  These are the first results of an observational program devoted to the
complete physical data of asteroids that could produce or feed meteoroid
streams. Our results are based on the optical observation at Pic du Midi
observatory in April 6-7, 2016 and January 17-18, 2018. We will present the
light curve of asteroid (259221) 2003 BA21, associated with Daytime Sextantids
(221 DSX) and November theta Aurigids (390 THA); the light curves and colors of
asteroid (363599) 2004 FG11, associated with Daytime zeta Perseids (172 ZPE) as
well as g-r and g-i; and the corresponding reflectances for the (85953) 1999
FK21, associated with Daytime eta Sagittariids (100 XSA). We will also present
the colors for two additional objects, namely, (5141) Tachibana and (43032)
1999 VR26.
