ORCID Profile
0000-0002-5606-3874
Current Organisations
The Hong Kong Polytechnic University
,
Hong Kong Polytechnic University
,
University of Sydney
Does something not look right? The information on this page has been harvested from data sources that may not be up to date. We continue to work with information providers to improve coverage and quality. To report an issue, use the Feedback Form.
In Research Link Australia (RLA), "Research Topics" refer to ANZSRC FOR and SEO codes. These topics are either sourced from ANZSRC FOR and SEO codes listed in researchers' related grants or generated by a large language model (LLM) based on their publications.
Astronomical and Space Instrumentation | Astronomical and Space Sciences | Photonics, Optoelectronics and Optical Communications | Cosmology and Extragalactic Astronomy | Photogrammetry and Remote Sensing | Optical Physics | Aerospace Engineering | Satellite, Space Vehicle and Missile Design and Testing | Polymers | Stellar Astronomy and Planetary Systems | Optical Physics Not Elsewhere Classified | Quantum Optics And Lasers
Expanding Knowledge in the Physical Sciences | Expanding Knowledge in Technology | Polymeric materials (e.g. paints) | Aerospace Equipment | Expanding Knowledge in the Environmental Sciences | Scientific Instruments | Physical sciences | Scientific instrumentation | Food Safety |
Publisher: SPIE
Date: 02-03-2020
DOI: 10.1117/12.2542848
Publisher: SPIE
Date: 22-07-2016
DOI: 10.1117/12.2234245
Publisher: The Optical Society
Date: 23-06-2017
DOI: 10.1364/OE.25.015549
Publisher: Optica Publishing Group
Date: 07-04-2010
DOI: 10.1364/OE.18.008430
Publisher: OSA
Date: 2018
Publisher: The Optical Society
Date: 16-11-2012
DOI: 10.1364/OE.20.027123
Publisher: SPIE
Date: 13-09-2012
DOI: 10.1117/12.925404
Publisher: Optica Publishing Group
Date: 2006
DOI: 10.1364/OE.14.001596
Abstract: We report smooth and broad continuum generation using a compact femtosecond Ti:Sapphire laser as a pump source and a tapered photonic crystal fibre as a nonlinear element. Spectral output is optimized for use in optical coherence tomography, providing a maximum longitudinal resolution of 1.5 microm in free space at 809 nm centre wavelength without use of additional spectral filtering.
Publisher: MyJove Corporation
Date: 20-04-2016
DOI: 10.3791/53326
Publisher: SPIE
Date: 10-07-2018
DOI: 10.1117/12.2313033
Publisher: Optica Publishing Group
Date: 04-2004
DOI: 10.1364/OL.29.000694
Abstract: Films of porous silica are deposited on the uniform waists of tapered fibers in minutes by a modified solgel dip coating method, inducing less than 0.2 dB of loss. The coated tapers are an ideal platform for realizing all-fiber devices that exploit evanescent-field interactions with the deposited porous film. As an ex le we demonstrate structural long-period gratings in which a periodic index variation in the film arises from the porosity variation produced by spatially varying exposure of the waist to a scanned CO2 laser beam. The long period grating is insensitive to temperature up to 800 degrees C.
Publisher: Institute of Electrical and Electronics Engineers (IEEE)
Date: 07-2020
Publisher: The Optical Society
Date: 06-09-2011
DOI: 10.1364/OE.19.018470
Publisher: Oxford University Press (OUP)
Date: 30-05-2011
Publisher: SPIE
Date: 22-07-2016
DOI: 10.1117/12.2231924
Publisher: IEEE
Date: 2006
Publisher: American Astronomical Society
Date: 16-01-2013
Publisher: OSA
Date: 2017
Publisher: IEEE
Date: 05-2011
Publisher: SPIE
Date: 28-09-2015
DOI: 10.1117/12.2195466
Publisher: IEEE
Date: 05-2011
Publisher: Optica Publishing Group
Date: 08-09-2022
DOI: 10.1364/OE.465639
Abstract: In astronomy and related fields there is a pressing need to efficiently inject light, transmitted through the atmosphere, into a single-mode fibre. However this is extremely difficult due to the large, rapidly changing aberrations imprinted on the light by the turbulent atmosphere. An adaptive optics system must be used, but its effectiveness is limited by non-common-path aberrations and insensitivity to certain crucial modes. Here we introduce a new concept device - the hybrid mode-selective photonic lantern - which incorporates both focal plane wavefront sensing and broadband single-mode fibre injection into a single photonic package. The fundamental mode of an input multimode fibre is directly mapped over a broad (1.5 to 1.8 μ m) bandwidth to a single-mode output fibre with minimal ( .1%) crosstalk, while all higher order modes are sent to a fast detector or spectrograph for wavefront sensing. This will enable an AO system optimised for maximum single-mode injection, sensitive to otherwise ‘blind’ modes and avoiding non-common-path wavefront-sensor aberrations.
Publisher: Optica Publishing Group
Date: 17-06-2021
DOI: 10.1364/JOSAB.423905
Abstract: Photonic devices (e.g., optical fibers, 2D waveguides) are commonly used on telescopes worldwide and have been hugely successful in terms of their scientific impact. Coupling light efficiently into photonic devices is critical because most astronomical sources generate low photon count rates at the detector, even when coupled to large telescope apertures. Recent developments in adaptive optics have helped to improve the coupling to optical fibers, although efficient coupling to single-mode fibers remains a challenge. We appraise the theoretical limits to this coupling efficiency in both diffraction limited and seeing limited conditions, and we review methods to improve coupling efficiency with a view to recent advances in astrophotonics.
