The ASAS-SN Catalog of Variable Stars VI: An All-Sky Sample of $\delta$ Scuti Stars

We characterize an all-sky catalog of ${\sim} 8,400$ $\delta$ Scuti variables in ASAS-SN, which includes ${\sim} 3,300$ new discoveries. Using distances from \textit{Gaia} DR2, we derive period-luminosity relationships (PLRs) for both the fundamental mode and overtone pulsators in the $W_{JK}$, $V$, Gaia DR2 $G$, $J$, $H$, $K_s$ and $W_1$ bands. We find that the overtone pulsators have a dominant overtone mode, with many sources pulsating in the second overtone or higher order modes. The fundamental mode pulsators have metallicity dependent periods, with $\log_{10} (\rm P){\sim}-1.1$ for $\rm [Fe/H]<-0.3$ and $\log_{10} (\rm P){\sim}-0.9$ for $\rm [Fe/H]>0$ which leads to a period-dependant scale height. Stars with $\rm P>0.100\,d$ are predominantly located close to the Galactic disk ($\rm |Z|<0.5\,kpc$). The median period at a scale height of $\rm Z{\sim}0\, kpc$ also increases with the Galactocentric radius $\rm R$, from $\log_{10} (\rm P){\sim}-0.94$ for sources with $\rm R>9\, kpc$ to $\log_{10} (\rm P){\sim}-0.85$ for sources with $\rm R<7\, kpc$, which is indicative of a radial metallicity gradient. To illustrate potential applications of this all-sky catalog, we obtained 30 min cadence, image subtraction TESS light curves for a sample of 10 fundamental mode and 10 overtone $\delta$ Scuti stars discovered by ASAS-SN. From this sample, we identified two new $\delta$ Scuti eclipsing binaries, ASASSN-V J071855.62$-$434247.3 and ASASSN-V J170344.20$-$615941.2 with short orbital periods of $\rm P_{orb}=2.6096$ d and $\rm P_{orb}=2.5347$ d respectively.
Comment: Accepted by MNRAS