M
Michael J. Kurtz
Researcher at Harvard University
Publications - 254
Citations - 9369
Michael J. Kurtz is an academic researcher from Harvard University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 51, co-authored 249 publications receiving 8968 citations. Previous affiliations of Michael J. Kurtz include CFA Institute & Smithsonian Astrophysical Observatory.
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Journal ArticleDOI
RVSAO 2.0: Digital Redshifts and Radial Velocities
Michael J. Kurtz,Douglas J. Mink +1 more
TL;DR: In this article, the authors developed a new methodology for building spectral templates for galaxy redshifts, using the new templates for the FAST spectrograph as an example, and showed that a two-dimensional spectral classification of galaxy spectra can be developed using their emission- and absorption-line templates as physically orthogonal basis vectors.
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The Updated Zwicky Catalog (UZC)
Emilio E. Falco,Michael J. Kurtz,Margaret J. Geller,John P. Huchra,J. Peters,Perry Berlind,Douglas J. Mink,Susan Tokarz,Barbara Elwell +8 more
TL;DR: The Zwicky catalog of galaxies (ZC) as discussed by the authors has been the basis for the Center for Astrophysics (CfA) redshift surveys based on it have relied on heterogeneous sets of galaxy coordinates and redshifts.
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Hectospec, the MMT's 300 Optical Fiber-Fed Spectrograph
Daniel G. Fabricant,Robert G. Fata,John Roll,Edward Hertz,Nelson Caldwell,Thomas Gauron,John C. Geary,Brian McLeod,Andrew Szentgyorgyi,Joseph Zajac,Michael J. Kurtz,Jack Barberis,Henry Bergner,Warren R. Brown,Maureen A. Conroy,Roger Eng,Margaret J. Geller,Richard E. Goddard,Michael F. Honsa,Mark Mueller,Douglas J. Mink,Mark Ordway,Susan Tokarz,Deborah Freedman Woods,William F. Wyatt,Harland W. Epps,Ian P. Dell'Antonio +26 more
TL;DR: The Hectospec as discussed by the authors is a 300 optical fiber fed spectrograph, which was used at the MMT for observing configurations within ∼300 s, and to an accuracy of ∼25 μm.
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Discovery of an Unbound Hypervelocity Star in the Milky Way Halo
TL;DR: The first example of a hypervelocity star ejected from the Galactic center, as predicted by Hills and later discussed by Yu & Tremaine, was discovered in this article. But the star's radial velocity vector points 174° from the galactic center, consistent with a Galactic center origin.
Journal ArticleDOI
Discovery of an Unbound Hyper-Velocity Star in the Milky Way Halo
TL;DR: The first example of a hyper-velocity star ejected from the Galactic center as predicted by Hill and later discussed by Yu & Tremaine was discovered in this paper. But the star was a hot blue B9 main sequence star with a heliocentric distance of ~55 kpc.