SPECTRUM OF THE BORDEAUX TRANSIT CIRCLE RESIDUALS

Citation
P. Benevidessoares et al., SPECTRUM OF THE BORDEAUX TRANSIT CIRCLE RESIDUALS, Astronomy and astrophysics, 278(1), 1993, pp. 293-300
Citations number
12
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
278
Issue
1
Year of publication
1993
Pages
293 - 300
Database
ISI
SICI code
0004-6361(1993)278:1<293:SOTBTC>2.0.ZU;2-2
Abstract
This paper discusses the residuals in right ascension and declination from the Bordeaux fully automated transit circle, corresponding to a t wo years period. It is shown that the solution can be improved by addi ng statistically significant terms to the reduction model. The correla tion between the residuals, considered as a sample of a stochastic sta tionary process, displays a weak dependence on the declination differe nce and may be treated as a function of a single variable, the right a scension lag. The characteristics of the autocorrelation curves can be interpreted as derived from a power spectrum with two components: a l ow frequency power law and a flat spectrum. A fitting gives S(nu) = 20 10(-6)nu-1.37 + 1.3 and S(nu) = 89 10(-6)nu-1.37 + 2.0 for the right ascension and declination residuals, respectively, where the frequency unit is Hz and the power spectrum is expressed in ('')2/Hz. The expre ssions are valid in the frequency interval from 3 10(-5) to 3 10(-2) H z. These spectra are compatible with Hog (1968). It is shown that a pa rt of the low frequency spectrum can be removed by the adoption of a r eduction model which includes empirical higher order terms.