activity
20052021
most citedHi-GAL: the Herschel infrared Galactic Plane Survey

614 citations · 1k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2021★ 82 cited

ALCHEMI: an ALMA Comprehensive High-resolution Extragalactic Molecular Inventory. Survey presentation and first results from the ACA array

S. Martín, J. G. Mangum, N. Harada +32

We used the Atacama Large Millimeter/submillimeter Array (ALMA), covering a nearly contiguous 289 GHz frequency range between 84.2 and 373.2 GHz, to image the continuum and spectra…

astro-ph.GA2012★ 28 cited

Small-scale structure in the interstellar medium: time-varying interstellar absorption towards κ Velorum

Keith T. Smith, Stephen J. Fossey, Martin A. Cordiner +4

Ultra-high spectral resolution observations of time-varying interstellar absorption towards κ Vel are reported, using the Ultra-High Resolution Facility on the Anglo-Australian Tel…

astro-ph.EP2011★ 116 cited

EChO - Exoplanet Characterisation Observatory

G. Tinetti, J. P. Beaulieu, T. Henning +131

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context…

astro-ph.GA2010★ 614 cited

Hi-GAL: the Herschel infrared Galactic Plane Survey

S. Molinari, the Hi-GAL Consortium

Hi-GAL, the Herschel infrared Galactic Plane Survey, is an Open Time Key Project of the Herschel Space Observatory. It will make an unbiased photometric survey of the inner Galacti…

astro-ph.SR2009★ 79 cited

Knots in the Helix Nebula found in H2

M. Matsuura, A. K. Speck, B. M. McHunu +6

We present a deep and wide field-of-view (4'x 7') image of the planetary nebula (PN) NGC 7293 (the Helix Nebula) in the 2.12 micron H2 v=1-0 S(1) line. The excellent seeing (0.4'')…

astro-ph2008★ 92 cited

Destruction of Molecular Gas Reservoirs in Early-Type Galaxies by Active Galactic Nucleus Feedback

Kevin Schawinski, Chris J. Lintott, Daniel Thomas +11

Residual star formation at late times in early-type galaxies and their progenitors must be suppressed in order to explain the population of red, passively evolving systems we see t…