Design and performance of SuperSpec: An on-chip, KID-based, mm-wavelength spectrometer

E. Shirokoff; P. S. Barry; C. M. Bradford; G. Chattopadhyay; P. Day; S. Doyle; S. Hailey-Dunsheath; M. I. Hollister; A. Kovács; H. G. Leduc; C. M. McKenney; Philip Mauskopf; H. T. Nguyen; R. O'Brient; S. Padin; T. J. Reck; L. J. Swenson; C. E. Tucker; J. Zmuidzinas

doi:10.1007/s10909-014-1122-8

Design and performance of SuperSpec: An on-chip, KID-based, mm-wavelength spectrometer

E. Shirokoff, P. S. Barry, C. M. Bradford, G. Chattopadhyay, P. Day, S. Doyle, S. Hailey-Dunsheath, M. I. Hollister, A. Kovács, H. G. Leduc, C. M. McKenney, Philip Mauskopf, H. T. Nguyen, R. O'Brient, S. Padin, T. J. Reck, L. J. Swenson, C. E. Tucker, J. Zmuidzinas

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

30 Scopus citations

Abstract

SuperSpec is an ultra-compact spectrometer-on-a-chip for mm and submm wavelength astronomy. Its very small size, wide spectral bandwidth, and highly multiplexed detector readout will enable construction of powerful multi-object spectrometers for observations of galaxies at high redshift. SuperSpec is a filter bank with planar, lithographed, superconducting transmission line resonator filters and lumped-element kinetic inductance detectors made from Titanium Nitride. We have built an 81 detector prototype that operates in the 195-310 GHz band. The prototype has a wide-band metal feed horn with a transition to microstrip that feeds the filter bank. The prototype has demonstrated optical filter bank channels with a range of resolving powers from 300 to 700, measured fractional frequency noise of 10^-17 Hz ^-1 at 1 Hz.

Original language	English (US)
Pages (from-to)	657-662
Number of pages	6
Journal	Journal of Low Temperature Physics
Volume	176
Issue number	5-6
DOIs	https://doi.org/10.1007/s10909-014-1122-8
State	Published - Sep 2014

Keywords

Kinetic inductance detectors
Millimeter-wavelength
Resonators
Spectroscopy

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Materials Science(all)
Condensed Matter Physics

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10.1007/s10909-014-1122-8

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Shirokoff, E., Barry, P. S., Bradford, C. M., Chattopadhyay, G., Day, P., Doyle, S., Hailey-Dunsheath, S., Hollister, M. I., Kovács, A., Leduc, H. G., McKenney, C. M., Mauskopf, P., Nguyen, H. T., O'Brient, R., Padin, S., Reck, T. J., Swenson, L. J., Tucker, C. E., & Zmuidzinas, J. (2014). Design and performance of SuperSpec: An on-chip, KID-based, mm-wavelength spectrometer. Journal of Low Temperature Physics, 176(5-6), 657-662. https://doi.org/10.1007/s10909-014-1122-8

Shirokoff, E, Barry, PS, Bradford, CM, Chattopadhyay, G, Day, P, Doyle, S, Hailey-Dunsheath, S, Hollister, MI, Kovács, A, Leduc, HG, McKenney, CM, Mauskopf, P, Nguyen, HT, O'Brient, R, Padin, S, Reck, TJ, Swenson, LJ, Tucker, CE & Zmuidzinas, J 2014, 'Design and performance of SuperSpec: An on-chip, KID-based, mm-wavelength spectrometer', Journal of Low Temperature Physics, vol. 176, no. 5-6, pp. 657-662. https://doi.org/10.1007/s10909-014-1122-8

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title = "Design and performance of SuperSpec: An on-chip, KID-based, mm-wavelength spectrometer",

abstract = "SuperSpec is an ultra-compact spectrometer-on-a-chip for mm and submm wavelength astronomy. Its very small size, wide spectral bandwidth, and highly multiplexed detector readout will enable construction of powerful multi-object spectrometers for observations of galaxies at high redshift. SuperSpec is a filter bank with planar, lithographed, superconducting transmission line resonator filters and lumped-element kinetic inductance detectors made from Titanium Nitride. We have built an 81 detector prototype that operates in the 195-310 GHz band. The prototype has a wide-band metal feed horn with a transition to microstrip that feeds the filter bank. The prototype has demonstrated optical filter bank channels with a range of resolving powers from 300 to 700, measured fractional frequency noise of 10-17 Hz -1 at 1 Hz.",

