Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers
SuperSpec is an on-chip filter bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors. SuperSpec technology will enable large-format spectroscopic integral field units suitable for high-redshift line intensity ma...
Gespeichert in:
| Veröffentlicht in: | Journal of low temperature physics 2020-05, Vol.199 (3-4), p.849-857 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 857 |
|---|---|
| container_issue | 3-4 |
| container_start_page | 849 |
| container_title | Journal of low temperature physics |
| container_volume | 199 |
| creator | Karkare, K. S. Barry, P. S. Bradford, C. M. Chapman, S. Doyle, S. Glenn, J. Gordon, S. Hailey-Dunsheath, S. Janssen, R. M. J. Kovács, A. LeDuc, H. G. Mauskopf, P. McGeehan, R. Redford, J. Shirokoff, E. Tucker, C. Wheeler, J. Zmuidzinas, J. |
| description | SuperSpec is an on-chip filter bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors. SuperSpec technology will enable large-format spectroscopic integral field units suitable for high-redshift line intensity mapping and multi-object spectrographs. In previous results, we have demonstrated noise performance in individual detectors suitable for photon noise-limited ground-based observations at excellent mm-wave sites. In these proceedings, we present the noise performance of a full
R
∼
275
spectrometer measured using deployment-ready RF hardware and software. We report typical noise equivalent powers through the full device of
∼
3
×
10
-
16
W
Hz
-
1
/
2
at expected sky loadings, which are photon noise dominated. Based on these results, we plan to deploy a six-spectrometer demonstration instrument to the Large Millimeter Telescope in early 2020. |
| doi_str_mv | 10.1007/s10909-020-02407-4 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1767044</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2396912076</sourcerecordid><originalsourceid>FETCH-LOGICAL-c412t-1ebb2e47186aeeabf9e1e69da99aaca042c6c22b4d436f82041aaf0a9633e2c13</originalsourceid><addsrcrecordid>eNp9kE1LAzEQhoMoWKt_wNOi5-jko0lzLNVWoVihit5Cms7aLd3NmmyF_nu3ruDNwzAwPO_L8BByyeCGAejbxMCAocChHQmayiPSYwMtqBYDfUx6AJxTzg07JWcpbQDADJXokffJbruloxjdPnsKRcLsGWMeYukqj1nIszust2FfYtXQaXQrzBa7GuOiRp-VJX1zX5jNKzpeF3V2ODYxlNhgTOfkJHfbhBe_u09eJ_cv4wc6m08fx6MZ9ZLxhjJcLjlKzYbKIbplbpChMitnjHPegeReec6XciWFyoccJHMuB2eUEMg9E31y1fWG1BQ2-aJBv_ahqtpfLNNKg5QtdN1BdQyfO0yN3YRdrNq_LBdGGcZBq5biHeVjSClibutYlC7uLQN70Gw7zbbVbH8020O16EKphasPjH_V_6S-ASdhf6k</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2396912076</pqid></control><display><type>article</type><title>Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers</title><source>Springer Online Journals</source><creator>Karkare, K. S. ; Barry, P. S. ; Bradford, C. M. ; Chapman, S. ; Doyle, S. ; Glenn, J. ; Gordon, S. ; Hailey-Dunsheath, S. ; Janssen, R. M. J. ; Kovács, A. ; LeDuc, H. G. ; Mauskopf, P. ; McGeehan, R. ; Redford, J. ; Shirokoff, E. ; Tucker, C. ; Wheeler, J. ; Zmuidzinas, J.</creator><creatorcontrib>Karkare, K. S. ; Barry, P. S. ; Bradford, C. M. ; Chapman, S. ; Doyle, S. ; Glenn, J. ; Gordon, S. ; Hailey-Dunsheath, S. ; Janssen, R. M. J. ; Kovács, A. ; LeDuc, H. G. ; Mauskopf, P. ; McGeehan, R. ; Redford, J. ; Shirokoff, E. ; Tucker, C. ; Wheeler, J. ; Zmuidzinas, J. ; Argonne National Laboratory (ANL), Argonne, IL (United States)</creatorcontrib><description>SuperSpec is an on-chip filter bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors. SuperSpec technology will enable large-format spectroscopic integral field units suitable for high-redshift line intensity mapping and multi-object spectrographs. In previous results, we have demonstrated noise performance in individual detectors suitable for photon noise-limited ground-based observations at excellent mm-wave sites. In these proceedings, we present the noise performance of a full
R
∼
275
