VizieR Online Data Catalog: Times of light minima for V410 Aur (Liao+, 2022)

CCD observations of V410 Aur have been carried out since 2006 by using the 1m and 60cm Cassegrain reflecting telescopes at Yunnan Observatories (YNOs; YNO-1m and YNO-60). We also monitored V410 Aur by using the 70cm telescope that was built in 2015 based on the cooperation between YNOs and the National Astronomical Research Institute of Thailand (NARIT), which is located at Lijiang Gaomeigu station of YNOs (LJ-70). Sixteen new eclipse times were obtained and are listed in Table 2 (therein Reference 16).

In order to determine stellar atmospheric parameters of V410 Aur, the spectra observations were performed on 2021 February 7 and October 20 by using the Beijing Faint Object Spectrograph and Camera (BFOSC) mounted on the 2.16m telescope in Xinglong station of National Astronomical Observatories, Chinese Academy of Sciences. See Section 2.2.

(2 data files).