activity
20022025
most citedThe Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager

345 citations · 1.2k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2025★ 6 cited

ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump

E. Schisano, S. Molinari, A. Coletta +51

High-mass stars and star clusters form from the fragmentation of massive dense clumps driven by gravity, turbulence, and magnetic fields. The ALMAGAL project observed cl…

astro-ph.GA2017★ 69 cited

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

astro-ph.GA2016★ 54 cited

Star formation laws in both Galactic massive clumps and external galaxies: An extensive study with dust continuum, HCN (4-3), and CS (7-6)

Tie Liu, Kee-Tae Kim, Hyunju Yoo +20

We observed 146 Galactic clumps in HCN (4-3) and CS (7-6) with the Atacama Submillimeter Telescope Experiment (ASTE) 10-m telescope. A tight linear relationship between star format…

astro-ph.GA2013★ 181 cited

MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey

J. M. Jackson, J. M. Rathborne, J. B. Foster +53

The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and chemical evolution of high-mass star-forming clumps. Exploiting the unique broad f…

astro-ph2003★ 37 cited

A parsec-scale flow associated with the IRAS 16547-4247 radio jet

K. J. Brooks, G. Garay, D. Mardones +1

IRAS 16547-4247 is the most luminous (6.2 x 10^4 Lsun) embedded young stellar object known to harbor a thermal radio jet. We report the discovery using VLT-ISAAC of a chain of H_2…

astro-ph2002★ 280 cited

The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager

T. J. Pearson, B. S. Mason, A. C. S. Readhead +23

Using the Cosmic Background Imager, a 13-element interferometer array operating in the 26-36 GHz frequency band, we have observed 40 sq deg of sky in three pairs of fields, each ~…