Publisher: IEEE
Date: 08-2011
Publisher: Oxford University Press (OUP)
Date: 17-08-2012
Publisher: IEEE
Date: 2006
Publisher: Oxford University Press (OUP)
Date: 13-01-2015
Publisher: IEEE
Date: 12-2010
Publisher: The Optical Society
Date: 22-08-2017
DOI: 10.1364/OE.25.021159
Publisher: MDPI AG
Date: 07-05-2022
DOI: 10.3390/RS14092244
Abstract: OpenHSI is an initiative to lower the barriers of entry and bring compact pushbroom hyperspectral imaging spectrometers to a wider audience. We present an open-source optical design that can be replicated with readily available commercial-off-the-shelf components, and an open-source software platform openhsi that simplifies the process of capturing calibrated hyperspectral datacubes. Some of the features that the software stack provides include: an ISO 19115-2 metadata editor, wavelength calibration, a fast smile correction method, radiance conversion, atmospheric correction using 6SV (an open-source radiative transfer code), and empirical line calibration. A pipeline was developed to customise the desired processing and make openhsi practical for real-time use. We used the OpenHSI optical design and software stack successfully in the field and verified the performance using calibration tarpaulins. By providing all the tools needed to collect documented hyperspectral datasets, our work empowers practitioners who may not have the financial or technical capability to operate commercial hyperspectral imagers, and opens the door for applications in new problem domains.
Publisher: The Optical Society
Date: 24-02-2015
DOI: 10.1364/OE.23.005723
Publisher: Informa UK Limited
Date: 07-09-2021
Publisher: SPIE
Date: 13-09-2012
DOI: 10.1117/12.925254
Publisher: SPIE
Date: 24-09-2012
DOI: 10.1117/12.925378
Publisher: Optica Publishing Group
Date: 2005
Abstract: We investigate the guidance properties of low-contrast photonic band gap fibres. As predicted by the antiresonant reflecting optical waveguide (ARROW) picture, band gaps were observed between wavelengths where modes of the high-index rods in the cladding are cutoff. At these wavelengths, leakage from the core by coupling to higher-order modes of the rods was observed directly. The low index contrast allowed for bend loss to be investigated unlike in index-guiding fibres, anomalous "centripetal" light leakage through the inside of the bend can occur.
Publisher: IEEE
Date: 08-2011
Publisher: Institute of Electrical and Electronics Engineers (IEEE)
Date: 04-2020
Publisher: Optica Publishing Group
Date: 14-09-2022
DOI: 10.1364/JOSAB.466227
Abstract: The photonic lantern (PL) is a tapered waveguide that can efficiently couple light into multiple single-mode optical fibers. Such devices are currently being considered for a number of tasks, including the coupling of telescopes and high-resolution, fiber-fed spectrometers, coherent detection, nulling interferometry, and vortex-fiber nulling. In conjunction with these use cases, PLs can simultaneously perform low-order focal-plane wavefront sensing. In this work, we provide a mathematical framework for the analysis of a PL wavefront sensor (PLWFS), deriving linear and higher-order reconstruction models as well as metrics through which sensing performance—in both the linear and nonlinear regimes—can be quantified. This framework can be extended to account for additional optics such as beam-shaping optics and vortex masks, and can be generalized for other wavefront sensing architectures. Finally, we provide initial numerical verification of our mathematical models by simulating a six-port PLWFS. In a forthcoming companion paper (Lin and Fitzgerald), we provide a more comprehensive numerical characterization of few-port PLWFSs, and consider how the sensing properties of these devices can be controlled and optimized.
Publisher: SPIE
Date: 22-08-2012
DOI: 10.1117/12.925819
Publisher: SPIE
Date: 06-07-2018
DOI: 10.1117/12.2311898
Publisher: Springer Science and Business Media LLC
Date: 29-04-2021
DOI: 10.1038/S41467-021-22769-X
Abstract: Characterisation of exoplanets is key to understanding their formation, composition and potential for life. Nulling interferometry, combined with extreme adaptive optics, is among the most promising techniques to advance this goal. We present an integrated-optic nuller whose design is directly scalable to future science-ready interferometric nullers: the Guided-Light Interferometric Nulling Technology, deployed at the Subaru Telescope. It combines four beams and delivers spatial and spectral information. We demonstrate the capability of the instrument, achieving a null depth better than 10 −3 with a precision of 10 −4 for all baselines, in laboratory conditions with simulated seeing applied. On sky, the instrument delivered angular diameter measurements of stars that were 2.5 times smaller than the diffraction limit of the telescope. These successes pave the way for future design enhancements: scaling to more baselines, improved photonic component and handling low-order atmospheric aberration within the instrument, all of which will contribute to enhance sensitivity and precision.
