Showing 101 - 120 results of 2,070 for search '"American Astronomical Society"', query time: 0.41s Refine Results
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    IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-wave Transient Catalog

    Published 2021
    “…© 2020. The American Astronomical Society. All rights reserved. Using the IceCube Neutrino Observatory, we search for high-energy neutrino emission coincident with compact binary mergers observed by the LIGO and Virgo gravitational-wave (GW) detectors during their first and second observing runs. …”
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  13. 113

    A Search for IceCube Events in the Direction of ANITA Neutrino Candidates by IceCube Collaboration, Arguelles Delgado, Carlos A, Axani, Spencer Nicholas, Collin, G. H., Conrad, Janet Marie, Diaz, Alejandro, Moulai, Marjon H.

    Published 2022
    “…© 2020. The American Astronomical Society. All rights reserved. During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. …”
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  14. 114

    Investigation of Two Fermi -LAT Gamma-Ray Blazars Coincident with High-energy Neutrinos Detected by IceCube

    Published 2021
    “…© 2019. The American Astronomical Society. All rights reserved.. After the identification of the gamma-ray blazar TXS 0506+056 as the first compelling IceCube neutrino source candidate, we perform a systematic analysis of all high-energy neutrino events satisfying the IceCube realtime trigger criteria. …”
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  15. 115

    Thermally Unstable Cooling Stimulated by Uplift: The Spoiler Clusters by Martz, CG, Mcnamara, BR, Nulsen, PEJ, Vantyghem, AN, Gingras, MJ, Babyk, IV, Russell, HR, Edge, AC, McDonald, Michael A., Tamhane, PD, Fabian, AC, Hogan, MT

    Published 2022
    “…© 2020. The American Astronomical Society. All rights reserved. Chandra X-ray observations are analyzed for five galaxy clusters whose atmospheric cooling times, entropy parameters, and ratios of cooling time to freefall time within the central galaxies lie below 1 Gyr, below 30 keV cm2, and between 20 ≲ min(t cool/t ff) ≲ 50, respectively. …”
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  16. 116

    Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-square-degree Survey

    Published 2021
    “…© 2020. The American Astronomical Society. All rights reserved.. We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. …”
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  17. 117

    Unveiling the Merger Dynamics of the Most Massive MaDCoWS Cluster at z = 1.2 from a Multiwavelength Mapping of Its Intracluster Medium Properties

    Published 2021
    “…© 2020. The American Astronomical Society. All rights reserved The characterization of the Intracluster Medium (ICM) properties of high-redshift galaxy clusters is fundamental to our understanding of large-scale structure formation processes. …”
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  18. 118

    A Metal-poor Damped Ly α System at Redshift 6.4 by Bañados, Eduardo, Rauch, Michael, Decarli, Roberto, Farina, Emanuele P, Hennawi, Joseph F, Mazzucchelli, Chiara, Venemans, Bram P, Walter, Fabian, Simcoe, Robert A., Prochaska, J Xavier, Cooper, Thomas, Davies, Frederick B, Chen, Shi-Fan S.

    Published 2022
    “…© 2019. The American Astronomical Society. All rights reserved. We identify a strong Lyα damping wing profile in the spectrum of the quasar P183+05 at z = 6.4386. …”
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  19. 119

    Bright Opportunities for Atmospheric Characterization of Small Planets: Masses and Radii of K2-3 b, c, and d and GJ3470 b from Radial Velocity Measurements and Spitzer Transits by Crossfield, Ian Jm, Berardo, David Anthony

    Published 2022
    “…© 2019. The American Astronomical Society. All rights reserved.. We report improved masses, radii, and densities for four planets in two bright M-dwarf systems, K2-3 and GJ3470, derived from a combination of new radial velocity and transit observations. …”
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  20. 120

    K2-291b: A Rocky Super-Earth in a 2.2 day Orbit

    Published 2021
    “…© 2019. The American Astronomical Society. All rights reserved.. K2-291 is a solar-type star with a radius of R ∗ = 0.899 ±0.034 R and mass of M ∗ = 0.934 ±0.038 M . …”
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