S. Guest

Gas near active galactic nuclei: A search for the 4.7 μm CO band

Mapping ices in protostellar environments on 1000 AU scales

ISOCAM observations in the Lockman Hole

Multiple protostellar systems

DeepU-B-Vimaging of the Lockman Hole with the LBT

ISOCAM observations in the Lockman Hole

Millimeter Observations of Obscured Spitzer 24 μm Sources

SPITZER QUASAR AND ULIRG EVOLUTION STUDY (QUEST). IV. COMPARISON OF 1 Jy ULTRALUMINOUS INFRARED GALAXIES WITH PALOMAR-GREEN QUASARS

Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas

ISOCAM observations in the Lockman Hole . II. The 14.3 μm deep survey: Data reduction, catalogue and source counts

The [Cii] 158 Micron Line Deficit in Ultraluminous Infrared Galaxies Revisited

A BACKWARD EVOLUTION MODEL FOR INFRARED SURVEYS: THE ROLE OF AGN– AND COLOR–L_TIRDISTRIBUTIONS

Mapping ices in protostellar environments on 1000 AU scales: Methanol-rich ice in the envelope of Serpens SMM 4

HERUS: A CO ATLAS FROM SPIRE SPECTROSCOPY OF LOCAL ULIRGs

AGN feedback in a galaxy merger: Multi-phase, galaxy-scale outflows with a fast molecular gas blob ~6 kpc away from IRAS F08572+3915

LINE DERIVED INFRARED EXTINCTION TOWARD THE GALACTIC CENTER

Herschel reveals a molecular outflow in a z = 2.3 ULIRG

ISOCAM‐CVF 5–12 Micron Spectroscopy of Ultraluminous Infrared Galaxies

Follow-up near-infrared spectroscopy of ultraluminous infrared galaxies\n observed by ISO

ISOCAM observations in the Lockman Hole. I. The 14.3 μm shallow survey: Data reduction, catalogue, and optical identifications

The data processing pipeline for the Herschel/SPIRE imaging Fourier Transform Spectrometer

The Isocam Responsivity in Orbit. Standard star photometry

The data processing pipeline for theHerschelSPIRE Fourier Transform Spectrometer

The data processing pipelines for the Herschel/SPIRE imaging Fourier transform spectrometer

The ISOCAM/LW Detector Dark Current Behaviour