The evolution of galaxy structure over cosmic time
CJ Conselice - Annual Review of Astronomy and Astrophysics, 2014 - annualreviews.org
I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …
Can minor merging account for the size growth of quiescent galaxies? New results from the CANDELS survey
AB Newman, RS Ellis, K Bundy… - The Astrophysical …, 2012 - iopscience.iop.org
The presence of extremely compact galaxies at z∼ 2 and their subsequent growth in
physical size has been the cause of much puzzlement. We revisit the question using deep …
physical size has been the cause of much puzzlement. We revisit the question using deep …
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 …
Bulge mass is king: the dominant role of the bulge in determining the fraction of passive galaxies in the Sloan Digital Sky Survey
We investigate the origin of galaxy bimodality by quantifying the relative role of intrinsic and
environmental drivers to the cessation (or 'quenching') of star formation in over half a million …
environmental drivers to the cessation (or 'quenching') of star formation in over half a million …
CEERS key paper. II. A first look at the resolved host properties of AGN at 3< z< 5 with JWST
We report on the host properties of five X-ray-luminous active galactic nuclei (AGN)
identified at 3< z< 5 in the first epoch of imaging from the Cosmic Evolution Early Release …
identified at 3< z< 5 in the first epoch of imaging from the Cosmic Evolution Early Release …
CEERS: Spatially Resolved UV and Mid-infrared Star Formation in Galaxies at 0.2< z< 2.5: The Picture from the Hubble and James Webb Space Telescopes
We present the mid-infrared (MIR) morphologies for 64 star-forming galaxies (SFGs) at 0.2<
z< 2.5 with stellar mass M*> 10 9 M⊙ using James Webb Space Telescope (JWST) Mid …
z< 2.5 with stellar mass M*> 10 9 M⊙ using James Webb Space Telescope (JWST) Mid …
How do minor mergers promote inside-out growth of ellipticals, transforming the size, density profile and dark matter fraction?
M Hilz, T Naab, JP Ostriker - Monthly Notices of the Royal …, 2013 - academic.oup.com
There is observational evidence for inside-out growth of giant elliptical galaxies since z≳ 2–
3, which is–in contrast to disc galaxies–not driven by in situ star formation. Many of the∼ …
3, which is–in contrast to disc galaxies–not driven by in situ star formation. Many of the∼ …
A CANDELS–3D-HST SYNERGY: RESOLVED STAR FORMATION PATTERNS AT 0.7< z< 1.5
S Wuyts, NMF Schreiber, EJ Nelson… - The Astrophysical …, 2013 - iopscience.iop.org
We analyze the resolved stellar populations of 473 massive star-forming galaxies at 0.7< z<
1.5, with multi-wavelength broadband imaging from CANDELS and Hα surface brightness …
1.5, with multi-wavelength broadband imaging from CANDELS and Hα surface brightness …
Spectroscopic confirmation of the rich z= 1.80 galaxy cluster JKCS 041 using the WFC3 grism: environmental trends in the ages and structure of quiescent galaxies
ABSTRACT We present Hubble Space Telescope imaging and grism spectroscopy in the
field of the distant galaxy cluster JKCS 041 using the Wide Field Camera 3. We confirm that …
field of the distant galaxy cluster JKCS 041 using the Wide Field Camera 3. We confirm that …
Early-type galaxies have been the predominant morphological class for massive galaxies since only z ∼ 1
Present-day massive galaxies are composed mostly of early-type objects. It is unknown
whether this was also the case at higher redshifts. In a hierarchical assembling scenario the …
whether this was also the case at higher redshifts. In a hierarchical assembling scenario the …