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Like most other configurable text editors, Atom enabled users to install third-party packages and themes to customize the features and looks of the editor. Packages could be installed, managed and published via Atom's package manager apm.
Tempo is a computer program to analyze radio observations of pulsars.Once enough observations are available, Tempo can deduce the pulsar rotation rate and phase, astrometric position and rates of change, and parameters of binary systems, by fitting models to pulse times of arrival measured at one or more terrestrial observatories. [1]
PyCBC is an open source software package primarily written in the Python programming language which is designed for use in gravitational-wave astronomy and gravitational-wave data analysis. [1] PyCBC contains modules for signal processing, FFT , matched filtering , gravitational waveform generation, among other tasks common in gravitational ...
The AtoM (previously ICA-AtoM) is a project originated by the International Council on Archives (ICA) that aimed to provide free license software that allows institutions to disseminate their archival holdings on the web. [2] Its last version in collaboration with the ICA was Release 1.3.2. [3]
This is a list of free and open-source software (FOSS) packages, computer software licensed under free software licenses and open-source licenses. Software that fits the Free Software Definition may be more appropriately called free software ; the GNU project in particular objects to their works being referred to as open-source . [ 1 ]
Pulsar: distributed pub-sub messaging system originally created at Yahoo; Qpid: AMQP messaging system in Java and C++; Ranger: a framework to enable, monitor and manage comprehensive data security across the Hadoop platform; Ratis: Java implementation for RAFT consensus protocol
A pulsar–neutron star system, e.g, PSR B1913+16. A pulsar and a normal star; e.g, PSR J0045−7319, a system that is composed of a pulsar and main-sequence B star. Theoretically, a pulsar-black hole system is possible and would be of enormous scientific interest but no such system has yet been identified.
The key property of a pulsar timing array is that the signal from a stochastic GW background will be correlated across the sightlines of pulsar pairs, while that from the other noise processes will not. [9] In the literature, this spatial correlation curve is called the Hellings-Downs curve or the overlap reduction function. [10]