activity
20092026
most citedCharacterization and on-sky demonstration of an integrated photonic spectrograph for astronomy

87 citations · 974 across the 46 of their papers we have counts for

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40 papers · 1 filter

astro-ph.IM2026

Pushing high angular resolution and high contrast observations on the VLTI from Y to L band with the Asgard instrumental suite: integration status and plans

Marc-Antoine Martinod, Michael J. Ireland, Denis Defrère +39

ESO's VLTI has a history of record-breaking discoveries in astrophysics using high-angular resolution instrumentation. Its latest visitor instrument, the Asgard instrumental suite,…

astro-ph.IM2026

Silencing the stellar glare with kernel-nulling and active phase control on photonic chips

Marc-Antoine Martinod, Vincent Foriel, Nick Cvetojevic +4

Characterizing exoplanets and finding biosignatures are among the hottest topics in astronomy. This quest is challenged by the brightness contrast between the faint planet and the…

astro-ph.IM2026

Characterization and on-sky testing of photonic, AWG-based astronomical spectrographs

Jeronimo Calderon-Gomez, Frantz Martinache, Nick Cvetojevic +14

Astrophotonics is a field that intends to meet the needs of next-generation instruments at a small footprint, low cost, and high stability, compared to bulk-optics-based alternativ…

astro-ph.IM2024★ 2 cited

Photonic chip for visible interferometry: laboratory characterization and comparison with the theoretical model

Manon Lallement, Sylvestre Lacour, Elsa Huby +15

Integrated optics are used to achieve astronomical interferometry inside robust and compact materials, improving the instruments stability and sensitivity. In order to perform diff…

astro-ph.IM2024★ 5 cited

Photonic beam-combiner for visible interferometry with SCExAO/FIRST: laboratory characterization and design optimization

Manon Lallement, Elsa Huby, Sylvestre Lacour +15

Integrated optics are used to achieve astronomical interferometry inside robust and compact materials, improving the instrument's stability and sensitivity. In order to perform dif…

astro-ph.IM2024★ 2 cited

Pushing high angular resolution and high contrast observations on the VLTI from Y to L band with the Asgard instrumental suite: integration status and plans

Marc-Antoine Martinod, Denis Defrère, Michael J. Ireland +35

ESO's Very Large Telescope Interferometer has a history of record-breaking discoveries in astrophysics and significant advances in instrumentation. The next leap forward is its new…

astro-ph.IM2024★ 1 cited

L-band nulling interferometry at the VLTI with Asgard/NOTT: status and plans

Denis Defrère, Romain Laugier, Marc-Antoine Martinod +43

NOTT (formerly Hi-5) is the L'-band (3.5-4.0~microns) nulling interferometer of Asgard, an instrument suite in preparation for the VLTI visitor focus. The primary scientific object…

astro-ph.IM2024★ 15 cited

Heimdallr, Baldr and Solarstein: designing the next generation of VLTI instruments in the Asgard suite

Adam K. Taras, J. Gordon Robertson, Fatme Allouche +11

High angular resolution imaging is an increasingly important capability in contemporary astrophysics. Of particular relevance to emerging fields such as the characterisation of exo…

astro-ph.IM2023★ 50 cited

2023 Astrophotonics Roadmap: pathways to realizing multi-functional integrated astrophotonic instruments

Nemanja Jovanovic, Pradip Gatkine, Narsireddy Anugu +77

Photonics offer numerous functionalities that can be used to realize astrophotonic instruments. The most spectacular example to date is the ESO Gravity instrument at the Very Large…

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.IM2023★ 5 cited

Single-aperture spectro-interferometry in the visible at the Subaru telescope with FIRST: First on-sky demonstration on Keho'oea (α Lyrae) and Hokulei (α Aurigae)

