Pi of the Sky in LSC-Virgo's em follow-up in O1 science run

© 2017 SPIE. Presented in this contribution are results gathered by Pi of the Sky during LSC-Virgo O1 science run. Pi of the Sky took part in LSC-Virgo's Electromagnetic (EM) Follow-up project during first science run of Advanced LIGO detectors between September 2015 and January 2016. LSC-Virgo...

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Main Authors: Zadrolny, A., Sokolowski, Marcin, Mankiewicz, L., Larnecki, A.
Format: Conference Paper
Published: 2017
Online Access:http://hdl.handle.net/20.500.11937/58001
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author Zadrolny, A.
Sokolowski, Marcin
Mankiewicz, L.
Larnecki, A.
author_facet Zadrolny, A.
Sokolowski, Marcin
Mankiewicz, L.
Larnecki, A.
author_sort Zadrolny, A.
building Curtin Institutional Repository
collection Online Access
description © 2017 SPIE. Presented in this contribution are results gathered by Pi of the Sky during LSC-Virgo O1 science run. Pi of the Sky took part in LSC-Virgo's Electromagnetic (EM) Follow-up project during first science run of Advanced LIGO detectors between September 2015 and January 2016. LSC-Virgo's EM Follow-up is aimed for searching electromagnetic counterparts to gravitational wave transient candidates. Observing an event both in EM and gravitational wave band might be a important step forward to multi-messenger astronomy. The aim of this paper is to show algorithms used by Pi of the Sky for analysing data taken during the first science run and to present the corresponding results. Concepts of algorithms for the next science run will also be discussed.
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spelling curtin-20.500.11937-580012017-11-20T08:58:08Z Pi of the Sky in LSC-Virgo's em follow-up in O1 science run Zadrolny, A. Sokolowski, Marcin Mankiewicz, L. Larnecki, A. © 2017 SPIE. Presented in this contribution are results gathered by Pi of the Sky during LSC-Virgo O1 science run. Pi of the Sky took part in LSC-Virgo's Electromagnetic (EM) Follow-up project during first science run of Advanced LIGO detectors between September 2015 and January 2016. LSC-Virgo's EM Follow-up is aimed for searching electromagnetic counterparts to gravitational wave transient candidates. Observing an event both in EM and gravitational wave band might be a important step forward to multi-messenger astronomy. The aim of this paper is to show algorithms used by Pi of the Sky for analysing data taken during the first science run and to present the corresponding results. Concepts of algorithms for the next science run will also be discussed. 2017 Conference Paper http://hdl.handle.net/20.500.11937/58001 10.1117/12.2281024 restricted
spellingShingle Zadrolny, A.
Sokolowski, Marcin
Mankiewicz, L.
Larnecki, A.
Pi of the Sky in LSC-Virgo's em follow-up in O1 science run
title Pi of the Sky in LSC-Virgo's em follow-up in O1 science run
title_full Pi of the Sky in LSC-Virgo's em follow-up in O1 science run
title_fullStr Pi of the Sky in LSC-Virgo's em follow-up in O1 science run
title_full_unstemmed Pi of the Sky in LSC-Virgo's em follow-up in O1 science run
title_short Pi of the Sky in LSC-Virgo's em follow-up in O1 science run
title_sort pi of the sky in lsc-virgo's em follow-up in o1 science run
url http://hdl.handle.net/20.500.11937/58001