ASASSN-25dc; a new candidate of a WZ Sge-type dwarf nova with the double
superoutburst
ASASSN-25dc was discovered by ASAS-SN on 2025-07-13.09 UTC at g=13.07. This
outburst is also observed by ATLAS, o~15.2 mag on 2025-07-07.8 UTC and
o~13.5 mag on 2025-07-10.9 UTC. The likely counterpart is Gaia
DR3 6129070308813533568 with G~21.0 mag, hence the outburst amplitude is
~7.0 mag.
This system underwent a short dip on 16-17th July, around 14.5 mag, and is
now recovering from the dip.
Lesedi telescope at Sutherland, Josch Hambsh, and Berto Monard have
reported the time-resolved observations of ASASSN-25dc. PDM analysis using
the overall data yields a single-peaked modulation with a period of
0.05991(4) d and an amplitude of 0.03 mag. Combining the 1-mag dip feature
on the light curve and short superhump period, ASASSN-25dc can be a similar
system to double-superoutburst WZ Sge-type dwarf novae, especially the
period-bouncer candidates ASASSN-15jd and ASASSN-16hg (see Kimura et al.
2016,2018).
https://arxiv.org/abs/1604.06344https://arxiv.org/abs/1803.03179
The ongoing second outburst should show the evolution of ordinary
superhumps. The hint of ordinary superhumps is seen in the observations on
17th July. Further time-resolved observations are encouraged.
Best regards,
Yusuke
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South African Astronomical Observatory, Postdoc fellow
Yusuke TAMPO / 反保 雄介
EMAIL: tampo(a)kusastro.kyoto-u.ac.jp
ALT. EMAIL: yusuke(a)saao.ac.za
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ASASSN-25df; new SU UMa-type dwarf nova
ASASSN-25df was discovered by ASAS-SN on 2025-07-28.02 UTC at g=13.51 mag.
The outburst amplitude is ~8.0 mag. ATLAS has also detected this outburst
since 2025-07-25.
https://vsx.aavso.org/index.php?view=detail.top&oid=10867883
Josch Hambsh reported the time-resolved observations. The observations
after 2025-08-02 show strong variations with an amplitude of ~0.1 mag. Due
to the short baselines because of its RA~12.5 hr, the superhump period is
not well constrained; a possible period is ~0.067 d, but other aliases are
equally possible.
Thus, I conclude that ASASSN-25df is a new SU UMa-type dwarf nova. A
waiting time of ~7 days before the appearance of ordinary superhumps
suggests that ASASSN-25df can be a WZ Sge-type dwarf nova.
Best regards,
Yusuke
--
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South African Astronomical Observatory, Postdoc fellow
Yusuke TAMPO / 反保 雄介
EMAIL: tampo(a)kusastro.kyoto-u.ac.jp
ALT. EMAIL: yusuke(a)saao.ac.za
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TCP J16271026-1030020: a new WZ Sge-type dwarf nova candidate possibly with
large-amplitude early superhump
TCP J16271026-1030020 was discovered by T. Kojima on 2025-07-25.52 UTC at
13.8 mag (unfiltered). ATLAS force photometry and ASASSN also detect this
outburst since 2025-07-22.3 UTC, peaking around g~12.6 mag. The Pan-STARRS1
counterpart is g=22.1(2) mag, giving the outburst amplitude of ~9.5 mag.
http://www.cbat.eps.harvard.edu/unconf/followups/J16271026-1030020.htmlhttps://vsx.aavso.org/index.php?view=detail.top&oid=10867693
I have obtained the low-resolution spectrum with the Lesedi telescope at
the SAAO Sutherland. This spectrum shows prominent Balmer, He II 4686, and
other He I emission lines with no absorption features. Itoh-san also
reported the time-resolved observations for ~45 min. The light curve shows
a modulation of ~0.2 mag.
These overall features suggest that TCP J16271026-1030020 is a new
large-amplitude dwarf nova, most likely a WZ Sge-type, showing relatively
large early superhump amplitude.
Further time-resolved observations (with multiple bands, if possible) and
time-resolved spectroscopy are encouraged.
Best regards,
Yusuke
--
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South African Astronomical Observatory, Postdoc fellow
Yusuke TAMPO / 反保 雄介
EMAIL: tampo(a)kusastro.kyoto-u.ac.jp
ALT. EMAIL: yusuke(a)saao.ac.za
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