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20182026
most citedA resonant sextuplet of sub-Neptunes transiting the bright star HD 110067

64 citations · 136 across the 17 of their papers we have counts for

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12 papers · 1 filter

astro-ph.EP2026

The Tierras Observatory: Ultra-Precise Photometry for Characterizing Exoplanets and Their Host Stars

Juliana García-Mejía, Patrick Tamburo, David Charbonneau +9

The Tierras Observatory is a fully robotic 1.3-m telescope at the Fred Lawrence Whipple Observatory in southern Arizona. Tierras achieves sub-part-per-thousand (ppt) photometric pr…

astro-ph.EP2026

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system

Pietro Leonardi, Alexandre Santerne, Luca Borsato +27

Characterizing long-period transiting exoplanets is inherently challenging due to the rarity and long duration of transit events. Yet, these systems provide unique insights into pl…

astro-ph.EP2026

RV and TTV Measurements of Two Transiting Long-Period Giants around TOI-4600

Tong Hu, Zitao Lin, Sharon X. Wang +27

TOI-4600b and c, originally identified by the Transiting Exoplanet Survey Satellite (TESS) and reported by I. Mireles et al. (2023), are a rare pair of transiting long-period giant…

astro-ph.EP2025

THYME XIII: Two young Neptunes orbiting a 75-Myr star in the Alpha Persei Cluster

Anne Dattilo, Andrew M. Vanderburg, Madyson G. Barber +28

Young planets with mass measurements are particularly valuable in studying atmospheric mass-loss processes, but these planets are rare and their masses difficult to measure due to…

astro-ph.EP2025

The Polar Orbit of TOI-2374 b, a Planet in the Neptunian Ridge

Samuel W. Yee, Patrick Tamburo, Gudmundur Stefánsson +11

The ``Neptunian ridge'' is a recently identified peak in the frequency of planets with sizes between that of Neptune and Saturn orbiting their host stars with periods between 3 and…

astro-ph.EP2025

A Ground-Based Transit Observation of the Long-Period Extremely Low-Density Planet HIP 41378 f

Juliana García-Mejía, Zoë L. de Beurs, Patrick Tamburo +25

We present a ground-based transit detection of HIP 41378 f, a long-period ( days), extremely low-density ( g cm) giant exoplanet in a dynamically com…

astro-ph.EP2025

Spot-Crossing Variations Confirm a Misaligned Orbit for a Planet Transiting an M Dwarf

Patrick Tamburo, Samuel W. Yee, Juliana García-Mejía +4

TOI-3884~b is an unusual 6.4~R planet orbiting an M4 host, whose transits display large and persistent spot-crossing events. We used the \textit{Tierras} Observatory to mo…

astro-ph.EP2025

The True Stellar Obliquity of a Sub-Saturn Planet from the Tierras Observatory and KPF

Patrick Tamburo, Samuel W. Yee, Juliana García-Mejía +7

We measure the true obliquity of TOI-2364, a K dwarf with a sub-Saturn-mass () transiting planet on the upper edge of the hot Neptune desert. We used new Rossiter-…

astro-ph.EP2023

TOI-4641b: An Aligned Warm Jupiter Orbiting a Bright (V=7.5) Rapidly Rotating F-star

Allyson Bieryla, George Zhou, Juliana García-Mejía +25

We report the discovery of TOI-4641b, a warm Jupiter transiting a rapidly rotating F-type star with a stellar effective temperature of 6560 K. The planet has a radius of 0.73 $R_{J…

astro-ph.EP2023★ 64 cited

A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067

R. Luque, H. P. Osborn, A. Leleu +149

Planets with radii between that of the Earth and Neptune (hereafter referred to as sub-Neptunes) are found in close-in orbits around more than half of all Sun-like stars. Yet, thei…

astro-ph.EP2020★ 2 cited

The HD 217107 Planetary System: Twenty Years of Radial Velocity Measurements

Mark R. Giovinazzi, Cullen H. Blake, Jason D. Eastman +13

The hot Jupiter HD 217107 b was one of the first exoplanets detected using the radial velocity (RV) method, originally reported in the literature in 1999. Today, precise RV measure…

astro-ph.EP2019★ 39 cited

Optimizing Ground-based Observations of O2 in Earth Analogs

Mercedes Lopez-Morales, Sagi Ben-Ami, Gonzalo Gonzalez-Abad +3

We present the result of calculations to optimize the search for molecular oxygen (O2) in Earth analogs transiting around nearby, low-mass stars using ground-based, high-resolution…