Search Results - "Panuzzo, Pasquale"
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DUST AND GAS IN THE MAGELLANIC CLOUDS FROM THE HERITAGE HERSCHEL KEY PROJECT. II. GAS-TO-DUST RATIO VARIATIONS ACROSS INTERSTELLAR MEDIUM PHASES
Published in The Astrophysical journal (20-12-2014)“…The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical evolution and life-cycle of dust in galaxies. We examine the relation…”
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THE SPATIAL DISTRIBUTION OF DUST AND STELLAR EMISSION OF THE MAGELLANIC CLOUDS
Published in The Astrophysical journal (10-12-2012)“…We study the emission by dust and stars in the Large and Small Magellanic Clouds, a pair of low-metallicity nearby galaxies, as traced by their spatially…”
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FIR/Submm Spectroscopy with Herschel: First Results from the VNGS and H-Atlas Surveys
Published in Open astronomy (01-01-2011)“…The FIR/submm window is one of the least-studied regions of the electromagnetic spectrum, yet this wavelength range is absolutely crucial for understanding the…”
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Drift removal by means of alternating least squares with application to Herschel data
Published in Signal processing (01-03-2015)“…We consider the problem of reconstructing an image observed with a linear, noisy instrument, the output of which is affected by a drift too, causing a slowly…”
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THE INFLUENCE OF SUPERNOVA REMNANTS ON THE INTERSTELLAR MEDIUM IN THE LARGE MAGELLANIC CLOUD SEEN AT 20-600 μm WAVELENGTHS
Published in The Astrophysical journal (20-01-2015)“…(ProQuest: ... denotes formulae and/or non-USASCII text omitted)We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and…”
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DUST AND GAS IN THE MAGELLANIC CLOUDS FROM THE HERITAGE HERSCHEL KEY PROJECT. I. DUST PROPERTIES AND INSIGHTS INTO THE ORIGIN OF THE SUBMILLIMETER EXCESS EMISSION
Published in The Astrophysical journal (20-12-2014)“…The dust properties in the Large and Small Magellanic clouds (LMC/SMC) are studied using the HERITAGE Herschel Key Project photometric data in five bands from…”
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The Influence of Supernova Remnants on the Interstellar Medium in the Large Magellanic Cloud Seen at 20-600 mum Wavelengths
Published in The Astrophysical journal (20-01-2015)“…We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and their influence on the environment at far-infrared (FIR) and…”
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Effects of dust scattering albedo and 2175-Å bump on ultraviolet colours of normal disc galaxies
Published in Monthly notices of the Royal Astronomical Society (21-07-2006)“…We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies by comparing observations in the ultraviolet (UV) with simulations by a…”
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Effects of dust scattering albedo and 2175 A bump on ultraviolet colours of normal disc galaxies
Published in Monthly notices of the Royal Astronomical Society (2006)“…We discuss dust properties in the interstellar medium (ISM) of nearby normal galaxies, by comparing observations in the ultraviolet (UV) with simulations by a…”
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PlotXY: a high quality plotting system for the Herschel Interactive Processing Environment (HIPE), and the astronomical community
Published 17-07-2012“…The Herschel Interactive Processing Environment (HIPE) was developed by the European Space Agency (ESA) in collaboration with NASA and the Herschel Instrument…”
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The Milky Way's halo in 6D: Gaia's Radial Velocity Spectrometer performance
Published 12-09-2016“…Gaia's Radial Velocity Spectrometer (RVS) has been operating in routine phase for over one year since initial commissioning. RVS continues to work well but the…”
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Mid Infrared Colors of Early Type Galaxies
Published in Astrophysics and space science (01-05-2001)“…We compare the mid infrared colors of early type galaxies with isochrones that suitably account for the effects of dust in the circumstellar envelopes of AGB…”
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Impacts of The Radiation Environment At L2 On Bolometers Onboard The Herschel Space Observatory
Published 24-07-2012“…We present the effects of cosmic rays on the detectors onboard the Herschel satellite. We describe in particular the glitches observed on the two types of…”
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Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
Published 08-12-2014“…A&A 575, A88 (2015) Since the launch of the Herschel Space Observatory, our understanding about the photo-dissociation regions (PDR) has taken a step forward…”
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The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 $\mu$m wavelengths
Published 21-10-2014“…We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and their influence on the environment at far-infrared (FIR) and…”
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Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission
Published 23-06-2014“…The dust properties in the Large and Small Magellanic Clouds are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500…”
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Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. II. Gas-to-Dust Ratio Variations across ISM Phases
Published 17-11-2014“…The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical evolution and lifecycle of dust in galaxies. We examine the relation…”
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Observing Extended Sources with the \Herschel SPIRE Fourier Transform Spectrometer
Published 24-06-2013“…The Spectral and Photometric Imaging Receiver (SPIRE) on the European Space Agency's Herschel Space Observatory utilizes a pioneering design for its imaging…”
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FIR/submm spectroscopy with Herschel: first results from the VNGS and H-ATLAS surveys
Published 06-12-2011“…Baltic Astronomy, 20, 371-378 (2011) The FIR/submm window is one of the least-studied regions of the electromagnetic spectrum, yet this wavelength range is…”
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