Corrections to optical activity of the transient X-ray source A0535+26/HDE 245770 (ATel#6528)
ATel #6585; F. Giovannelli (INAF-Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy), G. S. Bisnovatyi-Kogan (IKI - Space Research Institute, Moscow, Russia), I. Bruni (INAF-Osservatorio Astronomico di Bologna, Stazione astronomica di Loiano, Italy), F. Martinelli (Montecatini Val di Cecina Astronomical Centre, Montecatini Val di Cecina, Italy), M. Monaci (Montecatini Val di Cecina Astronomical Centre, Montecatini Val di Cecina, Italy), C. Rossi (Dpt. of Physics, Sapienza University, Roma, Italy)
on 16 Oct 2014; 17:55 UT
Credential Certification: Franco Giovannelli (franco.giovannelli@iaps.inaf.it)
Subjects: Optical, A Comment
Because of a mistake in our ATel#6528, which could cause scientific misunderstanding, we want to inform that the (JD 2456821) around which we planned the observations must be corrected with (JD 2456932), and the passage at the periastron of the neutron star is not 107 but 108 orbital periods after the 811205-E.
