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Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. the seventh year (2014-2015)
Kato T., Hambsch F., Dubovsky P., Kudzej I., Monard B., Miller I., Itoh H., Kiyota S., Masumoto K., Fukushima D., Kinoshita H., Maeda K., Mikami J., Matsuda R., Kojiguchi N., Kawabata M., Takenaka M., Matsumoto K., De Miguel E., Maeda Y., Ohshima T., Isogai K., Pickard R., Henden A., Kafka S., Akazawa H., Otani N., Ishibashi S., Ogi M., Tanabe K., Imamura K., Stein W., Kasai K., Vanmunster T., Starr P., Oksanen A., Pavlenko E., Antonyuk O., Antonyuk K., Sosnovskij A., Pit N., Babina J., Sklyanov A., Novák R., Dvorak S., Michel R., Masi G., Littlefield C., Ulowetz J., Shugarov S., Golysheva P., Chochol D., Krushevska V., Ruiz J., Tordai T., Morelle E., Sabo R., Maehara H., Richmond M., Katysheva N., Hirosawa K., Goff W., Dubois F., Logie L., Rau S., Voloshina I., Andreev M., Shiokawa K., Neustroev V., Sjoberg G., Zharikov S., James N., Bolt G., Crawford T., Buczynski D., Cook L., Kochanek C., Shappee B., Stanek K., Prieto J., Denisenko D., Nishimura H., Mukai M., Kaneko S., Ueda S., Stubbings R., Moriyama M., Schmeer P., Muyllaert E.
period and there was no strong indication of a period gap. We detected possible negative superhumps in Z
Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. the ninth year (2016-2017)
Kato T., Isogai K., Hambsch F., Vanmunster T., Itoh H., Monard B., Tordai T., Kimura M., Wakamatsu Y., Kiyota S., Miller I., Starr P., Kasai K., Shugarov S., Chochol D., Katysheva N., Zaostrojnykh A., Sekeráš M., Kuznyetsova Y., Kalinicheva E., Golysheva P., Krushevska V., Maeda Y., Dubovsky P., Kudzej I., Pavlenko E., Antonyuk K., Pit N., Sosnovskij A., Antonyuk O., Baklanov A., Pickard R., Kojiguchi N., Sugiura Y., Tei S., Yamamura K., Matsumoto K., Ruiz J., Stone G., Cook L., De Miguel E., Akazawa H., Goff W., Morelle E., Kafka S., Littlefield C., Bolt G., Dubois F., Brincat S., Maehara H., Sakanoi T., Kagitani M., Imada A., Voloshina I., Andreev M., Sabo R., Richmond M., Rodda T., Nelson P., Nazarov S., Mishevskiy N., Myers G., Denisenko D., Stanek K., Shields J., Kochanek C., Holoien T., Shappee B., Prieto J., Itagaki K., Nishiyama K., Kabashima F., Stubbings R., Schmeer P., Muyllaert E., Horie T., Shears J., Poyner G., Moriyama M.
collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016
Survey of period variations of superhumps in SU UMa-type dwarf novae. VII. the seventh year (2014-2015)
Kato T., Hambsch F., Dubovsky P., Kudzej I., Monard B., Miller I., Itoh H., Kiyota S., Masumoto K., Fukushima D., Kinoshita H., Maeda K., Mikami J., Matsuda R., Kojiguchi N., Kawabata M., Takenaka M., Matsumoto K., De Miguel E., Maeda Y., Ohshima T., Isogai K., Pickard R., Henden A., Kafka S., Akazawa H., Otani N., Ishibashi S., Ogi M., Tanabe K., Imamura K., Stein W., Kasai K., Vanmunster T., Starr P., Oksanen A., Pavlenko E., Antonyuk O., Antonyuk K., Sosnovskij A., Pit N., Babina J., Sklyanov A., Novák R., Dvorak S., Michel R., Masi G., Littlefield C., Ulowetz J., Shugarov S., Golysheva P., Chochol D., Krushevska V., Ruiz J., Tordai T., Morelle E., Sabo R., Maehara H., Richmond M., Katysheva N., Hirosawa K., Goff W., Dubois F., Logie L., Rau S., Voloshina I., Andreev M., Shiokawa K., Neustroev V., Sjoberg G., Zharikov S., James N., Bolt G., Crawford T., Buczynski D., Cook L., Kochanek C., Shappee B., Stanek K., Prieto J., Denisenko D., Nishimura H., Mukai M., Kaneko S., Ueda S., Stubbings R., Moriyama M., Schmeer P., Muyllaert E.
