We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength coverage spanning from the ultraviolet to the mid-infrared. Our atlas spans a broad range of galaxy types, including ellipticals, spirals, merging galaxies, blue compact dwarfs, and luminous infrared galaxies. We have combined ground-based optical drift-scan spectrophotometry with infrared spectroscopy from Spitzer and Akari with gaps in spectral coverage being filled using Multi-wavelength Analysis of Galaxy Physical Properties spectral energy distribution models. The spectroscopy and models were normalized, constrained, and verified with matched-aperture photometry measured from Swift, Galaxy Evolution Explorer, Sloan Digital Sky Survey, Two Micr...
We introduce a new empirical function for modeling the spectral energy distributions (SEDs) of galax...
We present a pan-chromatic analysis of an unprecedented sample of 1402 250 mu m selected galaxies at...
(abridged) We present STARDUST, a new self-consistent modelling of the spectral energy distributions...
We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength covera...
This is the archive for "An Atlas of Galaxy Spectral Energy Distributions From The UV to the Mid-Inf...
We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength covera...
The ultraviolet-to-radio continuum spectral energy distributions are presented for all 75 galaxies i...
We present 0.5-160 μm spectral energy distributions (SEDs) of galaxies, detected at 70 μm with the M...
We present a novel approach to photometric redshifts, one that merges the advantages of both the tem...
Combining far-infrared Herschel photometry from the PACS Evolutionary Probe (PEP) and Herschel Multi...
The All-wavelength Extended Groth Strip International Survey (AEGIS) team presents broad-band spectr...
The ultraviolet-to-radio continuum spectral energy distributions are presented for all 75 galaxies i...
Context. A new generation of spectral synthesis models has been developed in recent years, but there...
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 μm) spectral energy distributions (SEDs...
We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated...
We introduce a new empirical function for modeling the spectral energy distributions (SEDs) of galax...
We present a pan-chromatic analysis of an unprecedented sample of 1402 250 mu m selected galaxies at...
(abridged) We present STARDUST, a new self-consistent modelling of the spectral energy distributions...
We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength covera...
This is the archive for "An Atlas of Galaxy Spectral Energy Distributions From The UV to the Mid-Inf...
We present an atlas of 129 spectral energy distributions for nearby galaxies, with wavelength covera...
The ultraviolet-to-radio continuum spectral energy distributions are presented for all 75 galaxies i...
We present 0.5-160 μm spectral energy distributions (SEDs) of galaxies, detected at 70 μm with the M...
We present a novel approach to photometric redshifts, one that merges the advantages of both the tem...
Combining far-infrared Herschel photometry from the PACS Evolutionary Probe (PEP) and Herschel Multi...
The All-wavelength Extended Groth Strip International Survey (AEGIS) team presents broad-band spectr...
The ultraviolet-to-radio continuum spectral energy distributions are presented for all 75 galaxies i...
Context. A new generation of spectral synthesis models has been developed in recent years, but there...
We have fit the far-ultraviolet (FUV) to sub-millimeter (850 μm) spectral energy distributions (SEDs...
We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated...
We introduce a new empirical function for modeling the spectral energy distributions (SEDs) of galax...
We present a pan-chromatic analysis of an unprecedented sample of 1402 250 mu m selected galaxies at...
(abridged) We present STARDUST, a new self-consistent modelling of the spectral energy distributions...