D
Duilia F. de Mello
Researcher at The Catholic University of America
Publications - 147
Citations - 20036
Duilia F. de Mello is an academic researcher from The Catholic University of America. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 47, co-authored 147 publications receiving 18220 citations. Previous affiliations of Duilia F. de Mello include Chalmers University of Technology & California Institute of Technology.
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Journal ArticleDOI
UVUDF: UV Luminosity Functions at the Cosmic High Noon
Vihang Mehta,Claudia Scarlata,Marc Rafelski,Marc Rafelski,Timothy Gburek,Harry I. Teplitz,Anahita Alavi,Michael Boylan-Kolchin,Steven L. Finkelstein,Jonathan P. Gardner,Norman A. Grogin,Anton M. Koekemoer,Peter Kurczynski,Brian Siana,Alex Codoreanu,Duilia F. de Mello,Duilia F. de Mello,Kyoung-Soo Lee,Emmaris Soto +18 more
TL;DR: In this paper, the authors present the rest-1500 A UV luminosity functions (LF) for star-forming galaxies during the cosmic high noon, the peak of cosmic star formation rate at 1.5 < z < 3.
Journal ArticleDOI
Physical Properties of Sub-galactic Clumps at 0.5 $\leq z \leq$ 1.5 in the UVUDF
Emmaris Soto,Emmaris Soto,Duilia F. de Mello,Duilia F. de Mello,Marc Rafelski,Marc Rafelski,Jonathan P. Gardner,Harry I. Teplitz,Anton M. Koekemoer,Swara Ravindranath,Norman A. Grogin,Claudia Scarlata,P. Kurczynski,Eric Gawiser +13 more
TL;DR: In this paper, the authors measured the photometry of the clumps and determined the mass, age, and star formation rates (SFR) utilizing the SED-fitting code FAST.
Journal ArticleDOI
Star formation in H i tails: HCG 92, HCG 100 and six interacting systems
Duilia F. de Mello,Duilia F. de Mello,F. Urrutia-Viscarra,C. Mendes de Oliveira,S. Torres-Flores,Eleazar R. Carrasco,Eduardo Serra Cypriano +6 more
TL;DR: In this article, the authors present new Gemini spectra of 14 new objects found within the HI tails of Hickson Compact Groups 92 and 100, which confirm that these objects are members of the compact groups and have metallicities close to solar, with an average value of 12+log(O/H)approx.5.
Journal ArticleDOI
Structures of Local Galaxies Compared to High-Redshift Star-Forming Galaxies
Sara Petty,Sara Petty,Duilia F. de Mello,Duilia F. de Mello,Duilia F. de Mello,John S. Gallagher,Jonathan P. Gardner,Jennifer M. Lotz,C. Matt Mountain,Linda J. Smith,Linda J. Smith +10 more
TL;DR: In this paper, the second-order moment of the brightest 20% of the galaxy's flux (M {sub 20}), and the Sersic index (n) were used to classify galaxies as having merger, exponential disk, or bulge-like morphologies.
Journal ArticleDOI
Physical Properties of Sub-galactic Clumps at 0.5 ≤ Z ≤ 1.5 in the UVUDF
Emmaris Soto,Duilia F. de Mello,Marc Rafelski,Jonathan P. Gardner,Harry I. Teplitz,Anton M. Koekemoer,Swara Ravindranath,Norman A. Grogin,Claudia Scarlata,P. Kurczynski,Eric Gawiser +10 more
TL;DR: In this paper, the authors measured the photometry of clumps and determined the mass, age, and star formation rates (SFR) using the spectral energy distribution fitting code FAST.