activity
20052024
most citedX-rays from solar system objects

151 citations · 479 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2024★ 4 cited

High-Resolution Laboratory Measurements of M-shell Fe EUV Line Emission using EBIT-I

Alexander J. Fairchild, Natalie Hell, Peter Beiersdorfer +4

Solar physicists routinely utilize observations of Ar-like Fe IX and Cl-like Fe X emission to study a variety of solar structures. However, unidentified lines exist in the Fe IX an…

astro-ph.SR2019★ 18 cited

Laboratory Calibrations of Fe XII-XIV Line-Intensity Ratios for Electron Density Diagnostics

Thusitha P. Arthanayaka, Peter Beiersdorfer, Gregory V. Brown +5

We have used an electron beam ion trap to measure electron-density-diagnostic line-intensity ratios for extreme ultraviolet lines from F XII, XIII, and XIV at wavelengths of 185-20…

astro-ph.HE2018★ 12 cited

High-resolution Charge Exchange Spectra with L-shell Nickel Show Striking Differences from Models

G. L. Betancourt-Martinez, P. Beiersdorfer, G. V. Brown +7

We present the first high-resolution laboratory spectra of X-ray emission following L-shell charge exchange between nickel ions and neutral H2 and He. We employ the commonly used c…

astro-ph.HE2018★ 9 cited

Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions

Esra Bulbul, Adam Foster, Gregory V. Brown +10

Uncertainties in atomic models will introduce noticeable additional systematics in calculating the flux of weak dielectronic recombination (DR) satellite lines, affecting the detec…

physics.atom-ph2015

Atomic and Molecular Data: Division B / Commission 14

Lyudmila Mashonkina, Farid Salama, Glenn M. Wahlgren +6

Commission 14 has been operating for almost a century. It was one of the 32 Standing IAU Commissions and established in 1919. The main purpose of Commission 14 is to foster interac…

astro-ph.SR2012★ 1 cited

Non-thermal processes in coronae and beyond

K. Poppenhaeger, H. M. Guenther, P. Beiersdorfer +7

This contribution summarizes the splinter session "Non-thermal processes in coronae and beyond" held at the Cool Stars 17 workshop in Barcelona in 2012. It covers new developments…