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20022023
most citedSurvey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae

194 citations · 1.5k across the 37 of their papers we have counts for

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24 papers · 1 filter

astro-ph.SR2023

Spectroscopic distance, mass, and age estimations for APOGEE DR17

Alexander Stone-Martinez, Jon A. Holtzman, Julie Imig +3

We derive distances and masses of stars from the Sloan Digital Sky Survey (SDSS) Apache Point Observatory Galactic Evolution Experiment (APOGEE) Data Release 17 (DR17) using simple…

astro-ph.SR2022

Investigating the low-flux states in six Intermediate Polars

Ava E. Covington, Aarran W. Shaw, Koji Mukai +30

We present optical photometry of six intermediate polars that exhibit transitions to a low-flux state. For four of these systems, DW Cnc, V515 And, V1223 Sgr and RX J2133.7+5107, w…

astro-ph.SR2021★ 119 cited

Constraining the Evolution of Cataclysmic Variables via the Masses and Accretion Rates of their Underlying White Dwarfs

A. F. Pala, B. T. Gänsicke, D. Belloni +28

We report on the masses (), effective temperatures () and secular mean accretion rates () of 43 cataclysmic variable (CV) wh…

astro-ph.SR2021★ 48 cited

Populating the brown dwarf and stellar boundary: Five stars with transiting companions near the hydrogen-burning mass limit

Nolan Grieves, François Bouchy, Monika Lendl +52

We report the discovery of five transiting companions near the hydrogen-burning mass limit in close orbits around main sequence stars originally identified by the Transiting Exopla…

astro-ph.SR2019★ 16 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. X: The Tenth Year (2017)

Taichi Kato, Keisuke Isogai, Yasuyuki Wakamatsu +67

Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv/0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly duri…

astro-ph.SR2019★ 2 cited

CS Indi: SU UMa-Type Dwarf Nova with Long Precursor Outburst

Taichi Kato, Franz-Josef Hambsch, Berto Monard +3

We observed the 2018 November outburst of CS Ind and confirmed that it was a genuine superoutburst with a very long [0.12471(1) d in average] superhump period. The superoutburst wa…