activity
20222026
most citedAGN Feedback in SDSS-IV MaNGA: AGNs have Suppressed Central Star Formation Rates

37 citations · 111 across the 17 of their papers we have counts for

collaborators
Showing 2026Show all

6 papers · 1 filter

astro-ph.EP2026

The Mysterious Inspiral of WASP-12b: Why Obliquity Tides Cannot Drive Orbital Decay

Caleb Lammers, Yubo Su, Joshua N. Winn

WASP-12b's orbit is decaying, for unknown reasons. The planet's period is shrinking more rapidly than can be attributed to equilibrium tides or dynamical tides in a main-sequence s…

astro-ph.EP2026

Constraining Tidal Migration with the Hot Jupiter Population

Linhao Ma, Yubo Su, Samuel W. Yee +3

Hot Jupiters with orbital periods shorter than a few days have probably been affected by tidal orbital migration. We develop an analytical framework for constraining tidal migratio…

astro-ph.EP2026

POSEIDON III: The Aligned Orbit of the Hot Neptune Around the Hot Star WASP-195

Juan I. Espinoza-Retamal, Joshua N. Winn, Rafael Brahm +33

Stellar obliquities provide important clues as to the formation and migration histories of planetary systems, but measurements remain scarce for Neptune-mass planets, especially th…

astro-ph.EP2026

Constraining the Planetary Obliquity Distribution of Warm Jupiters

Caleb Lammers, Joshua N. Winn

Warm Jupiters are an intriguing class of planets with uncertain origins. Their planetary obliquities could help distinguish between different formation pathways: planet-planet scat…

astro-ph.EP2026

POSEIDON II: The Anti-Aligned Orbit of the Warm Neptune TOI-1710 A b

Juan I. Espinoza-Retamal, Hareesh Bhaskar, Joshua N. Winn +7

We present an observation of the Rossiter-McLaughlin effect for the TOI-1710 system with the NEID spectrograph on the WIYN 3.5 m telescope. The system hosts a warm Neptune ($P\sim2…

astro-ph.EP2026

TTV-Not-So-Fast: Uniqueness and Degeneracy in Perturbing Planet Parameters

Caleb Lammers, Joshua N. Winn

Nontransiting planets can reveal themselves through transit timing variations (TTVs), but inferring the properties of the perturbing planet is a highly degenerate inverse problem.…