Reconstruction of Galaxy Star Formation Histories through SED Fitting:The Dense Basis Approach [PDF]
, 2017 We introduce the dense basis method for Spectral Energy Distribution (SED) fitting. It accurately recovers traditional SED parameters, including M*, SFR, and dust attenuation, and reveals previously inaccessible information about the number and duration ...
Kartheik G. Iyer, E. Gawiser
semanticscholar +1 more source
The SEDs of interacting galaxies [PDF]
Proceedings of the International Astronomical Union, 2011 AbstractThe evolution of galaxies is greatly influenced by their interactions. As part of a program to study interacting galaxies, we have measured and modeled the spectral energy distributions (SEDs) from the ultraviolet (UV) to the far-infrared (FIR).
Elisabete da Cunha +10 more
openaire +4 more sources
Temperament influences on parenting and child psychopathology: Socio-economic disadvantage as moderator [PDF]
, 2008 Despite calls for research on how the socio-economic environment may be related to temperament we still do not know enough about the relationship between temperament and socio-economic disadvantage (SED).
Flouri, Eirini
core +2 more sources
Level and correlates of physical activity and sedentary behavior in patients with type 2 diabetes: a cross-sectional analysis of the italian diabetes and exercise study-2 [PDF]
, 2017 OBJECTIVE: Patients with type 2 diabetes usually show reduced physical activity (PA) and increased sedentary (SED)-time, though to a varying extent, especially for low-intensity PA (LPA), a major determinant of daily energy expenditure that is not ...
Antonio Nicolucci +12 more
core +4 more sources
Panchromatic SED modelling of spatially-resolved galaxies [PDF]
, 2018 We test the efficacy of the energy-balance spectral energy distribution (SED) fitting code Magphys for recovering the spatially-resolved properties of a simulated isolated disc galaxy, for which it was not designed. We perform 226,950 Magphys SED fits to
Daniel J B Smith, C. Hayward
semanticscholar +1 more source
SATMC: Spectral Energy Distribution Analysis Through Markov Chains [PDF]
, 2013 We present the general purpose spectral energy distribution (SED) fitting tool SED Analysis Through Markov Chains (SATMC). Utilizing Monte Carlo Markov Chain (MCMC) algorithms, SATMC fits an observed SED to SED templates or models of the user's choice to
Johnson, S. P. +3 more
core +1 more source
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
SED Constraints on the Highest-z Blazar Jet: QSO J0906+6930 [PDF]
, 2018 We report on Gemini, NuSTAR, and eight years of Fermi observations of the most distant blazar QSO J0906+6930 (z = 5.48). We construct a broadband spectral energy distribution (SED) and model the SED using a synchro-Compton model. The measurements yield a
H. An, R. Romani
semanticscholar +1 more source
Stokes−Einstein−Debye failure in molecular orientational diffusion: exception or rule? [PDF]
, 2014 The Stokes–Einstein–Debye (SED) expression is used routinely to relate orientational molecular diffusivity quantitatively to viscosity. However, it is well-known that Einstein’s equations are derived from hydrodynamic theory for the diffusion of a ...
Turton, David, Wynne, Klaas
core +1 more source
Spatially resolved star formation and dust attenuation in Mrk 848: Comparison of the integral field spectra and the UV-to-IR SED [PDF]
, 2018 We investigate the star formation history and the dust attenuation in the galaxy merger Mrk848. Thanks to the multiwavelength photometry from the ultraviolet (UV) to the infrared (IR), and MaNGA's integral field spectroscopy, we are able to study this ...
F. Yuan +7 more
semanticscholar +1 more source