Stellar Variability and Distance Indicators in the Near-infrared in Nearby Galaxies. I. RR Lyrae and Anomalous Cepheids in Draco dwarf spheroidal

Draco dwarf Spheroidal galaxy (dSph) is one of the nearest and the most dark matter dominated satellites of the Milky Way. We obtained multi-epoch near-infrared (NIR, JHKₛ) observations of the central region of Draco dSph covering a sky area of ~ 21'×21' using the WIRCam instrument at the 3.6-m Canada-France-Hawaii Telescope. Homogeneous JHKₛ time-series photometry for 212 RR Lyrae (173 fundamental-mode, 24 first-overtone, and 15 mixed-mode variables) and 5 Anomalous Cepheids in Draco dSph is presented and used to derive their period-luminosity relations at NIR wavelengths for the first-time. The small scatter of ~ 0.05~mag in these empirical relations for RR Lyrae stars is consistent with those in globular clusters and suggests a very small metallicity spread, up to ~0.2~dex, among these centrally located variables. Based on empirically calibrated NIR period-luminosity-metallicity relations for RR Lyrae in globular clusters, we determined a distance modulus to Draco dSph of μRRL = 19.557 ± 0.026 mag. The calibrated Kₛ-band period-luminosity relations for Anomalous Cepheids in the Draco dSph and the Large Magellanic Cloud exhibit statistically consistent slopes but systematically different zero-points, hinting at possible metallicity dependence of ~-0.3 mag~dex⁻¹. Finally, the apparent magnitudes of the tip of the red giant branch in I and J bands also agree well with their absolute calibrations with the adopted RR Lyrae distance to Draco. Our recommended ~1.5% precise RR Lyrae distance, DDraco = 81.55 ± 0.98 (statistical) ± 1.17 (systematic)~kpc, is the most accurate and precise distance to Draco dSph galaxy.