spectrometer measured using deployment-ready RF hardware and software. We report typical noise equivalent powers through the full device of
∼
3
×
10
-
16
W
Hz
-
1
/
2
at expected sky loadings, which are photon noise dominated. Based on these results, we plan to deploy a six-spectrometer demonstration instrument to the Large Millimeter Telescope in early 2020.</description><identifier>ISSN: 0022-2291</identifier><identifier>EISSN: 1573-7357</identifier><identifier>DOI: 10.1007/s10909-020-02407-4</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Broadband ; Characterization and Evaluation of Materials ; Condensed Matter Physics ; Detectors ; Filter banks ; Ground-based observation ; Inductance ; kinetic inductance detectors ; Large Millimeter Telescope ; Low temperature physics ; Magnetic Materials ; Magnetism ; Mapping ; Millimeter waves ; NEP ; Noise ; OTHER INSTRUMENTATION ; Photons ; Physics ; Physics and Astronomy ; Red shift ; ROACH2 ; Spectrographs ; spectrometer ; Spectrometers ; SuperSpec</subject><ispartof>Journal of low temperature physics, 2020-05, Vol.199 (3-4), p.849-857</ispartof><rights>Springer Science+Business Media, LLC, part of Springer Nature 2020</rights><rights>Springer Science+Business Media, LLC, part of Springer Nature 2020.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c412t-1ebb2e47186aeeabf9e1e69da99aaca042c6c22b4d436f82041aaf0a9633e2c13</citedby><cites>FETCH-LOGICAL-c412t-1ebb2e47186aeeabf9e1e69da99aaca042c6c22b4d436f82041aaf0a9633e2c13</cites><orcidid>0000-0002-5215-6993 ; 0000000252156993</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10909-020-02407-4$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10909-020-02407-4$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,314,776,780,881,27901,27902,41464,42533,51294</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1767044$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Karkare, K. S.</creatorcontrib><creatorcontrib>Barry, P. S.</creatorcontrib><creatorcontrib>Bradford, C. M.</creatorcontrib><creatorcontrib>Chapman, S.</creatorcontrib><creatorcontrib>Doyle, S.</creatorcontrib><creatorcontrib>Glenn, J.</creatorcontrib><creatorcontrib>Gordon, S.</creatorcontrib><creatorcontrib>Hailey-Dunsheath, S.</creatorcontrib><creatorcontrib>Janssen, R. M. J.</creatorcontrib><creatorcontrib>Kovács, A.</creatorcontrib><creatorcontrib>LeDuc, H. G.</creatorcontrib><creatorcontrib>Mauskopf, P.</creatorcontrib><creatorcontrib>McGeehan, R.</creatorcontrib><creatorcontrib>Redford, J.</creatorcontrib><creatorcontrib>Shirokoff, E.</creatorcontrib><creatorcontrib>Tucker, C.</creatorcontrib><creatorcontrib>Wheeler, J.</creatorcontrib><creatorcontrib>Zmuidzinas, J.</creatorcontrib><creatorcontrib>Argonne National Laboratory (ANL), Argonne, IL (United States)</creatorcontrib><title>Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers</title><title>Journal of low temperature physics</title><addtitle>J Low Temp Phys</addtitle><description>SuperSpec is an on-chip filter bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors. SuperSpec technology will enable large-format spectroscopic integral field units suitable for high-redshift line intensity mapping and multi-object spectrographs. In previous results, we have demonstrated noise performance in individual detectors suitable for photon noise-limited ground-based observations at excellent mm-wave sites. In these proceedings, we present the noise performance of a full
R
∼
275
spectrometer measured using deployment-ready RF hardware and software. We report typical noise equivalent powers through the full device of
∼
3
×
10
-
16
W
Hz
-
1
/
2
