Results 31 to 40 of about 9,672,606 (254)
Active galactic nuclei vs. host galaxy properties in the COSMOS field [PDF]
, 2017 Context. The coeval active galactic nuclei (AGN) and galaxy evolution and the observed local relations between super massive black holes (SMBHs) and galaxy properties suggest some sort of connection or feedback between the SMBH growth (i.e., the AGN ...
G. Lanzuisi +21 more
semanticscholar +1 more source
Properties of GRB host galaxies
Fourth Huntsville gamma-ray burst symposium, 1998 5 pages, AIPPROC LaTeX, to appear in "Gamma-Ray Bursts, 4th Huntsville Symposium," eds. C. Meegan, R.
Hartmann, Dieter H., Band, David L.
openaire +3 more sources
DEPENDENCE OF BARRED GALAXY FRACTION ON GALAXY PROPERTIES AND ENVIRONMENT [PDF]
The Astrophysical Journal, 2012 20 pages, 18 figures, accepted for publication in ...
Lee, Gwang-Ho +3 more
openaire +2 more sources
Hot Dust in Panchromatic SED Fitting: Identification of Active Galactic Nuclei and Improved Galaxy Properties [PDF]
, 2017 Forward modeling of the full galaxy SED is a powerful technique, providing self-consistent constraints on stellar ages, dust properties, and metallicities. However, the accuracy of these results is contingent on the accuracy of the model. One significant
J. Leja +3 more
semanticscholar +1 more source
The clustering properties of faint galaxies
The Astrophysical Journal, 1995 The two-point angular correlation function of galaxies, \wte, has been computed from a new survey of faint galaxies covering a 2 deg$^2$ area near the North Galactic Pole. This survey, which is complete to limiting magnitudes \jmag=24 and \fmag=23, samples angular scales as large as $1\degpoint5$.
Infante, L., Pritchet, C. J.
openaire +2 more sources
Two-phase galaxy formation: the evolutionary properties of galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2010 We use our model for the formation and evolution of galaxies within a two-phase galaxy formation scenario, showing that the high-redshift domain typically supports the growth of spheroidal systems, whereas at low redshifts the predominant baryonic growth mechanism is quiescent and may therefore support the growth of a disc structure.
Cook, Michael +4 more
openaire +3 more sources
COSMOS2015 photometric redshifts probe the impact of filaments on galaxy properties [PDF]
, 2017 The variation of galaxy stellar masses and colour types with the distance to projected cosmic filaments are quantified using the precise photometric redshifts of the COSMOS2015 catalogue extracted from Cosmological Evolution Survey (COSMOS) field (2 deg ...
C. Laigle +14 more
semanticscholar +1 more source
The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z≲6 [PDF]
, 2017 We explore the multiwavelength properties of AGN host galaxies for different classes of radio-selected AGN out to z ≲ 6 via a multiwavelength analysis of about 7700 radio sources in the COSMOS field.
I. Delvecchio +32 more
semanticscholar +1 more source
Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population [PDF]
Astrophysical Journal Letters, 2020 Using the PHANGS–ALMA CO(2–1) survey, we characterize molecular gas properties on ∼100 pc scales across 102,778 independent sightlines in 70 nearby galaxies. This yields the best synthetic view of molecular gas properties on cloud scales across the local
Jiayi Sun +36 more
semanticscholar +1 more source
Modelling the extinction properties of galaxies
Astrophysics and Space Science, 2001 Recently (Granato, Lacey, Silva et al. 2000, astro-ph/0001308) we have combined our spectrophotometric galaxy evolution code which includes dust reprocessing (GRASIL, Silva et al. 1998) with semi-analytical galaxy formation models (GALFORM, Cole et al. 1999).
Granato, G. L. +6 more
openaire +2 more sources