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
Dusty star-forming galaxies at high redshift
Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …
The CO-to-H2 Conversion Factor
CO line emission represents the most accessible and widely used tracer of the molecular
ISM. This renders the translation of observed CO intensity into total H2 gas mass critical to …
ISM. This renders the translation of observed CO intensity into total H2 gas mass critical to …
PHIBSS: unified scaling relations of gas depletion time and molecular gas fractions
This paper provides an update of our previous scaling relations between galaxy-integrated
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
molecular gas masses, stellar masses, and star formation rates (SFRs), in the framework of …
Tracing the total molecular gas in galaxies:[CII] and the CO-dark gas
Context. Molecular gas is a necessary fuel for star formation. The CO (1− 0) transition is
often used to deduce the total molecular hydrogen but is challenging to detect in low …
often used to deduce the total molecular hydrogen but is challenging to detect in low …
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 …
An empirical study of dust properties at the earliest epochs
We present an empirical analysis of the properties of dust-continuum emission in a sample
of 17 galaxies in the early Universe (4< z< 8) with well-sampled far-infrared spectral energy …
of 17 galaxies in the early Universe (4< z< 8) with well-sampled far-infrared spectral energy …
The evolving interstellar medium of star-forming galaxies since z= 2 as probed by their infrared spectral energy distributions
Using data from the mid-infrared to millimeter wavelengths for individual galaxies and for
stacked ensembles at 0.5< z< 2, we derive robust estimates of dust masses (M dust) for main …
stacked ensembles at 0.5< z< 2, we derive robust estimates of dust masses (M dust) for main …
ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
We report on the detection of the [C ii] 157.7 μ m emission from the Lyman break galaxy
(LBG) MACS0416_Y1 at z= 8.3113, by using the Atacama Large Millimeter/submillimeter …
(LBG) MACS0416_Y1 at z= 8.3113, by using the Atacama Large Millimeter/submillimeter …
Submillimeter galaxies as progenitors of compact quiescent galaxies
Three billion years after the big bang (at redshift z= 2), half of the most massive galaxies
were already old, quiescent systems with little to no residual star formation and extremely …
were already old, quiescent systems with little to no residual star formation and extremely …
Automated mining of the alma archive in the COSMOS field (A3COSMOS). II. cold molecular gas evolution out to redshift 6
We present new measurements of the cosmic cold molecular gas evolution out to redshift 6
based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) …
based on systematic mining of the Atacama Large Millimeter/submillimeter Array (ALMA) …