Submillimeter observations made with a rapid-scanning interferometer during the solar eclipse of June 30, 1973 are reported. Reduction, correction, and plotting...
Submillimeter Polarization Spectrum in the Vela C Molecular Cloud
Polarization maps of the Vela C molecular cloud were obtained at 250, 350, and 500 μm during the 2012 flight of the balloon-borne telescope BLASTPol. These...
Submillimeter Polarization Spectrum of the Carina Nebula
Linear polarization maps of the Carina Nebula were obtained at 250, 350, and 500 μm during the 2012 flight of the Balloon-borne Large Aperture Submillimeter...
Submillimeter-wave atmospheric and astrophysical spectroscopy
The paper describes some results and methods of work on the submillimeter spectrum and its application to atmospheric and astrophysical problems. The paper...
Submillimetre compactness as a critical dimension to understand the main sequence of star-forming galaxies
We study the interstellar medium (ISM) properties as a function of the molecular gas size for 77 infrared-selected galaxies at z ~ 1.3, having stellar masses 10...
Submillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks
Submillimetre galaxies represent a rapid growth phase of both star formation and massive galaxies. Mapping SMGs in galaxy protoclusters provides key insights...
Submillimetre galaxies reside in dark matter haloes with masses greater than 3×1011 solar masses
The extragalactic background light at far-infrared wavelengths comes from optically faint, dusty, star-forming galaxies in the Universe with star formation...
Subpercent constraints on the cosmological temperature evolution
The redshift dependence of the cosmic microwave background temperature is one of the key cosmological observables. In the standard cosmological model, one has T...
Substellar objects in star formation regions: A deep near infrared study in the Serpens cloud
We present near infrared (J, H and Ks) observations of a 5'× 10' sample field in the Serpens Star Formation region obtained with SOFI at the NTT. These...