Publisher: Walter de Gruyter GmbH
Date: 16-12-2013
Abstract: Multimode optical fibers have been primarily (and almost solely) used as “light pipes” in short distance telecommunications and in remote and astronomical spectroscopy. The modal properties of the multimode waveguides are rarely exploited and mostly discussed in the context of guiding light. Until recently, most photonic applications in the applied sciences have arisen from developments in telecommunications. However, the photonic lantern is one of several devices that arose to solve problems in astrophotonics and space photonics. Interestingly, these devices are now being explored for use in telecommunications and are likely to find commercial use in the next few years, particularly in the development of compact spectrographs. Photonic lanterns allow for a low-loss transformation of a multimode waveguide into a discrete number of single-mode waveguides and vice versa, thus enabling the use of single-mode photonic technologies in multimode systems. In this review, we will discuss the theory and function of the photonic lantern, along with several different variants of the technology. We will also discuss some of its applications in more detail. Furthermore, we foreshadow future applications of this technology to the field of nanophotonics.
Publisher: Optica Publishing Group
Date: 2005
Abstract: We report controlled hole expansion in photonic crystal fibres (PCFs) by heating the fibre while the holes were pressurised. This was done by post-processing an existing fibre, not during fibre fabrication. Small holes in an endlessly single-mode (ESM) PCF were inflated to become large holes. The large-hole PCF was then tapered to produce a "cobweb" PCF with a small highly-nonlinear core, interfaced to the ESM PCF at both ends by gradual transitions. The loss was less than 0.4 dB in the complete structure, which was used to demonstrate supercontinuum generation when pumped with a fs Ti:sapphire laser.
Publisher: Institute of Electrical and Electronics Engineers (IEEE)
Date: 09-2019
Publisher: Optica Publishing Group
Date: 2020
DOI: 10.1364/CLEOPR.2020.C6G_3
Abstract: We discuss the use of spatial mode sorters as coronagraphs capable of operating near the fundamental limits at small inner working angles.
Publisher: The Optical Society
Date: 13-04-2015
DOI: 10.1364/AOP.7.000107
Publisher: The Optical Society
Date: 10-01-2014
DOI: 10.1364/OE.22.001036
Publisher: IEEE
Date: 09-2015
Publisher: SPIE
Date: 11-06-2021
DOI: 10.1117/12.2600239
Publisher: SPIE
Date: 09-09-2019
DOI: 10.1117/12.2529212
Publisher: Springer Science and Business Media LLC
Date: 11-06-2018
DOI: 10.1038/S41598-018-27072-2
Abstract: We present a new technique allowing the fabrication of large modal count photonic lanterns for space- ision multiplexing applications. We demonstrate mode-selective photonic lanterns supporting 10 and 15 spatial channels by using graded-index fibres and microstructured templates. These templates are a versatile approach to position the graded-index fibres in the required geometry for efficient mode s ling and conversion. Thus, providing an effective scalable method for large number of spatial modes in a repeatable manner. Further, we demonstrate the efficiency and functionality of our photonic lanterns for optical communications. Our results show low insertion and mode dependent losses, as well as enhanced mode selectivity when spliced to few mode transmission fibres. These photonic lantern mode multiplexers are an enabling technology for future ultra-high capacity optical transmission systems.
Publisher: Optica Publishing Group
Date: 10-2002
Publisher: The Optical Society
Date: 19-12-2011
DOI: 10.1364/OE.20.000141
Publisher: OSA
Date: 2010
Publisher: Optica Publishing Group
Date: 09-11-2009
DOI: 10.1364/OE.17.021344
Publisher: SPIE
Date: 24-09-2012
DOI: 10.1117/12.925824
Publisher: Springer Science and Business Media LLC
Date: 26-03-2020
Publisher: IEEE
Date: 06-2007
Publisher: Informa UK Limited
Date: 03-04-2018
Publisher: SPIE
Date: 09-02-2012
DOI: 10.1117/12.916068
Publisher: Institute of Electrical and Electronics Engineers (IEEE)
Date: 2012
Publisher: SPIE
Date: 22-08-2012
DOI: 10.1117/12.925709
Publisher: OSA
Date: 2017
Publisher: The Optical Society
Date: 12-12-2014
DOI: 10.1364/OE.22.031575
Publisher: Institution of Engineering and Technology
Date: 2013
DOI: 10.1049/CP.2013.1680
Publisher: Institution of Engineering and Technology
Date: 2013
DOI: 10.1049/CP.2013.1681
Publisher: SPIE
Date: 09-08-2016
DOI: 10.1117/12.2232115
Publisher: IEEE
Date: 2006
Publisher: SPIE
Date: 24-09-2012
DOI: 10.1117/12.926483
Publisher: SPIE
Date: 16-07-2010
DOI: 10.1117/12.856348
Publisher: SPIE
Date: 16-07-2010
DOI: 10.1117/12.856347
Publisher: SPIE
Date: 13-09-2012
DOI: 10.1117/12.925791
Publisher: Oxford University Press (OUP)
Date: 11-12-2017
Publisher: Optica Publishing Group
Date: 2005
Abstract: Early work suggested that very large refractive index contrasts would be needed to create photonic bandgaps in two or three dimensionally periodic photonic crystals. It was then shown that in two-dimensionally periodic structures (such as photonic crystal fibres) a non-zero wavevector component in the axial direction permits photonic bandgaps for much smaller index contrasts. Here we experimentally demonstrate a photonic bandgap fibre made from two glasses with a relative index step of only 1%.
