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Canopus Photometry Software
The Photometric Light Curves and the Rotation Period of the Asteroid 3122 Florence
Canopus Photometry Software Free
Canopus Photometry Software Review
Canopus Photometry Software Update
MPO Canopus – Photometry The photometry side of Canopus is written primarily for lightcurve analysis and so many of its features are designed towards that end. Some of the methods used are different for asteroids than for variable star work but Canopus handles both. MPO Canopus software (BDW Publishing 2010) was used to perform differential photometry and period analysis. The data were binned in sets of 3 with a maximum time interval of 5 minutes. The bimodal composite lightcurve indicates period P = 3.4916 ± 0.0001 h and amplitude A = 0.59 ± 0.01 mag near opposition (Figure 1).
Abstract
This study presents our results of the 3122 Florence asteroid photometric observations. We focused on the light curve construction and on the subsequent rotation period determination. Duration of our observations spanned four nights during which we obtained three relatively high-quality light curves. Observational data have been combined into one file and by using the MOP Canopus software we have determined the value of the rotation period to be P = 2.352 pm 0.210 hours.
Canopus Photometry Software Free
Publication:
Pub Date:
July 2018
Bibcode:
Canopus Photometry Software Review
2018BlgAJ..29....3B
Keywords:
Canopus Photometry Software Update
minor planets;
near Earth objects;
3122 Florence;
photometry;
periods
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