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SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY

Title: SEARCH for TeV GAMMA-RAY EMISSION from POINT-LIKE SOURCES in the INNER GALACTIC PLANE with A PARTIAL CONFIGURATION of the HAWC OBSERVATORY
Authors: Abeysekara, AU; Abeysekara, AU; Alfaro, R; Alvarez, C; Alvarez, JD; Arceo, R; Arteaga-Velá Zquez, JC; Solares, HAA; Barber, AS; Baughman, BM; Bautista-Elivar, N; Reyes, ADB; Belmont, E; Benzvi, SY; Bernal, A; Braun, J; Caballero-Mora, KS; Capistrán, T; Carraminana, A; Casanova, S; Castillo, M; Cotti, U; Cotzomi, J; León, SCD; Fuente, EDL; León, CD; Deyoung, T; Diaz Hernandez, R; Dingus, BL; Duvernois, MA; Ellsworth, RW; Enriquez-Rivera, O; Fiorino, DW; Fraija, N; Garfias, F; González, MM; Goodman, JA; Gussert, M; Hampel-Arias, Z; Harding, JP; Hernandez, S; Hüntemeyer, P; Hui, CM; Imran, A; Iriarte, A; Karn, P; Kieda, D; Lara, A; Lauer, RJ; Lee, WH; Lennarz, D; Vargas, HL; Linnemann, JT; Longo, M; Raya, GL; Malone, K; Marinelli, A; Marinelli, SS; Martinez, H; Martinez, O; Martinez-Castro, J; Matthews, JA; Miranda-Romagnoli, P; Moreno, E; Mostafá, M; Nellen, L; Newbold, M; Noriega-Papaqui, R; Patricelli, B; Pelayo, R; Pérez-Pérez, EG; Pretz, J; Ren, Z; Riviere, C; Rosa-González, D; Salazar, H; Greus, FS; Sandoval, A; Schneider, M; Sinnis, G; Smith, AJ; Woodle, KS; Springer, RW; Taboada, I; Tibolla, O; Tollefson, K; Torres, I; Ukwatta, TN; Villasenor, L; Vrabel, K; Weisgarber, T; Westerhoff, S; Wisher, IG; Wood, J; Yapici, T; Yodh, GB; Younk, PW; Zaborov, D; Zepeda, A; Zhou, H
Source: Astrophysical Journal; vol 817, iss 1, 3-3; 0004-637X
Publisher Information: eScholarship, University of California 2016-01-20
Document Type: Electronic Resource
Abstract: A survey of the inner Galaxy region of Galactic longitude l ∈[+15,+50] and latitude b ∈ [-4, +4] is performed using one-third of the High Altitude Water Cherenkov Observatory, operated during ts construction phase. To address the ambiguities arising from unresolved sources in the data, we use a maximum likelihood technique to identify point source candidates. Ten sources and candidate sources are identified in this analysis. Eight of these are associated with known TeV sources but not all have ifferential fluxes that are compatible with previous measurements. Three sources are detected with significances >5 sigma; after accounting for statistical trials, and are associated with known TeV sources.
Index Terms: astroparticle physics; gamma rays: diffuse background; gamma rays: general; astro-ph.HE; Astronomy & Astrophysics; Astronomical and Space Sciences; Atomic; Molecular; Nuclear; Particle and Plasma Physics; Physical Chemistry; Physical Chemistry (incl. Structural); article
URL: https://escholarship.org/uc/item/1pw9z9sc; https://escholarship.org/
Availability: Open access content. Open access content; public
Note: application/pdf; Astrophysical Journal vol 817, iss 1, 3-3 0004-637X
Other Numbers: CDLER oai:escholarship.org:ark:/13030/qt1pw9z9sc; qt1pw9z9sc; https://escholarship.org/uc/item/1pw9z9sc; https://escholarship.org/; 1287337053
Contributing Source: UC MASS DIGITIZATION; From OAIster®, provided by the OCLC Cooperative.
Accession Number: edsoai.on1287337053
Database: OAIster