Publisher: SPIE-Intl Soc Optical Eng
Date: 03-2006
DOI: 10.1117/1.2181847
Publisher: SPIE
Date: 13-12-2020
DOI: 10.1117/12.2560626
Publisher: SPIE
Date: 15-05-2011
DOI: 10.1117/12.885672
Publisher: OSA
Date: 2017
Publisher: Cambridge University Press (CUP)
Date: 2017
DOI: 10.1017/PASA.2017.1
Abstract: Imaging bundles provide a convenient way to translate a spatially coherent image, yet conventional imaging bundles made from silica fibre optics typically remain expensive with large losses due to poor filling factors (~40%). We present the characterisation of a novel polymer imaging bundle made from poly(methyl methacrylate) (PMMA) that is considerably cheaper and a better alternative to silica imaging bundles over short distances (~1 m from the middle to the edge of a telescope’s focal plane). The large increase in filling factor (92% for the polymer imaging bundle) outweighs the large increase in optical attenuation from using PMMA (1 dB/m) instead of silica (10 −3 dB/m). We present and discuss current and possible future multi-object applications of the polymer imaging bundle in the context of astronomical instrumentation including: field acquisition, guiding, wavefront sensing, narrow-band imaging, aperture masking, and speckle imaging. The use of PMMA limits its use in low-light applications (e.g., imaging of galaxies) however, it is possible to fabricate polymer imaging bundles from a range of polymers that are better suited to the desired science.
Publisher: SPIE
Date: 18-07-2014
DOI: 10.1117/12.2055014
Publisher: The Optical Society
Date: 29-01-2016
DOI: 10.1364/AO.55.000811
Publisher: IEEE
Date: 07-2008
Publisher: IEEE
Date: 12-2010
Publisher: SPIE
Date: 22-07-2016
DOI: 10.1117/12.2233678
Publisher: Frontiers Media SA
Date: 14-01-2021
DOI: 10.3389/FAGRO.2020.601542
Abstract: Increasing concern for the ongoing availability and efficacy of herbicides is driving interest in the development of alternative physical and thermal weed control methods. Fortunately, improvements in weed detection through advancements in computing hardware and deep learning algorithms are creating an opportunity to use novel weed control tools, such as lasers, in large-scale cropping systems. For alternative control options, there are two key weed control timing opportunities, early and late post-crop emergence. Weed density for the early timing is typically higher, with a shorter window for control. Conversely, late post-emergent treatment of surviving and late-emerging weeds would occur in lower densities of larger and more variably sized weeds, given a prior weed control effort, but with a longer available weed control period. Research in laser weeding to date has primarily focused on early growth stage weeds and the ability of this approach to control larger weeds remains unknown. This study used a 25 W, 975 nm fiber-coupled diode laser to evaluate the opportunity for control of annual ryegrass ( Lolium rigidum Gaudin) and the influence of four different growth stages (three-leaf, seven-leaf, mid-tillering, and late-tillering). Annual ryegrass plants at each growth stage were treated using a laser-focused to a 5 mm diameter with five different irradiation durations developing energy densities of 1.3, 2.5, 6.4, 19.1, and 76.4 J mm −2 . At the three-leaf stage, all plants were controlled at 76.4 J mm −2 and 93.3% controlled at 19.1 J mm −2 . Complete control of seven-leaf plants was only achieved at 76.4 J mm −2 . Although laser treatments did not control mid-tillering stage plants, 76.4 J mm −2 reduced biomass by 60.2%. No similar reductions in biomass were recorded for the largest plants. This initial research assists in the development of novel weed control options in the context of large-scale conservation cropping systems. Future research should investigate the influence of laser treatments on additional weed species and the impact of increased laser power on larger weeds.
Publisher: SPIE
Date: 13-09-2012
DOI: 10.1117/12.925161
Publisher: Optica Publishing Group
Date: 21-10-2008
DOI: 10.1364/OL.33.002446
Abstract: A hollow-core microstructured polymer optical fiber is fabricated from polycarbonate material and guidance by inhibited coupling in a two-layer structure is demonstrated in two strong transmission bands with minimum losses of 9.0 dB/m at 800 nm and 3.1 dB/m at 1550 nm. The latter corresponds to a loss well below the polycarbonate material loss at this wavelength, and to our knowledge it is the lowest loss hollow-core polymer fiber reported to date. The short-term operational temperature limit of the fiber is shown to be 135 degrees C, significantly higher than that of conventional polymer optical fibers made of other polymers.
Publisher: SPIE-Intl Soc Optical Eng
Date: 29-06-2021
Publisher: Optica Publishing Group
Date: 06-02-2008
DOI: 10.1364/OL.33.000306
Abstract: We describe two all-fiber devices for converting light from the fundamental mode to the second-order set of modes in optical fibers. The first is made by controlled hole collapse in a photonic crystal fiber, and the second is a twisted fused coupler made from few-moded conventional fiber. As well as having applications within fiber optics, the devices can be used to generate azimuthally polarized free-space beams.
Publisher: OSA
Date: 2012
Publisher: Optica Publishing Group
Date: 04-09-2009
DOI: 10.1364/OL.34.002724
Publisher: Oxford University Press (OUP)
Date: 02-2012
Publisher: OSA
Date: 2015
Publisher: Oxford University Press (OUP)
Date: 05-11-2012
Publisher: Springer Science and Business Media LLC
Date: 18-01-2021
Publisher: OSA
Date: 2014
Publisher: OSA
Date: 2014
Publisher: SPIE
Date: 03-01-2020
DOI: 10.1117/12.2539992
Publisher: The Optical Society
Date: 08-10-2010
DOI: 10.1364/OE.18.022497
Publisher: IEEE
Date: 08-2011
Publisher: eScholarship
Date: 2015
Publisher: OSA
Date: 2010
Publisher: OSA
Date: 2010
Publisher: Optica Publishing Group
Date: 07-2005
DOI: 10.1364/OL.30.001629
Abstract: We report a new method for making low-loss interfaces between conventional single-mode fibers and photonic crystal fibers (PCFs). Adapted from the fabrication of PCF preforms from stacked tubes and rods, this method avoids the need for splicing and is versatile enough to interface to virtually any type of index-guiding silica PCF. We illustrate the method by forming interfaces to two problematic types of PCF, highly nonlinear and multicore. In particular, we believe this to be the first method capable of in idually coupling light into and out of all the cores of a fiber with multiple closely spaced cores, without input or output cross talk.
