Results 1 to 10 of about 1,514,532 (341)

Observation of high-energy neutrinos from the Galactic plane [PDF]

open access: yesScience, 2023
The origin of high-energy cosmic rays, atomic nuclei that continuously impact Earth’s atmosphere, is unknown. Because of deflection by interstellar magnetic fields, cosmic rays produced within the Milky Way arrive at Earth from random directions. However,
R. Abbasi   +388 more
exaly   +2 more sources

Chasing the identification of ASCA Galactic Objects (ChIcAGO): An X-ray survey of unidentified sources in the galactic plane. I : Source sample and initial results [PDF]

open access: bronze, 2013
We present the Chasing the Identification of ASCA Galactic Objects (ChIcAGO) survey, which is designed to identify the unknown X-ray sources discovered during the ASCA Galactic Plane Survey (AGPS).
Anderson, G.E.   +20 more
core   +6 more sources

Measurement of Ultra-High-Energy Diffuse Gamma-Ray Emission of the Galactic Plane from 10 TeV to 1 PeV with LHAASO-KM2A. [PDF]

open access: yesPhysical Review Letters, 2023
The diffuse Galactic γ-ray emission, mainly produced via interactions between cosmic rays and the interstellar medium and/or radiation field, is a very important probe of the distribution, propagation, and interaction of cosmic rays in the Milky Way.
Z. Cao   +278 more
semanticscholar   +1 more source

The SARAO MeerKAT 1.3 GHz Galactic Plane Survey [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
We present the SARAO MeerKAT Galactic Plane Survey (SMGPS), a 1.3 GHz continuum survey of almost half of the Galactic Plane (251○ ≤l ≤ 358○ and 2○ ≤l ≤ 61○ at |b| ≤ 1${_{.}^{\circ}}$5).
S. Goedhart   +129 more
semanticscholar   +1 more source

The FAST Galactic Plane Pulsar Snapshot survey: I. Project design and pulsar discoveries [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2021
Discovery of pulsars is one of the main goals for large radio telescopes. The Five-hundred-meter Aperture Spherical radio Telescope (FAST), that incorporates an L-band 19-beam receiver with a system temperature of about 20 K, is the most sensitive radio ...
J. Han   +36 more
semanticscholar   +1 more source

A global view on star formation: The GLOSTAR Galactic plane survey [PDF]

open access: yesAstronomy & Astrophysics, 2021
Context. The properties of the population of Galactic supernova remnants (SNRs) are essential to our understanding of the dynamics of the interstellar medium (ISM) in the Milky Way. However, the completeness of the catalog of Galactic SNRs is expected to
R. Dokara   +19 more
semanticscholar   +1 more source

Finding Quasars behind the Galactic Plane. I. Candidate Selections with Transfer Learning [PDF]

open access: yesAstrophysical Journal Supplement Series, 2021
Quasars behind the Galactic plane (GPQs) are important astrometric references and useful probes of Milky Way gas. However, the search for GPQs is difficult due to large extinctions and high source densities in the Galactic plane.
Yuming Fu   +6 more
semanticscholar   +1 more source

Survey of the Galactic Plane with the Cherenkov Telescope Array [PDF]

open access: yesInternational Conference on Rebooting Computing, 2021
Max-Planck-Institut fur Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany IRAP, Université de Toulouse, CNRS, UPS, CNES, F-31028 Toulouse, France AIM, CEA, CNRS, Université Paris-Saclay, Université Paris Diderot, Sorbonne Paris Cité, F-91191 Gif ...
Q. Remy   +6 more
semanticscholar   +1 more source

Update on the indication of a mass-dependent anisotropy above 1018.7 eV in the hybrid data of the Pierre Auger Observatory [PDF]

open access: yesEPJ Web of Conferences, 2023
We test for an anisotropy in the mass of arriving cosmic-ray primaries associated with the galactic plane. The sensitivity to primary mass is obtained through the depth of shower maximum, X max, extracted from hybrid events measured over a 14-year period
Mayotte Eric, Fitoussi Thomas
doaj   +1 more source

Microlensing Optical Depth and Event Rate in the OGLE-IV Galactic Plane Fields [PDF]

open access: yesAstrophysical Journal Supplement Series, 2020
Searches for gravitational microlensing events are traditionally concentrated on the central regions of the Galactic bulge but many microlensing events are expected to occur in the Galactic plane, far from the Galactic Center.
P. Mróz   +12 more
semanticscholar   +1 more source

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