activity
20022025
most citedAn optical bow shock around the nearby millisecond pulsar J2124-3358

44 citations · 121 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025★ 2 cited

Unlocking AGN Variability with Custom ZTF Photometry for High-Fidelity Light Curves and Robust Selection

P. Arévalo, P. Sánchez-Sáez, B. Sotomayor +3

(Abridged)We explore the potential of optical variability selection methods to identify AGN, including those challenging to detect with conventional techniques. Using the unprecede…

astro-ph.GA2022★ 15 cited

Orientation effects on cool gas absorption from gravitational-arc tomography of a z = 0.77 disc galaxy

A. Fernandez-Figueroa, S. Lopez, N. Tejos +11

We use spatially-resolved spectroscopy of a distant giant gravitational arc to test orientation effects on MgII absorption equivalent width (EW) and covering fraction (kappa) in th…

astro-ph.EP2020★ 41 cited

A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887

S. V. Jeffers, S. Dreizler, J. R. Barnes +29

The nearest exoplanets to the Sun are our best possibilities for detailed characterization. We report the discovery of a compact multi-planet system of super-Earths orbiting the ne…

astro-ph2005★ 19 cited

Observations in the 1.3 and 1.5 THz Atmospheric Windows with the Receiver Lab Telescope

D. P. Marrone, R. Blundell, E. Tong +5

The Receiver Lab Telescope (RLT) is a ground-based terahertz telescope; it is currently the only instrument producing astronomical data between 1 and 2 THz. The capabilities of the…

astro-ph2002★ 44 cited

An optical bow shock around the nearby millisecond pulsar J2124-3358

Bryan Gaensler, Heath Jones, Ben Stappers

We report the discovery of an H-alpha-emitting bow-shock nebula powered by the nearby millisecond pulsar J2124-3358. The bow shock is very broad, and is highly asymmetric about the…

astro-ph2002

The nature of ultraluminous X-ray sources in nearby galaxies

T. P. Roberts, M. R. Goad, M. J. Ward +2

The advanced capabilities of the Chandra and XMM-Newton observatories mean that, for the first time, the detailed study of the brightest point-like X-ray sources in nearby galaxies…