Showing 1–20 of 63 results
/ Date/ Name
Jan 8, 2019Dust opacity variations in the pre-stellar core L1544Sep 29, 2008Application of a Self-Similar Pressure Profile to Sunyaev-Zel'dovich Effect Data from Galaxy ClustersJun 21, 2021Thermodynamic evolution of the $z=1.75$ galaxy cluster IDCS J1426.5+3508Feb 16, 2021Large format imaging spectrograph for the Large Submillimeter Telescope (LST)Jan 21, 2015Resolving the Merging Planck Cluster PLCK G147.3-16.6 with GISMOAug 10, 2017VLA Radio Observations of the HST Frontier Fields Cluster Abell 2744: The Discovery of New Radio RelicsJan 15, 2017Chandra and JVLA observations of HST Frontier Fields cluster MACS J0717.5+3745Dec 22, 2016Sub-arcsecond imaging of the water emission in Arp 220Jun 10, 2025The MeerKAT Massive Distant Clusters Survey: Detection of Diffuse Radio Emission in Galaxy Clusters at $z > 1$Dec 30, 2020MERGHERS Pilot: MeerKAT discovery of diffuse emission in nine massive Sunyaev-Zel'dovich-selected galaxy clusters from ACTSep 30, 2022The 700 ks Chandra Spiderweb Field II: Evidence for inverse-Compton and thermal diffuse emission in the Spiderweb galaxyDec 15, 2022Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologuesJul 16, 2010Galaxy Clusters at z>=1: Gas Constraints from the Sunyaev-Zel'dovich ArrayJul 29, 2011Discovery of the correspondence between intra-cluster radio emission and a high pressure region detected through the Sunyaev-Zel'dovich effectMay 21, 2015Frontier Fields Clusters: Chandra and JVLA View of the Pre-Merging Cluster MACS J0416.1-2403Mar 24, 2015A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10$^{15}$M$_{\odot}$ Galaxy Cluster at z=0.7Jul 29, 2025The Atacama Cosmology Telescope: DR6 Sunyaev-Zel'dovich Selected Galaxy Clusters CatalogMar 14, 2019Mapping Galaxy Clusters in the Distant UniverseJun 11, 2014Galaxy Cluster Scaling Relations between Bolocam Sunyaev-Zel'dovich Effect and Chandra X-ray MeasurementsOct 27, 2016The Case for a Publicly Available, Well-Instrumented GBT Operating at 20-115 GHz