CONSTRUCTION OF THE INTERMEDIATE HIPPARCOS ASTROMETRIC CATALOG

被引：0

作者：

KOVALEVSKY, J

LINDEGREN, L

FROESCHLE, M

VANLEEUWEN, F

PERRYMAN, MAC

FALIN, JL

MIGNARD, F

PENSTON, MJ

PETERSEN, C

BERNACCA, PL

BUCCIARELLI, B

DONATI, F

HERING, R

HOG, E

LATTANZI, M

VANDERMAREL, H

SCHRIJVER, H

WALTER, HG

机构：

[1] LUND OBSERV, S-22100 LUND, SWEDEN

[2] ROYAL GREENWICH OBSERV, CAMBRIDGE CB3 0EZ, ENGLAND

[3] EUROPEAN SPACE AGCY, ESTEC, DIV ASTROPHYS, 2200 AG NOORDWIJK, NETHERLANDS

[4] COPENHAGEN UNIV OBSERV, DK-1350 COPENHAGEN K, DENMARK

[5] ASTROPHYS OBSERV, I-36102 ASIAGO, ITALY

[6] OSSERV ASTRON TORINO, I-10025 TURIN, ITALY

[7] CSS, I-10128 TURIN, ITALY

[8] ASTRON RECH INST, W-6900 HEIDELBERG, GERMANY

[9] DELFT UNIV TECHNOL, FAC GEODESY, 2629 JA DELFT, NETHERLANDS

[10] SRON, 3584 CA UTRECHT, NETHERLANDS

来源：

ASTRONOMY & ASTROPHYSICS | 1995年 / 304卷 / 01期

关键词：

ASTROMETRY; METHODS; DATA ANALYSIS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The data analysis methods for the determination of the astrometric parameters from observations by the Hipparcos satellite as used in FAST and NDAC consortia for the construction of intermediate 18-month and 30-month solutions are presented. The quality of the results depends upon calibrations of the instrumental parameters, examples of which are given. Results for the 18 and 30 month reductions are presented: these include histograms of the rms errors of each astrometric parameters, the FAST-NDAC differences as a function of coordinate, magnitude or colour index and results of a first attempt at combining the two solutions. The actual and pre-launch accuracy predictions are compared and discussed.

引用

页码：34 / 43

页数：10

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