Results 1 to 10 of about 6,945 (227)
Spectroscopic Confirmation of an Ultra-Massive Galaxy in a Protocluster at $z \sim 4.9$
We present spectroscopic confirmation of an ultra-massive galaxy (UMG) with $\log(M_\star/M_\odot) = 10.98 \pm 0.07$ at $z_\mathrm{spec} = 4.8947$ in the Extended Groth Strip (EGS), based on deep observations of Ly$\alpha$ emission with Keck/DEIMOS.
Stephanie M. Urbano Stawinski +10 more
doaj +1 more source
The S4G-WISE View of Global Star Formation in the Nearby Universe
In this work, we present source-tailored Wide-field Infrared Survey Explorer (WISE) mid-infrared photometry (at 3.4, 4.6, 12, and 23 μ m) of 2812 galaxies in the extended Spitzer Survey of Stellar Structure in Galaxies sample, and characterize the mid ...
M. E. Cluver +11 more
doaj +1 more source
J-PAS: A neural network approach to single stellar population characterisation
J-PAS (Javalambre Physics of the Accelerating Universe Astrophysical Survey) will present a groundbreaking photometric survey covering 8500 deg2 of the visible sky from Javalambre, capturing data in 56 narrow-band filters.
Domínguez Sánchez H. +30 more
doaj +1 more source
Working Group on Galaxy Photometry [PDF]
1. A tabular presentation has been adopted and the report does not cover work in the U.S.S.R. During the report period Circular No. 6 (Report on Prague Meeting) and a Technical Supplement, No. 6a, were distributed. Work on standard luminosity profiles for a few well-observed galaxies (NGC3115, 3379, 4486) progressed more slowly than expected, but ...
openaire +1 more source
Automated Computer Vision Cluster Identification in the Fireworks Galaxy
We present the integrated photometry, radii, and spatial distribution of young (≤25 Myr) star cluster candidates in NGC 6946. NGC 6946, also known as the Fireworks Galaxy, is a highly star-forming galaxy with numerous young massive clusters.
Debby Tran +7 more
doaj +1 more source
The China Space Station Telescope (CSST) will simultaneously conduct wide-field multiband photometric imaging and spectroscopic slitless surveys, poised to significantly advance cosmology and galaxy evolution research.
Yunkun Han +23 more
doaj +1 more source
Extragalactic science and cosmology with Stage IV galaxy surveys will rely almost exclusively on redshift measurements derived solely from photometry, which are subject to systematic and statistical uncertainties with numerous analysis choices.
Bryan R. Scott +2 more
doaj +1 more source
The Universe SPHEREx Will See: Empirically Based Galaxy Simulations and Redshift Predictions
We simulate galaxy properties and redshift estimation for SPHEREx, the next NASA Medium Class Explorer. To make robust models of the galaxy population and test the spectrophotometric redshift performance for SPHEREx, we develop a set of synthetic ...
Richard M. Feder +8 more
doaj +1 more source
RUBIES Spectroscopically Confirms the High Number Density of Quiescent Galaxies from 2 < z< 5
We present the number density of massive ( ${\mathrm{log}}({M}_{* }/{M}_{\odot })\gt 10.3$ ) quiescent galaxies at 2
Yunchong Zhang +23 more
doaj +1 more source
Star–galaxy classification in deep LSST data with random forest
Context. The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will produce unprecedentedly deep and wide photometric catalogues, enabling transformative studies of faint stellar systems such as the research of ultra-faint dwarf (UFD ...
Gatto M. +4 more
doaj +1 more source

