ASASSN-14bp: likely superoutburst According to ASAS-SN data, this object is most likely an SU UMa star with supercycles of 200-400 d (variable). Time-resolved photometry is encouraged. YYYYMMDD(UT) mag observer 20210102.8388 <129c (Yutaka Maeda) 20210114.7293 <135c (Yutaka Maeda) 20210119.628 145 (Rod Stubbings)