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19972026
most citedWhat Powers Ultra-luminous IRAS Galaxies?

1.2k citations · 48.4k across the 319 of their papers we have counts for

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Showing 2020Show all

15 papers · 1 filter

astro-ph.GA2020★ 49 cited

The KMOS Survey: Investigating the Origin of the Elevated Electron Densities in Star-Forming Galaxies at

Rebecca L. Davies, N. M. Förster Schreiber, R. Genzel +24

We investigate what drives the redshift evolution of the typical electron density () in star-forming galaxies, using a sample of 140 galaxies drawn primarily from KMOS$^{\rm 3…

astro-ph.GA2020★ 37 cited

Detection of faint stars near SgrA* with GRAVITY

GRAVITY Collaboration, R. Abuter, A. Amorim +58

The spin of the supermassive black hole that resides at the Galactic Centre can in principle be measured by accurate measurements of the orbits of stars that are much closer to Sgr…

astro-ph.GA2020★ 7 cited

Determining sub-parsec supermassive black hole binary orbits with infrared interferometry

J. Dexter, D. Lutz, T. T. Shimizu +12

Radial velocity monitoring has revealed the presence of moving broad emission lines in some quasars, potentially indicating the presence of a sub-parsec binary system. Phase-refere…

astro-ph.EP2020★ 128 cited

Direct confirmation of the radial-velocity planet Pic c

M. Nowak, S. Lacour, A. -M. Lagrange +90

Methods used to detect giant exoplanets can be broadly divided into two categories: indirect and direct. Indirect methods are more sensitive to planets with a small orbital period,…

astro-ph.GA2020★ 84 cited

The spatially resolved broad line region of IRAS 09149-6206

GRAVITY Collaboration, A. Amorim, W. Brandner +41

We present new near-infrared VLTI/GRAVITY interferometric spectra that spatially resolve the broad Br emission line in the nucleus of the active galaxy IRAS 09149-6206. We use t…

astro-ph.HE2020★ 71 cited

Dynamically important magnetic fields near the event horizon of Sgr A*

GRAVITY Collaboration, A. Jiménez-Rosales, J. Dexter +53

We study the time-variable linear polarisation of Sgr A* during a bright NIR flare observed with the GRAVITY instrument on July 28, 2018. Motivated by the time evolution of both th…