CEERS key paper. III. The diversity of galaxy structure and morphology at z= 3–9 with JWST
JS Kartaltepe, C Rose, BN Vanderhoof… - The Astrophysical …, 2023 - iopscience.iop.org
We present a comprehensive analysis of the evolution of the morphological and structural
properties of a large sample of galaxies at z= 3–9 using early James Webb Space …
properties of a large sample of galaxies at z= 3–9 using early James Webb Space …
Detailed decomposition of galaxy images. II. Beyond axisymmetric models
We present a two-dimensional (2D) fitting algorithm (Galfit, ver. 3) with new capabilities to
study the structural components of galaxies and other astronomical objects in digital images …
study the structural components of galaxies and other astronomical objects in digital images …
Structural parameters of galaxies in candels
A van der Wel, EF Bell, B Häussler… - The Astrophysical …, 2012 - iopscience.iop.org
We present global structural parameter measurements of 109,533 unique, H F160W-
selected objects from the CANDELS multi-cycle treasury program. Sérsic model fits for these …
selected objects from the CANDELS multi-cycle treasury program. Sérsic model fits for these …
GALAXY STRUCTURE AND MODE OF STAR FORMATION IN THE SFR–MASS PLANE FROM z∼ 2.5 TO z∼ 0.1
S Wuyts, NMF Schreiber, A van der Wel… - The Astrophysical …, 2011 - iopscience.iop.org
We analyze the dependence of galaxy structure (size and Sérsic index) and mode of star
formation (Σ SFR and SFR IR/SFR UV) on the position of galaxies in the star formation rate …
formation (Σ SFR and SFR IR/SFR UV) on the position of galaxies in the star formation rate …
Evolutionary paths of active galactic nuclei and their host galaxies
MY Zhuang, LC Ho - Nature Astronomy, 2023 - nature.com
The tight correlations between the masses of supermassive black holes (BHs) and the
properties of their host galaxies suggest that BHs co-evolve with galaxies. However, what is …
properties of their host galaxies suggest that BHs co-evolve with galaxies. However, what is …
IMFIT: a fast, flexible new program for astronomical image fitting
P Erwin - The Astrophysical Journal, 2015 - iopscience.iop.org
ABSTRACT I describe a new, open-source astronomical image-fitting program called imfit,
specialized for galaxies but potentially useful for other sources, which is fast, flexible, and …
specialized for galaxies but potentially useful for other sources, which is fast, flexible, and …
Galaxy And Mass Assembly (GAMA): structural investigation of galaxies via model analysis
We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled
independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey …
independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey …
An evolutionary continuum from nucleated dwarf galaxies to star clusters
Systematic studies,,–have revealed hundreds of ultra-compact dwarf galaxies (UCDs) in the
nearby Universe. With half-light radii rh of approximately 10–100 parsecs and stellar masses …
nearby Universe. With half-light radii rh of approximately 10–100 parsecs and stellar masses …
Structural properties of pseudo-bulges, classical bulges and elliptical galaxies: a Sloan Digital Sky Survey perspective
DA Gadotti - Monthly Notices of the Royal Astronomical Society, 2009 - academic.oup.com
We have performed 2D bulge/bar/disc decompositions using g, r and i-band images of a
representative sample of nearly 1000 galaxies from the Sloan Digital Sky Survey. We show …
representative sample of nearly 1000 galaxies from the Sloan Digital Sky Survey. We show …
Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy Size− Mass Relation at z< 1
L Kawinwanichakij, JD Silverman, X Ding… - The Astrophysical …, 2021 - iopscience.iop.org
Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …