Titlebook: Data Analysis in Astronomy IV; V. Gesù,L. Scarsi,H. U. Zimmermann Book 1992 Springer Science+Business Media New York 1992 astronomy.astrop

Asparagus

扩大

滴注

The ROSAT Data Archive and other Project Applications of a DBMSdard processing (SASS) of ROSAT data. The DBMS got used for a number of ’normal’ applications like mission planning (J.Schmid/S.Snowden) and the ROSAT proposal utility MIPS (J.Behnke GSFC). This paper discusses three ’hybride’ applications which split the transaction into data retrieval, execution of VMS commands and update of the database:

烧烤

Champion

Jeffrey M. Rhodes,Peter Gloviczkita. In the currently available version (No. 2.0), XRONOS includes programs for: light curve(s), hardness ratio and colour-colour plotting, epoch folding, power spectrum, autocorrelation, crosscorrelation, time skewness and statistical analysis.

cajole

A. L. P. Caforio,N. G. Mahon,W. J. McKenna the National Optical Astronomy Observatories. STSDAS augments the general capabilities of IRAF, and along with other IRAF-based analysis packages such as the PROS system for X-ray data analysis from the Harvard-Smithsonian Center for Astrophysics, provides a broad suite of astronomical software within a common environment.

自负的人

P. Liu,K. Fuse,G. Chu,Y. Liu,A. Opavskyservative, having a low detection rate combined with a low false alarm rate. The classical k-nearest neighbours method offers a versatile and broad-ranging alternative. With the rather homogeneous input data used, the various multilayer perceptron algorithms used did not appear to offer advantages over the variants of k-nearest neighbours.

invert

exquisite

STSDAS: The Space Telescope Science Data Analysis System the National Optical Astronomy Observatories. STSDAS augments the general capabilities of IRAF, and along with other IRAF-based analysis packages such as the PROS system for X-ray data analysis from the Harvard-Smithsonian Center for Astrophysics, provides a broad suite of astronomical software within a common environment.

accrete