at expected sky loadings, which are photon noise dominated. Based on these results, we plan to deploy a six-spectrometer demonstration instrument to the Large Millimeter Telescope in early 2020.</description><subject>Broadband</subject><subject>Characterization and Evaluation of Materials</subject><subject>Condensed Matter Physics</subject><subject>Detectors</subject><subject>Filter banks</subject><subject>Ground-based observation</subject><subject>Inductance</subject><subject>kinetic inductance detectors</subject><subject>Large Millimeter Telescope</subject><subject>Low temperature physics</subject><subject>Magnetic Materials</subject><subject>Magnetism</subject><subject>Mapping</subject><subject>Millimeter waves</subject><subject>NEP</subject><subject>Noise</subject><subject>OTHER INSTRUMENTATION</subject><subject>Photons</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Red shift</subject><subject>ROACH2</subject><subject>Spectrographs</subject><subject>spectrometer</subject><subject>Spectrometers</subject><subject>SuperSpec</subject><issn>0022-2291</issn><issn>1573-7357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWKt_wNOi5-jko0lzLNVWoVihit5Cms7aLd3NmmyF_nu3ruDNwzAwPO_L8BByyeCGAejbxMCAocChHQmayiPSYwMtqBYDfUx6AJxTzg07JWcpbQDADJXokffJbruloxjdPnsKRcLsGWMeYukqj1nIszust2FfYtXQaXQrzBa7GuOiRp-VJX1zX5jNKzpeF3V2ODYxlNhgTOfkJHfbhBe_u09eJ_cv4wc6m08fx6MZ9ZLxhjJcLjlKzYbKIbplbpChMitnjHPegeReec6XciWFyoccJHMuB2eUEMg9E31y1fWG1BQ2-aJBv_ahqtpfLNNKg5QtdN1BdQyfO0yN3YRdrNq_LBdGGcZBq5biHeVjSClibutYlC7uLQN70Gw7zbbVbH8020O16EKphasPjH_V_6S-ASdhf6k</recordid><startdate>20200501</startdate><enddate>20200501</enddate><creator>Karkare, K. S.</creator><creator>Barry, P. S.</creator><creator>Bradford, C. M.</creator><creator>Chapman, S.</creator><creator>Doyle, S.</creator><creator>Glenn, J.</creator><creator>Gordon, S.</creator><creator>Hailey-Dunsheath, S.</creator><creator>Janssen, R. M. J.</creator><creator>Kovács, A.</creator><creator>LeDuc, H. G.</creator><creator>Mauskopf, P.</creator><creator>McGeehan, R.</creator><creator>Redford, J.</creator><creator>Shirokoff, E.</creator><creator>Tucker, C.</creator><creator>Wheeler, J.</creator><creator>Zmuidzinas, J.</creator><general>Springer US</general><general>Springer Nature B.V</general><general>Springer</general><scope>AAYXX</scope><scope>CITATION</scope><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-5215-6993</orcidid><orcidid>https://orcid.org/0000000252156993</orcidid></search><sort><creationdate>20200501</creationdate><title>Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers</title><author>Karkare, K. S. ; Barry, P. S. ; Bradford, C. M. ; Chapman, S. ; Doyle, S. ; Glenn, J. ; Gordon, S. ; Hailey-Dunsheath, S. ; Janssen, R. M. J. ; Kovács, A. ; LeDuc, H. G. ; Mauskopf, P. ; McGeehan, R. ; Redford, J. ; Shirokoff, E. ; Tucker, C. ; Wheeler, J. ; Zmuidzinas, J.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c412t-1ebb2e47186aeeabf9e1e69da99aaca042c6c22b4d436f82041aaf0a9633e2c13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Broadband</topic><topic>Characterization and Evaluation of Materials</topic><topic>Condensed Matter Physics</topic><topic>Detectors</topic><topic>Filter banks</topic><topic>Ground-based observation</topic><topic>Inductance</topic><topic>kinetic inductance detectors</topic><topic>Large Millimeter Telescope</topic><topic>Low temperature physics</topic><topic>Magnetic Materials</topic><topic>Magnetism</topic><topic>Mapping</topic><topic>Millimeter waves</topic><topic>NEP</topic><topic>Noise</topic><topic>OTHER INSTRUMENTATION</topic><topic>Photons</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Red shift</topic><topic>ROACH2</topic><topic>Spectrographs</topic><topic>spectrometer</topic><topic>Spectrometers</topic><topic>SuperSpec</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Karkare, K. S.</creatorcontrib><creatorcontrib>Barry, P. S.</creatorcontrib><creatorcontrib>Bradford, C. M.</creatorcontrib><creatorcontrib>Chapman, S.</creatorcontrib><creatorcontrib>Doyle, S.</creatorcontrib><creatorcontrib>Glenn, J.</creatorcontrib><creatorcontrib>Gordon, S.</creatorcontrib><creatorcontrib>Hailey-Dunsheath, S.</creatorcontrib><creatorcontrib>Janssen, R. M. J.