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(Objective) We retrospectively analyzed clinical outcome, prognostic factors and adjuvant chemotherapy for bladder cancer patients with open radical cystectomy (ORC) combined with ileal conduit construction (ICC). (Patients and methods) From February 2005 to February 2019, 179 patients underwent ORC and ICC for invasive bladder cancer or BCG unresponsive non-muscle invasive bladder cancer. We investigated intraoperative and early postoperative complications, overall survival (OS), cancer-specific survival (CSS), and poor prognostic factors affecting OS. Furthermore, we evaluated the prognosis of patients with pT3,4 or pN1-3 depending on adjuvant chemotherapy. (Results) Clavien-Dindo Grade 4 or 5 complications were not occurred. The 5-year and 10-year OS probability were 71.1% and 57.4%, respectively, while the 5-year and 10-year CSS probability were 76.5% and 71.5%, respectively. Multivariate analysis revealed that male (HR = 2.70, 95%CI [0.97-7.51]), pT3,4 (HR = 1.83, 95%CI [1.05-3.21]), and pN1-3 (HR = 2.85, 95%CI [1.62-5.03]) were independent poor prognostic factors. Adjuvant chemotherapy significantly improved OS (p = 0.03) and CSS (p = 0.017) in pN1-3 patients. (Conclusion) ORC combined with ICC was an effective operative method, and good results were obtained. Adjuvant chemotherapy may be effective for patients with positive regional lymph nodes.

Continuing the project described by Kato et al. (2009a, arXiv:0905.1757), we collected times of superhump maxima for SU UMa-type dwarf novae mainly observed during the 2012-2013 season. We found three objects (V444 Peg, CSS J203937 and MASTER J212624) having strongly positive period derivatives despite the long orbital period (Porb). By using the period of growing stage (stage A) superhumps, we obtained mass ratios for six objects. We characterized nine new WZ Sge-type dwarf novae. We made a pilot survey of the decline rate of slowly fading part of SU UMa-type and WZ Sge-type outbursts. The decline time scale was found to generally follow the expected Porb^(1/4) dependence and WZ Sge-type outbursts also generally follow this trend. There are some objects which show slower decline rates, and we consider these objects good candidates for period bouncers. We also studied unusual behavior in some objects, including BK Lyn which made a transition from an ER UMa-type state to the novalike (standstill) state in 2013 and unusually frequent occurrence of superoutbursts in NY Ser and CR Boo. We applied least absolute shrinkage and selection operator (Lasso) power spectral analysis, which has been proven to be very effective in analyzing the Kepler data, to ground-based photometry of BK Lyn and detected the dramatic disappearance of the signal of negative superhumps in 2013. We suggested that the mass-transfer rates did not vary strongly between the ER UMa-type state and novalike state in BK Lyn, and this transition was less likely caused by a systematic variation of the mass-transfer rate., 83 pages, 95 figures, accepted for publication in PASJ

We report on photometric observations of WZ Sge-type dwarf novae, MASTER OT J211258.65+242145.4 and MASTER OT J203749.39+552210.3 which underwent outbursts in 2012. Early superhumps were recorded in both systems. During superoutburst plateau, ordinary superhumps with a period of 0.060291(4) d (MASTER J211258) and of 0.061307(9) d (MASTER J203749) in average were observed. MASTER J211258 and MASTER J203749 exhibited eight and more than four post-superoutburst rebrightenings, respectively. In the final part of the superoutburst, an increase in the superhump periods was seen in both systems. We have made a survey of WZ Sge-type dwarf novae with multiple rebrightenings, and confirmed that the superhump periods of WZ Sge-type dwarf novae with multiple rebrightenings were longer than those of WZ Sge-type dwarf novae without a rebrightening. Although WZ Sge-type dwarf novae with multiple rebrightenings have been thought to be the good candidates for period bouncers based on their low mass ratio (q) from inferred from the period of fully grown (stage B) superhumps, our new method using the period of growing superhumps (stage A superhumps), however, implies higher q than those expected from stage B superhumps. These q values appear to be consistent with the duration of the stage A superoutbursts, which likely reflects the growth time of the 3:1 resonance. We present a working hypothesis that the small fractional superhump excesses for stage B superhumps in these systems may be explained as a result that a higher gas pressure effect works in these systems than in ordinary SU UMa-type dwarf novae. This result leads to a new picture that WZ Sge-type dwarf novae with multiple rebrightenings and SU UMa-type dwarf novae without a rebrightening (they are not period bouncers) are located in the same place on the evolutionary track.