[
    {
        "id": "authors:38sgn-h0k15",
        "collection": "authors",
        "collection_id": "38sgn-h0k15",
        "cite_using_url": "https://authors.library.caltech.edu/records/38sgn-h0k15",
        "type": "book_section",
        "title": "NEW-MUSIC: The Next-generation Extended-Wavelength MUltiband Sub/millimeter Inductance Camera",
        "book_title": "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII",
        "author": [
            {
                "family_name": "Golwala",
                "given_name": "Sunil R.",
                "orcid": "0000-0002-1098-7174",
                "clpid": "Golwala-S-R"
            },
            {
                "family_name": "Beyer",
                "given_name": "Andrew",
                "orcid": "0000-0002-1045-1652",
                "clpid": "Beyer-Andrew"
            },
            {
                "family_name": "Cunnane",
                "given_name": "Daniel",
                "orcid": "0000-0001-8039-7914",
                "clpid": "Cunnane-Daniel"
            },
            {
                "family_name": "Day",
                "given_name": "Peter K.",
                "orcid": "0000-0002-3670-9017",
                "clpid": "Day-Peter-K"
            },
            {
                "family_name": "Defrance",
                "given_name": "Fabien",
                "orcid": "0000-0002-3746-5296",
                "clpid": "Defrance-Fabien"
            },
            {
                "family_name": "Frez",
                "given_name": "Clifford F.",
                "clpid": "Frez-Clifford-F"
            },
            {
                "family_name": "Huang",
                "given_name": "Xiaolan"
            },
            {
                "family_name": "Kim",
                "given_name": "Junhan",
                "orcid": "0000-0002-4274-9373",
                "clpid": "Kim-Junhan"
            },
            {
                "family_name": "Martin",
                "given_name": "Jean-Marc",
                "orcid": "0000-0002-9418-3420",
                "clpid": "Martin-Jean-Marc"
            },
            {
                "family_name": "Sayers",
                "given_name": "Jack",
                "orcid": "0000-0002-8213-3784",
                "clpid": "Sayers-J"
            },
            {
                "family_name": "Shu",
                "given_name": "Shibo",
                "orcid": "0000-0002-6370-2101"
            },
            {
                "family_name": "Yu",
                "given_name": "Shiling",
                "clpid": "Yu-Shiling"
            }
        ],
        "editor": [
            {
                "family_name": "Zmuidzinas",
                "given_name": "Jonas"
            },
            {
                "family_name": "Gao",
                "given_name": "Jian-Rong"
            }
        ],
        "abstract": "<p>The Next-generation Extended Wavelength-MUltiband Sub/millimeter Inductance Camera (NEW-MUSIC) on the Leighton Chajnantor Telescope (LCT) will be a first-of-its-kind, six-band, transmillimeter-wave (\"trans-mm\") polarimeter covering 2.4 octaves of spectral bandwidth to open a new window on the trans-mm time-domain frontier, in particular new frontiers in energy, density, time, and magnetic field. NEW-MUSIC's broad spectral coverage will also enable the use of the Sunyaev-Zeldovich effects to study accretion, feedback, and dust content in the hot gaseous haloes of galaxies and galaxy clusters. Six-band spectral energy distributions, with polarization information, will yield new insights into stellar and planetary nurseries. NEW-MUSIC will employ hierarchical, phased arrays of polarization-sensitive superconducting slot-dipole antennas, coupled to photolithographic bandpass filters, to nearly optimally populate LCT's 14&prime; field-of-view with six spectral bands over 80&ndash;420 GHz (1:5.25 spectral dynamic range; 2.4 octaves). Light will be routed to Al or AlMn microstripline-coupled, parallel-plate capacitor, lumped-element kinetic inductance detectors (MS-PPC-LEKIDs), an entirely new KID architecture that substantially enhances design flexibility while providing background-limited performance. Innovative, wide-bandwidth, etched silicon structures will be used to antireflection-treat the back-illuminated focal plane. NEW-MUSIC will cost-effectively reuse much of the MUSIC instrument, initially deploying a quarter-scale focal plane capable of the bulk of NEW-MUSIC science followed later by a full-FoV focal plane needed for NEW-MUSIC wide-area survey science.</p>",
        "doi": "10.1117/12.3021175",
        "isbn": "9781510675278",
        "publisher": "SPIE",
        "place_of_publication": "Bellingham, WA",
        "publication": "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII",
        "publication_date": "2024-08-16",
        "volume": "13102",
        "pages": "1310202"
    }
]