period and there was no strong indication of a period gap. We detected possible negative superhumps in Z
Survey of period variations of superhumps in SU UMa-type dwarf novae. IX. the ninth year (2016-2017)
Kato T., Isogai K., Hambsch F., Vanmunster T., Itoh H., Monard B., Tordai T., Kimura M., Wakamatsu Y., Kiyota S., Miller I., Starr P., Kasai K., Shugarov S., Chochol D., Katysheva N., Zaostrojnykh A., Sekeráš M., Kuznyetsova Y., Kalinicheva E., Golysheva P., Krushevska V., Maeda Y., Dubovsky P., Kudzej I., Pavlenko E., Antonyuk K., Pit N., Sosnovskij A., Antonyuk O., Baklanov A., Pickard R., Kojiguchi N., Sugiura Y., Tei S., Yamamura K., Matsumoto K., Ruiz J., Stone G., Cook L., De Miguel E., Akazawa H., Goff W., Morelle E., Kafka S., Littlefield C., Bolt G., Dubois F., Brincat S., Maehara H., Sakanoi T., Kagitani M., Imada A., Voloshina I., Andreev M., Sabo R., Richmond M., Rodda T., Nelson P., Nazarov S., Mishevskiy N., Myers G., Denisenko D., Stanek K., Shields J., Kochanek C., Holoien T., Shappee B., Prieto J., Itagaki K., Nishiyama K., Kabashima F., Stubbings R., Schmeer P., Muyllaert E., Horie T., Shears J., Poyner G., Moriyama M.
collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016
Superoutburst of CR Bootis: Estimation of mass ratio of a typical AMCVn star by stage A superhumps
Isogai K., Kato T., Ohshima T., Kasai K., Oksanen A., Masumoto K., Fukushima D., Maeda K., Kawabata M., Matsuda R., Kojiguchi N., Sugiura Y., Takeda N., Matsumoto K., Itoh H., Pavlenko E., Antonyuk K., Antonyuk O., Pit N., Sosnovskij A., Baklanov A., Babina J., Sklyanov A., Kiyota S., Hambsch F., Littlefield C., Maeda Y., Cook L., Masi G., Dubovsky P., Novák R., Dvorak S., Imada A., Nogami D.
of the main superoutburst in 2014, we detected growing superhumps (stage A superhumps) whose period was 0
Superhumps linked to X-ray emission: The superoutbursts of SSS J122221.7-311525 and GW Lib
.6 ks. We analysed the X-ray light curve and compared it with the behaviour of superhumps which were
OT J002656.6+284933 (CSS101212:002657+284933): An SU UMa-type dwarf nova with the longest superhump period
Kato T., Tordai T., Littlefield C., Kasai K., Shugarov S., Katysheva N., Zaostrojnykh A., Pickard R., De Miguel E., Antonyuk K., Antonyuk O., Pavlenko E., Pit N., Itoh H., Ruiz J., Isogai K., Kimura M., Wakamatsu Y., Vanmunster T., Stone G.
in that it s howed two post-outburst rebrightenings. It showed superhump evolution similar to short-period SU UMa
Survey of period variations of superhumps in SU UMa-type dwarf novae. VIII. The eighth year (2015-2016)
Kato T., Hambsch F., Monard B., Vanmunster T., Maeda Y., Miller I., Itoh H., Kiyota S., Isogai K., Kimura M., Imada A., Tordai T., Akazawa H., Tanabe K., Otani N., Ogi M., Ando K., Takigawa N., Dubovsky P., Kudzej I., Shugarov S., Katysheva N., Golysheva P., Gladilina N., Chochol D., Starr P., Kasai K., Pickard R., De Miguel E., Kojiguchi N., Sugiura Y., Fukushima D., Yamada E., Uto Y., Kamibetsunawa T., Tatsumi T., Takeda N., Matsumoto K., Cook L., Pavlenko E., Babina J., Pit N., Antonyuk O., Antonyuk K., Sosnovskij A., Baklanov A., Kafka S., Stein W., Voloshina I., Ruiz J., Sabo R., Dvorak S., Stone G., Andreev M., Antipin S., Zubareva A., Zaostrojnykh A., Richmond M., Shears J., Dubois F., Logie L., Rau S., Vanaverbeke S., Simon A., Oksanen A., Goff W., Bolt G., Ebski B., Kochanek C., Shappee B., Stanek K., Prieto J., Stubbings R., Muyllaert E., Hiraga M., Horie T., Schmeer P., Hirosawa K.
evolutionary path near the terminal stage of evolution of cataclysmic variables. Three objects (V452 Cas, KK
Electric and galvanomagnetic properties of CD₃AS₂-20 mol % MnAs composite under high pressure
Saypulaeva, L. A., Gadzhialiev, M. M., Alibekov, A. G., Melnikova, N. V., Zakhvalinskii, V. S.
, and magnetoresistance of the Cd₃As₂-20 mol % MnAs composite are investigated at pressures up to 9 GPa. The pressure
Superoutburst of CR Bootis: Estimation of mass ratio of a typical AMCVn star by stage A superhumps
Isogai K., Kato T., Ohshima T., Kasai K., Oksanen A., Masumoto K., Fukushima D., Maeda K., Kawabata M., Matsuda R., Kojiguchi N., Sugiura Y., Takeda N., Matsumoto K., Itoh H., Pavlenko E., Antonyuk K., Antonyuk O., Pit N., Sosnovskij A., Baklanov A., Babina J., Sklyanov A., Kiyota S., Hambsch F., Littlefield C., Maeda Y., Cook L., Masi G., Dubovsky P., Novák R., Dvorak S., Imada A., Nogami D.
of the main superoutburst in 2014, we detected growing superhumps (stage A superhumps) whose period was 0

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