Here is a list of the positions of regularly used System temperature calibrators:
RA(1950) Dec(1950)
Cas A 350.2953 58.558
Cyg A 299.43750 40.596
Tau A 82.8791 21.966
Vir A 187.074 12.668
Their flux densities are can be calculated from this table, where frequencies, `f', are given in MHz and flux densities, `S', are given in Jy:
log(S) = 5.745 - 0.770*log(f)This decreases at about ( 1.87-0.3*log(f) )% per year from the year 1986.
log(S) = 4.965 +0.085*log(f) - 0.178*log(f)*log(f)and from 2GHz to 31GHz
log(S) = 7.161 -1.242*log(f)
log(S) = 3.915 -0.299*log(f)
log(S) = 5.023 -0.856*log(f)
This gives the following antenna temperatures, for the nominal antenna gains:
Source 21cm 18cm Cas A(in 1980) 237K 209K Cyg A 179K 151K Tau A 107K 102K Vir A 24K 21K
There are also a few pointing calibrators, and their positions are given here:
RA(1950) Dec(1950)
3C123 68.4790 29.5720
3C218 138.9230 -11.8550
Here is a list of the positions of some spectral line calibrators:
RA(1950) Dec(1950) Wavelength Comment
W3 133.950 1.064 18cm OH masers
NML Cygnus 80.797 -1.922 18cm OH masers
Lockman Hole 159.242 57.333 21cm low HI density
@c________________________________________________________________