Abstract

A new method of dening the declination axis of the instrumental frame of an absolute transit circle cat- alog has been developed utilizing observations from stars over the entire sky rather than, as in the past, observations of just circumpolar stars. This method allows the plane- tary observations to be used directly to align the axes of the instrumental frame thus constructed with DE200. The alignment process has been simplied and recast so that it does not feed back into the denition of the in- strumental frame. A declination oset, which is unique to absolute transit circle observational catalogs, is discussed emphasizing the problem of its cross-correlation with ro- tation terms from the alignment process. When compared to \traditional methods, these new procedures give sim- ilar results for those quantities in common but they also produce additional adjustments that were not accounted for previously.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.