Astrophotonics -- current capabilities and the road ahead
arXiv:2408.15541 · doi:10.1364/AO.517018
Abstract
Astrophotonics represents a cutting-edge approach in observational astronomy. This paper explores the significant advancements and potential applications of astrophotonics, highlighting how photonic technologies stand to revolutionise astronomical instrumentation. Key areas of focus include photonic wavefront sensing and imaging, photonic interferometry and nulling, advanced chip fabrication methods, and the integration of spectroscopy and sensing onto photonic chips. The role of single-mode fibres in reducing modal noise, and the development of photonic integral field units (IFUs) and arrayed waveguide gratings (AWGs) for high-resolution, spatially resolved spectroscopy will be examined. As part of the Sydney regional-focus issue, this review aims to detail some of the current technological achievements in this field as well as to discuss the future trajectory of astrophotonics, underscoring its potential to unlock important new astronomical discoveries.
Published version available at https://opg.optica.org/ao/fulltext.cfm?uri=ao-63-24-6393&id=554618
References in corpus (84)
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
- First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer
- The Sydney-AAO Multi-object Integral field spectrograph (SAMI)
- First Results from the CHARA Array. II. A Description of the Instrument
- The SAMI Galaxy Survey: instrument specification and target selection
- The Subaru Coronagraphic Extreme Adaptive Optics system: enabling high-contrast imaging on solar-system scales
- The Photonic Lantern
- The Anglo-Australian Observatory's 2dF Facility
- Adaptive Optics for Astronomy
- Limits of Adaptive Optics for high contrast imaging
- Optical Interferometry in Astronomy
- The DESI Experiment Part II: Instrument Design
- Wavelength-scale stationary-wave integrated Fourier-transform spectrometry
- Optical Interferometry with Quantum Networks
- Low bend loss waveguides enable compact, efficient 3D photonic chips
- Michelson Interferometry with the Keck I Telescope
- Photonic Lantern
- Focal ratio degradation in lightly-fused hexabundles
- A superconducting focal plane array for ultraviolet, optical, and near-infrared astrophysics
- An integrated optics beam combiner for the second generation VLTI instruments
- Calibration and Pre-Compensation of Non-Common Path Aberrations for extreme Adaptive Optics
- Integrated optics for astronomical interferometry. I. Concept and astronomical applications
- Arrayed Waveguide Grating Spectrometers for Astronomical Applications: New Results
- On-sky speckle nulling demonstration at small angular separation with SCExAO
- Ultrafast laser inscription: an enabling technology for astrophotonics
- Characterization and on-sky demonstration of an integrated photonic spectrograph for astronomy
- GNOSIS: the first instrument to use fibre Bragg gratings for OH suppression
- Efficient injection from large telescopes into single-mode fibres: Enabling the era of ultra-precision astronomy
- The case for OH suppression at near-infrared wavelengths
- An all-photonic focal-plane wavefront sensor
- Symmetric polarization insensitive directional couplers fabricated by femtosecond laser waveguide writing
- The Asymmetric Pupil Fourier Wavefront Sensor
- First on-sky demonstration of an integrated-photonic nulling-interferometer: The GLINT instrument
- Starlight Demonstration of the Dragonfly Instrument: an Integrated Photonic Pupil Remapping Interferometer for High Contrast Imaging
- Developing arrayed waveguide grating spectrographs for multi-object astronomical spectroscopy
- Nulling Data Reduction and On-Sky Performance of the Large Binocular Telescope Interferometer
- Integrated photonic building blocks for next-generation astronomical instrumentation II: the multimode to single mode transition
- The MKID Exoplanet Camera for Subaru SCExAO
- Suppression of the near-infrared OH night sky lines with fibre Bragg gratings - first results
- 2023 Astrophotonics Roadmap: pathways to realizing multi-functional integrated astrophotonic instruments
- FIRST, a fibered aperture masking instrument. I. First on-sky test results
- Characterization of hexabundles: Initial results
- Integrated photonic building blocks for next-generation astronomical instrumentation I: the multimode waveguide
- Instruments without optics: an integrated photonic spectrograph
- Spectrographs for astrophotonics
- Efficient spectroscopy of exoplanets at small angular separations with vortex fiber nulling
- First demonstration of OH suppression in a high efficiency near-infrared spectrograph
- iLocater: A Diffraction-limited Doppler Spectrometer for the Large Binocular Telescope
- Fast & Furious focal-plane wavefront sensing
- Beating the classical limit: A diffraction-limited spectrograph for an arbitrary input beam
- Calibration of the island effect: Experimental validation of closed-loop focal plane wavefront control on Subaru/SCExAO
- High-performance 3D waveguide architecture for astronomical pupil-remapping interferometry
- Focal-plane wavefront sensing with photonic lanterns I: theoretical framework
- The Photonic TIGER: a multicore fiber-fed spectrograph
- Geometrically-controlled polarisation processing in an integrated photonic platform
- Asgard/NOTT: L-band nulling interferometry at the VLTI I. Simulating the expected high-contrast performance
- Space qualification of ultrafast laser written integrated waveguide optics
- Design of Optically Path Length Matched, Three-Dimensional Photonic Circuits Comprising Uniquely Routed Waveguides
- Potential of commercial SiN MPW platforms for developing mid/high-resolution integrated photonic spectrographs for astronomy
- Efficient detection and characterization of exoplanets within the diffraction limit: nulling with a mode-selective photonic lantern
- Low Wind Effect on VLT/SPHERE : impact, mitigation strategy, and results
- Photonic ring resonator filters for astronomical OH suppression
- Modal noise in an integrated photonic lantern fed diffraction-limited spectrograph
- Achromatic photonic tricouplers for application in nulling interferometry
- Characterizing Vibrations at the Subaru Telescope for the Subaru Coronagraphic Extreme Adaptive Optics instrument
- Design considerations of photonic lanterns for diffraction-limited spectrometry
- Final Design and On-Sky Testing of the iLocater SX Acquisition Camera: Broadband Single-Mode Fiber Coupling
- Quantum-Assisted Optical Interferometers: Instrument Requirements
- Achromatic design of a photonic tricoupler and phase shifter for broadband nulling interferometry
- Compact high-resolution spectrographs for large and extremely large telescopes: using the diffraction limit
- Design, simulation and characterization of integrated photonic spectrographs for Astronomy II: Low-aberration Generation-II AWG devices with three stigmatic points
- On the possibility of observable signatures of leptonium from astrophysical sources
- Vortex Fiber Nulling for Exoplanet Observations: Implementation and First Light
- Building hybridized 28-baseline pupil-remapping photonic interferometers for future high resolution imaging
- All-fiber photonic lantern multimode optical receiver with coherent adaptive optics beam combining
- Integrated Arbitrary Filter with Spiral Gratings: Design and Characterization
- Exploring intermediate (5-40AU) scales around AB Aurigae with the Palomar Fiber Nuller
- Astrophysical signatures of leptonium
- Learning the Lantern: Neural network applications to broadband photonic lantern modelling
- 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)
- Photonic beam-combiner for visible interferometry with SCExAO/FIRST: laboratory characterization and design optimization
- Polarization analysis of the VLTI and GRAVITY
- Astrophotonics: recent and future developments