Skip to content. | Skip to navigation
- Home
- About NRAO
- Science
- Observing
- Opportunities
- SRDP
-
VLASS
- News
- Science Themes & Impacts
- VLASS Data
- Community
- Public Outreach
- Library
- Pilot Survey
- Commensal Surveys
- VLASS 2.1 observations complete
- VLASS 2.2 observations to begin 2021/9/29
- VLASS 2.2 observations to begin early
- VLASS SE continuum users guide
- User-contributed software and scripts
- VLASS at AAS242 June 2023
- VLASS at AAS242 Abstracts
- Technical Implementation Plan
- VLASS pipeline versions
- ngVLA
- CASPER 2012
-
- CASPER Introduction
- The CASPER Collaboration for Radio Astronomy Signal Processing
- Introduction to the CASPER tools
- Python for Casper
- Tutorial Introductions
- DataDirect Networks—High Performance Storage Subsystems
- Hittite Corporation—High Performace ADCs
- The USRPA Flexible Mixed-Signal Platform for Scientific Instrumentation
- Black Hole Science with CASPER the Event Horizon Telescope
- Solar Burst Spectra with a CASPER-Based Correlator
- Science Update from the GMRT
- MeerKAT Status Update
- The LOFAR Station Correlator and Updates from CASPER at Oxford
- VEGAS: the VErsatile GBT Astronomical Spectrometer
- From MeerKAT to SKA-1s Dish Array: A Digital Perspective
- Scalable ROACH F-Engine for Correlators
- High Level Issues for the Implementation of Scientific Applications in High Performance Heterogeneous Systems
- FPGA/GPU Hybrid Correlator Design and Implementation
- An FPGA/GPU Correlator Prototype: Toward LEDA First Light
- Future Development Plans for the GMRT
- Design, Development and Testing of a GPU Based Backend for the GMRT
- CASPER Technology Use in the ALMA Phasing Project
- The ROACH-1 DBE Implementation for VLBA: A success story
- Xilinx Technology Update
- Arista Networks Technology
- New detection techniques for Ultra-High Energy Cosmic Rays, an R&D effort for wide-field microwave transient telescopes
- Real-time UWB 2-D Analog Fan Filters for Steerable Highly Selective Analog Aperture Arrays
- Digital Architectures for RF Real-time UWB Aperture-Array Beam Forming Using 2-D IIR Spatio-temporal Beam Filters
- Three-Dimensional 3-D Wave-Digital Filter Beamformer Architectures for RF Dense Aperture Array Applications
- Implementing Simulation Models for Multi-and many-core Processors
- Optimizing and Profiling the Processor-FPGA Interface Under Linux
- Mapping of Heterogeneous Instruments for Radio Astronomy
- Derivation of Low-Level ADC and Correlator Development Specifications From Telescope Level Specifications
- A System Engineering Plan for ROACHx
- Effective Testing in the CASPER Toolflow
- Design and Development of an ROACH 2 Based Digital FX Correlator for the EOVSA
- Direct Imaging with BEST-2
- Digitizing AmiBA for CO Intensity Mapping
- Development of FPGA Based Wide-Band Digital Backends for the Upgraded GMRT
- First Passive Radar Receiver Implementation with ROACH
- A Low Cost Disciplined Sampling Clock Using the WWVB 60KHz Broadcast
- A New Flexible Backend for the Parkes 21cm Multibeam Receiver
- MeerKAT Digitiser
- MeerKAT Digitizer Phase and Gain Stability
- ASIAA 10 Gsps ADC Board Development
The National Radio Astronomy Observatory is a facility of the National Science Foundation
operated under cooperative agreement by Associated Universities, Inc.
