For new users of the Skynet 20-meter radio telescope ...

Is an object a radio source? How powerful is it?

What question are you trying to answer? The most basic one is "does this object produce radio waves?" And if it does emit radio waves, how strong are they?
  • Here is how to find out.
    The "track" scan just points the telescope at one position and sits there for whatever length of time you tell it.
    (many people recently have done "track" scans on planets or star clusters or nebulas. Here is why this is usually not a useful observing method, and what to do instead.)

    The telescope sees a field of view that is often much larger than the angular size of the object, so the radiation detected by the telescope comes both from the object of interest and from the surrounding background and foreground. How much radiation is from the object, and how much from the background?
    With a "track" scan, you cannot tell.

    To find out what is coming from the object itself you need to observe both the object and the nearby surroundings, using either a "daisy" scan or an "on/off" scan.

    The daisy scan will scan the telescope across the object several times. If the object is detected, you will see a bump in the graph every time the telescope scans across the object.

    If you have set up a "daisy" scan with 4 petals, you should see 4 bumps in the graph. The height of those bumps tells you how much radiation is detected from the object. If there are no bumps, then the object has not been detected, and maybe does not emit radio waves at all.

    A daisy prescription:

  • set the minimum elevation to 20 degrees.
  • select "low resolution spectral/continuum mode"
  • select "daisy" as the sky pattern
  • set the radius to 150 arcminutes
  • set the number of petals to 4
  • set the integration time to 0.2
  • set the duration to 60 seconds.

    Look at the observation plots on the 20-meter web page. Look at the plot of power vs time. How much are the bumps above the baseline? That gives you the power in units of Kelvin.

    To convert to units of Janskys, to compare with references or with other radio telescopes, multiply by 16.

    Making Maps, i.e., radio images

    Maps are the way to make an image of an object. For a Map to make sense, your object needs to be big-- that is it needs to take up a lot of room in the sky. Most of the objects you are observing with the optical telescopes are only a few arc minutes across. The 20 Meter Telescope can't see any detail in these objects! You need something much larger in angular size-- like parts of our Milky Way, if you want to make a good map.

    Maps should be at least 6 degrees on a side (for 21 cm observations) to make a good map.
    More advice on maps

    Measuring Hydrogen Clouds in the Galaxy.

    With the radio telescope you can find out if our Milky Way Galaxy (and others) contain hydrogen atoms. Hydrogen atoms undergo an energy transition that produces energy in the form of radio waves that have a wavelength of 21cm, or a frequency of 1420.41 MHz.

    These are hydrogen ATOMS mind you, not ionized hydrogen or plasma like you find in stars. These atoms reside in clouds of cold gas that will one day coalesce into stars.

    To see if parts of our Milky Way contains cold hydrogen atoms, try this:

  • click on a location near the red line on the Skyviewer. The red line is the Milky Way's equator.
  • Type in a name for your observation
  • set the minimum elevation to 20 degrees
  • select "high resolution spectral/continuum mode" select "track"
  • set the duration to 60 seconds
  • everything else can stay the default values.
    More spectral line advice