activity
20022026
most citedThe DWARF project: Eclipsing binaries - precise clocks to discover exoplanets

58 citations · 570 across the 45 of their papers we have counts for

collaborators

45 papers

astro-ph.SR2026

Joint Observations of PTPS Targets (JOTA). Combined spectroscopic and photometric analysis of 16 SB1 systems

Robert Jaros, Andrzje Niedzielski, Sohaib Ali +9

Context. The Pennsylvania-Toruń Planet Search, which operates on a sample of 1000 northern-hemisphere stars, has been underway since 2004. Stars with radial velocity (RV) amp…

astro-ph.EP2024

Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission

Jack Schulte, Joseph E. Rodriguez, Allyson Bieryla +72

Hot Jupiters were many of the first exoplanets discovered in the 1990s, but in the decades since their discovery, the mysteries surrounding their origins remain. Here, we present n…

astro-ph.SR2022

HD 183986: a high-contrast SB2 system with a pulsating component

Martin Vaňko, Theodor Pribulla, Pavol Gajdoš +7

There is a small group of peculiar early-type stars on the main sequence that show different rotation velocities from different spectral lines. This inconsistency might be due to t…

astro-ph.SR2021★ 7 cited

V680 Mon -- a young mercury-manganese star in an eclipsing heartbeat system

E. Paunzen, S. Huemmerich, M. Fedurco +3

Chemically peculiar stars in eclipsing binary systems are rare objects that allow the derivation of fundamental stellar parameters and important information on the evolutionary sta…

astro-ph.EP2020★ 23 cited

Probing Transit Timing Variation and its Possible Origin with Twelve New Transits of TrES-3b

Vineet Kumar Mannaday, Parijat Thakur, Ing-Guey Jiang +15

We present twelve new transit light curves of the hot-Jupiter TrES-3b observed during to probe the transit timing variation (TTV). By combining the mid-transit times de…

astro-ph.SR2020★ 1 cited

Close eclipsing binary BD And: a triple system

T. Pribulla, L. Hambalek, E. Guenther +5

BD And is a fairly bright (V = 10.8), active and close (P = 0.9258 days) eclipsing binary. The cyclic variability of the apparent orbital period as well as third light in the light…