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HCN emission from translucent gas and UV-illuminated cloud edges revealed by wide-field IRAM 30 m maps of the Orion B GMC

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Revealing the CO X-factor in Dark Molecular Gas through Sensitive ALMA Absorption Observations

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The Astrophysical Journal Letters 889 (1) L4 (2020)
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Chemical Complexity in Local Diffuse and Translucent Clouds: Ubiquitous Linear C3H and CH3CN, a Detection of HC3N and an Upper Limit on the Abundance of CH2CN*

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The Role of Electron Excitation and Nature of Molecular Gas in Cluster Central Elliptical Galaxies

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A precise and accurate determination of the cosmic microwave background temperature atz= 0.89

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What Microwave Astronomical Spectroscopy can tell you about the Carriers of the DIBs

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Proceedings of the International Astronomical Union 9 (S297) 163 (2013)
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HERSCHEL/SPIRE SUBMILLIMETER SPECTRA OF LOCAL ACTIVE GALAXIES,

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