S
Susan G. Neff
Researcher at Goddard Space Flight Center
Publications - 174
Citations - 18806
Susan G. Neff is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 65, co-authored 171 publications receiving 17967 citations. Previous affiliations of Susan G. Neff include Advanced Technology Center.
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Journal ArticleDOI
The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
D. Christopher Martin,James L. Fanson,David Schiminovich,Patrick Morrissey,Peter G. Friedman,Tom A. Barlow,Tim Conrow,Robert Grange,Patrick N. Jelinsky,Bruno Milliard,Oswald H. W. Siegmund,Luciana Bianchi,Yong-Ik Byun,Jose Donas,Karl Forster,Timothy M. Heckman,Young-Wook Lee,Barry F. Madore,Barry F. Madore,Roger F. Malina,Susan G. Neff,R. Michael Rich,Todd Small,Frank Surber,Alexander S. Szalay,Barry Y. Welsh,Ted K. Wyder +26 more
TL;DR: Galaxy Evolution Explorer (GALEX) as mentioned in this paper performed the first space UV sky survey, including imaging and grism surveys in two bands (1350-1750 and 1750-2750?).
Journal ArticleDOI
The calibration and data products of GALEX
Patrick Morrissey,Tim Conrow,Tom A. Barlow,Todd Small,Mark Seibert,Ted K. Wyder,Tamás Budavári,Stéphane Arnouts,Peter G. Friedman,Karl Forster,D. Christopher Martin,Susan G. Neff,David Schiminovich,Luciana Bianchi,Jose Donas,Timothy M. Heckman,Young-Wook Lee,Barry F. Madore,Bruno Milliard,R. Michael Rich,Alexander S. Szalay,Barry Y. Welsh,Sukyoung K. Yi +22 more
TL;DR: Galaxy Evolution Explorer (GALEX) data releases have identical pipeline calibrations that are significantly improved over the GR1 data release, achieving photometric repeatability of 0.05 and 0.03 m(AB) in the FUV and NUV, respectively as mentioned in this paper.
Journal ArticleDOI
The GALEX Ultraviolet Atlas of Nearby Galaxies
Armando Gil de Paz,Armando Gil de Paz,Samuel Boissier,Barry F. Madore,Barry F. Madore,Mark Seibert,Y. H. Joe,Y. H. Joe,Alessandro Boselli,Ted K. Wyder,David A. Thilker,Luciana Bianchi,Soo-Chang Rey,Soo-Chang Rey,R. Michael Rich,Tom A. Barlow,Tim Conrow,Karl Forster,Peter G. Friedman,D. Christopher Martin,Patrick Morrissey,Susan G. Neff,David Schiminovich,Todd Small,Jose Donas,Timothy M. Heckman,Young-Wook Lee,Bruno Milliard,Alexander S. Szalay,Sukyoung K. Yi +29 more
TL;DR: In this article, the authors presented images, integrated photometry, and surface-brightness and color profiles for a total of 1034 nearby galaxies recently observed by the Galaxy Evolution Explorer (GALEX) satellite in its far-ultraviolet (FUV; λ_(eff) = 1516 A) and near-ult ultraviolet (NUV; Δ = 2267 A) bands.
Journal ArticleDOI
The GALEX Ultraviolet Atlas of Nearby Galaxies
A. Gil de Paz,Samuel Boissier,Barry F. Madore,Mark Seibert,Y. H. Joe,A. Boselli,Ted K. Wyder,David A. Thilker,Luciana Bianchi,Soo-Chang Rey,R. M. Rich,Tom A. Barlow,Tim Conrow,Karl Forster,Peter G. Friedman,D. C. Martin,Patrick Morrissey,Susan G. Neff,David Schiminovich,Todd Small,Jose Donas,Timothy M. Heckman,Young-Wook Lee,B. Milliard,Alexander S. Szalay,Sukyoung K. Yi +25 more
TL;DR: In this paper, the authors present images, integrated photometry, surface-brightness and color profiles for a total of 1034 nearby galaxies recently observed by the GALEX satellite in its far-ultraviolet (FUV; 1516A) and near-ult ultraviolet (NUV; 2267A) bands.
Journal ArticleDOI
The UV-Optical Galaxy Color-Magnitude Diagram. I. Basic Properties
Ted K. Wyder,D. Christopher Martin,David Schiminovich,Mark Seibert,Tamás Budavári,Marie Treyer,Tom A. Barlow,Karl Forster,Peter G. Friedman,Patrick Morrissey,Susan G. Neff,Todd Small,Luciana Bianchi,Jose Donas,Timothy M. Heckman,Young-Wook Lee,Barry F. Madore,Bruno Milliard,R. Michael Rich,Alexander S. Szalay,Barry Y. Welsh,Sukyoung K. Yi +21 more
TL;DR: In this article, the bivariate distribution of galaxies as a function of ultraviolet-optical colors and absolute magnitudes in the local universe was analyzed, and it was shown that approximately one-quarter of the color variation along the blue sequence is due to dust, with the remainder due to star formation history.