Cosmic star-formation history
Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …
Environmental Effects on Late‐Type Galaxies in Nearby Clusters
A Boselli, G Gavazzi - Publications of the Astronomical Society of …, 2006 - iopscience.iop.org
The transformations that take place in late‐type galaxies in the environment of rich clusters
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …
of galaxies at z= 0 are reviewed. From the handful of late‐type galaxies that inhabit local …
COSMOS2020: The galaxy stellar mass function-The assembly and star formation cessation of galaxies at 0.2< z≤ 7.5
Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …
within the modern landscape of galaxy evolution studies. These processes are indelibly …
The Herschel view of the dominant mode of galaxy growth from z= 4 to the present day
We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …
A unified multiwavelength model of galaxy formation
We present a new version of the galform semi-analytical model of galaxy formation. This
brings together several previous developments of galform into a single unified model …
brings together several previous developments of galform into a single unified model …
The evolution of the stellar mass functions of star-forming and quiescent galaxies to z= 4 from the COSMOS/UltraVISTA survey
We present measurements of the stellar mass functions (SMFs) of star-forming and
quiescent galaxies to z= 4 using a sample of 95,675 K s-selected galaxies in the …
quiescent galaxies to z= 4 using a sample of 95,675 K s-selected galaxies in the …
Galactic star formation and accretion histories from matching galaxies to dark matter haloes
We present a new statistical method to determine the relationship between the stellar
masses of galaxies and the masses of their host dark matter haloes over the entire cosmic …
masses of galaxies and the masses of their host dark matter haloes over the entire cosmic …
The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria
The ATLAS3D project is a multiwavelength survey combined with a theoretical modelling
effort. The observations span from the radio to the millimetre and optical, and provide …
effort. The observations span from the radio to the millimetre and optical, and provide …
Galaxy And Mass Assembly (GAMA): stellar mass estimates
This paper describes the first catalogue of photometrically derived stellar mass estimates for
intermediate-redshift (z< 0.65; median z= 0.2) galaxies in the Galaxy And Mass Assembly …
intermediate-redshift (z< 0.65; median z= 0.2) galaxies in the Galaxy And Mass Assembly …
[HTML][HTML] Review of particle physics
K Nakamura - Journal of Physics G: Nuclear and …, 2010 - bibliotecadigital.exactas.uba.ar
This biennial Review summarizes much of particle physics. Using data from previous
editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average …
editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average …