Norman Grogin
Johns Hopkins University
13 Papers
135 Citations
Norman Grogin is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 9, co-authored 13 publications. Previous affiliations of Norman Grogin include Max Planck Society & University of California, Santa Cruz.
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Papers
The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates
Guillermo Barro,P. G. Pérez-González,Antonio Cava,Gabriel B. Brammer,Viraj Pandya,Carmen Eliche Moral,P. Esquej,Helena Domínguez-Sánchez,Belen Alcalde Pampliega,Y. Guo,Anton M. Koekemoer,Jonathan R. Trump,Matthew L. N. Ashby,Nicolás Cardiel,Marco Castellano,C. J. Conselice,Mark Dickinson,Timothy Dolch,Jennifer L. Donley,Nestor Espino Briones,S. M. Faber,Giovanni Fazio,Henry C. Ferguson,S. L. Finkelstein,Adriano Fontana,Audrey Galametz,Jonathan P. Gardner,Eric Gawiser,M. Giavalisco,A. Grazian,Norman Grogin,Nimish P. Hathi,Shoubaneh Hemmati,Antonio Hernán-Caballero,D. D. Kocevski,David C. Koo,Dritan Kodra,K. S. Lee,Lihwai Lin,Ray A. Lucas,Bahram Mobasher,Elizabeth J. McGrath,Kirpal Nandra,Hooshang Nayyeri,Jeffrey A. Newman,Janine Pforr,Michael Peth,Marc Rafelski,L. Rodríguez-Muñoz,Mara Salvato,Mauro Stefanon,Arjen van der Wel,Steven P. Willner,Tommy Wiklind,Stijn Wuyts +54 more
TL;DR: In this article, the authors presented a WFC3 F160W (H-band) selected catalog containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts, and stellar parameters derived from the analysis of the multi-wavelength data.
EFFECTS OF DUST GEOMETRY IN Lyα GALAXIES AT z = 4.4
TL;DR: In this paper, the authors investigate the radiative transfer scenario with a new sample of six Ly? galaxy candidates in the GOODS CDF-S, selected at -->z = 4.4.
146
Effects of Dust Geometry in Lyman Alpha Galaxies at z = 4.4
TL;DR: In this article, the authors investigated the effect of a clump of inter-stellar medium (ISM) on the equivalent widths of Lyman alpha galaxies, and found that the EW was enhanced by 50% due to this dust.
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Improved photometric redshifts with surface luminosity priors
Lifang Xia,Seth H. Cohen,Sangeeta Malhotra,James E. Rhoads,Norman Grogin,Nimish P. Hathi,Rogier A. Windhorst,Nor Pirzkal,Chun Xu +8 more
TL;DR: In this article, the authors apply Bayesian statistics with prior probabilities of galaxy surface luminosity (SL) to improve photometric redshifts, and show that the addition of the SL prior probability helps break the degeneracy of SPZ redshift between low redshift 4000 u break galaxies and high redshift Lyman break galaxies which are mostly catastrophic outliers.
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Morphologies and Spectral Energy Distributions of Extremely Red Galaxies in the GOODS-South Field
Leonidas A. Moustakas,Stefano Casertano,Christopher J. Conselice,Mark Dickinson,Peter R. Eisenhardt,Henry C. Ferguson,Mauro Giavalisco,Norman Grogin,Anton M. Koekemoer,Ray A. Lucas,Bahram Mobasher,Bahram Mobasher,Casey Papovich,Alvio Renzini,Rachel S. Somerville,Daniel Stern +15 more
TL;DR: In this paper, the authors constructed a large, complete sample of 275 extremely red objects (EROs; K_s 3.35; AB) with deep HST/ACS imaging in B_435, V_606, i_775, and z_850, and well-calibrated photometric redshifts.
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