The Recent Developmental Status of SNEGRAF: a Web-Based Gravitational Wave Signal Analyzer. (arXiv:1912.08571v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Eguchi_S/0/1/0/all/0/1">Satoshi Eguchi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Shibagaki_S/0/1/0/all/0/1">Shota Shibagaki</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hayama_K/0/1/0/all/0/1">Kazuhiro Hayama</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kotake_K/0/1/0/all/0/1">Kei Kotake</a>

Unveiling physical processes in a supernova is one of challenging topics of
modern physics and astrophysics since that event is due to particle physics on
a stellar scale and tightly related to nucleosynthesis in Universe.
Multi-messenger astronomy, a combination, such as of electromagnetic-wave,
gravitational-wave, and neutrino observations, will be a breakthrough to the
puzzle. To boost the research, we released a web-based gravitational wave
signal analyzer “SuperNova Event Gravitational-wave-display in Fukuoka
(SNEGRAF)” last year (Eguchi et al. 2019). We are now working on an integration
of the application with the RIDGE pipeline, which is for a coherent network
analysis between the LIGO, VIRGO, and KAGRA observations (Hayama et al. 2007),
and implemented in MATLAB. In the basic design phase, we decided to wrap RIDGE
with a simple Python script and make it listen for connections from SNEGRAF.
This design enables these two programs to be hosted on different servers
independently, and minimizes the cyber risks of RIDGE. In this paper, we report
the current developmental status of our system.

Unveiling physical processes in a supernova is one of challenging topics of
modern physics and astrophysics since that event is due to particle physics on
a stellar scale and tightly related to nucleosynthesis in Universe.
Multi-messenger astronomy, a combination, such as of electromagnetic-wave,
gravitational-wave, and neutrino observations, will be a breakthrough to the
puzzle. To boost the research, we released a web-based gravitational wave
signal analyzer “SuperNova Event Gravitational-wave-display in Fukuoka
(SNEGRAF)” last year (Eguchi et al. 2019). We are now working on an integration
of the application with the RIDGE pipeline, which is for a coherent network
analysis between the LIGO, VIRGO, and KAGRA observations (Hayama et al. 2007),
and implemented in MATLAB. In the basic design phase, we decided to wrap RIDGE
with a simple Python script and make it listen for connections from SNEGRAF.
This design enables these two programs to be hosted on different servers
independently, and minimizes the cyber risks of RIDGE. In this paper, we report
the current developmental status of our system.

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