Results 11 to 20 of about 1,014 (183)
Galaxy surface photometry [PDF]
We describe galaxy surface photometry based on fitting ellipses to the isophotes of the galaxies. Example galaxies with different isophotal shapes are used to illustrate the process, including how the deviations from elliptical isophotes are quantified using Fourier expansions.
Milvang-Jensen Bo, Jørgensen Inger
exaly +4 more sources
Cosmology with Galaxy Photometry Alone
We present the first cosmological constraints using only the observed photometry of galaxies. Villaescusa-Navarro et al. recently demonstrated that the internal physical properties of a single simulated galaxy contain a significant amount of cosmological
ChangHoon Hahn +3 more
exaly +4 more sources
The DESI PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) Mock Challenge
The PRObabilistic Value-added Bright Galaxy Survey (PROVABGS) catalog will provide measurements of galaxy properties, such as stellar mass ( M _* ), star formation rate (SFR), stellar metallicity ( Z ), and stellar age ( t _age ), for >10 million ...
ChangHoon Hahn +18 more
doaj +1 more source
Improved GALEX UV Photometry for 700,000 SDSS Galaxies
The Galaxy Evolution Explorer (GALEX) satellite performed the first and only large-area UV survey, which in tandem with the Sloan Digital Sky Survey (SDSS) has facilitated modeling of the spectral energy distributions of low-redshift galaxies and the ...
Chandler Osborne +4 more
doaj +1 more source
We present PopSED , a framework for the population-level inference of galaxy properties from photometric data. Unlike the traditional approach of first analyzing individual galaxies and then combining the results to determine the physical properties of ...
Jiaxuan Li +3 more
doaj +1 more source
Surface Photometry of Nearby Field Galaxies: The Data [PDF]
We have obtained integrated spectra and multi-filter photometry for a repre- sentative sample of ~200 nearby galaxies. These galaxies span the entire Hubble sequence in morphological type, as well as a wide range of luminosities (M_B = -14 to -22) and colors (B-R=0.4 to 1.8).
Jansen, RA +3 more
openaire +3 more sources
The void galaxy survey: photometry, structure and identity of void galaxies [PDF]
We analyze photometry from deep B-band images of 59 void galaxies in the Void Galaxy Survey (VGS), together with their near-infrared 3.6$μ$m and 4.5$μ$m Spitzer photometry. The VGS galaxies constitute a sample of void galaxies that were selected by a geometric-topological procedure from the SDSS DR7 data release, and which populate the deep interior of
B. Beygu +7 more
openaire +4 more sources
Photometry of Remote Galaxy Clusters [PDF]
New data on the colors of galaxies in distant, rich clusters of galaxies are presented. Of seven clusters examined having z<0.20, all exhibit color distributions indicating that a significant proportion of the member galaxies are undergoing star formation. The one cluster studied with z<0.20 clearly shows a reduced fraction of such galaxies.
H. Butcher, A. Oemler, D. Wells
openaire +1 more source
The Farmer: A Reproducible Profile-fitting Photometry Package for Deep Galaxy Surveys
While space-borne optical and near-infrared facilities have succeeded in delivering a precise and spatially resolved picture of our Universe, their small survey area is known to underrepresent the true diversity of galaxy populations.
J. R. Weaver +19 more
doaj +1 more source
Study photometric properties of spiral galaxy NGC 4448 using CCD camera with multiband filters
The goal of our study is to perform detailed multiband surface photometry of the spiral galaxy NGC 4448 and its brightest star-forming regions. The structure and composition of the stellar population in the surface brightness galaxy NGC 4448 was studied
Sinan H. Ali
doaj +1 more source

