E
Erica J. Nelson
Researcher at Harvard University
Publications - 160
Citations - 11405
Erica J. Nelson is an academic researcher from Harvard University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 44, co-authored 105 publications receiving 9623 citations. Previous affiliations of Erica J. Nelson include Yale University & Max Planck Society.
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Journal ArticleDOI
3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE–MASS DISTRIBUTION SINCE z = 3
A. van der Wel,Marijn Franx,P. G. van Dokkum,Rosalind E. Skelton,Ivelina Momcheva,Katherine E. Whitaker,Gabriel B. Brammer,Eric F. Bell,Hans-Walter Rix,Stijn Wuyts,Henry C. Ferguson,Bradford P. Holden,Guillermo Barro,Anton M. Koekemoer,Yu-Yen Chang,Elizabeth J. McGrath,B. Haussler,B. Haussler,Avishai Dekel,Peter Behroozi,Michele Fumagalli,Joel Leja,Britt Lundgren,Michael V. Maseda,Erica J. Nelson,David A. Wake,David A. Wake,Shannon G. Patel,Ivo Labbé,Sandra M. Faber,Norman A. Grogin,Dale D. Kocevski +31 more
TL;DR: In this paper, the galaxy size-mass distribution over the redshift range 0 3 × 10{sup 9} M {sub ☉}, and steep, R{sub eff}∝M{sub ∗}{sup 0.75}, for early-type galaxies with stellar mass > 2 × 10,sup 10} M{sub ǫ, and the intrinsic scattermore is ≲0.2 dex for all galaxy types and redshifts.
Journal ArticleDOI
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
Rosalind E. Skelton,Katherine E. Whitaker,Ivelina Momcheva,Gabriel B. Brammer,Pieter G. van Dokkum,Ivo Labbé,Marijn Franx,Arjen van der Wel,Rachel Bezanson,Rachel Bezanson,Elisabete da Cunha,Mattia Fumagalli,Natascha M. Förster Schreiber,Mariska Kriek,Joel Leja,Britt Lundgren,Daniel Magee,Danilo Marchesini,Michael V. Maseda,Erica J. Nelson,Pascal Oesch,Camilla Pacifici,Shannon G. Patel,Sedona H. Price,Hans-Walter Rix,Tomer Tal,David A. Wake,David A. Wake,Stijn Wuyts +28 more
TL;DR: In this paper, a photometric analysis of the CANDELS and 3D-HST HST imaging and the ancillary imaging data at wavelengths 0.3-8 μm is presented, where objects were selected in the WFC3 near-IR bands and their spectral energy distributions were determined by carefully taking the effects of the point-spread function in each observation into account.
Journal ArticleDOI
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies
Ivelina Momcheva,Gabriel B. Brammer,Pieter van Dokkum,Rosalind E. Skelton,Katherine E. Whitaker,Erica J. Nelson,Mattia Fumagalli,Michael V. Maseda,Joel Leja,Marijn Franx,Hans-Walter Rix,Rachel Bezanson,Elisabete da Cunha,Claire Dickey,Natascha M. Förster Schreiber,Garth D. Illingworth,Mariska Kriek,Ivo Labbé,Johannes U. Lange,Britt Lundgren,Daniel Magee,Danilo Marchesini,Pascal Oesch,Camilla Pacifici,Shannon G. Patel,Sedona H. Price,Tomer Tal,David A. Wake,Arjen van der Wel,Stijn Wuyts +29 more
TL;DR: In this article, the authors presented reduced data and data products from the 3D-HST survey, a 248-orbit HST Treasury program, which obtained WFC3 G141 grism spectroscopy in four of the five CANDELS fields: AEGIS, COSMOS, GOODS-S, and UDS, along with WFC 3 $H 140$ imaging.
Journal ArticleDOI
The 3d-hst survey: hubble space telescope wfc3/g141 grism spectra, redshifts, and emission line measurements for ∼100,000 galaxies
Ivelina Momcheva,Gabriel B. Brammer,Pieter van Dokkum,Rosalind E. Skelton,Katherine E. Whitaker,Erica J. Nelson,Mattia Fumagalli,Michael V. Maseda,Joel Leja,Marijn Franx,Hans-Walter Rix,Rachel Bezanson,Elisabete da Cunha,Claire Dickey,Natascha M. Förster Schreiber,Garth D. Illingworth,Mariska Kriek,Ivo Labbé,Johannes U. Lange,Britt Lundgren,Daniel Magee,Danilo Marchesini,Pascal Oesch,Camilla Pacifici,Shannon G. Patel,Sedona H. Price,Tomer Tal,David A. Wake,David A. Wake,Arjen van der Wel,Stijn Wuyts +30 more
TL;DR: The 3D-HST Treasury Program as mentioned in this paper has been used for the 3D design of the HST's three-dimensional (3D) HST-HWST array.
Journal ArticleDOI
The KMOS3D survey: design, first results, and the evolution of galaxy kinematics from 0.7 ≤ z ≤ 2.7
Emily Wisnioski,N. M. Förster Schreiber,Stijn Wuyts,E. Wuyts,K. Bandara,David J. Wilman,R. Genzel,Ralf Bender,Ric Davies,Matteo Fossati,Philipp Lang,J. T. Mendel,Alessandra Beifiori,Gabriel B. Brammer,Jeffrey C. C. Chan,M. H. Fabricius,Y. Fudamoto,Sandesh K. Kulkarni,Jaron Kurk,Dieter Lutz,Erica J. Nelson,Ivelina Momcheva,David J. Rosario,R. P. Saglia,Stella Seitz,Linda J. Tacconi,P. G. van Dokkum +26 more
TL;DR: In this article, the authors present the KMOS3D survey, a new integral field survey of over 600 galaxies at 0.7 1, implying that the star-forming main sequence is primarily composed of rotating galaxies at both redshift regimes.