Optimizing photonic ring-resonator filters for OH-suppressed near-infrared astronomy

Pufan Liu; David A. Czaplewski; Simon Ellis; Robert Kehoe; Kyler Kuehn; Harold M. Spinka; Nathaniel P. Stern; David G. Underwood; Steve Kuhlmann

doi:10.1364/AO.421383

Optimizing photonic ring-resonator filters for OH-suppressed near-infrared astronomy

Pufan Liu^*, David A. Czaplewski, Simon Ellis, Robert Kehoe, Kyler Kuehn, Harold M. Spinka, Nathaniel P. Stern, David G. Underwood, Steve Kuhlmann

^*Corresponding author for this work

Australian Astronomical Optics

Research output: Contribution to journal › Article › peer-review

1 Citation (Scopus)

Abstract

Near-infrared wavelength observations are crucial for understanding numerous fields of astrophysics, such as supernova cosmology and positronium annihilation detection.However, current ground-based observations suffer from an enormous background due to OH emission in the upper atmosphere. One promising way to solve this problem is to use ring-resonator filters to suppress OH emission lines. In this work, we discuss our optimization of ring-resonator filter performance from five perspectives: Resonance wavelength matching, polarizationindependent operation, low insertion loss, low-loss coupling to astronomical instruments, and broadband operation. In the end, we discuss next steps needed for reliable supernova and positronium observations, thus providing a roadmap for future advances in near-infrared astronomy.

Original language	English
Pages (from-to)	3865-3873
Number of pages	9
Journal	Applied Optics
Volume	60
Issue number	13
DOIs	https://doi.org/10.1364/AO.421383
Publication status	Published - 1 May 2021

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@article{4a4adb08601543f690dd8c4d78cdd796,

title = "Optimizing photonic ring-resonator filters for OH-suppressed near-infrared astronomy",

abstract = "Near-infrared wavelength observations are crucial for understanding numerous fields of astrophysics, such as supernova cosmology and positronium annihilation detection.However, current ground-based observations suffer from an enormous background due to OH emission in the upper atmosphere. One promising way to solve this problem is to use ring-resonator filters to suppress OH emission lines. In this work, we discuss our optimization of ring-resonator filter performance from five perspectives: Resonance wavelength matching, polarizationindependent operation, low insertion loss, low-loss coupling to astronomical instruments, and broadband operation. In the end, we discuss next steps needed for reliable supernova and positronium observations, thus providing a roadmap for future advances in near-infrared astronomy. ",

author = "Pufan Liu and Czaplewski, {David A.} and Simon Ellis and Robert Kehoe and Kyler Kuehn and Spinka, {Harold M.} and Stern, {Nathaniel P.} and Underwood, {David G.} and Steve Kuhlmann",

year = "2021",

month = may,

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doi = "10.1364/AO.421383",

language = "English",

volume = "60",

pages = "3865--3873",

journal = "Applied Optics",

issn = "1559-128X",

publisher = "Optical Society of America (OSA)",

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Optimizing photonic ring-resonator filters for OH-suppressed near-infrared astronomy. / Liu, Pufan; Czaplewski, David A.; Ellis, Simon; Kehoe, Robert; Kuehn, Kyler; Spinka, Harold M.; Stern, Nathaniel P.; Underwood, David G.; Kuhlmann, Steve.

In: Applied Optics, Vol. 60, No. 13, 01.05.2021, p. 3865-3873.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - Optimizing photonic ring-resonator filters for OH-suppressed near-infrared astronomy

AU - Liu, Pufan

AU - Czaplewski, David A.

AU - Ellis, Simon

AU - Kehoe, Robert

AU - Kuehn, Kyler

AU - Spinka, Harold M.

AU - Stern, Nathaniel P.

AU - Underwood, David G.

AU - Kuhlmann, Steve

PY - 2021/5/1

Y1 - 2021/5/1

N2 - Near-infrared wavelength observations are crucial for understanding numerous fields of astrophysics, such as supernova cosmology and positronium annihilation detection.However, current ground-based observations suffer from an enormous background due to OH emission in the upper atmosphere. One promising way to solve this problem is to use ring-resonator filters to suppress OH emission lines. In this work, we discuss our optimization of ring-resonator filter performance from five perspectives: Resonance wavelength matching, polarizationindependent operation, low insertion loss, low-loss coupling to astronomical instruments, and broadband operation. In the end, we discuss next steps needed for reliable supernova and positronium observations, thus providing a roadmap for future advances in near-infrared astronomy.

AB - Near-infrared wavelength observations are crucial for understanding numerous fields of astrophysics, such as supernova cosmology and positronium annihilation detection.However, current ground-based observations suffer from an enormous background due to OH emission in the upper atmosphere. One promising way to solve this problem is to use ring-resonator filters to suppress OH emission lines. In this work, we discuss our optimization of ring-resonator filter performance from five perspectives: Resonance wavelength matching, polarizationindependent operation, low insertion loss, low-loss coupling to astronomical instruments, and broadband operation. In the end, we discuss next steps needed for reliable supernova and positronium observations, thus providing a roadmap for future advances in near-infrared astronomy.

UR - http://www.scopus.com/inward/record.url?scp=85105270891&partnerID=8YFLogxK

U2 - 10.1364/AO.421383

DO - 10.1364/AO.421383

M3 - Article

C2 - 33983324

AN - SCOPUS:85105270891

VL - 60

SP - 3865

EP - 3873

JO - Applied Optics

JF - Applied Optics

SN - 1559-128X

IS - 13

ER -

Optimizing photonic ring-resonator filters for OH-suppressed near-infrared astronomy

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