J/MNRAS/466/1567     Sou323 ICRF reference sample            (Liu+, 2017)

Test of source selection for constructing a more stable and uniform celestial reference frame. Liu N., Liu J.-C., Zhu Z. <Mon. Not. R. Astron. Soc., 466, 1567-1574 (2017)> =2017MNRAS.466.1567L 2017MNRAS.466.1567L (SIMBAD/NED BibCode)
ADC_Keywords: Fundamental catalog ; Positional data ; VLBI Keywords: catalogues - astrometry - reference systems Abstract: We aim to evaluate the possibility of improving the International Celestial Reference System realization starting from the ICRF2 catalogue by investigating the coordinate time series of radio sources observed by the very long baseline interferometry between 1979 and 2016. Sources with long observational history are selected as the candidates and the least-squares fits with special handling of the weights are performed to derive the linear drifts of the source coordinates. Then the sources are sorted, based on the normalized linear drift (i) over the whole sky, and (ii) in four homolographic areas divided by declinations. The axial stability of the reference system and sky distribution defined by the selected sources are evaluated, which are acted as the criterion for the final source lists. With our improved source selection scheme, two groups of sources are proposed and considered suitable for defining a more stable and homogeneous celestial reference system compared to the second version of the current International Celestial Reference Frame (ICRF2). The number of sources in the final lists are 323 and 294, respectively, and the global rotations of the axes derived from apparent motion of the sources are about two times better th Description: With the coordinate time series over 30yr, some of ICRF2 defining appear to be unstable and not suitable for defining a celestial frame. We have applied an improved selection scheme to pick out suitable sources as candidates. Finally, two sets of sources that show improved axial stability and sky distribution are recommended (Sou323 and Sou294). Only Sou323 is available. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 101 323 Time-series statistical information of sources in Sou323 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [ICRF] 6- 21 A16 --- ICRF ICRF designation (JHHMMSS.s+DDMMSS) 24- 31 A8 --- IERS IERS source name (HHMM+DDd, B1950) 36- 39 F4.2 --- pm/e_pm Ratio of proper motion on proper motion error 42- 47 F6.1 uas/yr dpmRA* Liner drift in pmRA*cosDE 50- 55 F6.1 uas/yr dpmDE Liner drift in pmDE 60- 63 F4.2 mas WdevRA* Weighted standard deviation in RA*cosDE 68- 71 F4.2 mas WdevDE Weighted standard deviation in DE 76- 79 F4.2 mas WAdevRA* Weighted Allan deviation in RA*cosDE 84- 87 F4.2 mas WAdevDE Weighted Allan deviation in DE 92- 95 F4.1 yr Tobs Observation span 98-101 I4 --- Nses Number of seasons -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 15-Oct-2019
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line