activity
20012023
most citedThe Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey

1.5k citations · 4k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2023★ 3 cited

Metal-poor stars observed with the Magellan Telescope. IV. Neutron-capture element signatures in 27 main-sequence stars

Mohammad K. Mardini, Anna Frebel, Leyatt Betre +3

Based on high-resolution spectra obtained with Magellan/MIKE, we present a chemo-dynamical analysis for 27 near main-sequence turnoff metal-poor stars, including 20 stars analyzed…

astro-ph.SR2017★ 23 cited

The remarkable outburst of the highly evolved post-period-minimum dwarf nova SSS J122221.7-311525

V. V. Neustroev, T. R. Marsh, S. V. Zharikov +22

We report extensive 3-yr multiwavelength observations of the WZ Sge-type dwarf nova SSS J122221.7-311525 during its unusual double superoutburst, the following decline and in quies…

astro-ph.SR2016★ 31 cited

The Gaia-ESO Survey: the inner disk, intermediate-age open cluster Trumpler 23

J. C. Overbeek, E. D. Friel, P. Donati +33

Context: Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a Rgc ~6 kpc. It is in a crowded field very close to the Galactic plane and…

astro-ph.GA2016★ 78 cited

The Gaia-ESO Survey: Probes of the inner disk abundance gradient

H. R. Jacobson, E. D. Friel, L. Jilkova +41

The nature of the metallicity gradient inside the solar circle (R_GC < 8 kpc) is poorly understood, but studies of Cepheids and a small sample of open clusters suggest that it stee…

astro-ph.SR2016★ 27 cited

New Neutron-Capture Measurements in 23 Open Clusters. I. The R-Process

Jamie C. Overbeek, Eileen D. Friel, Heather R. Jacobson

Neutron-capture elements, those with Z > 35, are the least well-understood in terms of nucleosynthesis and formation environments. The rapid neutron-capture, or r-process, elements…

astro-ph.SR2016★ 80 cited

The Gaia-ESO Survey: Sodium and aluminium abundances in giants and dwarfs - Implications for stellar and Galactic chemical evolution

R. Smiljanic, D. Romano, A. Bragaglia +40

Stellar evolution models predict that internal mixing should cause some sodium overabundance at the surface of red giants more massive than ~ 1.5--2.0 Msun. The surface aluminium a…