activity
20202026
most citedDetermination of the Local Hubble Constant from Virgo Infall Using TRGB Distances

32 citations · 111 across the 25 of their papers we have counts for

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Showing astro-ph.IMShow all

23 papers · 1 filter

astro-ph.IM2026

The Photonic Lantern Nuller: from concept to laboratory and on-sky demonstrations

Yinzi Xin, Nemanja Jovanovic, Dimitri Mawet +18

This thesis work presents the conceptual design and experimental characterization of the Photonic Lantern Nuller instrument, which uses a multimode-to-single-mode demultiplexing wa…

astro-ph.IM2026

Instrumental artifacts in photonic lantern spectroastrometry and their mitigation with PLred

Yoo Jung Kim, Michael P. Fitzgerald, Malena Bloom +10

Spectroastrometry is a powerful spectral-differential technique for probing angular scales below the resolution limit, but it is also well known to be susceptible to instrumental a…

astro-ph.IM2026

FIRST-PL: Commissioning the first visible photonic lantern spectrograph for sub-diffraction-limit astronomy on Subaru/SCExAO

Sebastien Vievard, Elsa Huby, Sylvestre Lacour +18

FIRST-PL (Fibered Imager foR a Single Telescope - Photonic Lantern) is a newly commissioned visible-light instrument on Subaru/SCExAO achieving spectroscopy below the diffraction l…

astro-ph.IM2026

Tricouplers for nulling interferometry with photonic integrated circuits

Anusha Pai Asnodkar, Nemanja Jovanovic, Harry-Dean Kenchington Goldsmith +7

Solar System analog gas giants and habitable-zone terrestrial planets are observationally elusive to conventional exoplanet detection and characterization techniques, i.e. transits…

astro-ph.IM2026

Technologies and novel components for broadband splitting and coupling in pairwise and nulling interferometry

Harry-Dean Kenchington Goldsmith, Nemanja Jovanovic, Anusha Pai Asnodkar +9

Passive and active photonic components are central to the continued development of astronomical photonic integrated circuits (PICs), although achieving broadband achromatic perform…

astro-ph.IM2026

Quantum-optimal coronagraphy with spatial mode sorting for direct exoplanet observations

Yinzi Xin, Sebastiaan Haffert, Yoo Jung Kim +1

Conventional coronagraphs struggle to reach the theoretical limit of exoplanet detection at close separations to the star, particularly when the telescope has a complex aperture or…

astro-ph.IM2026

Experimentally-determined performance limits for joint imaging and wavefront sensing with a photonic lantern

Aditya R. Sengupta, Vincent Chambouleyron, Rebecca Jensen-Clem +16

The photonic lantern (PL) is a focal-plane wavefront sensor (WFS) that can be used for second-stage control of extreme adaptive optics (AO) systems. While the number of sensed mode…

astro-ph.IM2026

Combining spectroscopy and wavefront control at deep contrast with photonic lanterns

Mona El Morsy, Olivier Guyon, Barnaby Norris +7

HWO aims to directly image objects orbiting Sun-like stars, using a 6-m telescope capable of high-contrast imaging () and spectroscopy to search for biosignatures in plan…

astro-ph.IM2026

Tri-coupler geometries for achromatic nulling interferometry in the near-infrared

Harry-Dean Kenchington Goldsmith, Nemanja Jovanovic, Anusha Pai Asnodkar +4

Astrophotonics is central to the next generation of astronomical instrumentation, enabling compact photonic integrated circuits for both ground-based observatories and future space…

astro-ph.IM2025★ 2 cited

On-sky Demonstration of Subdiffraction-limited Astronomical Measurement Using a Photonic Lantern

Yoo Jung Kim, Michael P. Fitzgerald, Sébastien Vievard +18

Resolving fine details of astronomical objects provides critical insights into their underlying physical processes. This drives in part the desire to construct ever-larger telescop…

astro-ph.IM2025

Implicit Electric Field Conjugation with the Photonic Lantern Nuller

Yinzi Xin, Daniel Echeverri, Nemanja Jovanovic +12

The Photonic Lantern Nuller (PLN) is an instrument concept designed to characterize exoplanets within a single beam-width from its host star. The PLN leverages the spatial symmetry…

astro-ph.IM2024

Spectral characterization of a 3-port photonic lantern for application to spectroastrometry

