papers

Publications (38)

physics.optics2024

Advancing on-chip Kerr optical parametric oscillation towards coherent applications covering the green gap

Yi Sun, Jordan Stone, Xiyuan Lu +3

Optical parametric oscillation (OPO) in Kerr microresonators can efficiently transfer near-infrared laser light into the visible spectrum. To date, however, chromatic dispersion ha…

physics.optics2025

All-Optical Noise Quenching of An Integrated Frequency Comb

Gregory Moille, Pradyoth Shandilya, Jordan Stone +2

Integrated frequency combs promise transformation of lab-based metrology into disruptive real-world applications. These microcombs are, however, sensitive to stochastic thermal flu…

astro-ph.EP2015

The LEECH Exoplanet Imaging Survey: Characterization of the Coldest Directly Imaged Exoplanet, GJ 504 b, and Evidence for Super-Stellar Metallicity

Andrew J. Skemer, Caroline V. Morley, Neil T. Zimmerman +39

As gas giant planets and brown dwarfs radiate away the residual heat from their formation, they cool through a spectral type transition from L to T, which encompasses the dissipati…

astro-ph.GA2018

Detection of intrinsic source structure at ~3 Schwarzschild radii with Millimeter-VLBI observations of SAGITTARIUS A*

Ru-Sen Lu, Thomas P. Krichbaum, Alan L. Roy +53

We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A*, at 1.3 mm (230 GHz). The observations w…

physics.optics2023

Two-Dimensional Nonlinear Mixing Between a Dissipative Kerr Soliton and Continuous Waves for a Higher-Dimension Frequency Comb

Gregory Moille, Christy Li, Jordan Stone +6

Dissipative Kerr solitons (DKSs) intrinsically exhibit two degrees of freedom through their group and phase rotation velocity. Periodic extraction of the DKS into a waveguide produ…

astro-ph.IM2020

Betelgeuse scope: Single-mode-fibers-assisted optical interferometer design for dedicated stellar activity monitoring

Narsireddy Anugu, Katie M. Morzinski, Josh Eisner +12

Betelgeuse has gone through a sudden shift in its brightness and dimmed mysteriously. This is likely caused by a hot blob of plasma ejected from Betelgeuse and then cooled to obscu…

physics.optics2021

Hybrid-mode-family Kerr optical parametric oscillation for robust coherent light generation on chip

Feng Zhou, Xiyuan Lu, Ashutosh Rao +5

Optical parametric oscillation (OPO) using the third-order nonlinearity () in integrated photonics platforms is an emerging approach for coherent light generation, and ha…

astro-ph.EP2026

From Young to Older Disks: JWST/MIRI Evidence for Fading Molecular Emission and Hints for Elevated C/O in Upper Scorpius

Chengyan Xie, Ilaria Pascucci, Feng Long +23

We present JWST/MIRI spectroscopy of 14 disks in the older (~5-10 Myr) Upper Scorpius (USco) association and use slab of gas in local thermal equilibrium to infer basic gas propert…

astro-ph.IM2018

ALES: Overview and Upgrades

Andrew J. Skemer, Philip Hinz, Jordan Stone +4

The Arizona Lenslets for Exoplanet Spectroscopy (ALES) is the world's first AO-fed thermal infrared integral field spectrograph, mounted inside the Large Binocular Telescope Interf…

astro-ph.HE2013

An 8 hour characteristic time-scale in submillimetre light curves of Sagittarius A*

Jason Dexter, Brandon Kelly, Geoffrey C. Bower +4

We compile and analyse long term (~10 year) submillimetre (1.3, 0.87, 0.43 mm, submm) wavelength light curves of the Galactic centre black hole, Sagittarius A*. The 0.87 and 0.43 m…

astro-ph.EP2023

Direct images and spectroscopy of a giant protoplanet driving spiral arms in MWC 758

Kevin Wagner, Jordan Stone, Andrew Skemer +23

Understanding the driving forces behind spiral arms in protoplanetary disks remains a challenge due to the faintness of young giant planets. MWC 758 hosts such a protoplanetary dis…

physics.optics2023

Fourier synthesis dispersion engineering of photonic crystal microrings for broadband frequency combs

Gregory Moille, Xiyuan Lu, Jordan Stone +2

Dispersion engineering of microring resonators is crucial for optical frequency comb applications, to achieve targeted bandwidths and powers of individual comb teeth. However, conv…

astro-ph.SR2018

The TRENDS High-Contrast Imaging Survey. VII. Discovery of a Nearby Sirius-like White Dwarf System (HD 169889)