Publisher: Optica Publishing Group
Date: 11-05-2010
DOI: 10.1364/AO.49.002749
Publisher: The Optical Society
Date: 09-07-2012
DOI: 10.1364/OE.20.016671
Publisher: OSA
Date: 2016
Publisher: OSA
Date: 2014
Publisher: AIP Publishing
Date: 17-03-2014
DOI: 10.1063/1.4869129
Abstract: We report an in-fiber magnetic field sensor based on magneto-driven optical loss effects, while being implemented in a ferrofluid infiltrated microstructured polymer optical fiber. We demonstrate that magnetic field flux changes up to 2000 gauss can be detected when the magnetic field is applied perpendicular to the fiber axis. In addition, the sensor exhibits high polarization sensitivity for the interrogated wavelengths, providing the possibility of both field flux and direction measurements. The underlying physical and guidance mechanisms of this sensing transduction are further investigated using spectrophotometric, light scattering measurements, and numerical simulations, suggesting photonic Hall effect as the dominant physical, transducing mechanism.
Publisher: IEEE
Date: 05-2008
Publisher: Oxford University Press (OUP)
Date: 13-08-2018
Publisher: Oxford University Press (OUP)
Date: 17-08-2017
Publisher: SPIE
Date: 06-07-2018
DOI: 10.1117/12.2309893
Publisher: No publisher found
Date: 2009
Publisher: No publisher found
Publisher: SPIE
Date: 06-01-2020
DOI: 10.1117/12.2539883
Publisher: Optica Publishing Group
Date: 23-06-2021
DOI: 10.1364/AO.420855
Abstract: By combining integral field spectroscopy with extreme adaptive optics, we are now able to resolve objects close to the diffraction limit of large telescopes, exploring new science cases. We introduce an integral field unit designed to couple light with a minimal plate scale from the SCExAO facility at NIR wavelengths to a single-mode spectrograph. The integral field unit has a 3D-printed micro-lens array on top of a custom single-mode multi-core fiber, to optimize the coupling of light into the fiber cores. We demonstrate the potential of the instrument via initial results from the first on-sky runs at the 8.2 m Subaru Telescope with a spectrograph using off-the-shelf optics, allowing for rapid development with low cost.
Publisher: SPIE
Date: 04-03-2019
DOI: 10.1117/12.2507478
Publisher: Springer Science and Business Media LLC
Date: 06-12-2011
DOI: 10.1038/NCOMMS1584
Abstract: A long-standing and profound problem in astronomy is the difficulty in obtaining deep near-infrared observations due to the extreme brightness and variability of the night sky at these wavelengths. A solution to this problem is crucial if we are to obtain the deepest possible observations of the early Universe, as redshifted starlight from distant galaxies appears at these wavelengths. The atmospheric emission between 1,000 and 1,800 nm arises almost entirely from a forest of extremely bright, very narrow hydroxyl emission lines that varies on timescales of minutes. The astronomical community has long envisaged the prospect of selectively removing these lines, while retaining high throughput between them. Here we demonstrate such a filter for the first time, presenting results from the first on-sky tests. Its use on current 8 m telescopes and future 30 m telescopes will open up many new research avenues in the years to come.
Publisher: IEEE
Date: 08-2011
Publisher: Optica Publishing Group
Date: 07-04-2008
DOI: 10.1364/OE.16.005642
Abstract: We propose a guidance mechanism in hollow-core optical fibres dominated by antiresonant reflection from struts of solid material in the cladding. Resonances with these struts determine the high loss bands of the fibres, and vector effects become important in determining the width of these bands through the non-degeneracy of the TE and TM polarised strut modes near cut-off. Away from resonances the light is confined through the inhibited coupling mechanism. This is demonstrated in a square lattice hollow-core microstructured polymer optical fibre.
Publisher: SPIE
Date: 28-07-2014
DOI: 10.1117/12.2055597
Publisher: American Astronomical Society
Date: 10-2022
Abstract: 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 greatly increase the expected number of detectable planets, which scales inversely with the inner working angle. The vortex fiber nuller (VFN) is an instrument concept designed to characterize exoplanets within a single beam width. It requires few optical elements and is compatible with many coronagraph designs as a complementary characterization tool. However, the peak throughput for planet light is limited to about 20%, and the measurement places poor constraints on the planet location and flux ratio. We propose to augment the VFN design by replacing its single-mode fiber with a six-port mode-selective photonic lantern, retaining the original functionality while providing several additional ports that reject starlight but couple planet light. We show that the photonic lantern can also be used as a nuller without a vortex. We present monochromatic simulations characterizing the response of the photonic lantern nuller (PLN) to astrophysical signals and wavefront errors, and show that combining exoplanet flux from the nulled ports significantly increases the overall throughput of the instrument. We show using synthetically generated data that the PLN detects exoplanets more effectively than the VFN. Furthermore, with the PLN, the exoplanet can be partially localized, and its flux ratio constrained. The PLN has the potential to be a powerful characterization tool complementary to traditional coronagraphs in future high-contrast instruments.
