Preface |
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Acknowledgements |
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xv | |
Organizing committee |
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xvii | |
Conference photograph |
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xviii | |
Conference participants |
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xx | |
Introduction |
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Reification of galaxies: cognitive astrophysics and the multiwavelength inverse problem |
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1 | (1) |
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Section 1 Population Synthesis |
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Population synthesis at the crossroads |
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2 | (10) |
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Effects of Non-Solar Abundance Ratios on Star Spectra: Observations versus Models |
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12 | (4) |
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Spectral models of stellar populations resolved in chemical abundances |
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16 | (4) |
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The importance of nebular emission for SED modeling of distant star-forming galaxies |
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20 | (6) |
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NBursts+phot: parametric recovery of galaxy star formation histories from the simultaneous fitting of spectra and broad-band spectral energy distributions |
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26 | (3) |
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An empirical spectral library of chemically well characterized stars for stellar population modelling |
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29 | (3) |
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A first glance into the Spectral Energy Distributions of Single Stellar Populations in the Infrared range |
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32 | (3) |
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Stellar population models in the UV: I. Characterisation of the New Generation Stellar Library |
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35 | (3) |
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Beyond model fitting SEDs |
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38 | (4) |
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SED fitting with MCMC: methodology and application to large galaxy surveys |
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42 | (4) |
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A Bayesian approach to quantify the uncertainties in the determination of galaxy properties derived from spectral fits |
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46 | (3) |
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What can the UV SED tell us about primitive galaxies? |
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49 | (4) |
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Hα and FUV luminosities from a stochastically formed stellar population |
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53 | (3) |
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The UV upturn phenomenon in the hierarchical universe |
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56 | (3) |
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Star formation history and the SED of galaxies: insights from resolved stars |
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59 | (4) |
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Direct constraints on the impact of TP-AGB stars on the SED of galaxies from near-infrared spectroscopy |
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63 | (3) |
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Spectral fitting of SDSS passive galaxies with α-enhanced single stellar populations |
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66 | (3) |
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Multi-component parametric inversion of galaxy kinematics and stellar populations using full spectral fitting |
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69 | (3) |
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Section 2 Understanding the Emergent SEDs of Local Universe Galaxies |
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Chemical and physical properties of interstellar dust |
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72 | (10) |
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The processing of radiation by dust in galaxies |
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82 | (10) |
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Section 2-1 Understanding the Emergent SEDs of Local Universe Galaxies: Spiral and Dwarf Galaxies |
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A detailed dust energy balance study of the Sombrero galaxy |
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92 | (5) |
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Investigations of dust heating in M81, M83 and NGC 2403 with Herschel and Spitzer |
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97 | (4) |
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The Herschel-SPIRE Local Galaxies Guaranteed Time Programs |
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The dust distribution in late-type low surface brightness disks |
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101 | (3) |
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The 3-dimensional structure of NGC 891 and M51 |
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104 | (3) |
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Stellar and dust SED modelling of the Whirlpool interacting galaxy system |
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107 | (5) |
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Hot, cold dust in M31: the resolved SED of Andromeda |
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112 | (5) |
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The MPIA Herschel Andromeda Team |
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Resolved optical-infrared SEDs of galaxies: universal relations and their break-down on local scales |
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117 | (5) |
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Spectral Energy Distributions of a set of H II regions in M33 (HerM33es) |
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122 | (3) |
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Variation in the dust spectral index across M33 |
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125 | (3) |
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New HErschel Multi-wavelength Extragalactic Survey of Edge-on Spirals (NHEMESES) |
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128 | (4) |
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Ionization of the diffuse gas in galaxies: hot low-mass evolved stars at work |
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132 | (3) |
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Detection of a large amount of diffuse extraplanar dust in NGC 891 |
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135 | (3) |
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On the nature of the peculiarsuperthin LSB galaxy UGC 12281 |
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138 | (3) |
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Low Metallicity ISM: excess submillimetre emission and CO-free H2 gas |
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141 | (8) |
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The Herschel SAG2 consortium |
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Characterisation of the submillimeter excess in dwarf galaxies: Presentation of the Herschel Dwarf Galaxies Survey |
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149 | (3) |
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The Herschel SAG2 Consortium |
