L. Piazzo

activity

20112021

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 · 577 across the 8 of their papers we have counts for

collaborators

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3 papers · 1 filter

astro-ph.GA2021★ 106 cited

The Hi-GAL compact source catalogue -- II. The 360° catalogue of clump physical properties

D. Elia, M. Merello, S. Molinari +29

We present the $36 0^{\circ}$ catalogue of physical properties of Hi-GAL compact sources, detected between 70 and 500 $μ$ m. This release not only completes the analogous catalogue pre…

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.GA2013★ 119 cited

The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5

D. Elia, S. Molinari, Y. Fukui +17

We present the first Herschel PACS and SPIRE photometric observations in a portion of the outer Galaxy ( $216. 5^{\circ} ≲ ℓ ≲ 225. 5^{\circ}$ and $-2^{\circ} \lesssi…

The Hi-GAL compact source catalogue -- II. The 360° catalogue of clump physical properties

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∘)

The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5

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 ( $- 71. 0^{\circ} < ℓ < 67. 0^{\circ}$ )