M
Michael V. Maseda
Researcher at Leiden University
Publications - 151
Citations - 6925
Michael V. Maseda is an academic researcher from Leiden University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 32, co-authored 102 publications receiving 5498 citations. Previous affiliations of Michael V. Maseda include Max Planck Society & University of Wisconsin-Madison.
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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 MUSE Hubble Ultra Deep Field Survey. I. Survey description, data reduction, and source detection
Roland Bacon,Simon Conseil,David Mary,Jarle Brinchmann,Jarle Brinchmann,Martin C. Shepherd,Mohammad Akhlaghi,Peter M. Weilbacher,Laure Piqueras,Lutz Wisotzki,David J. Lagattuta,Benoît Epinat,Benoît Epinat,Adrien Guérou,Adrien Guérou,Hanae Inami,Sebastiano Cantalupo,Jean-Baptiste Courbot,Jean-Baptiste Courbot,Thierry Contini,Johan Richard,Michael V. Maseda,Rychard Bouwens,Nicolas Bouché,Wolfram Kollatschny,Joop Schaye,Raffaella Anna Marino,Roser Pello,Christian Herenz,Bruno Guiderdoni,Marcella Carollo +30 more
TL;DR: The MUSE Hubble Ultra Deep Survey (MUSE-UDSS) dataset as discussed by the authors is the most complete dataset of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h exposure in a single 1.15 arcmin 2 field.