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*   CRL2688, NGC7027, section above) are left unchanged, but these are not
*   inconsistent with Loup.
*   Note that we still have not gone through all the sources in the list.!!
*
*   The catalogue gives T_A* (peak) for the 2-1 line. More informative, however, are the integrated line intensities
*   in the comment line (in K km/s), which largely determine how easy it is to detect a line. Note that JCMT 2-1
*   data followed by J are typically low by about a factor of 1.3 - 1.5 (telescope heavily deformed due to conebar
*   welding.
*
* 20070717 Notes reflect new positional accuracies : L1 L2 L3 original Loup qualities (<1", 1-5", >5");
*                                                  : /H and /T reflect updates by Hipparcos & Tycho (uncertainty of <1")
* 20060530 Notes reflect new positional accuracies : /2M reflect updates by 2MASS (catalog II/246)
*
* 20140910 Modifications based on M13BN01 and M14AN01:
*          Vlsr, Tpeak, Vrange derived from HARP CO(3-2) spectra
*          Under comments is indicated whether source is good for RxA, HARP, or both: A, H, AH
*          and Tpeak, Integrated intensity for CO(2-1) and CO(3-2)
*
*
*               RA & DEC                   Eq  Vlsr     Tpeak   Vrange              PM1        PM2     Parallax Comments
*- -- -- -- -- -- --  -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- -- --