The translation that Tyma Gaidash links to in the comments explains what these terms mean: they are the orbital positions of Venus, Earth, Jupiter, and Saturn at time $t$ years. So the value for a given planet is $360^\circ/P_\text{orb}$, where $P_\text{orb}$ is its orbital period in earth years.
The Royal Astronomical Society of Canada's Calgary Centre has this web page which gives the orbital periods of the planets in years to a very high precision (strangely, it gives the orbital period of Earth as $1.0000007$ years, which perhaps somebody can explain in the comments):
$$\begin{array}{c|c|c|}
& P_\text{orb} & 360^\circ/P_\text{orb} \\ \hline
\text{Venus} & 0.61517237 & 585.2018^\circ \\ \hline
\text{Jupiter} & 11.8663142 & 30.3380^\circ \\ \hline
\text{Saturn} & 29.47305083 & 12.2145^\circ \\ \hline
\end{array}$$
This clearly shows that "585° dot 26" should be interpreted as $585.26^\circ$, and similarly for Jupiter and Saturn. The third column matches your quoted figures to better than one part in $2000$; if we interpreted the last two digits as arcminutes, the match would be no better than one part in $80$.
Updated to add: The Calgary Centre's Larry McNish was kind enough to reply to my query about that $1.0000007$:
It was the result of applying Kepler's third law to the published JPL values for the planetary orbits as they were back in 2009.
I've attached the spreadsheet (which had a JPL value of the semi-major axis for the Earth's orbit as 1.00000018 a.u.)
Either because I used too many digits of precision in the answer or because it was measured as sidereal years.
365.256622 / 1.0000007 = 365.25636632054357561949706635205 which is very close to the number of days in a sidereal year
https://en.wikipedia.org/wiki/Earth%27s_orbit 365.256363004 days[13]