Asteroid phase curves using sparse and dense photometry
<p align="justify">We present a phase-curve computation method capable of combining sparse survey data, like relative photometry with dense differential measurements. Combining those types of data allows to obtain phase-curves parameters for large number of asteroids for which using traditional approach would not be sufficient.</p> <p align="justify">Using traditional dense ground-based photometry collected at Astronomical Observatory Institute of Adam Mickiewicz University in Pozna&#324; alongside with absolute Gaia measurements we were able to perform more accurate lightcurve amplitude correction and then derive the phase-slope parameter &#946; of the phase-curve separately for each opposition which met our selection criteria. We show preliminary results for 31 oppositions of 24 asteroids.</p> <p align="justify">In the future we plan to create a large photometric database containing sparse and dense photometry from various publicly available data sources (Gaia, ATLAS, K2, LSST, TESS, VISTA and others) which will include absolute, relative and differential photometry.</p> <p align="justify"><strong>Acknowledgments: </strong>This work has been supported by grant No. 2017/25/B/ST9/00740 from the National Science Centre, Poland.</p>