A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications
Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavele...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lowitz, A. E. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media New York 2014 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Springer US, 1969, 176(2014), 3-4 vom: 21. Feb., Seite 504-510 |
|---|---|
| Übergeordnetes Werk: |
volume:176 ; year:2014 ; number:3-4 ; day:21 ; month:02 ; pages:504-510 |
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| DOI / URN: |
10.1007/s10909-014-1133-5 |
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OLC2036822215 |
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| 520 | |a Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. | ||
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10.1007/s10909-014-1133-5 doi (DE-627)OLC2036822215 (DE-He213)s10909-014-1133-5-p DE-627 ger DE-627 rakwb eng 530 VZ Lowitz, A. E. verfasserin aut A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. Kinetic inductance detector Transition edge sensor Millimeter wave detector Barrentine, E. M. aut Golwala, S. R. aut Timbie, P. T. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 21. Feb., Seite 504-510 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:21 month:02 pages:504-510 https://doi.org/10.1007/s10909-014-1133-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 21 02 504-510 |
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10.1007/s10909-014-1133-5 doi (DE-627)OLC2036822215 (DE-He213)s10909-014-1133-5-p DE-627 ger DE-627 rakwb eng 530 VZ Lowitz, A. E. verfasserin aut A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. Kinetic inductance detector Transition edge sensor Millimeter wave detector Barrentine, E. M. aut Golwala, S. R. aut Timbie, P. T. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 21. Feb., Seite 504-510 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:21 month:02 pages:504-510 https://doi.org/10.1007/s10909-014-1133-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 21 02 504-510 |
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10.1007/s10909-014-1133-5 doi (DE-627)OLC2036822215 (DE-He213)s10909-014-1133-5-p DE-627 ger DE-627 rakwb eng 530 VZ Lowitz, A. E. verfasserin aut A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. Kinetic inductance detector Transition edge sensor Millimeter wave detector Barrentine, E. M. aut Golwala, S. R. aut Timbie, P. T. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 21. Feb., Seite 504-510 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:21 month:02 pages:504-510 https://doi.org/10.1007/s10909-014-1133-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 21 02 504-510 |
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10.1007/s10909-014-1133-5 doi (DE-627)OLC2036822215 (DE-He213)s10909-014-1133-5-p DE-627 ger DE-627 rakwb eng 530 VZ Lowitz, A. E. verfasserin aut A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. Kinetic inductance detector Transition edge sensor Millimeter wave detector Barrentine, E. M. aut Golwala, S. R. aut Timbie, P. T. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 21. Feb., Seite 504-510 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:21 month:02 pages:504-510 https://doi.org/10.1007/s10909-014-1133-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 21 02 504-510 |
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10.1007/s10909-014-1133-5 doi (DE-627)OLC2036822215 (DE-He213)s10909-014-1133-5-p DE-627 ger DE-627 rakwb eng 530 VZ Lowitz, A. E. verfasserin aut A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media New York 2014 Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. Kinetic inductance detector Transition edge sensor Millimeter wave detector Barrentine, E. M. aut Golwala, S. R. aut Timbie, P. T. aut Enthalten in Journal of low temperature physics Springer US, 1969 176(2014), 3-4 vom: 21. Feb., Seite 504-510 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:176 year:2014 number:3-4 day:21 month:02 pages:504-510 https://doi.org/10.1007/s10909-014-1133-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_22 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2185 GBV_ILN_4126 GBV_ILN_4323 AR 176 2014 3-4 21 02 504-510 |
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Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. © Springer Science+Business Media New York 2014 |
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Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. © Springer Science+Business Media New York 2014 |
| abstract_unstemmed |
Abstract Kinetic inductance detectors (KIDs) show promise as a competitive technology for astronomical observations over a wide range of wavelengths. We are interested in comparing the fundamental limitations to the sensitivity of KIDs with that of transition edge sensors (TESs) at millimeter wavelengths, specifically over the wavelengths required for studies of the Cosmic Microwave Background (CMB). We calculate the total fundamental noise arising from optical and thermal excitations in TESs and KIDs for a variety of bath temperatures and optical loading scenarios for applications at millimeter wavelengths. Special consideration is given to the case of ground-based observations of 100 GHz radiation with a 100 mK bath temperature, conditions consistent with the planned second module of the QUBIC telescope, a CMB instrument Battistelli (Astropart Phys 34:705, 2011). Under these conditions, a titanium nitride KID with optimized critical temperature pays a few percent noise penalty compared to a typical optimized TES. © Springer Science+Business Media New York 2014 |
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| title_short |
A Comparison of Fundamental Noise in Kinetic Inductance Detectors and Transition Edge Sensors for Millimeter-Wave Applications |
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https://doi.org/10.1007/s10909-014-1133-5 |
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Barrentine, E. M. Golwala, S. R. Timbie, P. T. |
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