output
19942026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2016 · astro-ph.SRShow all

18 papers · 2 filters

astro-ph.SR2016★ 14 cited

A 16-Year Photometric Campaign on the Eclipsing Novalike Variable DW Ursae Majoris

D. R. S. Boyd, E. de Miguel, J. Patterson +29

We present an analysis of photometric observations of the eclipsing novalike variable DW UMa made by the CBA consortium between 1999 and 2015. Analysis of 372 new and 260 previousl…

astro-ph.SR2016★ 4 cited

Post-common envelope PN, fundamental or irrelevant?

Orsola De Marco, T. Reichardt, R. Iaconi +6

One in 5 planetary nebulae are ejected from common envelope binary interactions but Kepler Space Telescope results are already showing this proportion to be larger. Their propertie…

astro-ph.SR2016★ 257 cited

The Kepler Follow-Up Observation Program. I. A Catalog of Companions to Kepler Stars from High-Resolution Imaging

E. Furlan, D. R. Ciardi, M. E. Everett +16

We present results from high-resolution, optical to near-IR imaging of host stars of Kepler Objects of Interest (KOIs), identified in the original Kepler field. Part of the data we…

astro-ph.SR2016★ 139 cited

The Mount Wilson Observatory S-index of the Sun

Ricky Egeland, Willie Soon, Sallie Baliunas +3

The most commonly used index of stellar magnetic activity is the instrumental flux scale of singly-ionized calcium H & K line core emission, S, developed by the Mount Wilson Observ…

astro-ph.SR2016★ 25 cited

SCExAO and GPI Band Photometry and Integral Field Spectroscopy of the Young Brown Dwarf Companion to HD 1160

Eugenio V. Garcia, Thayne Currie, Olivier Guyon +51

We present high signal-to-noise ratio, precise photometry and band (\gpiwave~m) spectroscopy of HD 1160 B, a young substellar companion discovered from the Gemini NICI…

astro-ph.SR2016★ 23 cited

A Catalog of Calibrator Stars for Next-Generation Optical Interferometers

Samuel J. Swihart, E. Victor Garcia, Keivan G. Stassun +3

Benchmark stars with known angular diameters are key to calibrating interferometric observations. With the advent of optical interferometry, there is a need for suitably bright, we…