[
    {
        "id": "authors:1rxer-jt836",
        "collection": "authors",
        "collection_id": "1rxer-jt836",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190528-131400152",
        "type": "monograph",
        "title": "Census of the Local Universe (CLU) Narrow-Band Survey I: Galaxy Catalogs from Preliminary Fields",
        "author": [
            {
                "family_name": "Cook",
                "given_name": "David O.",
                "orcid": "0000-0002-6877-7655",
                "clpid": "Cook-David-O"
            },
            {
                "family_name": "Kasliwal",
                "given_name": "Mansi M.",
                "orcid": "0000-0002-5619-4938",
                "clpid": "Kasliwal-M-M"
            },
            {
                "family_name": "Van Sistine",
                "given_name": "Angela",
                "orcid": "0000-0003-4131-173X",
                "clpid": "Van-Sistine-A"
            },
            {
                "family_name": "Kaplan",
                "given_name": "David L.",
                "orcid": "0000-0001-6295-2881",
                "clpid": "Kaplan-D-L"
            },
            {
                "family_name": "Sutter",
                "given_name": "Jessica S.",
                "orcid": "0000-0002-9183-8102",
                "clpid": "Sutter-J-S"
            },
            {
                "family_name": "Kupfer",
                "given_name": "Thomas",
                "orcid": "0000-0002-6540-1484",
                "clpid": "Kupfer-T"
            },
            {
                "family_name": "Shupe",
                "given_name": "David L.",
                "orcid": "0000-0003-4401-0430",
                "clpid": "Shupe-David-L"
            },
            {
                "family_name": "Laher",
                "given_name": "Russ R.",
                "orcid": "0000-0003-2451-5482",
                "clpid": "Laher-R-R"
            },
            {
                "family_name": "Masci",
                "given_name": "Frank J.",
                "orcid": "0000-0002-8532-9395",
                "clpid": "Masci-F-J"
            },
            {
                "family_name": "Dale",
                "given_name": "Daniel A.",
                "orcid": "0000-0002-5782-9093",
                "clpid": "Dale-D-A"
            },
            {
                "family_name": "Sesar",
                "given_name": "Branimir",
                "orcid": "0000-0002-0834-3978",
                "clpid": "Sesar-B"
            },
            {
                "family_name": "Brady",
                "given_name": "Patrick R.",
                "orcid": "0000-0002-4611-9387",
                "clpid": "Brady-P-R"
            },
            {
                "family_name": "Yan",
                "given_name": "Lin",
                "orcid": "0000-0003-1710-9339",
                "clpid": "Yan-Lin"
            },
            {
                "family_name": "Ofek",
                "given_name": "Eran O.",
                "orcid": "0000-0002-6786-8774",
                "clpid": "Ofek-E-O"
            },
            {
                "family_name": "Reitze",
                "given_name": "David H.",
                "clpid": "Reitze-D-H"
            },
            {
                "family_name": "Kulkarni",
                "given_name": "Shrinivas R.",
                "orcid": "0000-0001-5390-8563",
                "clpid": "Kulkarni-S-R"
            }
        ],
        "abstract": "We present the Census of the Local Universe (CLU) narrow-band survey to search for emission-line (H\u03b1) galaxies. CLU-H\u03b1 has imaged \u22483\u03c0 of the sky (26,470 deg^2) with 4 narrow-band filters that probe a distance out to 200 Mpc. We have obtained spectroscopic follow-up for galaxy candidates in 14 preliminary fields (101.6 deg^2) to characterize the limits and completeness of the survey. In these preliminary fields, CLU can identify emission lines down to an H\u03b1 flux limit of 10^(\u221214) erg s^(\u22121) cm^(\u22122) at 90\\% completeness, and recovers 83% (67%) of the H\u03b1 flux from catalogued galaxies in our search volume at the \u03a3=2.5 (\u03a3=5) color excess levels. The contamination from galaxies with no emission lines is 61% (12%) for \u03a3=2.5 (\u03a3=5). Also, in the regions of overlap between our preliminary fields and previous emission-line surveys, we recover the majority of the galaxies found in previous surveys and identify an additional \u2248300 galaxies. In total, we find 90 galaxies with no previous distance information, several of which are interesting objects: 7 blue compact dwarfs, 1 green pea, and a Seyfert galaxy; we also identified a known planetary nebula. These objects show that the CLU-H\u03b1 survey can be a discovery machine for objects in our own Galaxy and extreme galaxies out to intermediate redshifts. However, the majority of the CLU-H\u03b1 galaxies identified in this work show properties consistent with normal star-forming galaxies. CLU-H\u03b1 galaxies with new redshifts will be added to existing galaxy catalogs to focus the search for the electromagnetic counterpart to gravitational wave events.",
        "doi": "10.48550/arXiv.1710.05016",
        "publisher": "arXiv",
        "publication_date": "2017-10-13"
    }
]