Automatic observation rendering (AMORE) (Ng, 2002)

Details Automatic observation rendering (AMORE) (Ng, 2002) Automatic observation rendering (AMORE) (Ng, 2002)

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33921129n&link_type=abstract

VizieR On-line Data Catalog: J/A+A/392/1129. Originally published in: 2002A&A...392.1129N

Astronomy and Astrophysics

Astrophysics

Models: Evolutionary, Photometry

Scientific paper

Tablea1.dat provides AMORE with the test population as specified in Sect. 4.3.1. See 2.6.2, 2.6.3, 2.6.4, 2.6.5 and 4.2 for additional details. Tablea2.dat contains the results of running AMORE with one of the astrophysical parameters fixed at its original value. These tests provide an indication about the influence of one parameter on the retrieval of the remaining parameters, see Sects. 4.3.3 and 5.3 for additional details. Tablea3.dat contains the results of running AMORE with one of the parameters fixed at one sigma from its original value. These tests provide an indication about the influence of one parameter on the retrieval of the remaining parameters - in particular, how the remaining parameters balance this mis-match by moving away from their optimal value (see Sects. 4.3.4 and 5.4 of the paper for additional details). (3 data files).

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