Here, you see the sky coverage of our commonly used SiO
pointing sources. By clicking on any source, you can see the SiO(2-1)
line spectrum of that source. During observations you may observe any
pointing source, depending on the distance to the sun and your source,
to check the telescope's pointing.
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- The numbers in parenthesis denote the last peak temperature value observed.
- The coordinate system is in R.A. (Horizontal) and Declination (Vertical).
J2000.0
- The pointing data was obtained using the SESIS 100 GHz Receiver.
- Monitoring of the pointing sources is conducted by Francisco
Azagra
- Data from pointing run May 1st 2002 (2.2" / 2.0")