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Dust in dwarf galaxies: The case of NGC 4214 |
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152 | (4) |
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Modeling the dust Spectral Energy Distribution of NGC 4214 |
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156 | (3) |
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A Multi-wavelength MOCASSIN model of the Magellanic-type galaxy NGC 4449 |
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159 | (4) |
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Identification of Spitzer-IRS staring mode targets in the Magellanic Clouds |
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163 | (3) |
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The SG view of stellar mass, mid-IR dust, and evolved, intermediate-age stars in nearby galaxies |
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166 | (4) |
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The peculiar dust properties of the LMC and their implications on modelling SEDs of galaxies |
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170 | (3) |
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Spikes in the SED and ripples in the outskirts of galaxies |
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173 | (7) |
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TYPHOON observations of the Lindsay-Shapley Ring |
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180 | (3) |
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Section 2-2 Understanding the Emergent SEDs of Local Universe Galaxies: Starburst Galaxies and Active Galactic Nuclei |
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Sources of X-rays from galaxies |
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183 | (10) |
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Optical SED models of galaxy mergers |
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193 | (5) |
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The SEDs of interacting galaxies |
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198 | (4) |
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A Spitzer study of interacting luminous and ultra-luminous infrared galaxies |
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202 | (3) |
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A new model for the infrared emission of IRAS F10214+4724 |
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205 | (5) |
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Properties of mid- to far-infrared dust emission in the nearby superwind galaxy M82 |
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210 | (3) |
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The SED of the nearby H I-massive LIRG HIZOA J0836--43: from the NIR to the radio domain |
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213 | (5) |
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Retrieving the stellar content in distant starbursts |
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218 | (3) |
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What makes a galaxy radio-loud? |
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221 | (3) |
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Spectral energy distributions of quasars selected in the mid-infrared |
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224 | (4) |
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The Mid-Infrared luminosity function of galaxies using the AKARI mid-infrared All-Sky Survey Catalogue |
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228 | (3) |
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Optically faint radio sources: reborn AGN? |
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231 | (3) |
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Stellar populations in the centers of nearby galaxies |
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234 | (3) |
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Multiwavelength data for bright active galaxies |
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237 | (3) |
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Section 2-3 Understanding the Emergent SEDs of Local Universe Galaxies: Early Type Galaxies |
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Young stars in nearby early-type galaxies: SED fitting based on ultraviolet (UV) and optical imaging |
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240 | (4) |
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The star-formation histories of early-type galaxies from ATLAS3D |
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244 | (4) |
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Constrain the stellar population gradient of elliptical galaxies with SED |
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248 | (3) |
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Outer stellar disks of lenticular galaxies |
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251 | (3) |
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Dust and PAHs in X-ray plasma of elliptical galaxies |
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254 | (5) |
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Dusty early-type galaxies and passive spirals |
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259 | (3) |
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The Herschel-ATLAS and GAMA collaborations |
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Using GAMA and H-ATLAS data to explore the cold dust properties of early-type galaxies |
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262 | (3) |
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Age-dating Stellar Populations of Luminous Red Galaxies |
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265 | (3) |
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Section 2-4 Understanding the Emergent SEDs of Local Universe Galaxies: Multiwavelength Surveys |
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Panchromatic properties of galaxies in wide-field optical spectroscopic and photometric surveys |
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268 | (11) |
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Far-IR to Submm SEDs for local galaxies: Herschel, Planck and the HRS |
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279 | (4) |
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The Herschel Reference Sample Team |
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The spectral energy distributions of the entire Herschel Reference Survey |
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283 | (3) |
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The Herschel-SPIRE Local Galaxies Guaranteed Time Programs |
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Far-infrared and sub-millimeter properties of SDSS galaxies in the Herschel ATLAS SDP Field |
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286 | (3) |
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Far Infrared Luminosity Function of Local Galaxies in the AKARI Deep Field South |
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289 | (3) |
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MAGPHYS: a publicly available tool to interpret observed galaxy SEDs |
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292 | (5) |
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Fitting the full SED of galaxies to put constraints on dust attenuation and star formation determinations |
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297 | (4) |
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Measuring SEDs for individualgalaxy components |
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301 | (5) |
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Dust effects on the derived Sersic indexes of disks and bulges in spiral galaxies |
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306 | (3) |
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Publicly available database for spectral line measurements of SDSS DR7 galaxies |
