Orsay Survey of Atomic Hydrogen in the Galactic Plane
Joachim Köppen Strasbourg Feb. 2013
This applet shows the results of a survey of the Galactic Plane
at the radio line of atomic hydrogen at 21 cm wavelength, done with
the 3.3m diameter radio telescope in Orsay, south of Paris, near
Orly airport, built and operated by J.J.Maintoux.
The data are shown in a false colour longitude-vrad map for galactic
longitude (from 4° to 240° in steps of 2°) and radial velocity from
-200 to +200 km/s.
Here are brief instructions:
- File Info gives some technical details of the data file
- freq.smooth allows to apply a smoothing of the spectra
over an intervall of the indicated number of frequency points.
- Long-Vrad map is a false colour map of the intensity
as a function of galactic longitude and radial velocity.
- clicking on the map will display the x, y, and z values of
that point, i.e. longitude, radial velocity, and intensity.
- drag & zoom: click this button, then drag the mouse
over the portion of the map that you want to be zoomed.
- unzoom brings back the full view.
- the Map colour coding can be chosen among several options.
The coding is shown as a thin bar at the right hand side of
the map, from minimum to maximum value of the chosen range.
- one may chose between autorange or manual cuts.
For the latter, the min and max values can be entered in the
fields below the button.
- the white vertical line indicates the longitude whose spectrum
can be plotted.
- x-y map is a false colour map of the intensity
as if we would look down on the Galactic Plane.
The white line indicates the line-of-sight at the longitude chosen
with the stepping buttons.
Note: the colour coding is identical to the one of the l-v map.
- Gauss fit allows to fit the spectrum of a galactic longitude
with Gaussian components of different radial velocities.
- empty button will show green if the corresponding component
has been chosen and is displayed.
- grab: click this for a chosen component, then click on the
plot where you want the Gaussian curve's peak to be placed.
- c is the center velocity. One can also enter the value manually,
followed by hitting the Enter key.
- w is the FWHM of the component.
- h is the peak value of the component.
- Sum curve shows the sum of all chosen components,,
components shows all individual components.
- plot shows the spectrum at a galactic longitude.
Clicking on the plot will display the x=radial velocity and y=intensity
of that point.
- with the buttons -50 ... +50 one can step back and
forth in longitude.
- Output shows the displayed spectrum (including smoothing)
at the chosen longitude as a numerical table. It can be copied
and pasted into a text editor.
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last update: Feb. 2013 J.Köppen