scispace - formally typeset
S

Suzanne C. Madden

Researcher at Université Paris-Saclay

Publications -  42
Citations -  7481

Suzanne C. Madden is an academic researcher from Université Paris-Saclay. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 18, co-authored 42 publications receiving 6975 citations. Previous affiliations of Suzanne C. Madden include French Alternative Energies and Atomic Energy Commission & DSM.

Papers
More filters
Journal ArticleDOI

The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory

Albrecht Poglitsch, +83 more
TL;DR: The Photodetector Array Camera and Spectrometer (PACS) as discussed by the authors is one of the three science instruments on ESA's far infrared and sub-mil- limetre observatory.
Journal ArticleDOI

The Herschel-SPIRE instrument and its in-flight performance

Matthew Joseph Griffin, +189 more
TL;DR: The Spectral and Photometric Imaging REceiver (SPIRE) is the Herschel Space Observatory's sub-millimetre camera and spectrometer as discussed by the authors, which is used for image and spectroscopic data acquisition.
Journal ArticleDOI

Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (SAGE). I. Overview and Initial Results

TL;DR: The SAGE Legacy project as discussed by the authors performed a uniform and unbiased imaging survey of the Large Magellanic Cloud (LMC; 7° × 7°) using the IRAC (3.6, 4.5, 5.8, and 8 μm) and MIPS (24, 70, and 160μm) instruments on board the Spitzer Space Telescope.
Journal ArticleDOI

High-Resolution Imaging of Molecular Gas and Dust in the Antennae (NGC 4038/39): Super Giant Molecular Complexes

TL;DR: In this paper, the authors presented new aperture synthesis CO maps of the Antennae (NGC 4038/39) obtained with the Caltech Millimeter Array, revealing the large extent of the extranuclear region of star formation (the "overlap region"), which dominates the CO emission from this system.
Journal ArticleDOI

Dust in an extremely metal-poor galaxy: mid-infrared observations of SBS 0335-052

TL;DR: In this paper, the metal deficient (Z = Z_sun/41) Blue Compact Dwarf Galaxy (BCD) SBS 0335-052 was observed with ISOCAM between 5 and 17 mic.