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FERMI -LAT OBSERVATIONS OF THE DIFFUSE γ-RAY EMISSION: IMPLICATIONS FOR COSMIC RAYS AND THE INTERSTELLAR MEDIUM
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On the Problem of the Most Efficient Tests of Statistical Hypotheses
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Infrared Excess and Molecular Clouds: A Comparison of New Surveys of Far‐Infrared and H i 21 Centimeter Emission at High Galactic Latitudes
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FERMI OBSERVATIONS OF CASSIOPEIA AND CEPHEUS: DIFFUSE GAMMA-RAY EMISSION IN THE OUTER GALAXY
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Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the “dark gas” in our Galaxy
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FERMI LARGE AREA TELESCOPE STUDY OF COSMIC RAYS AND THE INTERSTELLAR MEDIUM IN NEARBY MOLECULAR CLOUDS
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Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties
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E ( B – V ), N (H I), AND N (H 2 )
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GAMMA-RAY OBSERVATIONS OF THE ORION MOLECULAR CLOUDS WITH THE FERMI LARGE AREA TELESCOPE
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The dark Molecular gas
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THE SPECTRUM AND MORPHOLOGY OF THE FERMI BUBBLES
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Planck intermediate results: XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies⋆
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FAINT EXTENDED OH EMISSION FROM THE LOCAL INTERSTELLAR MEDIUM IN THE DIRECTION l ≈ 108°, b ≈ 5°
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Evolution of dust properties in an interstellar filament
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The Milky Way in Molecular Clouds: A New Complete CO Survey
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THE ATOMIC-TO-MOLECULAR TRANSITION IN GALAXIES. II: H I AND H 2 COLUMN DENSITIES
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Changes of dust Opacity with Density in the Orion a Molecular Cloud
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Planck early results. XXI. Properties of the interstellar medium in the Galactic plane
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Effects of magnetic fields on the cosmic-ray ionization of molecular cloud cores
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The Millennium Arecibo 21 Centimeter Absorption‐Line Survey. II. Properties of the Warm and Cold Neutral Media
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A HIGH-RESOLUTION STUDY OF THE H I-H 2 TRANSITION ACROSS THE PERSEUS MOLECULAR CLOUD
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The Relation Between gas and dust in the Taurus Molecular Cloud
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August 2010 |
${\rm H\,\scriptsize{I}}$, CO, AND PLANCK / IRAS DUST PROPERTIES IN THE HIGH LATITUDE CLOUD COMPLEX, MBM 53, 54, 55 AND HLCG 92 – 35. POSSIBLE EVIDENCE FOR AN OPTICALLY THICK ${\rm H\,\scriptsize{I}}$ ENVELOPE AROUND THE CO CLOUDS
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November 2014 |
THE FERMI LARGE AREA TELESCOPE ON ORBIT: EVENT CLASSIFICATION, INSTRUMENT RESPONSE FUNCTIONS, AND CALIBRATION
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October 2012 |
High-Energy Cosmic-Ray Diffusion in Molecular Clouds: a Numerical Approach
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GIANT GAMMA-RAY BUBBLES FROM FERMI -LAT: ACTIVE GALACTIC NUCLEUS ACTIVITY OR BIPOLAR GALACTIC WIND?
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The photodissociation and chemistry of interstellar CO
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A Large Catalog of Accurate Distances to Molecular Clouds from ps1 Photometry
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A Large Scale 12 CO (J=1−0) Survey toward the Chamaeleon Region with NANTEN
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Characterization and Physical Explanation of Energetic Particles on Planck HFI Instrument
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Plasma Diagnostics of the Interstellar Medium with Radio Astronomy
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Skillful statistical models to predict seasonal wind speed and solar radiation in a Yangtze River estuary case study
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Planck pre-launch status: HFI ground calibration
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Joint 3D modelling of the polarized Galactic synchrotron and thermal dust foreground diffuse emission
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January 2011 |
IceCube sensitivity for low-energy neutrinos from nearby supernovae ( Corrigendum )
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Planck 2013 results. XVII. Gravitational lensing by large-scale structure
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Planck 2013 results. XVI. Cosmological parameters
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Flux upper limits for 47 AGN observed with H.E.S.S. in 2004−2011
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Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck -HFI observations
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The Herschel Reference Survey
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On the proper kinetic quadrupole CMB removal and the quadrupole anomalies
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