[
    {
        "id": "authors:2e09p-hjt94",
        "collection": "authors",
        "collection_id": "2e09p-hjt94",
        "cite_using_url": "https://authors.library.caltech.edu/records/2e09p-hjt94",
        "type": "conference_item",
        "title": "Highly sensitive far-IR KIDs for PRIMA: optical characterization of a 25-micron array",
        "book_title": "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII",
        "author": [
            {
                "family_name": "Foote",
                "given_name": "Logan M.",
                "orcid": "0000-0002-4162-8609",
                "clpid": "Foote-Logan"
            },
            {
                "family_name": "Albert",
                "given_name": "Chris",
                "clpid": "Albert-Chris"
            },
            {
                "family_name": "Basu Thakur",
                "given_name": "Ritoban",
                "orcid": "0000-0002-3351-3078",
                "clpid": "Basu-Thakur-Ritoban"
            },
            {
                "family_name": "Day",
                "given_name": "Peter K.",
                "orcid": "0000-0002-3670-9017"
            },
            {
                "family_name": "Cothard",
                "given_name": "Nicholas F.",
                "orcid": "0000-0002-6151-6292",
                "clpid": "Cothard-Nicholas-F"
            },
            {
                "family_name": "Hailey-Dunsheath",
                "given_name": "Steve",
                "orcid": "0000-0002-8504-7988",
                "clpid": "Hailey-Dunsheath-S"
            },
            {
                "family_name": "Echternach",
                "given_name": "Pierre M.",
                "orcid": "0000-0001-9643-5110",
                "clpid": "Echternach-Pierre-M"
            },
            {
                "family_name": "Eom",
                "given_name": "Byeong Ho",
                "orcid": "0000-0002-0976-0861",
                "clpid": "Eom-Byeong-Ho"
            },
            {
                "family_name": "Janssen",
                "given_name": "Reinier M. J.",
                "orcid": "0000-0001-9122-9668",
                "clpid": "Janssen-Reinier-M-J"
            },
            {
                "family_name": "Kane",
                "given_name": "Elijah",
                "clpid": "Kane-Elijah"
            },
            {
                "family_name": "Leduc",
                "given_name": "Henry G.",
                "orcid": "0000-0002-6721-5271",
                "clpid": "Leduc-Henry-G"
            },
            {
                "family_name": "Liu",
                "given_name": "Lun-Jun",
                "orcid": "0009-0004-1270-2373",
                "clpid": "Liu-Lun-Jun"
            },
            {
                "family_name": "Nguyen",
                "given_name": "Hien T.",
                "clpid": "Nguyen-Hien-T"
            },
            {
                "family_name": "Glenn",
                "given_name": "Jason",
                "orcid": "0000-0001-7527-2017"
            },
            {
                "family_name": "Bradford",
                "given_name": "Charles M.",
                "orcid": "0000-0001-5261-7094",
                "clpid": "Bradford-C-M"
            },
            {
                "family_name": "Zmuidzinas",
                "given_name": "Jonas",
                "orcid": "0000-0002-3330-5439",
                "clpid": "Zmuidzinas-J"
            }
        ],
        "editor": [
            {
                "family_name": "Zmuidzinas",
                "given_name": "Jonas"
            },
            {
                "family_name": "Gao",
                "given_name": "Jian-Rong"
            }
        ],
        "abstract": "<div class=\"DetailStyles-module__abstractContent___KAqNh\">\n<div>The PRobe far-Infrared Mission for Astrophysics (PRIMA) is a future cryogenic space observatory that will revolutionize study of evolving galaxies and forming planetary systems with highly-sensitive far-infrared (far-IR) imaging and spectroscopy. PRIMA&rsquo;s spectrometer, the Far-InfraRed Enhanced Survey Spectrometer (FIRESS), will deploy kilo-pixel aluminum kinetic inductance detector (KID) arrays covering wavelengths from 24-235 &mu;m. Here we present optical characterization of a prototype FIRESS array operating at 25 &mu;m. We employ a blackbody modulation technique to measure the detector responsivity, and discuss methods for reducing 1/f noise from the multi-tone readout electronics. We measure an NEP below 3.5 &times; 10<sup>&minus;20</sup> W/ &radic; Hz at 10 Hz accross the array, which exceeds the requirement to be limited by the astrophysical background limit for PRIMA&rsquo;s FIRESS spectrometer. We discuss limitations of the multi-tone readout and compare results to measurements with a single-tone readout system.</div>\n</div>",
