Searching for the mHz variability in the TESS observations of nova-like cataclysmic variables

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Table 2.

Used system parameters.

object	m_WD	ṁ_acc	i
	(M_⊙)	(M_⊙/yr)	(deg)
AH Men	0.35/0.55 ^(a)	3 × 10⁻¹⁰^(a)	20 ^(a)
BB Dor	0.8 ^(b)	10⁻⁹^(b)	< 10 ^(b)
KQ Mon	0.6 ^(c)	10⁻⁹^(c)	60–75 ^(c)
KR Aur	0.7 ^(d)		< 40 ^(d)
	0.6 ^(e)	3 × 10⁻¹⁰^(e)	41 ^(e)
	0.59 ± 0.17 ^(f)		38 ^(f)
	$0 . 94_{- 0.11}^{+ 0.15}$ $0.94^{+0.15}_{-0.11}$ ^(g)		47 ^(g)
MV Lyr	0.73 ± 0.10 ^(h)	3 × 10⁻⁹⁽ⁱ⁾	12 ^(h)
QU Car	0.6–1.2 ^(j)	10⁻⁷–10⁻⁶^(j)	40–60 ^(j)
TT Ari	0.57 ^(k)	4 × 10⁻⁹^(k)	17–22.5 ^(k)
V592 Cas	$1 . 4_{- 0.6}^{+ 1.0}$ $1.4^{+1.0}_{-0.6}$ ^(l)		28 ^(l)
V795 Her	0.8 ^(e)	10⁻¹⁰^(e)	41 ^(e)

AC Cnc			75.6 ^(f)
DW UMa			82 ^(f)
LX Ser			90 ^(f)
RR Pic			65 ^(f)
RW Tri			70.5 ^(f)
TV Col			70 ^(f)
UU Aqr			78 ^(f)
UX UMa			70 ^(f)
V348 Pup			81.1 ^(f)

Notes. The first part is for systems with an f_b detection, while the second part is only for systems with red noise PDSs.

References:^(a)Gänsicke & Koester (1999), ^(b)Godon et al. (2008), ^(c)Wolfe et al. (2013), ^(d)Shafter (1983), ^(e)Mizusawa et al. (2010), ^(f)Ritter & Kolb (2003), ^(g)Rodríguez-Gil et al. (2020), ^(h)Hoard et al. (2004), ⁽ⁱ⁾Linnell et al. (2005), ^(j)Linnell et al. (2008), ^(k)Belyakov et al. (2010), ^(l)Huber et al. (1998).

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