activity
19982026
most citedA large light-mass component of cosmic rays at 10^{17} - 10^{17.5} eV from radio observations

156 citations · 698 across the 44 of their papers we have counts for

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Showing 2020Show all

7 papers · 1 filter

astro-ph.GA2020★ 13 cited

A search for radio jets from massive young stellar objects. Association of radio jets with H2O and CH3OH masers

U. Kavak, A. Sanchez-Monge, A. Lopez-Sepulcre +5

Recent theoretical and observational studies debate the similarities between the formation process of high-mass (>8 Msun) and low-mass stars. The formation of low-mass star formati…

astro-ph.EP2020★ 12 cited

The surface of (1) Ceres in visible light as seen by Dawn/VIR

B. Rousseau, M. C. De Sanctis, A. Raponi +9

We study the surface of Ceres at visible wavelengths, as observed by the Visible and InfraRed mapping spectrometer (VIR) onboard the Dawn spacecraft, and analyze the variations of…

astro-ph.HE2020★ 41 cited

Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run

K. L. Page, P. A. Evans, A. Tohuvavohu +41

The Neil Gehrels Swift Observatory followed up 18 gravitational wave (GW) triggers from the LIGO/Virgo collaboration during the O3 observing run in 2019/2020, performing approximat…

astro-ph.GA2020★ 23 cited

Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers

Onur Çatmabacak, Robert Feldmann, Daniel Anglés-Alcázar +3

The concurrent growth of supermassive black holes (SMBHs) and their host galaxies remains to be fully explored, especially at high redshift. While often understood as a consequence…

astro-ph.HE2020★ 19 cited

Discovery of delayed spin-up behavior following two large glitches in the Crab pulsar, and the statistics of such processes

M. Y. Ge, S. N. Zhang, F. J. Lu +130

Glitches correspond to sudden jumps of rotation frequency () and its derivative () of pulsars, the origin of which remains not well understood yet, partly because the jum…

astro-ph.HE2020★ 21 cited

High-energy characteristics of the accretion-powered millisecond pulsar IGR J17591-2342 during its 2018 outburst

L. Kuiper, S. S. Tsygankov, M. Falanga +4

IGR J17591-2342 is a recently INTEGRAL discovered accreting millisecond X-ray pulsar that went into outburst around July 21, 2018. To better understand the physics acting in these…