Title: (55638) 2002 VE95
Content:  The rotation period of  is poorly defined and has ambiguous results with multiple alternative period solutions in between 4.90 and 10 hours. In December 2002, a rotational lightcurve of this object was obtained from photometric observations by astromomers from the Sierra Nevada Observatory in Spain. Lightcurve analysis gave a poorly defined period of 6.76 hours with a brightness variation of 0.08 magnitude (U=1+). Two years later in December 2004, it was revisited by the same astronomers, obtaining another poorly defined period of 9.97 hours with an amplitude of 0.05 magnitude (U=1+). Other observations by Sheppard only determined an amplitude of less than 0.06 magnitude (U=1).
Title: (391211) 2006 HZ51
Content:  As of 2018, n rotational lightcurve of has been obtained from photometric observations. The body's rotation period, pole and shape remains unknown.
Title: 986 Amelia
Content:  In October 2000, a rotational lightcurve of Amelia was obtained from photometric observations by American amateur astronomer Robert A. Koff at the Thornton Observatory in Colorado. Lightcurve analysis gave a well-defined rotation period of 9.52 hours with a brightness amplitude of 0.43 magnitude (U=3). In December 2006, a concurring period determination of 0.396533 d was made by astronomers Raymond Poncy, Enric Forné, Hiromi Hamanowa, Hiroko Hamanowa and Hilari Pallarés (U=3). In 2016, a modeled lightcurves using photometric data from various sources, rendered a concurring sidereal period of 9.519 h and two spin axes of (80.0°, 30.0°) and (282.0°, 30.0°) in ecliptic coordinates.
Title: (89830) 2002 CE
Content:  In October 2004, a rotational lightcurve of was obtained from photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory. Lightcurve analysis gave a rotation period of 2.6149 hours with a low brightness amplitude of 0.09 magnitude (U=2-). Several longer periods are also possible.
Title: (481394) 2006 SF6
Content:  In September 2018, a rotational lightcurve of  was obtained from photometric observations by Brian Warner and Robert Stephens at the Center for Solar System Studies in California. Lightcurve analysis gave a rotation period of 11.517 hours with a very high brightness amplitude of 0.97 magnitude (U=3), indicative of a highly elongated non-spherical shape. The two photometrists revisited the object in October 2019 and obtained a similar result of 11.495 hours with an even higher magnitude of 1.07 (U=3-).
Title: (65407) 2002 RP120
Content:  In October 2010, a rotational lightcurve of  was obtained from photometric observations by French amateur astronomer René Roy. Lightcurve analysis gave a rotation period of 200 hours with a brightness amplitude of 0.6 magnitude, indicative of an elongated, non-spherical shape (U=2). With a rotation period above 100 hours, it is a typical slow rotator.
Title: 920 Rogeria
Content:   In October 2010, a rotational lightcurve of Rogeria was obtained from photometric observations by Thomas A. Polakis at the Command Module Observatory in Arizona. Lightcurve analysis gave a rotation period of 12.244 hours with a brightness variation of 0.31 magnitude (U=3−). A tentative period determination of 9.05 hours with an amplitude of 0.21 magnitude was made by French amateur French astronomer René Roy in July 2012 (U=2−). Another observation by Petr Pravec and Peter Kušnirák at Ondřejov Observatory in June 2007 gave a period of 8.09 hours (U=2−). In 2016, a modeled lightcurve gave a concurring sidereal period of 12.575 hours using data from the Uppsala Asteroid Photometric Catalogue, the Palomar Transient Factory survey, and individual observers (such as above), as well as sparse-in-time photometry from the NOFS, the Catalina Sky Survey, and the La Palma surveys. The study also determined two spin axes of (238.0°, −15.0°) and (47.0°, −35.0°) in ecliptic coordinates (λ,&thinsp;β).
Title: 894 Erda
Content:  In June 2006, a rotational lightcurve of Erda was obtained from photometric observations by David Higgins at Hunters Hill Observatory, Australia, and by Rui Gonçalves at Linhaceira Observatory in Portugal. Lightcurve analysis gave a well-defined rotation period of 4.69 hours with a brightness variation of 0.27 magnitude, significantly higher than previous observations had measured (U=3). The observers also found no indication of a previously speculated companion. The result supersedes observations from July 2001, when both Robert Stephens and Laurent Bernasconi determined a period of 4.69 and 4.69 hours with an amplitude of 0.05 and 0.06 magnitude, respectively.
Title: (127546) 2002 XU93
Content:  As of 2018, no rotational lightcurve of this object has been obtained from photometric observations. The object's rotation period, pole and shape remain unknown.
Title: (22149) 2000 WD49
Content:  In July 2006, a first rotational lightcurve of  was obtained from photometric observations by Italian amateur astronomer Silvano Casulli. Lightcurve analysis gave a rotation period of 7.84 hours with a brightness amplitude of 0.20 magnitude (U=2).

Question: Verify the following claims with "True" or "False": Its epoch date is 2006.12.31 and its rotation period is 95040.0.
Answer: True