- vsnet-alert - ooruri.kusastro.kyoto-u.ac.jp

[vsnet-alert 28037] TCP J23291172+4127354: new eclipsing WZ Sge-type dwarf nova
by Yusuke Tampo 07 Dec '24

07 Dec '24

TCP J23291172+4127354: new eclipsing WZ Sge-type dwarf nova TCP J23291172+4127354 was discovered by Y. Nakamura on 2024-12-04.5385 at 14.1 mag (unfiltered). The counterpart in Pan-STARRS1 is g= 21.6 mag (objID= 157753522991272187), hence the outburst amplitude is ~7.5 mag. http://www.cbat.eps.harvard.edu/unconf/followups/J23291172+4127354.html https://www.aavso.org/vsx/index.php?view=detail.top&oid=2390566 Time-resolved observations reported by Itoh-san on the 5th and 6th Dec show double-peaked profiles and superposed eclipses. Its period and amplitude are obtained as 0.05693(2) d and ~0.5 mag (0.3 mag hump + 0.3 mag eclipse). Thus TCP J23291172+4127354 is a new (and yet another!) eclipsing WZ Sge-type dwarf nova. This would be another nice target for time-resolved photometries. Best regards, Yusuke -- ---------------------------------------------- South African Astronomical Observatory, Postdoc fellow 反保雄介　Yusuke TAMPO MAIL: tampo(a)kusastro.kyoto-u.ac.jp MAIL: yusuke(a)saao.ac.za ----------------------------------------------

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[vsnet-alert 28034] Gaia DR3 3130088774241620608: confirmation as a WZ Sge-type dwarf nova
by Yusuke Tampo 05 Dec '24

05 Dec '24

Gaia DR3 3130088774241620608: confirmation as a WZ Sge-type dwarf nova Itoh-san and J. Hambsch have reported the time-resolved observations of Gaia DR3 3130088774241620608 = TCP J06330104+0303350. The light curve shows a large-amplitude double-hump profile and superposed eclipses. Combining with AAVSO observations by J. Zhao, I obtained the early superhump+eclipse period as 0.05786(1) d. The orbital profile amplitude is ~0.5 mag; 0.3 mag early superhump plus 0.3 mag eclipse. Therefore, Gaia DR3 3130088774241620608 is now confirmed as an eclipsing WZ Sge-type. Time-resolved observations are strongly encouraged! best regards, Yusuke 2024年11月29日(金) 15:56 Yusuke Tampo <tampo(a)kusastro.kyoto-u.ac.jp>: > > TCP J06330104+0303350 = Gaia DR3 3130088774241620608 > > TCP J06330104+0303350 was discovered by T. Kojima on 2024-11-28.76 at > 13.9 mag and now brightened to V=13.4 mag according to TOCP reports. > http://www.cbat.eps.harvard.edu/unconf/followups/J06330104+0303350.html > > This system has already been pointed as a WZ Sge-type cataclysmic > variable candidate in Inight et al 2024, named Gaia DR3 > 3130088774241620608. > https://www.aavso.org/vsx/index.php?view=detail.top&oid=2389763 > https://ui.adsabs.harvard.edu/abs/2024MNRAS.tmp.2451I/abstract > > This outburst is a great opportunity to determine its outburst nature > as well as derive its superhump periods. > Time-resolved observations are encouraged. > > Best regards > Yusuke > > -- > ---------------------------------------------- > > South African Astronomical Observatory, Postdoc fellow > 反保雄介　Yusuke TAMPO > MAIL: tampo(a)kusastro.kyoto-u.ac.jp > MAIL: yusuke(a)saao.ac.za > > ---------------------------------------------- -- ---------------------------------------------- South African Astronomical Observatory, Postdoc fellow 反保雄介　Yusuke TAMPO MAIL: tampo(a)kusastro.kyoto-u.ac.jp MAIL: yusuke(a)saao.ac.za ----------------------------------------------

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[vsnet-alert 28035] TCP J01330474+3913194: new eclipsing WZ Sge star
by Kojiguchi 03 Dec '24

03 Dec '24

TCP J01330474+3913194: new eclipsing WZ Sge Star Itoh-san has reported time-resolved observations. Moriyama-san has also reported snapshots. The light curve shows an overlapping profile of early superhumps and eclipses. The period and amplitude are 0.0551(1) d and about 0.8 mag, respectively. Further observations are encouraged.

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[vsnet-alert 28033] TCP J06330104+0303350 = Gaia DR3 3130088774241620608
by Yusuke Tampo 29 Nov '24

29 Nov '24

TCP J06330104+0303350 = Gaia DR3 3130088774241620608 TCP J06330104+0303350 was discovered by T. Kojima on 2024-11-28.76 at 13.9 mag and now brightened to V=13.4 mag according to TOCP reports. http://www.cbat.eps.harvard.edu/unconf/followups/J06330104+0303350.html This system has already been pointed as a WZ Sge-type cataclysmic variable candidate in Inight et al 2024, named Gaia DR3 3130088774241620608. https://www.aavso.org/vsx/index.php?view=detail.top&oid=2389763 https://ui.adsabs.harvard.edu/abs/2024MNRAS.tmp.2451I/abstract This outburst is a great opportunity to determine its outburst nature as well as derive its superhump periods. Time-resolved observations are encouraged. Best regards Yusuke -- ---------------------------------------------- South African Astronomical Observatory, Postdoc fellow 反保雄介　Yusuke TAMPO MAIL: tampo(a)kusastro.kyoto-u.ac.jp MAIL: yusuke(a)saao.ac.za ----------------------------------------------

