R
Rosalind E. Skelton
Researcher at Yale University
Publications - 134
Citations - 14041
Rosalind E. Skelton is an academic researcher from Yale University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 50, co-authored 128 publications receiving 12159 citations. Previous affiliations of Rosalind E. Skelton include University of Cape Town & 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.
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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
CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 < z < 2.5
Katherine E. Whitaker,Marijn Franx,Joel Leja,Pieter G. van Dokkum,Alaina Henry,Rosalind E. Skelton,Mattia Fumagalli,Ivelina Momcheva,Gabriel B. Brammer,Ivo Labbé,Erica J. Nelson,Jane R. Rigby +11 more
TL;DR: In this article, the authors constrain the slope of the star formation rate (log�) to stellar mass (logM) relation down to log(M⋆/M⊙) = 8.4.
Journal ArticleDOI
3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope
Gabriel B. Brammer,Pieter G. van Dokkum,Marijn Franx,Mattia Fumagalli,Shannon G. Patel,Hans-Walter Rix,Rosalind E. Skelton,Mariska Kriek,Erica J. Nelson,Kasper B. Schmidt,Rachel Bezanson,Elisabete da Cunha,Dawn K. Erb,Xiaohui Fan,Natascha M. Förster Schreiber,Garth D. Illingworth,Ivo Labbé,Joel Leja,Britt Lundgren,Dan Magee,Danilo Marchesini,Patrick J. McCarthy,Ivelina Momcheva,Ivelina Momcheva,Adam Muzzin,Ryan Quadri,Charles C. Steidel,Tomer Tal,David Wake,Katherine E. Whitaker,Anna Williams +30 more
TL;DR: 3D-HST as discussed by the authors is a near-infrared spectroscopic Treasury program with the Hubble Space Telescope for studying the physical processes that shape galaxies in the distant universe.
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.