Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
High-redshift star formation in the Atacama large millimetre/submillimetre array era
JA Hodge, E da Cunha - Royal Society Open Science, 2020 - royalsocietypublishing.org
The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …
Physical models of galaxy formation in a cosmological framework
Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …
challenges in astrophysics today due to the vast range of scales and numerous physical …
Ionised gas kinematics and dynamical masses of z≳ 6 galaxies from JADES/NIRSpec high-resolution spectroscopy
A de Graaff, HW Rix, S Carniani, KA Suess… - Astronomy & …, 2024 - aanda.org
We explore the kinematic gas properties of six 5.5< z< 7.4 galaxies in the JWST Advanced
Deep Extragalactic Survey (JADES), using high-resolution JWST/NIRSpec multi-object …
Deep Extragalactic Survey (JADES), using high-resolution JWST/NIRSpec multi-object …
Evolution of the Size–Mass Relation of Star-forming Galaxies Since z= 5.5 Revealed by CEERS
E Ward, A de la Vega, B Mobasher… - The Astrophysical …, 2024 - iopscience.iop.org
We combine deep imaging data from the CEERS early release JWST survey and Hubble
Space Telescope imaging from CANDELS to examine the size–mass relation of star-forming …
Space Telescope imaging from CANDELS to examine the size–mass relation of star-forming …
What causes the formation of discs and end of bursty star formation?
As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
Morpheus reveals distant disk galaxy morphologies with jwst: The first ai/ml analysis of jwst images
The dramatic first images with JWST demonstrated its power to provide unprecedented
spatial detail for galaxies in the high-redshift universe. Here, we leverage the resolution and …
spatial detail for galaxies in the high-redshift universe. Here, we leverage the resolution and …
Theoretical challenges in galaxy formation
T Naab, JP Ostriker - Annual review of astronomy and …, 2017 - annualreviews.org
Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …
evolution. Over the decades the field has made significant progress. It is now possible to …
Cool gas in high-redshift galaxies
CL Carilli, F Walter - Annual Review of Astronomy and …, 2013 - annualreviews.org
Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …
Structure and kinematics of early-type galaxies from integral field spectroscopy
M Cappellari - Annual review of astronomy and astrophysics, 2016 - annualreviews.org
Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …
The size evolution of star-forming and quenched galaxies in the IllustrisTNG simulation
We analyse scaling relations and evolution histories of galaxy sizes in TNG100, part of the
IllustrisTNG simulation suite. Observational qualitative trends of size with stellar mass, star …
IllustrisTNG simulation suite. Observational qualitative trends of size with stellar mass, star …