Showing 1–20 of 211 results
/ Date/ Name
Nov 2, 2012Tearing the Veil: interaction of the Orion Nebula with its neutral environmentJan 19, 2006Extreme superstarclustersNov 24, 2004Dissecting starburst galaxies with infrared observationsNov 27, 1998Discovery of distant high luminosity infrared galaxiesJan 21, 1998Observations and diagnostic use of highly redshifted fine structure linesOct 23, 2000Can dusty Lyman break galaxies produce the submillimeter counts and background? Lessons from lensed Lyman break galaxiesNov 10, 2000Lessons from lensed Lyman break galaxies: can dusty Lyman break galaxies produce the submillimetre counts and background?Jun 13, 1997Star formation at high redshift as traced by near-infrared Halpha surveysMay 29, 1998Dust and molecular gas in high redshift radio galaxiesJan 11, 2001Starbursts in ultraluminous infrared galaxies - fueling and propertiesJun 23, 2011Water vapor emission reveals a highly obscured, star forming nuclear region in the QSO host galaxy APM08279+5255 at z=3.9Aug 9, 2001Probing the evolution of galaxies using redshifted H-alpha emissionJan 17, 2000H2 emission as a diagnostic of physical processes in starforming galaxiesJun 6, 2007First CO J=6-5, 4-3 detections in local ULIRGs: the dense gas in Mrk231, and its colling budgetFeb 8, 2012The molecular gas in Luminous Infrared Galaxies II: extreme physical conditions, and their effects on the X_{co} factorSep 30, 2012An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: High resolution 870um source countsFeb 2, 2022The ALMA REBELS Survey: Efficient Ly$α$ Transmission of UV-Bright z$\simeq$7 Galaxies from Large Velocity Offsets and Broad Line WidthsFeb 5, 2023Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep SurveyApr 7, 2024Physical Properties of the Southwest Outflow Streamer in the Starburst Galaxy NGC 253 with ALCHEMIMay 19, 2020VLA-ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): Total Cold Gas Masses and CO Line Ratios for z=2-3 "Main Sequence" Galaxies