activity
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

collaborators

22 papers

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.SR2026

Six New Eclipsing AM CVn Binaries from the Zwicky Transient Facility

Aaron Householder, Kevin B. Burdge, Yapeng Zhang +16

We present the discovery of six new eclipsing AM CVn binaries, helium-accreting ultracompact systems in which a cool donor eclipses the accreting white dwarf. The systems were foun…

astro-ph.IM2026

Optimal Photon Counting with Fast, Low Noise Astronomical Imagers

Jack T. Dinsmore, Christopher Layden, Roger W. Romani +9

Measuring rapid astrophysical phenomena requires many short exposures, which suffer from repeated read noise. A variety of recent technologies are achieving sub-electron read noise…

astro-ph.SR2026

Conspicuous Gas, Cryptic Dust: Spectroscopy and Chromaticity of Complex Periodic Variables

Luke G. Bouma, Facundo Perez Paolino, Lynne A. Hillenbrand +17

Complex periodic variables (CPVs) are young low-mass stars whose light curves show periodic dips indicative of transiting corotating material. The origin and composition of this ma…

astro-ph.IM2026

The Lightspeed project: high-speed, ultra-low read noise imaging and polarimetry for the Magellan telescopes

Christopher Layden, Kevin Burdge, John J. Piotrowski +12

Lightspeed will be an ultra-fast (> kHz), ultra-low read noise, multicolor (ugriz + IR) imager for the 6.5 meter Magellan Clay telescope. In a single-channel configuration, Lightsp…

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.SR2026

An eclipsing 8.56 minute orbital period mass-transferring binary

Emma T. Chickles, Joheen Chakraborty, Kevin B. Burdge +34

We report the discovery of ATLAS J101342.5-451656.8 (hereafter ATLAS J1013-4516), an 8.56 minute orbital period mass transferring AM Canum Venaticorum binary with mean Gaia magnitu…

astro-ph.IM2026

proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope

Christopher Layden, Kevin Burdge, Gabor Furesz +9

proto-Lightspeed is a new instrument that has been commissioned on the Nasmyth East port of the Magellan Clay Telescope at Las Campanas Observatory to deliver high-speed optical im…

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.IM2020

The Tierras Observatory: An ultra-precise photometer to characterize nearby terrestrial exoplanets

Juliana García-Mejía, David Charbonneau, Daniel Fabricant +4

We report on the status of the Tierras Observatory, a refurbished 1.3-m ultra-precise fully-automated photometer located at the F. L. Whipple Observatory atop Mt. Hopkins, Arizona.…

astro-ph.IM2020

Characterization of a multi-etalon array for ultra-high resolution spectroscopy

Surangkhana Rukdee, Sagi Ben-Ami, Andrew Szentgyorgyi +3

The upcoming Extremely Large Telescopes (ELTs) are expected to have the collecting area required to detect potential biosignature gases in the atmosphere of rocky planets around ne…

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…

astro-ph.IM2019★ 12 cited

First radial velocity results from the MINiature Exoplanet Radial Velocity Array (MINERVA)

Maurice L. Wilson, Jason D. Eastman, Matthew A. Cornachione +52

The MINiature Exoplanet Radial Velocity Array (MINERVA) is a dedicated observatory of four 0.7m robotic telescopes fiber-fed to a KiwiSpec spectrograph. The MINERVA mission is to d…

astro-ph.IM2018★ 19 cited

High Resolution Spectroscopy using Fabry Perot Intereferometer Arrays: An Application to Searches for O in Exoplanetary Atmospheres

Sagi Ben-Ami, Mercedes López-Morales, Juliana Garcia-Mejia +2

We present a novel implementation for extremely high resolution spectroscopy using custom-designed Fabry Perot Interferometer (FPI) arrays. For a given telescope aperture at the se…