C
Christopher N. A. Willmer
Researcher at University of Arizona
Publications - 110
Citations - 9972
Christopher N. A. Willmer is an academic researcher from University of Arizona. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 42, co-authored 110 publications receiving 9188 citations. Previous affiliations of Christopher N. A. Willmer include Steward Health Care System.
Papers
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Journal ArticleDOI
Star Formation in AEGIS Field Galaxies since z = 1.1: The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-forming Galaxies
Kai G. Noeske,Benjamin J. Weiner,Sandra M. Faber,Casey Papovich,David C. Koo,Rachel S. Somerville,Kevin Bundy,Christopher J. Conselice,Jeffrey A. Newman,David Schiminovich,E. Le Floc'h,Alison L. Coil,George H. Rieke,Jennifer M. Lotz,Joel R. Primack,Pauline Barmby,Michael C. Cooper,Martin Davis,Richard S. Ellis,Giovanni G. Fazio,Puragra Guhathakurta,J.-S. Huang,Susan A. Kassin,D. C. Martin,Andrew C. Phillips,R. M. Rich,Todd Small,Christopher N. A. Willmer,G. W. Wilson +28 more
TL;DR: In this paper, the authors analyzed star formation as a function of stellar mass (M☉) and redshift z in the All-Wavelength Extended Groth Strip International Survey.
Journal ArticleDOI
Galaxy luminosity functions to z∼ 1 from DEEP2 and COMBO-17: Implications for red galaxy formation
Sandra M. Faber,Christopher N. A. Willmer,Christian Wolf,David C. Koo,Benjamin J. Weiner,Jeffrey A. Newman,Myungshin Im,Alison L. Coil,C. Conroy,Michael C. Cooper,Michael Davis,Douglas P. Finkbeiner,Brian F. Gerke,Karl Gebhardt,Edward J. Groth,Puragra Guhathakurta,Justin Harker,Nick Kaiser,Susan A. Kassin,M. Kleinheinrich,N. P. Konidaris,Richard G. Kron,Lihwai Lin,Lihwai Lin,G. A. Luppino,Darren Madgwick,Klaus Meisenheimer,Kai G. Noeske,Andrew C. Phillips,Vicki L. Sarajedini,Ricardo P. Schiavon,Luc Simard,Alexander S. Szalay,Nicole P. Vogt,Renbin Yan +34 more
TL;DR: The DEEP2 and COMBO-17 surveys are compared to study luminosity functions of red and blue galaxies to z ~ 1, and the results imply that the number and total stellar mass of blue galaxies have been substantially constant since z = 1, whereas those of red galaxies (near L*) have been significantly rising as mentioned in this paper.
Journal ArticleDOI
Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation
S. M. Faber,Christopher N. A. Willmer,Christian Wolf,David C. Koo,Ben Weiner,J. A. Newman,Myungshin Im,Alison L. Coil,C. Conroy,M. C. Cooper,Michael Davis,D. P. Finkbeiner,Brian F. Gerke,Karl Gebhardt,Edward J. Groth,P. Guhathakurta,Justin Harker,Nick Kaiser,Susan A. Kassin,M. Kleinheinrich,N. P. Konidaris,L. Lin,G. A. Luppino,Darren Madgwick,K. Meisenheimer K. G. Noeske,Andrew C. Phillips,Vicki L. Sarajedini,Luc Simard,Alexander S. Szalay,N. P. Vogt,R. Yan +30 more
TL;DR: In this paper, the DEEP2 and COMBO-17 surveys are used to study the evolution of the luminosity function of red and blue galaxies to $z \sim 1$ Schechter function fits show that, since $z = 1$, $M^*_B$ dims by $\sim$ 1.3 mag per unit redshift for both color classes, while red galaxies has formally nearly quadrupled.
Journal ArticleDOI
The DEEP2 Galaxy Redshift Survey: The Galaxy Luminosity Function to z ~ 1
Christopher N. A. Willmer,S. M. Faber,David C. Koo,Benjamin J. Weiner,J. A. Newman,Alison L. Coil,A. J. Connolly,C. Conroy,Michael C. Cooper,Michael Davis,Douglas P. Finkbeiner,Brian F. Gerke,Puragra Guhathakurta,Justin Harker,Nick Kaiser,Susan A. Kassin,N. P. Konidaris,L. Lin,G. A. Luppino,Darren Madgwick,Kai G. Noeske,Andrew C. Phillips,Renbin Yan +22 more
TL;DR: The evolution of the B-band galaxy luminosity function is measured using a sample of more than 11,000 galaxies with spectroscopic redshifts from the DEEP2 Redshift Survey.
Journal ArticleDOI
Evolution of the dusty infrared luminosity function from z = 0 to z = 2.3 using observations from Spitzer
Benjamin Magnelli,David Elbaz,Ranga-Ram Chary,Mark Dickinson,D. Le Borgne,David T. Frayer,Christopher N. A. Willmer +6 more
TL;DR: In this paper, the authors derived the infrared luminosity function (LF) over the last 4/5ths of cosmic time using deep 24 and 70 μm imaging of the GOODS North and South fields.