Astrophotonics: astronomy and modern optics
arXiv:2003.12485 · doi:10.1007/s00159-021-00134-7
Abstract
Much of the progress in Astronomy has been driven by instrumental developments, from the first telescopes to fiber fed spectrographs. In this review we describe the field of astrophotonics, a combination of photonics and astronomical instrumentation that has the potential to drive the next generation of developements. We begin with the science cases that have been identified as possibly benefiting from astrophotonic devices. We then discuss devices, methods and developments in the field along with the advantages they provide. We conclude by describing possible future developments in the field and their influence on astronomy.
arXiv comment99 pages, 7 figures - Invited review article for The Astronomy and Astrophysics Review. Submitted on 9 Nov 2018, Resubmission 8 Nov 2020
References in corpus (172)
- The Sloan Digital Sky Survey: Technical Summary
- Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant
- Temporal solitons in optical microresonators
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- A terrestrial planet candidate in a temperate orbit around Proxima Centauri
- Closest Star Seen Orbiting the Supermassive Black Hole at the Centre of the Milky Way
- The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
- The MUSE second-generation VLT instrument
- Optical Images of an Exosolar Planet 25 Light Years from Earth
- Possible Gravitational Microlensing of a Star in the Large Magellanic Cloud
- Universal Dynamics of Kerr Frequency Comb Formation in Microresonators
- A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
- The SAURON project. I. The panoramic integral-field spectrograph
- Southern Massive Stars at High Angular Resolution: Observational Campaign and Companion Detection
- First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer
- A probable giant planet imaged in the Beta Pictoris disk
- The Sydney-AAO Multi-object Integral field spectrograph (SAMI)
- Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole
- The SAMI Galaxy Survey: instrument specification and target selection
- Relativistic redshift of the star S0-2 orbiting the Galactic center supermassive black hole
- An Update on Monitoring Stellar Orbits in the Galactic Center
- The Subaru Coronagraphic Extreme Adaptive Optics system: enabling high-contrast imaging on solar-system scales
- A planetary system as the origin of structure in Fomalhaut's dust belt
- The Photonic Lantern
- PIONIER: a 4-telescope visitor instrument at VLTI
- Theoretical Limits on Extrasolar Terrestrial Planet Detection with Coronagraphs
- Imaging the Surface of Altair
- LkCa 15: A Young Exoplanet Caught at Formation?
- Asymmetric features in the protoplanetary disk MWC758
- HST/NICMOS Imaging of Disks and Envelopes Around Very Young Stars
- Searching for Exoplanets Using a Microresonator Astrocomb
- The Palomar Testbed Interferometer
- ISO spectroscopy of gas and dust: from molecular clouds to protoplanetary disks
- Combining high-dispersion spectroscopy (HDS) with high contrast imaging (HCI): Probing rocky planets around our nearest neighbors
- Spectro-astrometric imaging of molecular gas within protoplanetary disk gaps
- On the Interferometric Sizes of Young Stellar Objects
- Wavelength-scale stationary-wave integrated Fourier-transform spectrometry
- ROTSE All Sky Surveys for Variable Stars I: Test Fields
- Phase-Induced Amplitude Apodization of Telescope Pupils for Extrasolar Terrestrial Planet Imaging
- Near-Infrared Spectroscopy of the Extrasolar Planet HR 8799 b
- Performance of AAOmega: the AAT multi-purpose fibre-fed spectrograph
- The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)
- Optical Vectorial Vortex Coronagraphs using Liquid Crystal Polymers: theory, manufacturing and laboratory demonstration
- Self-aligning universal beam coupler
- PALM-3000: Exoplanet Adaptive Optics for the 5-meter Hale Telescope
- Ices in the edge-on disk CRBR 2422.8-3423: Spitzer spectroscopy and Monte Carlo radiative transfer modeling
- Structure of Herbig AeBe disks at the milliarcsecond scale A statistical survey in the H band using PIONIER-VLTI
- The Vector Vortex Coronagraph: Laboratory Results and First Light at Palomar Observatory
- Three-dimensional mid-infrared photonic circuits in chalcogenide glass
- EXPRES: A Next Generation RV Spectrograph in the Search for Earth-like Worlds
- First light of the VLT planet finder SPHERE. IV. Physical and chemical properties of the planets around HR8799
- Review of small-angle coronagraphic techniques in the wake of ground-based second-generation adaptive optics systems
- Taking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest
- In the Shadow of the Transiting Disk: Imaging epsilon Aurigae in Eclipse
- SOPHIE+: First results of an octagonal-section fiber for high-precision radial velocity measurements
- A VLT/NACO Survey for Triple and Quadruple Systems among Visual Pre-Main Sequence Binaries