Publisher: OSA
Date: 2015
Publisher: Springer New York
Date: 06-06-2013
Publisher: The Optical Society
Date: 29-11-2018
DOI: 10.1364/OE.26.032777
Publisher: SPIE
Date: 04-08-2016
DOI: 10.1117/12.2230740
Publisher: SPIE
Date: 08-07-2014
DOI: 10.1117/12.2055638
Publisher: IEEE
Date: 09-2012
Publisher: The Optical Society
Date: 13-07-2017
DOI: 10.1364/OE.25.017530
Publisher: IEEE
Date: 07-2009
Publisher: SPIE
Date: 04-08-2016
DOI: 10.1117/12.2232126
Publisher: OSA
Date: 2017
Publisher: Optica Publishing Group
Date: 10-2005
DOI: 10.1364/OL.30.002545
Abstract: A taper transition can couple light between a multimode fiber and several single-mode fibers. If the number of single-mode fibers matches the number of spatial modes in the multimode fiber, the transition can have low loss in both directions. This enables the high performance of single-mode fiber devices to be attained in multimode fibers. We report an experimental proof of concept by using photonic crystal fiber techniques to make the transitions, demonstrating a multimode fiber filter with the transmission spectrum of a single-mode fiber grating.
Publisher: The Optical Society
Date: 06-01-2015
DOI: 10.1364/OE.23.000224
Publisher: Optica Publishing Group
Date: 26-01-2007
DOI: 10.1364/OL.32.000328
Abstract: We have used two different photonic crystal fiber (PCF) techniques to make all-fiber mode converters. An LP(01) to LP(11) mode converter was made by the ferrule technique on a drawing tower, and an LP(01) to LP(02) mode converter was made by controlled hole inflation of an existing PCF on a tapering rig. Both devices rely on adiabatic propagation rather than resonant coupling so high extinction was achieved across a wide wavelength range.
Publisher: IEEE
Date: 07-2007
Publisher: Optica Publishing Group
Date: 23-06-2021
DOI: 10.1364/AO.421560
Abstract: Celestially, positronium (Ps) has been observed only through gamma-ray emission produced by its annihilation. However, in its triplet state, a Ps atom has a mean lifetime long enough for electronic transitions to occur between quantum states. This produces a recombination spectrum observable in principle at near IR wavelengths, where angular resolution greatly exceeding that of the gamma-ray observations is possible. However, the background in the near IR is dominated by extremely bright atmospheric hydroxyl (OH) emission lines. In this paper, we present the design of a diffraction-limited spectroscopic system using novel photonic components—a photonic lantern, OH fiber Bragg grating filters, and a photonic TIGER 2D pseudo-slit—to observe the Ps Balmer alpha line at 1.3122 µm for the first time, to our knowledge.
Publisher: SPIE
Date: 06-2012
DOI: 10.1117/12.922700
Publisher: Elsevier BV
Date: 02-2017
Publisher: SPIE
Date: 04-08-2014
DOI: 10.1117/12.2055584
Publisher: Springer Science and Business Media LLC
Date: 21-10-2020
DOI: 10.1038/S41467-020-19117-W
Abstract: Adaptive optics (AO) is critical in astronomy, optical communications and remote sensing to deal with the rapid blurring caused by the Earth’s turbulent atmosphere. But current AO systems are limited by their wavefront sensors, which need to be in an optical plane non-common to the science image and are insensitive to certain wavefront-error modes. Here we present a wavefront sensor based on a photonic lantern fibre-mode-converter and deep learning, which can be placed at the same focal plane as the science image, and is optimal for single-mode fibre injection. By measuring the intensities of an array of single-mode outputs, both phase and litude information on the incident wavefront can be reconstructed. We demonstrate the concept with simulations and an experimental realisation wherein Zernike wavefront errors are recovered from focal-plane measurements to a precision of 5.1 × 10 −3 π radians root-mean-squared-error.
Publisher: Optica Publishing Group
Date: 25-10-2023
DOI: 10.1364/JOSAB.502962
Publisher: Optica Publishing Group
Date: 2006
DOI: 10.1364/OE.14.006188
Abstract: We demonstrate a cascaded nonlinear process using pump conversion to 742 nm by four-wave mixing in the normal dispersion regime then continuum generation by modulation instability to generate bright single-mode visible continuum with an average power up to -20 dBm/nm, from a compact 1064 nm infrared source in a monolithic single-mode photonic crystal fibre with a tapered section in one end.
