Improved Photometric Accuracy and the Creation of an All-sky High-Accuracy Stellar Standard System

Details Improved Photometric Accuracy and the Creation of an All-sky High-Accuracy Stellar Standard System Improved Photometric Accuracy and the Creation of an All-sky High-Accuracy Stellar Standard System

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..364...77m&link_type=abstract

The Future of Photometric, Spectrophotometric and Polarimetric Standardization, ASP Conference Series, Vol. 364, Proceedings of

Astronomy and Astrophysics

Astrophysics

Scientific paper

Some astrophotometry problems require accuracy within 0.001m-0.003m mag, both in the random and systematic sense. Many research teams are planning now to carry out new sky surveys. These surveys will be made in different photometric systems and each photometric system will need its own standards. Thus, the main problem of photometric standardization becomes a task to construct the fundamental photometric catalog. Magnitudes of stars in the catalog have to be easily transformed to any specified photometric system without sacrifice of accuracy.

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