Justin R. Crepp, Erica J. Gonzales, Brendan P. Bowler +8

Monitoring the long-term radial velocity (RV) and acceleration of nearby stars has proven an effective method for directly detecting binary and substellar companions. Some fraction…

astro-ph.SR2020

First Images of the Protoplanetary Disk Around PDS 201

Kevin Wagner, Jordan Stone, Ruobing Dong +11

Scattered light imaging has revealed nearly a dozen circumstellar disks around young Herbig Ae/Be starsenabling studies of structures in the upper disk layers as potential signs…

physics.optics2022

High-performance microresonator optical parametric oscillator on a silicon chip

Edgar F. Perez, Gregory Moille, Xiyuan Lu +3

Optical parametric oscillation (OPO) is distinguished by its wavelength access, that is, the ability to flexibly generate coherent light at wavelengths that are dramatically differ…

astro-ph.IM2023

The Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy (SCALES): driving science cases and expected outcomes

Steph Sallum, Andrew Skemer, Deno Stelter +34

The Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy (SCALES) is a m, high-contrast integral field spectrograph (IFS) currently being built for Keck Observ…

astro-ph.SR2020

ELT Imaging of MWC 297 from the 23-m LBTI: Complex Disk Structure and a Companion Candidate

Steph Sallum, Josh Eisner, Jordan Stone +3

Herbig Ae/Be stars represent the early outcomes of star formation and the initial stages of planet formation at intermediate stellar masses. Understanding both of these processes r…

astro-ph.GA2016

Persistent Asymmetric Structure of Sagittarius A* on Event Horizon Scales

Vincent L. Fish, Michael D. Johnson, Sheperd S. Doeleman +69

The Galactic Center black hole Sagittarius A* (Sgr A*) is a prime observing target for the Event Horizon Telescope (EHT), which can resolve the 1.3 mm emission from this source on…

physics.optics2025

Parasitic loss in microring-waveguide coupling and its impact on wideband nonlinear photonics

Yi Sun, Daniel Pimbi, Xiyuan Lu +4

Microring resonators enable the enhancement of nonlinear frequency mixing processes, generating output fields at frequencies that widely differ from the inputs, in some cases by mo…

astro-ph.EP2025

Orbital Modeling of HII 1348B: An Eccentric Young Substellar Companion in the Pleiades

Gabriel Weible, Kevin Wagner, Jordan Stone +4

Brown dwarfs with known physical properties (e.g., age and mass) are essential for constraining models of the formation and evolution of substellar objects. We present new high-con…

astro-ph.IM2022

Design of SCALES: A 2-5 Micron Coronagraphic Integral Field Spectrograph for Keck Observatory

Andrew Skemer, R. Deno Stelter, Stephanie Sallum +49

We present the design of SCALES (Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy) a new 2-5 micron coronagraphic integral field spectrograph under construction fo…

physics.optics2026

Self-aligned optical microcomb emerging between octave separated lasers

Grégory Moille, Pradyoth Shandilya, Jordan Stone +11

Optical frequency combs (OFCs) are frequency rulers essential for precision metrology, next generation navigation, and testing of fundamental physics. Despite intense efforts, chip…

astro-ph.IM2019

Status of commissioning stabilized infrared Fizeau interferometry with LBTI

Eckhart Spalding, Phil Hinz, Katie Morzinski +5

The Large Binocular Telescope Interferometer (LBTI) has the longest baseline in the world, 22.7 m, for performing astronomical interferometry in Fizeau mode, which involves beam co…

astro-ph.IM2023

Simulating medium-spectral-resolution exoplanet characterization with SCALES angular/reference differential imaging

Aditi Desai, Stephanie E. Sallum, Ravinder Banyal +30

SCALES (Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy) is a 2 - 5 micron high-contrast lenslet-based integral field spectrograph (IFS) designed to characterize…

astro-ph.IM2018

Towards controlled Fizeau observations with the Large Binocular Telescope

Eckhart Spalding, Phil Hinz, Steve Ertel +2

The Large Binocular Telescope Interferometer (LBTI) can perform Fizeau interferometry in the focal plane, which accesses spatial information out to the LBT's full 22.7-m edge-to-ed…

physics.optics2018

Thermal and Nonlinear Dissipative-Soliton Dynamics in Kerr Microresonator Frequency Combs