- A complex multi-notch astronomical filter to suppress the bright infrared sky
- SPIRou: the near-infrared spectropolarimeter/high-precision velocimeter for the Canada-France-Hawaii telescope
- Spatially resolved spectroscopy of the exoplanet HR 8799 c
- An integrated optics beam combiner for the second generation VLTI instruments
- Astrophotonics: a new era for astronomical instruments
- The HOSTS survey for exozodiacal dust: Observational results from the complete survey
- Integrated optics for astronomical interferometry. I. Concept and astronomical applications
- Exo--Zodiacal Dust Levels for Nearby Main Sequence Stars
- Medium-resolution integral-field spectroscopy for high-contrast exoplanet imaging: Molecule maps of the Pictoris system with SINFONI
- High-Contrast Observations in Optical and Infrared Astronomy
- Circumstellar structure of RU Lupi down to au scales
- No Sun-like dynamo on the active star Andromedae from starspot asymmetry
- Interferometer Observations of Subparsec-scale Infrared Emission in the Nucleus of NGC 4151
- Arrayed Waveguide Grating Spectrometers for Astronomical Applications: New Results
- A near-infrared interferometric survey of debris-disc stars. IV. An unbiased sample of 92 southern stars observed in H-band with VLTI/PIONIER
- The All Sky Automated Survey
- Imaging the spinning gas and dust in the disc around the supergiant A[e] star HD62623
- Ultrafast Laser Inscription of a 121-Waveguide Fan-Out for Astrophotonics
- Mid-infrared guided optics: a perspective for astronomical instruments
- 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
- Inner Rim of A Molecular Disk Spatially Resolved in Infrared CO Emission Lines
- A dust-parallax distance of 19 megaparsecs to the supermassive black hole in NGC 4151
- Demonstration of a Near-IR Laser Comb for Precision Radial Velocity Measurements in Astronomy
- The W. M. Keck Observatory infrared vortex coronagraph and a first image of HIP79124 B
- Ring-apodized vortex coronagraphs for obscured telescopes. I. Transmissive ring apodizers
- Panchromatic observations and modeling of the HV Tau C edge-on disk
- L'-band AGPM vector vortex coronagraph's first light on VLT/NACO: Discovery of a late-type companion at two beamwidths from an F0V star
- First on-sky demonstration of an integrated-photonic nulling-interferometer: The GLINT instrument
- Developing arrayed waveguide grating spectrographs for multi-object astronomical spectroscopy
- Starlight Demonstration of the Dragonfly Instrument: an Integrated Photonic Pupil Remapping Interferometer for High Contrast Imaging
- 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
- A Frequency Comb calibrated Solar Atlas
- Photonic spatial reformatting of stellar light for diffraction-limited spectroscopy
- Improving Interferometric Null Depth Measurements using Statistical Distributions: Theory and First Results with the Palomar Fiber Nuller
- Optical vortex coronagraphs on ground-based telescopes
- Discovery of an Optically Thick, Edge-on Disk around the Herbig Ae star PDS 144N
- Laboratory demonstration of a mid-infrared AGPM vector vortex coronagraph
- Coronagraphic Low Order Wavefront Sensor: Principle and Application to a Phase-Induced Amplitude Coronagraph
- First-light LBT nulling interferometric observations: warm exozodiacal dust resolved within a few AU of eta Corvi
- A 2MASS Survey for Brown Dwarfs Towards the Hyades
- High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)
- Vigorous atmospheric motion in the red supergiant star Antares
- Theia: Faint objects in motion or the new astrometry frontier
- Characterization of hexabundles: Initial results
- FIRST, a fibered aperture masking instrument. I. First on-sky test results
- Integrated optics for astronomical interferometry. II. First laboratory white-light interferograms
- Multiband processing of multimode light: combining 3D photonic lanterns with waveguide Bragg gratings
- Astrointerferometry with discrete optics
- An infrared integrated optic astronomical beam combiner for stellar interferometry at 3-4 microns
- On-sky performance of the QACITS pointing control technique with the Keck/NIRC2 vortex coronagraph
- Instruments without optics: an integrated photonic spectrograph
- Simulating the Exoplanet Yield of a Space-based MIR Interferometer Based on Kepler Statistics
- VLTI monitoring of the dust formation event of the Nova V1280 Sco
- Extreme adaptive optics imaging with a clear and well-corrected off-axis telescope sub-aperture
- Demonstration of an efficient, photonic-based astronomical spectrograph on an 8-m telescope
- iLocater: A Diffraction-limited Doppler Spectrometer for the Large Binocular Telescope
- Integrated optics prototype beam combiner for long baseline interferometry in the L and M bands
- First demonstration of OH suppression in a high efficiency near-infrared spectrograph
