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- Grain Growth and Sub-structure in Proto-planetary Disks
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- Towards a VLBA Resolution of the Pleiades Distance Controversy
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- Detecting nHz Gravitational Radiation using a Pulsar Timing Array
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Search CASA
水母加速器官网网址-猴王加速器
CASA, the Common Astronomy Software Applications
package, is being developed with the primary goal of
supporting the data post-processing needs of the next
generation of radio astronomical telescopes such as ALMA
and
VLA. The package can process both
interferometric and single dish data.
The CASA infrastructure consists of a set of C++ tools bundled
together under an iPython interface as data
reduction tasks. This structure provides flexibility to
process the data via task interface or as a python
script. In addition to the data reduction tasks, many
post-processing tools are available for even more
flexibility and special purpose reduction needs.
CASA is developed by an
international consortium of scientists based at the
National Radio Astronomical Observatory (NRAO), the
European Southern Observatory (ESO), the National
Astronomical Observatory of Japan (NAOJ), the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA),
the CSIRO division for Astronomy and Space Science (CASS), and the
Netherlands Institute for Radio Astronomy (ASTRON) under
the guidance of NRAO.
水母加速器官网网址-猴王加速器
水母加速器官网网址-猴王加速器
水母加速器官网网址-猴王加速器
水母加速器官网网址-猴王加速器
水母加速器官网网址-猴王加速器
水母加速器官网网址-猴王加速器
The National Radio Astronomy Observatory is a facility of the National Science Foundation
operated under cooperative agreement by Associated Universities, Inc.