Publisher: SPIE
Date: 09-06-2011
DOI: 10.1117/12.900529
Publisher: The Optical Society
Date: 17-04-2014
DOI: 10.1364/OE.22.009920
Publisher: SPIE
Date: 25-04-2008
DOI: 10.1117/12.780822
Publisher: SPIE
Date: 07-08-2014
DOI: 10.1117/12.2055623
Publisher: American Astronomical Society
Date: 05-12-2012
Publisher: SPIE
Date: 14-03-2019
DOI: 10.1117/12.2511917
Publisher: The Optical Society
Date: 31-10-2018
DOI: 10.1364/OE.26.030042
Publisher: Springer Science and Business Media LLC
Date: 21-06-2019
DOI: 10.1038/S41598-019-45082-6
Abstract: Quantum entanglement is arguably the cornerstone which differentiates the quantum realm from its classical counterpart. While entanglement can reside in any photonic degree of freedom, polarization permits perhaps the most straightforward manipulation due to the widespread availability of standard optical elements such as waveplates and polarizers. As a step towards a fuller exploitation of entanglement in other degrees of freedom, in this work we demonstrate control over the transverse spatial structure of light at the single-photon level. In particular we integrate in our setup all the technologies required for: (i) fibre-based photon pair generation, (ii) deterministic and broadband single-photon spatial conversion relying on a passive optical device, and (iii) single-photon transmission, while retaining transverse structure, over 400 m of few-mode fibre. In our experiment, we employ a mode selective photonic lantern multiplexer with the help of which we can convert the transverse profile of a single photon from the fundamental mode into any of the supported higher-order modes. We also achieve conversion to an incoherent or coherent addition of two user-selected higher order modes by addressing different combinations of inputs in the photonic lantern multiplexer. The coherent nature of the addition, and extraction of usable orbital angular momentum at the single-photon level, is further demonstrated by far-field diffraction through a triangular aperture. Our work could enable studies of photonic entanglement in the transverse modes of a fibre and could constitute a key resource quantum for key distribution with an alphabet of scalable dimension.
Publisher: Institute of Electrical and Electronics Engineers (IEEE)
Date: 2011
Publisher: The Optical Society
Date: 04-02-2016
DOI: 10.1364/OE.24.002919
Publisher: EDP Sciences
Date: 08-2017
Publisher: Optica Publishing Group
Date: 25-08-2006
DOI: 10.1364/OL.31.002672
Abstract: We demonstrate low-loss anamorphic transitions between circular and rectangular fiber cores with aspect ratios up to 5:1, and hence improved coupling from a diode laser by using only a spherical lens. Differential hole pressurization and localized heating of a stock photonic crystal fiber inflates the holes at different rates. Some holes are plugged in the fiber end face where pressure is applied, so they remain at ambient pressure. Alternatively, holes of different sizes expand at different rates because the effective pressure due to surface tension differs.
Publisher: IEEE
Date: 08-2011
Publisher: SPIE
Date: 13-12-2020
DOI: 10.1117/12.2561514
Publisher: Optica Publishing Group
Date: 03-12-2008
DOI: 10.1364/AO.47.006497
Abstract: An enhanced magnetic Faraday effect is demonstrated in cobalt nanoparticle-doped polymer optical fiber. Magneto-optically induced rotation of the plane of polarization proportional to both the dopant particle concentration and the magnetic field strength is demonstrated. Potential applications include magnetic field sensors, current sensors, and in-fiber optical isolators.
Publisher: The Optical Society
Date: 19-08-2015
DOI: 10.1364/OL.40.003966
Publisher: OSA
Date: 2018
Publisher: Optica Publishing Group
Date: 26-06-2004
Abstract: Submicron-diameter tapered fibres and photonic crystal fibre cores, both of which are silica-air waveguides with low dispersion at 532 nm, were made using a conventional tapering process. In just cm of either waveguide, ns pulses from a low-power 532-nm microchip laser generated a single-mode supercontinuum broad enough to fill the visible spectrum without spreading far beyond it.
Publisher: Elsevier BV
Date: 03-2017
Publisher: Oxford University Press (OUP)
Date: 20-11-2015
Publisher: The Optical Society
Date: 27-01-2014
DOI: 10.1364/OE.22.002216
Publisher: The Optical Society
Date: 26-06-2017
DOI: 10.1364/OE.25.015614
Publisher: SPIE
Date: 10-07-2018
DOI: 10.1117/12.2312895
Publisher: Optica Publishing Group
Date: 23-10-2023
Publisher: Cambridge University Press (CUP)
Date: 08-2012
DOI: 10.1017/S1743921313013264
Abstract: The ‘holy grail’ of exoplanet research today is the detection of an earth-like planet: a rocky planet in the habitable zone around a main-sequence star. Extremely precise Doppler spectroscopy is an indispensable tool to find and characterize earth-like planets however, to find these planets around solar-type stars, we need nearly one order of magnitude better radial velocity (RV) precision than the best current spectrographs provide. Recent developments in astrophotonics (Bland-Hawthorn & Horton 2006, Bland-Hawthorn et al . 2010) and adaptive optics (AO) enable single mode fiber (SMF) fed, high resolution spectrographs, which can realize the next step in precision. SMF feeds have intrinsic advantages over multimode fiber or slit coupled spectrographs: The intensity distribution at the fiber exit is extremely stable, and as a result the line spread function of a well-designed spectrograph is fully decoupled from input coupling conditions, like guiding or seeing variations (Ihle et al . 2010). Modal noise, a limiting factor in current multimode fiber fed instruments (Baudrand & Walker 2001), can be eliminated by proper design, and the diffraction limited input to the spectrograph allows for very compact instrument designs, which provide excellent optomechanical stability. A SMF is the ideal interface for new, very precise wavelength calibrators, like laser frequency combs (Steinmetz et al . 2008, Osterman et al . 2012), or SMF based Fabry-Perot Etalons (Halverson et al . 2013). At near infrared wavelengths, these technologies are ready to be implemented in on-sky instruments, or already in use. We discuss a novel concept for such a spectrograph.
