activity
20042012
most citedCatalogs of Hot White Dwarfs in the Milky Way from GALEX's Ultraviolet Sky Surveys. Constraining Stellar Evolution

125 citations · 347 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2012★ 11 cited

A New Grid of Synthetic Spectra for the Analysis of [WC]-type Central Stars of Planetary Nebulae

Graziela R. Keller, James E. Herald, Luciana Bianchi +2

We present a comprehensive grid of synthetic stellar-atmosphere spectra, suitable for the analysis of high resolution spectra of hydrogen-deficient post-Asymptotic Giant Branch (po…

astro-ph.SR2010★ 125 cited

Catalogs of Hot White Dwarfs in the Milky Way from GALEX's Ultraviolet Sky Surveys. Constraining Stellar Evolution

Luciana Bianchi, Boryana Efremova, James Herald +4

We present comprehensive catalogs of hot star candidates in the Milky Way, selected from GALEX far-UV (FUV, 1344-1786 AA) and near-UV (NUV, 1771-2831 AA) imaging. The FUV and NUV p…

astro-ph.CO2009★ 22 cited

Extreme UV QSOs

Luciana Bianchi, John B. Hutchings, Boryana Efremova +3

We present a sample of spectroscopically confirmed QSOs with FUV-NUV color (as measured by GALEX photometry) bluer than canonical QSO templates and than the majority of known QSOs.…

astro-ph2007★ 1 cited

GALEX Ultraviolet photometry of NGC 2420: searching for WDs

C. De Martino, L. Bianchi, I. Pagano +2

We present color-magnitude diagrams of the open cluster NGC 2420, obtained from Galaxy Evolution Explorer (GALEX) ultraviolet images in FUV and NUV bands and Sloan Digital Sky Surv…

astro-ph2006★ 74 cited

Statistical Properties of the GALEX/SDSS matched source catalogs, and classification of the UV sources

Luciana Bianchi, Lino Rodriguez-Merino, Maurice Viton +30

We use the Galaxy Evolution Explorer (GALEX) Medium and All-Sky-Imaging Survey (MIS & AIS) data from the first public data release (GR1), matched to the Sloan Digital Sky Survey (S…

astro-ph2005★ 22 cited

Discovery of NeVII in the Winds of Hot Evolved Stars

J. E. Herald, L. Bianchi, J. D. Hillier

We show that a strong P-Cygni feature seen in the far-UV spectra of some very hot (Teff >~ 85 kK) central stars of planetary nebulae (CSPN), which has been previously identified as…