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R Lopez-Coto

Explore the profile of R Lopez-Coto including associated specialties, affiliations and a list of published articles. Areas
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Articles 10
Citations 15
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Recent Articles
1.
Abe H, Abe S, Acciari V, Aniello T, Ansoldi S, Antonelli L, et al.
Phys Rev Lett . 2023 Feb; 130(6):061002. PMID: 36827578
Linelike features in TeV γ rays constitute a "smoking gun" for TeV-scale particle dark matter and new physics. Probing the Galactic Center region with ground-based Cherenkov telescopes enables the search...
2.
Acciari V, Ansoldi S, Antonelli L, Arbet Engels A, Baack D, Babic A, et al.
Phys Rev Lett . 2020 Jul; 125(2):021301. PMID: 32701326
On January 14, 2019, the Major Atmospheric Gamma Imaging Cherenkov telescopes detected GRB 190114C above 0.2 TeV, recording the most energetic photons ever observed from a gamma-ray burst. We use...
3.
Albert A, Alfaro R, Alvarez C, Angeles Camacho J, Arteaga-Velazquez J, Arunbabu K, et al.
Phys Rev Lett . 2020 Apr; 124(13):131101. PMID: 32302173
Because of the high energies and long distances to the sources, astrophysical observations provide a unique opportunity to test possible signatures of Lorentz invariance violation (LIV). Superluminal LIV enables the...
4.
Abeysekara A, Albert A, Alfaro R, Angeles Camacho J, Arteaga-Velazquez J, Arunbabu K, et al.
Phys Rev Lett . 2020 Feb; 124(2):021102. PMID: 32004015
We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting...
5.
Lopez-Coto R, Parsons R, Hinton J, Giacinti G
Phys Rev Lett . 2019 Jan; 121(25):251106. PMID: 30608860
Cosmic ray electrons and positrons are tracers of particle propagation in the interstellar medium (ISM). A recent measurement performed using the High Energy Stereoscopic System extends the all-electron (electron+positron) spectrum...
6.
Abeysekara A, Albert A, Alfaro R, Alvarez C, Alvarez J, Arceo R, et al.
Nature . 2018 Nov; 564(7736):E38. PMID: 30482938
In this Letter, owing to a production error, the penultimate version of the PDF was published. The HTML version was always correct. The PDF has been corrected online.
7.
Abeysekara A, Albert A, Alfaro R, Alvarez C, Alvarez J, Arceo R, et al.
Nature . 2018 Oct; 562(7725):82-85. PMID: 30283106
SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star)....
8.
Abdallah H, Abramowski A, Aharonian F, Benkhali F, Anguner E, Arakawa M, et al.
Phys Rev Lett . 2018 Jun; 120(20):201101. PMID: 29864326
Spectral lines are among the most powerful signatures for dark matter (DM) annihilation searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the...
9.
Abeysekara A, Albert A, Alfaro R, Alvarez C, Alvarez J, Arceo R, et al.
Science . 2017 Nov; 358(6365):911-914. PMID: 29146808
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using...
10.
Aleksic J, Ansoldi S, Antonelli L, Antoranz P, Babic A, Bangale P, et al.
Science . 2014 Nov; 346(6213):1080-4. PMID: 25378461
Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry but...