Showing 1–20 of 153 results
/ Date/ Name
May 17, 2011The extended atmospheres of Mira variables probed by VLTI, VLBA, and APEXMar 4, 2009CO line emission in the halo of a radio galaxy at z=2.6Feb 8, 2009A new search for distant radio galaxies in the Southern hemisphere -- III. Optical spectroscopy and analysis of the MRCR--SUMSS sampleOct 16, 2009Multi-wavelength properties of Spitzer-selected starbursts at z~2Oct 16, 2023The Quasar Feedback Survey: characterising CO excitation in quasar host galaxiesAug 5, 2022Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913Mar 11, 2013ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxiesSep 5, 2018Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early UniverseSep 26, 2019Prevalence of SED turndown among classical Be stars: Are all Be stars close binaries?Jul 28, 2020A wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecastJul 20, 2020High molecular gas content and star formation rates in local galaxies that host quasars, outflows and jetsNov 19, 2019VLT/SINFONI study of black hole growth in high redshift radio-loud quasars from the CARLA surveyJun 27, 2020Optical and near-infrared observations of the SPT2349-56 proto-cluster core at z = 4.3Aug 28, 2015Sub-kiloparsec Imaging of Cool Molecular Gas in Two Strongly Lensed Dusty, Star-Forming GalaxiesMay 19, 2017Are we seeing accretion flows in a 250kpc-sized Ly-alpha halo at z=3?Apr 15, 2013An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South: Source catalog and multiplicitySep 12, 2013SPT 0538-50: Physical conditions in the ISM of a strongly lensed dusty star-forming galaxy at z=2.8Nov 14, 2013Silicon isotopic abundance toward evolved stars and its application for presolar grainsOct 21, 2013Searching for large-scale structures around high-redshift radio galaxies with HerschelOct 5, 2016Gas kinematics in powerful radio galaxies at z~2: Energy supply from star formation, AGN, and radio jet