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您现在的位置是:虫虫源码 > Python > 光度校准仪器的恒星大小和过滤功能

光度校准仪器的恒星大小和过滤功能

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Stellar Instrumental Magnitudes + Filter Functions -> Calibration Email big.macs.calibrate@gmail.com for updates/notifications An implementation of algorithms described in Kelly et al. 2014 (http://arxiv.org/abs/1208.0602) Updated 8/25/12 Author List P. L. Kelly, A. von der Linden, D. Applegate, M. Allen, S. W. Allen, P. R. Burchat, D. L. Burke, H. Ebeling, P. Capak, O. Czoske, D. Donovan, A. Mantz, and R. G. Morris 1-2% Color Calibration Big MACS is a Python program that estimates an accurate photometric calibration from only an input catalog of stellar magnitudes and filter transmission functions. The user does not have to measure color terms which can be difficult to characterize. Supplied with filter transmission functions, Big MACS synthesizes an expected stellar locus for your data and then simultaneously solves for all unknown zeropoints when fitti

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big-macs-calibrate
EXAMPLES
FILTERS
fit_locus.py
lociCAS.fits
LOCUS_SPECTRA
munari.sed
PLOTS
README
sqlcl.py
utilities.py
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