SaprEMo: a simplified algorithm for predicting detections of electromagnetic transients in surveys. Issue 1 (21st December 2018)

• Record Type: Journal Article
• Authors: Vinciguerra, S; Branchesi, M; Ciolfi, R; Mandel, I; Neijssel, C J; Stratta, G
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 484:Issue 1(2019)
• Page Start: 332
• Page End: 344
• Publication Date: 2018-12-21
• Subjects: gravitational waves -- methods: data analysis -- catalogues -- surveys -- stars: neutron -- X-rays: bursts; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty3490
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: The multiwavelength detection of GW170817 has inaugurated multimessenger astronomy. The next step consists in interpreting observations coming from population of gravitational wave sources. We introduce saprEMo, a tool aimed at predicting the number of electromagnetic signals characterized by a specific light curve and spectrum, expected in a particular sky survey. By looking at past surveys, saprEMo allows us to constrain models of electromagnetic emission or event rates. Applying saprEMo to proposed astronomical missions/observing campaigns provides a perspective on their scientific impact and tests the effect of adopting different observational strategies. For our first case study, we adopt a model of spin-down-powered X-ray emission predicted for a binary neutron star merger producing a long-lived neutron star. We apply saprEMo on data collected by XMM–Newton and Chandra and during 10 4 s of observations with the mission concept THESEUS . We demonstrate that our emission model and binary neutron star merger rate imply the presence of some signals in the XMM–Newton catalogues. We also show that the new class of X-ray transients found by Bauer et al. in the Chandra Deep Field-South is marginally consistent with the expected rate. Finally, by studying the mission concept THESEUS, we demonstrate the substantial impact of a much larger field of view in searches of X-ray transients.