contact us [[mailto:cade@irap.omp.eu|cade@irap.omp.eu]] if you require CHIMPS maps at a different angular resolution for your science. Data from CHIMPS2 will be incorporated as it becomes publicly available.*/
^  __**13CO(3-2)**__  ^  __**C18O(3 -2)**__  ^
|  <html><div id="aladin-lite-div-chimps13CO" class="aladin-lite-container"></div></html>  |  <html><div id="aladin-lite-div-chimpsC18O" class="aladin-lite-container"></div></html>  |

=== References ===
  * 'CHIMPS: the 13CO/C18O(3 -2) Heterodyne Inner Milky Way Plane Survey ', Rigby, A. et al, 2016, MNRAS, 456, 3, 2885 https://ui.adsabs.harvard.edu/abs/2016MNRAS.456.2885R/abstract

=== Maps ===
13CO(3-2) Integrated Intensity: [[http://cade.irap.omp.eu/documents/Ancillary/CHIMPS/CHIMPS_13CO_MOM0_1_32768_partial.fits|CHIMPS_13CO_MOM0_1_32768_partial.fits]]

C18O(3 -2) Integrated Intensity: [[http://cade.irap.omp.eu/documents/Ancillary/CHIMPS/CHIMPS_C18O_MOM0_1_32768_partial.fits|CHIMPS_C18O_MOM0_1_32768_partial.fits]]


<html>
<script src="lib/scripts/aladin-btns.js"></script>
<script>
// Broadcast a table given a hub connection.
var chimps13CO = function(connection) {
    var msg = new samp.Message("image.load.fits",
    {"url": "http://cade.irap.omp.eu/documents/Ancillary/CHIMPS/CHIMPS_13CO_MOM0_1_32768_partial.fits","name":"CHIMPS 13CO (3-2)"} );
    connection.notifyAll([msg]);
};
var chimpsC18O = function(connection) {
      var msg = new samp.Message("image.load.fits",
      {"url": "http://cade.irap.omp.eu/documents/Ancillary/CHIMPS/	CHIMPS_C18O_MOM0_1_32768_partial.fits","name":"CHIMPS C18O (3-2)"} );
      connection.notifyAll([msg]);
};

// Aladin visualizations
jQuery().ready(function($){
    var aladin_01 = A.aladin('#aladin-lite-div-chimps13CO', {zoom:30});
    aladin_01.setFrame('Galactic');
    aladin_01.gotoPosition(35, 0);
    aladin_01.setImageSurvey(aladin_01.createImageSurvey(
        'CHIMPS_13CO_MOM0', 'CHIMPS_13CO_MOM0',
        'http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CHIMPS_13CO_MOM0/',
        'Galactic', 3
    ));
    aladin_01.getBaseImageLayer().getColorMap().update('rainbow');

    var aladin_02 = A.aladin('#aladin-lite-div-chimpsC18O', {zoom:30});
    aladin_02.setFrame('Galactic');
    aladin_02.gotoPosition(35, 0);
    aladin_02.setImageSurvey(aladin_02.createImageSurvey(
        'CHIMPS_C18O_MOM0', 'CHIMPS_C18O_MOM0',
        'http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CHIMPS_C18O_MOM0/',
        'Galactic', 3
    ));
    aladin_02.getBaseImageLayer().getColorMap().update('rainbow');
});
</script>
</html>

===HiPS ===

Enter the following URLs in Aladin ("Files" then "Use directly a URL"):\\
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CHIMPS_13CO_MOM0\\
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/CHIMPS_C18O_MOM0\\

=== Known Issues ===


=== Version History ===
  * v1 CADE maps, March 2022*/
 
=== Original WCS Data ===
http://dx.doi.org/10.11570/16.0001

=== Project PI Website ===
https://ajrigby.github.io/#research
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