A very rapidly rotating white dwarf in nova YZ Reticuli
G. J. M. Luna (1,2), N. Rawat (3), R. Angeloni (4), M. Orio (5,6), S. Scaringi (7,8), A. Dobrotka (9), and J. Magdolen (9) ((1) UNAHUR, (2) Conicet, (3) South African Astronomical Observatory, (4) International Gemini Observatory/NSF NOIRLab

TL;DR
This paper reports the discovery of a rapidly rotating white dwarf in YZ Reticuli, identified through multi-instrument timing analysis, revealing a stable 37.69 s rotation period indicative of an Intermediate Polar system.
Contribution
It provides the first definitive measurement of the white dwarf's true rotation period in YZ Reticuli, confirming its nature as a fast-spinning magnetic white dwarf in an Intermediate Polar.
Findings
White dwarf rotation period is 37.69131 seconds.
The 42.61 s signal in TESS is a Nyquist alias.
The white dwarf's stability rules out transient oscillations.
Abstract
YZ Ret (Nova Reticuli 2020) is the first VY Scl-type nova-like variable observed to undergo a classical nova eruption. Following the outburst, timing analysis of 20-s cadence TESS data revealed a periodicity at approximately 42 s, suggesting a possible classification as a fast-spinning Intermediate Polar. To definitively identify the nature of this modulation, we performed a multi-instrument timing analysis using high-speed ground-based photometry Zorro/Gemini South (1 s cadence) and the South African Astronomical Observatory (5 s cadence) alongside TESS Sector 97 observations. Our ground-based data reveal a highly coherent period of 37.69131 +- 0.00001 s, which we identify as the true rotation period of the white dwarf. We demonstrate that the apparent 42.61 s signal in the TESS data is a Nyquist alias of this fundamental frequency. Furthermore, the signal amplitude in the TESS data is…
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