The direct access to the interior of the Sun has been possible, over the past 25 years, by successfully applying seismic techniques to detect and to...
HELP project - a dreamed-of multiwavelength dataset for SED fitting: The influence of used models for the main physical properties of galaxies
The Herschel Extragalactic Legacy Project (HELP) focuses to publish an astronomical multiwavelength catalogue of millions of objects over 1300 deg 2 of the...
HERSCHEL OH SPECTROSCOPY OF SEYFERT, LINER, AND STARBURST GALAXIES
We select a sample of 179 local (0 ≤ z 0.35) galaxies from the Hershel Science Archive to investigate possible relationships between the 65μm, 71μm, 79μm, 84μm...
The Herschel Reference Survey is a Herschel guaranteed time key project and will be a benchmark study of dust in the nearby universe. The survey will complement...
We present the first study of the far-infrared (FIR) properties of high-redshift, radio-selected ultraluminous infrared galaxies (ULIRGs) using deep...
Herschel-SPIRE spectroscopy of nearby Seyfert galaxies
We present the 450-1550 GHz spectra of three nearby Seyfert galaxies (NGC1068, NGC7130 and NGC7582) taken with the Herschel SPIRE FTS. For the case of NGC1068...
Herschel-SPIRE: design, ground test results, and predicted performance
SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for Herschel. It comprises a three-band camera operating at 250...
Herschel-SPIRE: design, performance, and scientific capabilities
SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for the European Space Agency's Herschel Space Observatory. It...
Herschel/PACS: Constraining clumping in the intermediate wind region of OB stars
At present, it is well established that previously accepted mass-loss rates (Ṁ) of luminous OB stars may be overestimated when clumping is neglected. Our...