</creatorcontrib><creatorcontrib>Kovács, A.</creatorcontrib><creatorcontrib>LeDuc, H. G.</creatorcontrib><creatorcontrib>Mauskopf, P.</creatorcontrib><creatorcontrib>McGeehan, R.</creatorcontrib><creatorcontrib>Redford, J.</creatorcontrib><creatorcontrib>Shirokoff, E.</creatorcontrib><creatorcontrib>Tucker, C.</creatorcontrib><creatorcontrib>Wheeler, J.</creatorcontrib><creatorcontrib>Zmuidzinas, J.</creatorcontrib><creatorcontrib>Argonne National Laboratory (ANL), Argonne, IL (United States)</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Journal of low temperature physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Karkare, K. S.</au><au>Barry, P. S.</au><au>Bradford, C. M.</au><au>Chapman, S.</au><au>Doyle, S.</au><au>Glenn, J.</au><au>Gordon, S.</au><au>Hailey-Dunsheath, S.</au><au>Janssen, R. M. J.</au><au>Kovács, A.</au><au>LeDuc, H. G.</au><au>Mauskopf, P.</au><au>McGeehan, R.</au><au>Redford, J.</au><au>Shirokoff, E.</au><au>Tucker, C.</au><au>Wheeler, J.</au><au>Zmuidzinas, J.</au><aucorp>Argonne National Laboratory (ANL), Argonne, IL (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers</atitle><jtitle>Journal of low temperature physics</jtitle><stitle>J Low Temp Phys</stitle><date>2020-05-01</date><risdate>2020</risdate><volume>199</volume><issue>3-4</issue><spage>849</spage><epage>857</epage><pages>849-857</pages><issn>0022-2291</issn><eissn>1573-7357</eissn><abstract>SuperSpec is an on-chip filter bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors. SuperSpec technology will enable large-format spectroscopic integral field units suitable for high-redshift line intensity mapping and multi-object spectrographs. In previous results, we have demonstrated noise performance in individual detectors suitable for photon noise-limited ground-based observations at excellent mm-wave sites. In these proceedings, we present the noise performance of a full
R
∼
275
spectrometer measured using deployment-ready RF hardware and software. We report typical noise equivalent powers through the full device of
∼
3
×
10
-
16
W
Hz
-
1
/
2
at expected sky loadings, which are photon noise dominated. Based on these results, we plan to deploy a six-spectrometer demonstration instrument to the Large Millimeter Telescope in early 2020.</abstract><cop>New York</cop><pub>Springer US</pub><doi>10.1007/s10909-020-02407-4</doi><tpages>9</tpages><orcidid>https://orcid.org/0000-0002-5215-6993</orcidid><orcidid>https://orcid.org/0000000252156993</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0022-2291 |
| ispartof | Journal of low temperature physics, 2020-05, Vol.199 (3-4), p.849-857 |
| issn | 0022-2291 1573-7357 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1767044 |
| source | Springer Online Journals |
| subjects | Broadband Characterization and Evaluation of Materials Condensed Matter Physics Detectors Filter banks Ground-based observation Inductance kinetic inductance detectors Large Millimeter Telescope Low temperature physics Magnetic Materials Magnetism Mapping Millimeter waves NEP Noise OTHER INSTRUMENTATION Photons Physics Physics and Astronomy Red shift ROACH2 Spectrographs spectrometer Spectrometers SuperSpec |
| title | Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-04T19%3A34%3A45IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Full-Array%20Noise%20Performance%20of%20Deployment-Grade%20SuperSpec%20mm-Wave%20On-Chip%20Spectrometers&rft.jtitle=Journal%20of%20low%20temperature%20physics&rft.au=Karkare,%20K.%20S.&rft.aucorp=Argonne%20National%20Laboratory%20(ANL),%20Argonne,%20IL%20(United%20States)&rft.date=2020-05-01&rft.volume=199&rft.issue=3-4&rft.spage=849&rft.epage=857&rft.pages=849-857&rft.issn=0022-2291&rft.eissn=1573-7357&rft_id=info:doi/10.1007/s10909-020-02407-4&rft_dat=%3Cproquest_osti_%3E2396912076%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2396912076&rft_id=info:pmid/&rfr_iscdi=true |