E
Evan N. Kirby
Researcher at California Institute of Technology
Publications - 223
Citations - 13194
Evan N. Kirby is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Milky Way. The author has an hindex of 58, co-authored 207 publications receiving 11901 citations. Previous affiliations of Evan N. Kirby include Space Telescope Science Institute & University of California, Irvine.
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Journal ArticleDOI
The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts
Jeffrey A. Newman,Michael C. Cooper,Marc Davis,S. M. Faber,Alison L. Coil,Alison L. Coil,Puragra Guhathakurta,David C. Koo,Andrew C. Phillips,Charlie Conroy,Charlie Conroy,Aaron A. Dutton,Douglas P. Finkbeiner,Brian F. Gerke,David J. Rosario,Benjamin J. Weiner,Christopher N. A. Willmer,Renbin Yan,Justin Harker,Susan A. Kassin,Susan A. Kassin,Nicholas P. Konidaris,Kamson Lai,Darren Madgwick,Kai G. Noeske,Gregory D. Wirth,Andrew J. Connolly,Nick Kaiser,Evan N. Kirby,Brian C. Lemaux,Lihwai Lin,Jennifer M. Lotz,Gerard A. Luppino,Christian Marinoni,Daniel J. Matthews,Anne J. Metevier,Ricardo P. Schiavon +36 more
TL;DR: The DEEP2 Galaxy Redshift Survey (DEEP2) as discussed by the authors is the largest high-precision redshift survey of galaxies at z ~ 1 completed to date, covering an area of 2.8 deg^2 divided into four separate fields observed to a limiting apparent magnitude of R_(AB) = 24.1.
Journal ArticleDOI
The Universal Stellar Mass-Stellar Metallicity Relation for Dwarf Galaxies
Evan N. Kirby,Judith G. Cohen,Puragra Guhathakurta,Lucy Cheng,James S. Bullock,Anna Gallazzi,Anna Gallazzi +6 more
TL;DR: In this paper, spectroscopic metallicities of individual stars in seven gas-rich dwarf irregular galaxies (dIrrs) were analyzed and it was shown that dIrrs obey the same mass-metallicity relation as the dwarf spheroidal (dSph) satellites of both the Milky Way and M31: Z_* ∝ M_*^(0.30±0.02).
Journal ArticleDOI
The All-Wavelength Extended Groth Strip International Survey(AEGIS) Data Sets
Mark E. Davis,Puragra Guhathakurta,Nicholas P. Konidaris,Jeffrey A. Newman,M. L. N. Ashby,A. D. Biggs,Pauline Barmby,Kevin Bundy,Scott Chapman,Alison L. Coil,Christopher J. Conselice,Michael C. Cooper,Darren J. Croton,Peter Eisenhardt,Richard S. Ellis,Sandra M. Faber,Taotao Fang,Giovanni G. Fazio,Antonis Georgakakis,Brian F. Gerke,W. M. Goss,Stephen D. J. Gwyn,Justin Harker,Andrew M. Hopkins,J.-S. Huang,Rob Ivison,Susan A. Kassin,Evan N. Kirby,Anton M. Koekemoer,David C. Koo,Elise S. Laird,E. Le Floc'h,Lihwai Lin,Lihwai Lin,Jennifer M. Lotz,Philip J. Marshall,D. C. Martin,Anne J. Metevier,Leonidas A. Moustakas,Kirpal Nandra,Kai G. Noeske,Casey Papovich,Andrew C. Phillips,R. M. Rich,George H. Rieke,Dimitra Rigopoulou,Samir Salim,David Schiminovich,Luc Simard,Ian Smail,Todd Small,Benjamin J. Weiner,Christopher N. A. Willmer,Steven Willner,Gillian Wilson,Edward L. Wright,Renbin Yan +56 more
TL;DR: The All-Wavelength Extended Groth Strip International Survey (AEGIS) as mentioned in this paper was proposed to study the physical properties and evolutionary processes of galaxies at z = 1.5.
Journal ArticleDOI
Uncovering Extremely Metal-Poor Stars in the Milky Way’s Ultrafaint Dwarf Spheroidal Satellite Galaxies*
TL;DR: In this paper, the authors presented the first spectroscopic metallicities at [Fe/H ] < − 3.0 of stars in a dwarf galaxy, with individual stellar metallicities as low as [ Fe/H] = −3.3.
Journal ArticleDOI
Uncovering Extremely Metal-Poor Stars in the Milky Way's Ultra-Faint Dwarf Spheroidal Satellite Galaxies
TL;DR: In this article, the authors presented the first spectroscopic metallicities at [Fe/H] < 3.0 of stars in a dwarf galaxy, with individual stellar metallicities as low as [Fe /H] = -3.3.