D. Polychroni

activity

20132017

most citedProperties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy (

- 71. 0^{\circ} < ℓ < 67. 0^{\circ}

)

201 citations · 252 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2017★ 201 cited

Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ( $- 71. 0^{\circ} < ℓ < 67. 0^{\circ}$ )

D. Elia, S. Molinari, E. Schisano +83

Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 $μ$ m. We present a band-merged catalogue of spatia…

astro-ph.GA2016

Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues. First data release for Inner Milky Way: +68°> l > -70°

S. Molinari, E. Schisano, D. Elia +62

(Abridged) We present the first public release of high-quality data products (DR1) from Hi-GAL, the {\em Herschel} infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite…

astro-ph.GA2013★ 51 cited

Herschel Observations of the W3 GMC: Clues to the Formation of Clusters of High-Mass Stars

A. Rivera-Ingraham, P. G. Martin, D. Polychroni +22

The W3 GMC is a prime target for the study of the early stages of high-mass star formation. We have used Herschel data from the HOBYS key program to produce and analyze column dens…

Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy (−71.0∘<ℓ<67.0∘)

Hi-GAL, the Herschel infrared Galactic Plane Survey: photometric maps and compact source catalogues. First data release for Inner Milky Way: +68°> l > -70°

Herschel Observations of the W3 GMC: Clues to the Formation of Clusters of High-Mass Stars

Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ( $- 71. 0^{\circ} < ℓ < 67. 0^{\circ}$ )