116 datasets found

Keywords: Spectral energy distribution

Filter Results
  • Gamma-Ray spectral energy in HAWC J1825-134 region

    The Earth is bombarded by ultrarelativistic particles, known as cosmic rays (CRs). CRs with energies up to a few PeV (=1015eV), the knee in the particle spectrum, are believed...
  • BAT AGN spectroscopic survey. XI. IR photometry

    We quantify the luminosity contribution of active galactic nuclei (AGNs) to the 12{mu}m, mid-infrared (MIR; 5-38{mu}m), and total IR (5-1000{mu}m) emission in the local AGNs...
  • Far-infrared SED measurements of massive galaxies

    Massive Population II galaxies undergoing the first phase of vigorous star formation after the initial Population III stage should have high energy densities and silicate-rich...
  • ASTRAL: reference spectra for evolved M stars

    The Hubble Space Telescope (HST) Treasury Program Advanced Spectral Library Project: Cool Stars was designed to collect representative, high-quality UV spectra of eight evolved...
  • "Super-deblended" dust emission in galaxies. I.

    We present a new technique to measure multi-wavelength "super-deblended" photometry from highly confused images, which we apply to Herschel and ground-based far-infrared (FIR)...
  • FIR-mm data of YSOs in star-forming regions

    Far-infrared and (sub)millimeter fluxes can be used to study dust in protoplanetary disks, the building blocks of planets. Here, we combine observations from the Herschel Space...
  • Composite SEDs of type 1 and type 2 QSOs

    We present observed mid-infrared and optical colors and composite spectral energy distributions (SEDs) of type 1 (broad-line) and 2 (narrow-line) quasars selected from Sloan...
  • Intrinsic far-IR SED of luminous AGNs

    The range of currently proposed active galactic nucleus (AGN) far-infrared templates results in uncertainties in retrieving host galaxy information from infrared observations...
  • Multiwavelength obs. of BL Lac in 2012-2013

    BL Lac, the eponymous blazar, flared to historically high levels at millimeter, infrared, X-ray, and gamma-ray wavelengths in 2012. We present observations made with Herschel,...
  • GRB 120326A, 100418A & 100901A multi-wavelength obs.

    We present multi-wavelength observations and modeling of gamma-ray bursts (GRBs) that exhibit a simultaneous re-brightening in their X-ray and optical light curves, and are also...
  • WISE ELIRGs and comparison with QSOs

    We present 20 Wide-field Infrared Survey Explorer (WISE)-selected galaxies with bolometric luminosities L_bol_>10^14^L_{sun}, including five with infrared luminosities...
  • SED fitting results of HETDEX pilot survey

    We use broadband photometry extending from the rest-frame UV to the near-IR to fit the individual spectral energy distributions of 63 bright (L(Ly{alpha})>10^43^ erg/s)...
  • SEDs of type I AGN in COSMOS. I. XMM-COSMOS

    The "Cosmic Evolution Survey" (COSMOS) enables the study of the spectral energy distributions (SEDs) of active galactic nuclei (AGNs) because of the deep coverage and rich...
  • IR SEDs of 24um z~0.3-3 galaxies

    In this paper, we characterize the infrared spectral energy distributions (SEDs) of mid-IR-selected z~0.3-3.0 and L_IR_~10^11^-10^13^L_{sun} galaxies, and study how their SEDs...
  • SED of Fermi bright blazars

    We have conducted a detailed investigation of the broadband spectral properties of the {gamma}-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS, Cat....
  • Low-resolution SED templates for AGNs and galaxies

    We present a set of low-resolution empirical spectral energy distribution (SED) templates for active galactic nuclei (AGNs) and galaxies in the wavelength range from 0.03um to...
  • SED of the Fermi blazars

    We complied the optical, X-ray, and {gamma}-ray data for 54 Fermi blazars and studied the relationship between the broadband spectral index {alpha}ox and {alpha}x{gamma}, as...
  • SED of cluster radio galaxies

    To explore the high-frequency radio spectra of galaxies in clusters, we used NRAO's Very Large Array at four frequencies, 4.9-43GHz, to observe 139 galaxies in low redshift...
  • Star forming galaxy templates

    We show that measures of star formation rates (SFRs) for infrared galaxies using either single-band 24um or extinction-corrected Pa{alpha} luminosities are consistent in the...
  • SEDs of ELAIS-S1 mid-IR sources

    We present the broadband SEDs of the largest available highly complete (72%) spectroscopic sample of MIR-selected galaxies and AGNs at intermediate redshift. The sample contains...
You can also access this registry using the API (see API Docs).