keywords = "Kinetic inductance detectors, Millimeter-wavelength, Resonators, Spectroscopy",

author = "E. Shirokoff and Barry, {P. S.} and Bradford, {C. M.} and G. Chattopadhyay and P. Day and S. Doyle and S. Hailey-Dunsheath and Hollister, {M. I.} and A. Kov{\'a}cs and Leduc, {H. G.} and McKenney, {C. M.} and Philip Mauskopf and Nguyen, {H. T.} and R. O'Brient and S. Padin and Reck, {T. J.} and Swenson, {L. J.} and Tucker, {C. E.} and J. Zmuidzinas",

note = "Funding Information: Acknowledgments This project is supported by NASA Astrophysics Research and Analysis (APRA) Grant No. 399131.02.06.03.43. ES, CMM, and LJS acknowledge support from the W. M. Keck Institute for Space Studies. MIH, LJS, and TR acknowledge support from the NASA Postdoctoral Program. PSB acknowledges the continuing support from the Science and Technology Facilities Council Ph.D. studentship programme and grant programmes ST/G002711/1 and ST/J001449/1. Device fabrication was performed the JPL Microdevices Laboratory.",

year = "2014",

month = sep,

doi = "10.1007/s10909-014-1122-8",

language = "English (US)",

volume = "176",

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T1 - Design and performance of SuperSpec

T2 - An on-chip, KID-based, mm-wavelength spectrometer

AU - Shirokoff, E.

AU - Barry, P. S.

AU - Bradford, C. M.

AU - Chattopadhyay, G.

AU - Day, P.

AU - Doyle, S.

AU - Hailey-Dunsheath, S.

AU - Hollister, M. I.

AU - Kovács, A.

AU - Leduc, H. G.

AU - McKenney, C. M.

AU - Mauskopf, Philip

AU - Nguyen, H. T.

AU - O'Brient, R.

AU - Padin, S.

AU - Reck, T. J.

AU - Swenson, L. J.

AU - Tucker, C. E.

AU - Zmuidzinas, J.

N1 - Funding Information: Acknowledgments This project is supported by NASA Astrophysics Research and Analysis (APRA) Grant No. 399131.02.06.03.43. ES, CMM, and LJS acknowledge support from the W. M. Keck Institute for Space Studies. MIH, LJS, and TR acknowledge support from the NASA Postdoctoral Program. PSB acknowledges the continuing support from the Science and Technology Facilities Council Ph.D. studentship programme and grant programmes ST/G002711/1 and ST/J001449/1. Device fabrication was performed the JPL Microdevices Laboratory.

PY - 2014/9

Y1 - 2014/9

N2 - SuperSpec is an ultra-compact spectrometer-on-a-chip for mm and submm wavelength astronomy. Its very small size, wide spectral bandwidth, and highly multiplexed detector readout will enable construction of powerful multi-object spectrometers for observations of galaxies at high redshift. SuperSpec is a filter bank with planar, lithographed, superconducting transmission line resonator filters and lumped-element kinetic inductance detectors made from Titanium Nitride. We have built an 81 detector prototype that operates in the 195-310 GHz band. The prototype has a wide-band metal feed horn with a transition to microstrip that feeds the filter bank. The prototype has demonstrated optical filter bank channels with a range of resolving powers from 300 to 700, measured fractional frequency noise of 10-17 Hz -1 at 1 Hz.

AB - SuperSpec is an ultra-compact spectrometer-on-a-chip for mm and submm wavelength astronomy. Its very small size, wide spectral bandwidth, and highly multiplexed detector readout will enable construction of powerful multi-object spectrometers for observations of galaxies at high redshift. SuperSpec is a filter bank with planar, lithographed, superconducting transmission line resonator filters and lumped-element kinetic inductance detectors made from Titanium Nitride. We have built an 81 detector prototype that operates in the 195-310 GHz band. The prototype has a wide-band metal feed horn with a transition to microstrip that feeds the filter bank. The prototype has demonstrated optical filter bank channels with a range of resolving powers from 300 to 700, measured fractional frequency noise of 10-17 Hz -1 at 1 Hz.

KW - Kinetic inductance detectors

KW - Millimeter-wavelength

KW - Resonators

KW - Spectroscopy

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ER -

Design and performance of SuperSpec: An on-chip, KID-based, mm-wavelength spectrometer

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Keywords

ASJC Scopus subject areas

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