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309 | (3) |
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Probing the opacity of local Universe GAMA galaxies using attenuation-inclination relations |
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312 | (3) |
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The unusual multi-wavelength SED of two optical dropout galaxies |
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315 | (2) |
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Section 3 Star-Formation in Galaxies |
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What triggers star formation in galaxies? |
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317 | (13) |
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The energetics of turbulent molecular gas and star formation |
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330 | (7) |
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The dust emission SED of X-ray emitting regions in Stephan's Quintet |
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337 | (5) |
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AKARI observations of the multiphase intergalactic medium of Stephan's Quintet |
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342 | (3) |
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Radial variations of the SFHs of dwarf irregular galaxies |
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345 | (4) |
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Star formation properties in barred galaxies |
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349 | (3) |
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Environmental dependence of SFRs in late-type GAMA galaxies |
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352 | (5) |
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AKARI/IRC broadband mid-infrared data as an indicator of the Star Formation Rate |
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357 | (3) |
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Section 4 The Panchromatic View of the Milky Way |
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Cosmic-Ray induced diffuse emissions from the Milky Way and Local Group galaxies |
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360 | (5) |
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The H.E.S.S. view of the Milky Way in TeV light |
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365 | (6) |
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The Galactic Centre - a laboratory for starburst galaxies (?) |
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371 | (8) |
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The star formation rate in the Milky Way: Results from stars and planetary nebulae |
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379 | (3) |
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Section 5 Linking Low- and High-Energy Properties of Galaxies |
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High-energy emission from galaxies: the star-formation/gamma-ray connection |
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382 | (7) |
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Dark gas: a new possible link between low and high-energy phenomena |
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389 | (4) |
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Cosmic rays and high energy emission from starburst galaxies |
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393 | (4) |
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Cosmic ray production and emission in M82 |
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397 | (3) |
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The resolved radio--FIR correlation in nearby galaxies with Herschel and Spitzer |
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400 | (4) |
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No evidence for evolution in the Far-Infrared-Radio correlation out to z ~ 2 in the ECDFS |
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404 | (3) |
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The non-thermal broadband spectral energy distribution of radio galaxies |
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407 | (4) |
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The challenging SED of AP Librae |
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411 | (3) |
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Very high energy γ-radiation from the radio quasar 4C 21.35 |
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414 | (3) |
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Synchrotron radiation from giant e± pair halos |
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417 | (3) |
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Constraints on the optical-IR extragalactic background from γ-ray absorption studies |
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420 | (9) |
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Spectrophotometric measurement of the Extragalacic Background Light |
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429 | (8) |
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Cosmic Optical Background: the view from Pioneer 10/11 |
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437 | (5) |
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An empirical approach to the extragalactic background light from AEGIS galaxy SED-type fractions |
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442 | (4) |
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Section 6 Understanding the Cosmological Evolution of Emergent SEDs |
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Panchromatic radiation from galaxies as a probe of galaxy formation and evolution |
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446 | (10) |
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Photometric studies of PAH emission from distant infrared galaxies |
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456 | (4) |
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The AKARI extragalactic team |
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Minor-merger-driven growth of early-type galaxies over the last 8 billion years |
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460 | (5) |
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Charting the evolution of the ages and metallicities of massive galaxies since z = 0.7 |
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465 | (3) |
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Determining the average SFR of K+A galaxies |
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468 | (3) |
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High resolution SMA imaging of (ultra)-luminous infrared galaxies |
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471 | (4) |
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Multi-wavelength probes of distant lensed galaxies |
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475 | (7) |
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Cosmic Infrared Background ExpeRiment (CIBER): A probe of Extragalactic Background Light from reionization |
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482 | (7) |
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Evolutionary Map of the Universe |
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489 | (5) |
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Extragalactic science with ALMA |
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494 | (2) |
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The UK ALMA Regional Centre Node |
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Looking at the distant universe with the MeerKAT Array (LADUMA) |
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496 | (4) |
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Conference Summary |
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500 | (8) |
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Author index |
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508 | |