Luigi Spinoglio astrophysicien italien
Spinoglio, Luigi
Spinoglio, L.
VIAF ID: 202296249 (Personal)
Permalink: http://viaf.org/viaf/202296249
Preferred Forms
- 100 0 _ ‡a Luigi Spinoglio ‡c astrophysicien italien
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- 100 1 _ ‡a Spinoglio, Luigi
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- 100 1 _ ‡a Spinoglio, Luigi
4xx's: Alternate Name Forms (7)
Works
Title | Sources |
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An astronomical observatory at CONCORDIA (dome C, Antarctica) : [proceedings from the 3rd Arena Conference held in Frascati, Italy, 11-15 May 2009] | |
The dust scaling relations of theHerschelReference Survey | |
EVIDENCE FOR CO SHOCK EXCITATION IN NGC 6240 FROMHERSCHELSPIRE SPECTROSCOPY | |
FAR-INFRARED LINE SPECTRA OF ACTIVE GALAXIES FROM THEHERSCHEL/PACS SPECTROMETER: THE COMPLETE DATABASE | |
FAR-IR/SUBMILLIMETER SPECTROSCOPIC COSMOLOGICAL SURVEYS: PREDICTIONS OF INFRARED LINE LUMINOSITY FUNCTIONS FORz< 4 GALAXIES | |
Feedback and Feeding in the Context of Galaxy Evolution with SPICA: Direct Characterisation of Molecular Outflows and Inflows | |
Filaments in the Lupus molecular clouds | |
FIR colours and SEDs of nearby galaxies observed with Herschel | |
FISICA | |
FPGA based control system for space instrumentation | |
From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt Survey | |
Galaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR Spectroscopy | |
The gas-to-dust mass ratio of Centaurus A as seen by Herschel | |
Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range | |
Heating of the molecular gas in the massive outflow of the local ultraluminous-infrared and radio-loud galaxy 4C12.50 | |
The Herschel and JCMT Gould belt surveys: constraining dust properties in the Perseus B1 clump with PACS, SPIRE, and SCUBA-2 | |
The Herschel comprehensive (U)LIRG emission survey (HERCULES): CO ladders, fine structure lines, and neutral gas cooling | |
The Herschel Exploitation of Local Galaxy Andromeda | |
Herschel observations of Cen A: stellar heating of two extragalactic dust clouds | |
Herschel observations of water vapour in Markarian 231 | |
The Herschel reference survey: dust in early-type galaxies and across the Hubble sequence | |
Herschel-SPIRE observations of the disturbed galaxy NGC 4438 | |
Hi-GAL: The Herschel Infrared Galactic Plane Survey | |
High‐excitation OH and H2O Lines in Markarian 231: The Molecular Signatures of Compact Far‐infrared Continuum Sources | |
High-resolution, 3D radiative transfer modeling | |
The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratios | |
The imprint of rapid star formation quenching on the spectral energy distributions of galaxies | |
Investigations of dust heating in M81, M83 and NGC 2403 with the Herschel Space Observatory | |
Ionisation impact of high-mass stars on interstellar filaments | |
Ionization compression impact on dense gas distribution and star formation | |
ISO-LWS two-colour diagram of young stellar objects | |
The JCMT Gould Belt Survey: first results from the SCUBA-2 observations of the Ophiuchus molecular cloud and a virial analysis of its prestellar core population | |
Linking dust emission to fundamental properties in galaxies: the low-metallicity picture | |
Millimetron—a large Russian-European submillimeter space observatory | |
The Nature of the Mid-Infrared Population from Optical Identifications of the ELAIS-S1 Sample | |
On the origin of M81 group extended dust emission | |
An Overview of the Dwarf Galaxy Survey (PASP, 125, 600, [2013])—Corrigendum | |
THE PHYSICAL CHARACTERISTICS OF THE GAS IN THE DISK OF CENTAURUS A USING THEHERSCHEL SPACE OBSERVATORY | |
Pillars and globules at the edges of H ii regions | |
Probing the Baryon Cycle of Galaxies with SPICA Mid- and Far-Infrared Observations | |
Probing the high-redshift universe with SPICA: Toward the epoch of reionisation and beyond | |
Probing the molecular interstellar medium of M82 withHerschel-SPIRE spectroscopy | |
Quantifying the heating sources for mid-infrared dust emissions in galaxies: the case of M 81 | |
Reconstructing the density and temperature structure of prestellar cores fromHerscheldata: A case study for B68 and L1689B | |
Regional variations in the dense gas heating and cooling in M51 from Herschel far-infrared spectroscopy | |
The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83 | |
A resolved analysis of cold dust and gas in the nearby edge-on spiral NGC 891 | |
Revealing the cold dust in low-metallicity environments. I. Photometry analysis of the Dwarf Galaxy Survey with Herschel | |
SAFARI digital processing unit: performance analysis of the SpaceWire links in case of a LEON3-FT based CPU | |
Searching for Heavily Obscured AGN at High Redshift with the SAFARI-SPICA Spectro-Photometer | |
Short time scale variability of the BL Lacertae object OJ 287 in the near-infrared | |
Spatially resolved stellar, dust, and gas properties of the post-interacting whirlpool galaxy system | |
SPICA—A Large Cryogenic Infrared Space Telescope: Unveiling the Obscured Universe | |
SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust | |
SPIRE imaging of M 82: Cool dust in the wind and tidal streams | |
SpitzerIRS High‐Resolution Spectroscopy of the 12 μm Seyfert Galaxies. I. First Results | |
Star formation and dust heating in the FIR bright sources of M83 | |
Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey (Corrigendum) | |
Submm/FIR Astronomy in Antarctica: Potential for a large telescope facility | |
TheHerschelview of the on-going star formation in the Vela-C molecular cloud | |
Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales | |
Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-zUniverse | |
Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA | |
A traffic analyzer for multiple SpaceWire links | |
Unbiased Large Spectroscopic Surveys of Galaxies Selected by SPICA Using Dust Bands | |
WHAT DETERMINES THE DENSITY STRUCTURE OF MOLECULAR CLOUDS? A CASE STUDY OF ORION B WITHHERSCHEL |