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[vsnet-alert 28032] ASASSN-24gv - new SU UMa-type dwarf nova
by Yusuke Tampo 29 Nov '24

29 Nov '24

ASASSN-24gv - new SU UMa-type dwarf nova ASASSN-24gv is a new CV candidate discovered by ASAS-SN at 15.25 mag on 2024-11-25. The quiescence counterpart is the g=22.34(2) star in the YMCA catalog, thus outburst amplitude is ~7 mag. Our time-resolved observations at SAAO on 2024-11-28 detected likely superhumps with a period of ~0.06 d and amplitude of 0.12 mag, classifying ASASSN-24gv as an SU UMa-type dwarf nova. Further observations are encouraged to establish its superhump period. Best regards, Yusuke -- ---------------------------------------------- South African Astronomical Observatory, Postdoc fellow 反保雄介　Yusuke TAMPO MAIL: tampo(a)kusastro.kyoto-u.ac.jp MAIL: yusuke(a)saao.ac.za ----------------------------------------------

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[vsnet-alert 28030] TCPJ00205034+3628247: superhumps
by Katsuki Muraoka 29 Nov '24

29 Nov '24

TCPJ00205034+3628247: superhumps Stephen M. Brincat reported time-resolved observations of TCPJ00205034+3628247. This object started showing superhumps with an amplitude of ~0.3 mag andperiodicity of around 0.051 d. Further observations are encouraged. Best Regards, Katsuki

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[vsnet-alert 28029] ASASSN-24gm: new WZ Sge-type dwarf nova
by Yusuke Tampo 13 Nov '24

13 Nov '24

ASASSN-24gm: new WZ Sge-type dwarf nova South African Astronomical Observatory team and Josch Hambsch have reported the time-resolved observations of ASASSN-24gm. Observations on 12 Nov. at SAAO detected clear superhumps, ~16 d after its discovery by ASAS-SN on 27th Oct. The tentative superhumps period is 0.0602(1) d, while 1-d aliases are still possible. Combining its short superhump period, large outburst amplitude of 8.4 mag, and long waiting time for superhump appearance, ASASSN-24gm is likely a new WZ Sge-type dwarf nova. Further observations are encouraged. Best regards, Yusuke -- ---------------------------------------------- South African Astronomical Observatory, Postdoc fellow Yusuke TAMPO MAIL: tampo(a)kusastro.kyoto-u.ac.jp MAIL: yusuke(a)saao.ac.za ----------------------------------------------

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[vsnet-alert 28028] QZ Vir superoutburst
by 大島誠人 12 Nov '24

12 Nov '24

Dear collegues, QZ Vir (= T Leo) is now undergoing a superoutburst. Although this object can be observed just before the dawn, please observe superhumps of this object if possible. Tomohito Ohshima

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[vsnet-alert 28027] GOTO065054.49+593624.51: end of the type-E rebrighening
by Yusuke Tampo 31 Oct '24

31 Oct '24

GOTO065054.49+593624.51: end of the type-E rebrighening According to the most recent ATLAS forced photometry and AAVSO observations by Nikola Antonov, Arto Oksanen, and Klaus Wenzel, this object dimmed around 18th mag on 2024-10-30, likely an end of its type E brightening. As type-E-rebrighening systems typically show additional short-lived brightenings, daily snapshots are still encouraged. Best regards, Yusuke #ATLAS forced photometry #UTC mag band observer 20241004.59088 13.215 c atlas 20241004.59451 13.214 c atlas 20241004.61565 13.207 c atlas 20241004.63368 13.206 c atlas 20241006.61241 13.714 o atlas 20241006.63332 13.715 o atlas 20241006.63517 13.712 o atlas 20241006.64267 13.727 o atlas 20241008.60186 13.596 c atlas 20241008.60503 13.613 c atlas 20241008.62933 13.615 c atlas 20241008.64262 13.630 c atlas 20241012.56768 13.963 c atlas 20241012.57085 13.963 c atlas 20241012.57629 13.959 c atlas 20241012.59150 13.954 c atlas 20241016.57534 14.505 o atlas 20241016.57716 14.503 o atlas 20241016.59971 14.498 o atlas 20241016.60560 14.498 o atlas 20241020.46639 14.542 o atlas 20241020.47092 14.542 o atlas 20241020.47409 14.578 o atlas 20241020.50475 14.478 o atlas 20241024.52590 14.645 o atlas 20241024.52771 14.656 o atlas 20241024.53178 14.666 o atlas 20241024.54710 14.594 o atlas 20241030.54204 17.807 c atlas 20241030.55202 17.790 c atlas 20241030.55437 17.759 c atlas 20241030.56083 17.819 c atlas 20241030.56415 17.775 c atlas 20241030.56882 18.013 c atlas 20241030.57205 17.835 c atlas -- ---------------------------------------------- South African Astronomical Observatory, Postdoc fellow 反保雄介 Yusuke TAMPO MAIL: tampo(a)kusastro.kyoto-u.ac.jp MAIL: yusuke(a)saao.ac.za ----------------------------------------------

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[vsnet-alert 28026] maintenance power outrage
by Katsuki Muraoka 31 Oct '24

31 Oct '24

Dear, VSNET members, I'm Katsuki Muraoka, a M2 student of Kyoto University. I must inform you all that there will be a maintenance power outage for the Kyoto Univ. building on this weekend, so VSNET server must be shut down in advance. The shutdown is scheduled to occur around 16:00 JST on November 2nd (UTC: 07:00), and the system is scheduled to be restored at around 17:30 JST (UTC: 08:30) on November 3rd. Thank you for your cooperation. Katsuki Muraoka

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