Showing 1–20 of 42 results
/ Date/ Name
Oct 1, 2025JADES Data Release 4 -- Paper II: Data reduction, analysis and emission-line fluxes of the complete spectroscopic sampleDec 8, 2022Identification and properties of intense star-forming galaxies at redshifts z>10Feb 7, 2022The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope III. Integral-field spectroscopyFeb 7, 2022The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope IV. Capabilities and predicted performance for exoplanet characterizationAug 11, 2011Far infrared constraints on the contamination by dust obscured galaxies of high-z dropout searchesFeb 10, 2020Molecular gas and star formation activity in LIRGs in clusters at intermediate redshiftsFeb 7, 2022The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope I. Overview of the instrument and its capabilitiesJul 9, 2019The impact of cosmic rays on the sensitivity of JWST/NIRSpecFeb 7, 2022The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope II. Multi-object spectroscopy (MOS)Aug 9, 2022Optical throughput and sensitivity of JWST NIRSpecJan 31, 2023In-orbit Performance of the Near-Infrared Spectrograph NIRSpec on the James Webb Space TelescopeMay 20, 2010LoCuSS: A Herschel view of obscured star formation in Abell 1835Oct 9, 2013Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing SurveyMay 20, 2010LoCuSS: Probing Galaxy Transformation Physics with HerschelOct 15, 2013[CII] and 12CO(1-0) Emission Maps in HLSJ091828.6+514223: A Strongly Lensed Interacting System at z=5.24Aug 3, 2015A complete census of Herschel-detected infrared sources within the HST Frontier FieldsMay 20, 2010Deep Herschel view of obscured star formation in the Bullet clusterMay 20, 2010The Herschel Lensing Survey (HLS): overviewMay 20, 2010Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshiftsDec 20, 2018Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2$\lesssim$$z$$\lesssim$0.9