Jordan Stone, Travis Briles, Tara Drake +4

We explore the dynamical response of dissipative Kerr solitons to changes in pump power and detuning and show how thermal and nonlinear processes couple these parameters to the fre…

astro-ph.IM2015

First Light with ALES: A 2-5 Micron Adaptive Optics Integral Field Spectrograph for the LBT

Andrew J. Skemer, Philip Hinz, Manny Montoya +9

Integral field spectrographs are an important technology for exoplanet imaging, due to their ability to take spectra in a high-contrast environment, and improve planet detection se…

astro-ph.IM2023

Recovering simulated planet and disk signals using SCALES aperture masking

Mackenzie Lach, Steph Sallum, Ravinder Banyal +29

The Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy (SCALES) instrument is a lenslet-based integral field spectrograph that will operate at 2 to 5 microns, imagin…

astro-ph.IM2023

The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems: Best Practices for Data Collection in Cycle 2 and Beyond

Sasha Hinkley, Beth Biller, Andrew Skemer +35

We present a set of recommended best practices for JWST data collection for members of the community focussed on the direct imaging and spectroscopy of exoplanetary systems. These…

astro-ph.SR2020

Thermal Emission in the Southwest Clump of VY CMa

Michael S. Gordon, Terry J. Jones, Roberta M. Humphreys +6

We present high spatial resolution LBTI/NOMIC images of VY CMa and its massive outflow feature, the Southwest (SW) Clump. Combined with high-resolution imaging from HS…

astro-ph.IM2021

Imaging low-mass planets within the habitable zones of nearby stars with ground-based mid-infrared imaging

Kevin Wagner, Steve Ertel, Jordan Stone +8

Giant exoplanets on 10-100 au orbits have been directly imaged around young stars. The peak of the thermal emission from these warm young planets is in the near-infrared (~1-5 micr…

physics.optics2023

Kerr-Induced Synchronization of a Cavity Soliton to an Optical Reference

Gregory Moille, Jordan Stone, Michal Chojnacky +4

The phase-coherent frequency division of a stabilized optical reference laser to the microwave domain is made possible by optical frequency combs (OFCs). Fundamentally, OFC-based c…

astro-ph.IM2026

Upgrading LBTI/NOMIC with a quadruple annular groove phase mask and GeoSnap detector for imaging nearby, habitable-zone exoplanets

Kevin Wagner, Manny Montoya, Steve Ertel +32

The paper describes two upgrades to the Large Binocular Telescope Interferometer’s NOMIC camera—a quadruple annular groove phase mask coronagraph and a new Teledyne GeoSnap detecto…

#coronagraph#mid-infrared imaging#exoplanet detection#interferometry
physics.soc-ph2025

The Probability of Vacuum Metastability and Artificial Vacuum Decay: Expert Survey Results

Jordan Stone, Youssef Saleh, Darryl Wright +1

Vacuum decay posits that the universe's apparent vacuum is metastable and could transition to a lower-energy state. According to current physics models, if such a transition occurr…

physics.optics2025

All-Optical Azimuthal Trapping of Dissipative Kerr Multi-Solitons for Relative Noise Suppression

Pradyoth Shandilya, Shao-Chien Ou, Jordan Stone +4

Temporal cavity solitons, or dissipative Kerr solitons (DKS) in integrated microresonators, are essential for deployable metrology technologies. Such applications favor the lowest…

physics.optics2024

On-chip Kerr parametric oscillation with integrated heating for enhanced frequency tuning and control

Jordan Stone, Daron Westly, Gregory Moille +1

Nonlinear microresonators can convert light from chip-integrated sources into new wavelengths within the visible and near-infrared spectrum. For most applications, such as the inte…

astro-ph.EP2020

On the Chemical Abundance of HR 8799 and the Planet c

Ji Wang, Jason Wang, Bo Ma +10

Comparing chemical abundances of a planet and the host star reveals the origin and formation path. Stellar abundance is measured with high-resolution spectroscopy. Planet abundance…

physics.app-ph2017

An Integrated-Photonics Optical-Frequency Synthesizer

Daryl T. Spencer, Tara Drake, Travis C. Briles +24

Integrated-photonics microchips now enable a range of advanced functionalities for high-coherence applications such as data transmission, highly optimized physical sensors, and har…