        "doi": "10.1117/12.3020228",
        "isbn": "9781510675278",
        "publisher": "SPIE",
        "place_of_publication": "Bellingham, WA",
        "publication_date": "2024-08-16",
        "pages": "131020D"
    },
    {
        "id": "authors:hnmyx-er004",
        "collection": "authors",
        "collection_id": "hnmyx-er004",
        "cite_using_url": "https://authors.library.caltech.edu/records/hnmyx-er004",
        "type": "conference_item",
        "title": "Development of an ultra-sensitive 210-micron array of KIDs for far-IR astronomy",
        "book_title": "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII",
        "author": [
            {
                "family_name": "Kane",
                "given_name": "Elijah",
                "clpid": "Kane-Elijah"
            },
            {
                "family_name": "Albert",
                "given_name": "Chris",
                "clpid": "Albert-Chris"
            },
            {
                "family_name": "Cothard",
                "given_name": "Nicholas F.",
                "orcid": "0000-0002-6151-6292"
            },
            {
                "family_name": "Hailey-Dunsheath",
                "given_name": "Steve",
                "orcid": "0000-0002-8504-7988",
                "clpid": "Hailey-Dunsheath-S"
            },
            {
                "family_name": "Echternach",
                "given_name": "Pierre M.",
                "orcid": "0000-0001-9643-5110",
                "clpid": "Echternach-Pierre-M"
            },
            {
                "family_name": "Foote",
                "given_name": "Logan M.",
                "orcid": "0000-0002-4162-8609",
                "clpid": "Foote-Logan"
            },
            {
                "family_name": "Janssen",
                "given_name": "Reinier M. J.",
                "orcid": "0000-0001-9122-9668",
                "clpid": "Janssen-Reinier-M-J"
            },
            {
                "family_name": "LeDuc",
                "given_name": "Henry G.",
                "orcid": "0000-0002-6721-5271",
                "clpid": "LeDuc-Henry-G"
            },
            {
                "family_name": "Liu",
                "given_name": "Lun-Jun",
                "orcid": "0009-0004-1270-2373",
                "clpid": "Liu-Lun-Jun"
            },
            {
                "family_name": "Nguyen",
                "given_name": "Hien T.",
                "clpid": "Nguyen-Hien-T"
            },
            {
                "family_name": "Glenn",
                "given_name": "Jason",
                "orcid": "0000-0001-7527-2017"
            },
            {
                "family_name": "Bradford",
                "given_name": "Charles M.",
                "orcid": "0000-0001-5261-7094",
                "clpid": "Bradford-C-M"
            },
            {
                "family_name": "Zmuidzinas",
                "given_name": "Jonas",
                "orcid": "0000-0002-3330-5439",
                "clpid": "Zmuidzinas-J"
            }
        ],
        "editor": [
            {
                "family_name": "Zmuidzinas",
                "given_name": "Jonas"
            },
            {
                "family_name": "Gao",
                "given_name": "Jian-Rong"
            }
        ],
        "abstract": "<div class=\"DetailStyles-module__abstractContent___KAqNh\">\n<div>The Probe far-Infrared Mission for Astrophysics (PRIMA) is a proposed space observatory which will use arrays of thousands of kinetic inductance detectors (KIDs) to perform low- and moderate-resolution spectroscopy throughout the far-infrared. The detectors must have noise equivalent powers (NEPs) at or below 1&times;10<sup>&minus;19</sup>&nbsp;W Hz<sup>&minus;1/2</sup>&nbsp;to be subdominant to noise from sky backgrounds and thermal noise from PRIMA&rsquo;s cryogenically cooled primary mirror. Using a Radio Frequency System on a Chip for multitone readout, we measure the NEPs of detectors on a flight-like array designed to observe at a wavelength of 210 &mu;m. We find that 92% of the KIDs measured have an NEP below 1 &times; 10<sup>&minus;19</sup>&nbsp;W Hz<sup>&minus;1/2</sup> at a noise frequency of 10 Hz.</div>\n</div>",
        "doi": "10.1117/12.3020346",
        "isbn": "9781510675278",
        "publisher": "SPIE",
        "place_of_publication": "Bellingham, WA",
        "publication_date": "2024-08-16",
        "pages": "131021K"
    }
]