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dc.contributor.authorJovanovic, N
dc.contributor.authorGatkine, P
dc.contributor.authorAnugu, N
dc.contributor.authorAmezcua-Correa, R
dc.contributor.authorThakur, RB
dc.contributor.authorBeichman, C
dc.contributor.authorBender, CF
dc.contributor.authorBerger, J-P
dc.contributor.authorBigioli, A
dc.contributor.authorBland-Hawthorn, J
dc.contributor.authorBourdarot, G
dc.contributor.authorBradford, CM
dc.contributor.authorBroeke, R
dc.contributor.authorBryant, J
dc.contributor.authorBundy, K
dc.contributor.authorCheriton, R
dc.contributor.authorCvetojevic, N
dc.contributor.authorDiab, M
dc.contributor.authorDiddams, SA
dc.contributor.authorDinkelaker, AN
dc.contributor.authorDuis, J
dc.contributor.authorEikenberry, S
dc.contributor.authorEllis, S
dc.contributor.authorEndo, A
dc.contributor.authorFiger, DF
dc.contributor.authorFitzgerald, MP
dc.contributor.authorGris-Sanchez, I
dc.contributor.authorGross, S
dc.contributor.authorGrossard, L
dc.contributor.authorGuyon, O
dc.contributor.authorHaffert, SY
dc.contributor.authorHalverson, S
dc.contributor.authorHarris, RJ
dc.contributor.authorHe, J
dc.contributor.authorHerr, T
dc.contributor.authorHottinger, P
dc.contributor.authorHuby, E
dc.contributor.authorIreland, M
dc.contributor.authorJenson-Clem, R
dc.contributor.authorJewell, J
dc.contributor.authorJocou, L
dc.contributor.authorKraus, S
dc.contributor.authorLabadie, L
dc.contributor.authorLacour, S
dc.contributor.authorLaugier, R
dc.contributor.authorŁawniczuk, K
dc.contributor.authorLin, J
dc.contributor.authorLeifer, S
dc.contributor.authorLeon-Saval, S
dc.contributor.authorMartin, G
dc.contributor.authorMartinache, F
dc.contributor.authorMartinod, M-A
dc.contributor.authorMazin, BA
dc.contributor.authorMinardi, S
dc.contributor.authorMonnier, JD
dc.contributor.authorMoreira, R
dc.contributor.authorMourard, D
dc.contributor.authorNayak, AS
dc.contributor.authorNorris, B
dc.contributor.authorObrzud, E
dc.contributor.authorPerraut, K
dc.contributor.authorReynaud, F
dc.contributor.authorSallum, S
dc.contributor.authorSchiminovich, D
dc.contributor.authorSchwab, C
dc.contributor.authorSerbayn, E
dc.contributor.authorSoliman, S
dc.contributor.authorStoll, A
dc.contributor.authorTang, L
dc.contributor.authorTuthill, P
dc.contributor.authorVahala, K
dc.contributor.authorVasisht, G
dc.contributor.authorVeilleux, S
dc.contributor.authorWalter, AB
dc.contributor.authorWollack, EJ
dc.contributor.authorXin, Y
dc.contributor.authorYang, Z
dc.contributor.authorYerolatsitis, S
dc.contributor.authorZhang, Y
dc.contributor.authorZou, C-L
dc.date.accessioned2023-12-18T11:36:07Z
dc.date.issued2023-10-30
dc.date.updated2023-12-16T00:48:52Z
dc.description.abstractPhotonic technologies 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 Telescope in Chile that combines the light-gathering power of four 8 m telescopes through a complex photonic interferometer. Fully integrated astrophotonic devices stand to offer critical advantages for instrument development, including extreme miniaturization when operating at the diffraction-limit, as well as 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 for example 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, complex beam combiners to enable long baseline interferometry with for example, 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, to name a few. In this roadmap, we identify 24 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.en_GB
dc.description.sponsorshipNational Science Foundation (NSF)en_GB
dc.description.sponsorshipNASAen_GB
dc.format.extent042501-
dc.identifier.citationVol. 5(4), article 042501en_GB
dc.identifier.doihttps://doi.org/10.1088/2515-7647/ace869
dc.identifier.grantnumber2109232en_GB
dc.identifier.grantnumberHST-HF2-51478.001-Aen_GB
dc.identifier.urihttp://hdl.handle.net/10871/134810
dc.identifierORCID: 0000-0001-6017-8773 (Kraus, Stefan)
dc.identifierScopusID: 24481487500 (Kraus, Stefan)
dc.language.isoenen_GB
dc.publisherIOP Publishingen_GB
dc.rights© 2023 The Author(s). Published by IOP Publishing Ltd. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en_GB
dc.subjectastrophotonicsen_GB
dc.subjectspectrographen_GB
dc.subjectlanternsen_GB
dc.subjectdetectorsen_GB
dc.subjectPICsen_GB
dc.subjecthybridizationen_GB
dc.subjectintegrationen_GB
dc.title2023 Astrophotonics Roadmap: pathways to realizing multi-functional integrated astrophotonic instrumentsen_GB
dc.typeArticleen_GB
dc.date.available2023-12-18T11:36:07Z
dc.identifier.issn2515-7647
dc.descriptionThis is the final version. Available on open access from IOP Publishing via the DOI in this recorden_GB
dc.descriptionData availability statement: The data that support the findings of this study are available upon reasonable request from the authors.en_GB
dc.identifier.eissn2515-7647
dc.identifier.journalJournal of Physics: Photonicsen_GB
dc.relation.ispartofJournal of Physics Photonics, 5(4)
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
dcterms.dateAccepted2023-07-18
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2023-10-30
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2023-12-18T11:32:52Z
refterms.versionFCDVoR
refterms.dateFOA2023-12-18T11:36:09Z
refterms.panelBen_GB
refterms.dateFirstOnline2023-10-30


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© 2023 The Author(s). Published by IOP Publishing Ltd. Open access. Original content from
this work may be used
under the terms of the
Creative Commons
Attribution 4.0 licence.
Any further distribution
of this work must
maintain attribution to
the author(s) and the title
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Except where otherwise noted, this item's licence is described as © 2023 The Author(s). Published by IOP Publishing Ltd. Open access. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.