S
Sedona H. Price
Researcher at Max Planck Society
Publications - 143
Citations - 8917
Sedona H. Price is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 41, co-authored 118 publications receiving 6977 citations. Previous affiliations of Sedona H. Price include California Institute of Technology & University of California, Berkeley.
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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.
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The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 ? z ? 3.8
Mariska Kriek,Alice E. Shapley,Naveen A. Reddy,Brian Siana,Alison L. Coil,Bahram Mobasher,William R. Freeman,Laura de Groot,Sedona H. Price,Ryan L. Sanders,Irene Shivaei,Gabriel B. Brammer,Ivelina Momcheva,Rosalind E. Skelton,Pieter G. van Dokkum,Katherine E. Whitaker,James Aird,Mojegan Azadi,Marc Kassis,James S. Bullock,Charlie Conroy,Charlie Conroy,Romeel Davé,Dušan Kereš,Mark R. Krumholz +24 more
TL;DR: The MOSFIRE Deep Evolution Field (MOSDEF) survey as discussed by the authors was the first large-scale deep evolution field (DEDF) survey, which aims to obtain moderate-resolution (R = 3000-3650) rest-frame optical spectra (∼3700-7000 Å) for ∼1500 galaxies at in three well-studied CANDELS fields: AEGIS, COSMOS, and GOODS-N. In addition, 55 additional galaxies were serendipitously detected.
Journal ArticleDOI
THE MOSDEF SURVEY: MEASUREMENTS OF BALMER DECREMENTS AND THE DUST ATTENUATION CURVE AT REDSHIFTS z ∼ 1.4–2.6*
Naveen A. Reddy,Mariska Kriek,Alice E. Shapley,William R. Freeman,Brian Siana,Alison L. Coil,Bahram Mobasher,Sedona H. Price,Ryan L. Sanders,Irene Shivaei +9 more
TL;DR: In this article, the authors used early observations from the MOSFIRE Deep Evolution Field survey (DESF) to measure the dust attenuation curve of z? 2 galaxies and found that the difference in the total attenuation of the ionized gas and stellar continuum correlates strongly with SFR.