- Modal noise prediction in fibre-spectroscopy I: Visibility and the coherent model
- The Infrared Imaging Spectrograph (IRIS) for TMT: Instrument Overview
- Gliese 49: Activity evolution and detection of a super-Earth
- Discovery of an extended debris disk around the F2V star HD 15745
- Optimizing the subwavelength grating of L-band Annular Groove Phase Masks for high coronagraphic performance
- High-performance 3D waveguide architecture for astronomical pupil-remapping interferometry
- Conceptual Design of the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS) for the Subaru Telescope
- The Photonic TIGER: a multicore fiber-fed spectrograph
- Milli-arcsecond images of the Herbig Ae star HD 163296
- Astrophotonics: molding the flow of light in astronomical instruments
- 'Modal-noise' in single-mode fibers: A cautionary note for high precision radial velocity instruments
- The Infrared Imaging Spectrograph (IRIS) for TMT: Instrument Overview
- Design of Optically Path Length Matched, Three-Dimensional Photonic Circuits Comprising Uniquely Routed Waveguides
- ARGOS at the LBT. Binocular laser guided ground layer adaptive optics
- Rugate filters for OH-suppressed imaging at near-infrared wavelengths
- Fabrication tolerant chalcogenide mid-infrared multimode interference coupler design with application for Bracewell nulling interferometry
- Efficient photonic reformatting of celestial light for diffraction-limited spectroscopy
- Applications of Integrated Photonic Spectrographs in Astronomy
- Generation of optical frequency combs via four-wave mixing processes for low- and medium-resolution astronomy
- Modal noise in an integrated photonic lantern fed diffraction-limited spectrograph
- Phase-Induced Amplitude Apodization on centrally obscured pupils: design and first laboratory demonstration for the Subaru Telescope pupil
- First fringes with an integrated-optics beam combiner at 10 um - A new step towards instrument miniaturization for mid-infrared interferometry
- Photonic ring resonator filters for astronomical OH suppression
- A detector interferometric calibration experiment for high precision astrometry
- High Contrast Imaging in the Visible: First Experimental Results at the Large Binocular Telescope
- FIRST, a fibered aperture masking instrument II. Spectroscopy of the Capella binary system at the diffraction limit
- Three years of SPHERE: the latest view of the morphology and evolution of protoplanetary discs
- Can stellar activity make a planet seem misaligned?
- Diffraction-limited integral-field spectroscopy for extreme adaptive optics systems with the Multi-Core fiber-fed Integral-Field Unit
- Micro-lens array as tip-tilt sensor for single-mode fiber coupling
- Technology challenges for space interferometry: the option of mid-infrared integrated optics
- Development of a New, Precise Near-infrared Doppler Wavelength Reference: A Fiber Fabry-Perot Interferometer
- Development of integrated mode reformatting components for diffraction-limited spectroscopy
- PRAXIS: a low background NIR spectrograph for fibre Bragg grating OH suppression
- Mid-infrared laser light nulling experiment using single-mode conductive waveguides
- Beam combination schemes and technologies for the Planet Formation Imager (PFI)
- Development of high resolution arrayed waveguide grating spectrometers for astronomical applications: first results
- High dynamic range imaging with a single-mode pupil remapping system : a self-calibration algorithm for redundant interferometric arrays
- The ESPRI project: astrometric exoplanet search with PRIMA I. Instrument description and performance of first light observations
- On-chip spectro-detection for fully integrated coherent beam combiners
- Multicore fibre photonic lanterns for precision radial velocity science
- Photonic Technologies for a Pupil Remapping Interferometer
- Spatially resolved H2 emission from the disk around T Tau N
- Vortex-phase filtering technique for extracting spatial information from unresolved sources
- Preliminary results on the characterization and performances of ZBLAN fiber for infrared spectrographs
- The spatial extent of Polycyclic Aromatic Hydrocarbons emission in the Herbig star HD 179218
- Infrared Interferometry and AGNs: Parsec-scale Disks and Dusty Outflows
- A Broadband Scalar Vortex Coronagraph
- The metrology system of the VLTI instrument GRAVITY
- AGILIS: Agile Guided Interferometer for Longbaseline Imaging Synthesis - Demonstration and concepts of reconfigurable optical imaging interferometers
- Chalcogenide glass planar MIR couplers for future chip based Bracewell interferometers
- Science Requirements and Trade-offs for the MOSAIC Instrument for the European ELT
- Photonics-based mid-infrared interferometry: 4-year results of the ALSI project and future prospects
- Strategies for spectroscopy on Extremely Large Telescopes. II - Diverse field spectroscopy
- CubeSats as pathfinders for planetary detection: the FIRST-S satellite