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 / ๅไฟ ้ไป
EMAIL: tampo(a)kusastro.kyoto-u.ac.jp
ALT. EMAIL: yusuke(a)saao.ac.za
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