Low Latency transient search of Gravitational Waves for the Advanced Detectors

Drago, Marco

アイテム詳細

登録内容を編集ファイル形式で保存

一時保存へ追加

タグ情報を表示リリース履歴を表示詳細要約

公開

成果報告書

Low Latency transient search of Gravitational Waves for the Advanced Detectors

MPS-Authors

/persons/resource/persons180430

Drago, Marco
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

External Resource

There are no locators available

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

フルテキスト (公開)

1507.02871.pdf
(プレプリント), 297KB

付随資料 (公開)

There is no public supplementary material available

引用

Drago, M. (submitted). Low Latency transient search of Gravitational Waves for the Advanced Detectors.

引用: https://hdl.handle.net/11858/00-001M-0000-0027-F40C-F

要旨

The reliability of the first detection is one of the most interesting challenges for the gravitational wave community. To increase the detection confidence, the LIGO and Virgo collaboration have already started coincident observations between gravitational waves detectors and other astronomical instruments, like electromagnetic or neutrino detectors. This can be done in two directions: searching for gravitational waves triggered by the electromagnetic informations, or pointing the electromagnetic telescopes to the sky position given in real time by the gravitational wave analysis. The success of the latter case depends strongly on the analysis speed of gravitational wave pipelines to analyze data and extract any gravitational wave candidate with as much information as possible. In this paper we discuss the case of the coherent Waveburst pipeline, the main pipeline used in the past scientific LIGO-Virgo analyses for the search of gravitational wave transients, reporting the capability of making an all-sky and all-time analysis and the analysis speed performance.