Yoo Jung Kim, Michael P. Fitzgerald, Jonathan Lin +10

Spectroastrometry, which measures wavelength-dependent shifts in the center of light, is well-suited for studying objects whose morphology changes with wavelength at very high angu…

astro-ph.IM2024

On the Potential of Spectroastrometry with Photonic Lanterns

Yoo Jung Kim, Michael P. Fitzgerald, Jonathan Lin +5

We investigate the potential of photonic lantern (PL) fiber fed spectrometers for two-dimensional spectroastrometry. Spectroastrometry, a technique for studying small angular scale…

astro-ph.IM2024★ 4 cited

Spectroscopy using a visible photonic lantern at the Subaru telescope: Laboratory characterization and first on-sky demonstration on Ikiiki (α Leo) and `Aua (α Ori)

Sébastien Vievard, Manon Lallement, Sergio Leon-Saval +23

Photonic lanterns are waveguide devices enabling high throughput single mode spectroscopy and high angular resolution. We aim to present the first on-sky demonstration of a photoni…

astro-ph.IM2024

Visible Photonic Lantern integration, characterization and on-sky testing on Subaru/SCExAO

Sébastien Vievard, Manon Lallement, Sergio Leon-Saval +23

A Photonic Lantern (PL) is a novel device that efficiently converts a multi-mode fiber into several single-mode fibers. When coupled with an extreme adaptive optics (ExAO) system a…

astro-ph.IM2024★ 5 cited

Laboratory demonstration of a Photonic Lantern Nuller in monochromatic and broadband light

Yinzi Xin, Daniel Echeverri, Nemanja Jovanovic +11

Photonic lantern nulling (PLN) is a method for enabling the detection and characterization of close-in exoplanets by exploiting the symmetries of the ports of a mode-selective phot…

astro-ph.IM2024

Coherent Imaging with Photonic Lanterns

Yoo Jung Kim, Michael P. Fitzgerald, Jonathan Lin +4

Photonic Lanterns (PLs) are tapered waveguides that gradually transition from a multi-mode fiber geometry to a bundle of single-mode fibers (SMFs). They can efficiently couple mult…

astro-ph.IM2023

Real-time experimental demonstrations of a photonic lantern wavefront sensor

Jonathan W. Lin, Michael P. Fitzgerald, Yinzi Xin +12

The direct imaging of an Earth-like exoplanet will require sub-nanometric wavefront control across large light-collecting apertures, to reject host starlight and detect the faint p…

astro-ph.IM2023

Spectroastrometry and Imaging Science with Photonic Lanterns on Extremely Large Telescopes

Yoo Jung Kim, Michael P. Fitzgerald, Jonathan Lin +11

Photonic lanterns (PLs) are tapered waveguides that gradually transition from a multi-mode fiber geometry to a bundle of single-mode fibers. In astronomical applications, PLs can e…

astro-ph.IM2023

Focal-plane wavefront sensing with photonic lanterns II: numerical characterization and optimization

Jonathan Lin, Michael P. Fitzgerald, Yinzi Xin +5

We present numerical characterizations of the wavefront sensing performance for few-mode photonic lantern wavefront sensors (PLWFSs). These characterizations include calculations o…

astro-ph.IM2023

The path to detecting extraterrestrial life with astrophotonics

Nemanja Jovanovic, Yinzi Xin, Michael P. Fitzgerald +20

Astrophysical research into exoplanets has delivered thousands of confirmed planets orbiting distant stars. These planets span a wide ranges of size and composition, with diversity…

astro-ph.IM2023

Photonic spectro-interferometry with SCExAO/FIRST at the Subaru Telescope: towards H-alpha imaging of protoplanets

Sébastien Vievard, Manon Lallement, Elsa Huby +27

FIRST is a post Extreme Adaptive-Optics (ExAO) spectro-interferometer operating in the Visible (600-800 nm, R~400). Its exquisite angular resolution (a sensitivity analysis of on-s…

astro-ph.IM2022★ 22 cited

Efficient detection and characterization of exoplanets within the diffraction limit: nulling with a mode-selective photonic lantern

Yinzi Xin, Nemanja Jovanovic, Garreth Ruane +9

Coronagraphs allow for faint off-axis exoplanets to be observed, but are limited to angular separations greater than a few beam widths. Accessing closer-in separations would greatl…