Sébastien Vievard, Elsa Huby, Sylvestre Lacour +20

FIRST is a spectro-interferometer combining, in the visible, the techniques of aperture masking and spatial filtering thanks to single-mode fibers. This instrument aims to deliver…

astro-ph.IM2023★ 4 cited

High-contrast detection of exoplanets with a kernel-nuller at the VLTI

Peter Marley Chingaipe, Frantz Martinache, Nick Cvetojevic +5

Context: The conventional approach to direct imaging has been the use of a single aperture coronagraph with wavefront correction via extreme adaptive optics. Such systems are limit…

astro-ph.IM2023★ 1 cited

High-angular resolution and high-contrast VLTI observations from Y to L band with the Asgard instrumental suite

Marc-Antoine Martinod, Denis Defrère, Michael Ireland +17

The Very Large Telescope Interferometer is one of the most proficient observatories in the world for high angular resolution. Since its first observations, it has hosted several in…

astro-ph.IM2022★ 2 cited

An all-photonic, dynamic device for flattening the spectrum of a laser frequency comb for precise calibration of radial velocity measurements

Nemanja Jovanovic, Pradip Gatkine, Boqiang Shen +9

Laser frequency combs are fast becoming critical to reaching the highest radial velocity precisions. One shortcoming is the highly variable brightness of the comb lines across the…

astro-ph.IM2022★ 1 cited

Controlling petals using fringes: discontinuous wavefront sensing through sparse aperture interferometry at Subaru/SCExAO

Vincent Deo, Sébastien Vievard, Nick Cvetojevic +9

Low wind and petaling effects, caused by the discontinuous apertures of telescopes, are poorly corrected -- if at all -- by commonly used workhorse wavefront sensors (WFSs). Wavefr…

astro-ph.IM2022

Statistical tests with multi-wavelength Kernel-phase analysis for the detection and characterization of planetary companions

Mamadou N'Diaye, David Mary, Frantz Martinache +4

Kernel phase is a method to interpret stellar point source images by considering their formation as the analytical result of an interferometric process. Using Fourier formalism, th…

astro-ph.IM2022★ 2 cited

3-beam self-calibrated Kernel nulling photonic interferometer

Nick Cvetojevic, Frantz Martinache, Peter Chingaipe +6

The use of interferometric nulling for the direct characterization of extrasolar planets is an exciting prospect, but one that faces many practical challenges when deployed on tele…

astro-ph.IM2021★ 11 cited

Building hybridized 28-baseline pupil-remapping photonic interferometers for future high resolution imaging

Nick Cvetojevic, Barnaby R. M. Norris, Simon Gross +7

One key advantage of single-mode photonic technologies for interferometric use is their ability to easily scale to an ever increasing number of inputs without a major increase in t…

astro-ph.IM2020★ 1 cited

FIRST, a Pupil-Remapping Fiber Interferometer at the Subaru Telescope: on-sky results

Sébastien Vievard, Elsa Huby, Sylvestre Lacour +13

FIRST, the Fibered Imager foR a Single Telescope, is a spectro-imager using single-mode fibers for pupil remapping, allowing measurements beyond the telescope diffraction limit. In…

astro-ph.IM2020★ 5 cited

Capabilities of a fibered imager on an extremely large telescope

Sebastien Vievard, Nick Cvetojevic, Elsa Huby +11

FIRST, the Fibered Imager foR a Single Telescope instrument, is an ultra-high angular resolution spectro-imager, able to deliver calibrated images and measurements beyond the teles…

astro-ph.IM2020★ 12 cited

Kernel nullers for an arbitrary number of apertures

Romain Laugier, Nick Cvetojevic, Frantz Martinache

The use of interferometric nulling for the direct detection of extrasolar planets is in part limited by the extreme sensitivity of the instrumental response to tiny optical path di…

astro-ph.IM2020★ 10 cited

Astronomical Applications of Multi-Core Fiber Technology

Nemanja Jovanovic, Robert J. Harris, Nick Cvetojevic

Optical fibers have altered astronomical instrument design by allowing for a complex, often large instrument to be mounted in a remote and stable location with respect to the teles…

astro-ph.IM2020★ 7 cited

Angular differential kernel phases

Romain Laugier, Frantz Martinache, Nick Cvetojevic +7

To reach its optimal performance, Fizeau interferometry requires that we work to resolve instrumental biases through calibration. One common technique used in high contrast imaging…