Publisher: The Optical Society
Date: 24-10-2013
DOI: 10.1364/OE.21.026103
Publisher: IEEE
Date: 10-2016
Publisher: OSA
Date: 2014
Publisher: The Optical Society
Date: 05-2012
DOI: 10.1364/OE.20.011232
Publisher: Optica Publishing Group
Date: 2008
DOI: 10.1364/OE.16.001142
Abstract: We report on the fabrication and characterization of hollow-core photonic bandgap fibers that do not suffer from surface mode coupling within the photonic bandgap of the cladding. This enables low attenuation over the full spectral width of the bandgap--we measured a minimum loss of 15 dB/km and less than 50 dB/km over 300 nm for a fiber operating at 1550 nm. As a result of the increased bandwidth, the fiber has reduced dispersion and dispersion slope--by a factor of almost 2 compared to previous fibers. These features are important for several applications in high-power ultrashort pulse compression and delivery. Realizing these advances has been possible due to development of a modified fabrication process which makes the production of low-loss hollow-core fibers both simpler and quicker than previously.
Publisher: Oxford University Press (OUP)
Date: 08-01-2020
Abstract: Ground-based near-infrared (NIR) astronomy is severely h ered by the forest of atmospheric emission lines resulting from the rovibrational decay of OH molecules in the upper atmosphere. The extreme brightness of these lines, as well as their spatial and temporal variability, makes accurate sky subtraction difficult. Selectively filtering these lines with OH suppression instruments has been a long standing goal for NIR spectroscopy. We have shown previously the efficacy of fibre Bragg gratings (FBGs) combined with photonic lanterns for achieving OH suppression. Here we report on PRAXIS, a unique NIR spectrograph that is optimized for OH suppression with FBGs. We show for the first time that OH suppression (of any kind) is possible with high overall throughput (18 per cent end-to-end), and provide ex les of the relative benefits of OH suppression.
Publisher: IEEE
Date: 2008
Publisher: Institute of Electrical and Electronics Engineers (IEEE)
Date: 07-2012
Publisher: The Optical Society
Date: 14-07-2015
DOI: 10.1364/OE.23.018888
Publisher: IMPERIAL COLLEGE PRESS
Date: 08-2012
DOI: 10.1142/P782
Publisher: IEEE
Date: 05-2011
Publisher: Optica Publishing Group
Date: 2020
DOI: 10.1364/CLEOPR.2020.PDP_1
Abstract: We present a new type of wavefront sensor based on a fibre-mode-converter and deep learning. By only measuring intensities of the single-mode outputs array, both phase and litude on the incident wavefront can be reconstructed.
Publisher: Oxford University Press (OUP)
Date: 16-05-2013
DOI: 10.1093/MNRAS/STT677
Publisher: IOP Publishing
Date: 10-2023
Abstract: Photonic technologies offer numerous functionalities that can be used to realize astrophotonic instruments. The most spectacular ex le to date is the ESO Gravity instrument at the Very Large Telescope in Chile that combines the light-gathering power of four 8-m telescopes through a complex photonic interferometer. Fully integrated astrophotonic devices offer critical advantages for instrument development, including extreme miniaturization when operating at the diffraction-limit, plus integration, superior thermal and mechanical stabilization owing to the small footprint, and high replicability offering significant cost savings. Numerous astrophotonic technologies have been developed to address shortcomings of conventional instruments to date, including the development of photonic lanterns to convert from multimode inputs to single mode outputs, complex aperiodic fiber Bragg gratings to filter OH emission from the atmosphere, beam combiners enabling long baseline interferometry with for ex le, ESO Gravity, and laser frequency combs for high precision spectral calibration of spectrometers. Despite these successes, the facility implementation of photonic solutions in astronomical instrumentation is currently limited because of 1) low throughputs from coupling to fibers, coupling fibers to chips, propagation and bend losses, device losses, etc., 2) difficulties with scaling to large channel count devices needed for large bandwidths and high resolutions, and 3) efficient integration of photonics with detectors. In this roadmap, we identify 23 key areas that need further development. We outline the challenges and advances needed across those areas covering design tools, simulation capabilities, fabrication processes, the need for entirely new components, integration and hybridization and the characterization of devices. To realize these advances the astrophotonics community will have to work cooperatively with industrial partners who have more advanced manufacturing capabilities. With the advances described herein, multi-functional integrated instruments will be realized leading to novel observing capabilities for both ground and space based platforms, enabling new scientific studies and discoveries.
Publisher: The Optical Society
Date: 11-07-2014
DOI: 10.1364/OE.22.017497
Location: United Kingdom of Great Britain and Northern Ireland
Start Date: 01-2010
End Date: 01-2013
Amount: $285,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 12-2017
End Date: 12-2024
Amount: $4,619,950.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2018
End Date: 12-2021
Amount: $468,671.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2019
End Date: 12-2021
Amount: $656,639.00
Funder: Australian Research Council
View Funded ActivityStart Date: 05-2016
End Date: 12-2017
Amount: $175,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 07-2013
End Date: 12-2014
Amount: $315,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 2015
End Date: 12-2015
Amount: $430,000.00
Funder: Australian Research Council
View Funded ActivityStart Date: 02-2013
End Date: 01-2014
Amount: $300,000.00
Funder: Australian Research Council
View Funded Activity