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Multimessenger Analysis Strategy for Core-Collapse Supernova Search: Gravitational Waves and Low-energy Neutrinos

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Odysse Halim, Claudio Casentini, Marco Drago, Viviana Fafone, Kate Scholberg, Carlo Francesco Vigorito, and Giulia Pagliaroli

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VIR-0717A-21

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10:22, Tuesday, 22 June, 2021

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halim

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https://tds.virgo-gw.eu/ql/?c=16965

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- The cosmic merger rate density evolution of compact binaries formed in young star clusters and in isolated binaries (VIR-0312B-20)
- The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution (VIR-0719B-20)
- The document on data release policy (VIR-0648B-20)
- The first 100 ms of a long-lived magnetized neutron star formed in a binary neutron star merger (VIR-0363A-19)
- The host galaxies of double compact objects across cosmic time (VIR-0503A-19)
- The hunt for environmental noise in Virgo during the third observing run (VIR-0520D-20)
- The impact of hydrogen-rich envelope, dredge-up and 12 C(α, γ) 16 O rate on the pair instability black hole mass gap (VIR-0780B-20)
- The kilonova of GW190425-like events (VIR-0134A-20)
- The properties of merging neutron stars and black holes across cosmic time (VIR-0016A-19)
- The research on amorphous coatings for future GW detectors (Proceedings TAUP 2019) (VIR-1048A-19)
- The search of higher multipole radiation in gravitational waves from compact binary coalescences by a minimally-modelled pipeline (VIR-0761A-21)
- Thermodynamic conditions of matter in neutron star mergers (contribution to a EPJ special issue on the impact of GW170817 on the nuclear EOS) (VIR-0236C-19)
- Tool based on un-modeled transient search to extract Post merger neutron stars properties (VIR-0440A-17)
- Torino group presentation (VIR-0735A-18)
- Total-variation methods for gravitational-wave denoising: performance tests on Advanced LIGO data (VIR-0331A-18)
- Towards asteroseismology of core-collapse supernovae with gravitational-wave observations - II. Spacetime perturbations (VIR-0410A-18)
- Towards the AdV computing model update: CDP part (to be presented at ECC meeting) (VIR-0706C-18)
- Understanding gravitational-wave emission from core-collapse supernovae (VIR-0156A-19)
- Unmodeled characterization of post-merger gravitational wave emission from binary neutron stars coalescence (VIR-0213A-20)
- Update circular for LIGO/Virgo G270580: candidate retraction (VIR-0514A-17)
- Update on ER14 cWB online Virgo contribution (VIR-0323A-19)
- Upgrades of coherentWaveBurst for burst searches in the O2 run (VIR-0437A-16)
- VIRGO-the-future (my personal vision) (VIR-0486B-20)
- VW Presentation - Expanding Core-Collapse Supernova Search Horizon of Multimessenger Detectors (VIR-0069A-20)
- Virgo offline computing and data processing (VIR-0541A-19)
- Virgo offline computing and data processing (VIR-0782A-18)
- Virgo-week PE_slides (VIR-0848A-17)
- Was GW190814 a Black Hole - Strange Quark Star system? (VIR-0812A-21)
- Wavegraph clustering for coherent waveburst - Principles, applications, improvements. (VIR-0259A-16)
- Wavegraph updates: method paper & O2 results (VIR-0673A-17)
- Wavelet graphs for the detection of gravitational waves: application to eccentric binary black holes (VIR-0091A-19)
- Wavelet-based search for gravitational wave detection - Updates (VIR-0026F-17)
- What can be learned from a proto-neutron star's mass and radius? (VIR-0001A-21)
- Working with Gravitational-Wave sky localizations: new methods and implementations (VIR-0630A-19)
- Xpipeline closed-box results: the effects of adding Virgo on the global sensitivity of the network for the O2 GRBs with 3 Detectors online (updated with 50% Upper Limits) (VIR-0538D-18)
- cWB ER13 offline analysis (VIR-0093A-19)
- cWB low latency: ER13 and O3 plans (VIR-0039B-19)
- cWB offline O2 searches related to CBC sources (VIR-0825A-17)
- coherent Waveburst, a pipeline for unmodeled gravitational-wave data analysis (VIR-0310C-20)
- coherentWaveBurst contribution to current LVC papers (VIR-0387A-20)

Presentation requests

- Invitations received by members of the Collaboration, to present Virgo or parts of it, must be forwarded to the VEB. In order to ensure a fair distribution of talks to individuals and institutions, the VEB will select a speaker from the Collaboration, trying to keep a good balance between respecting the wishes of conference organizers and the requirement of a fair share of presentations among Collaboration members and the need to promote young colleagues.
- Full Virgo Collaboration Publication and Presentation Rules are available here.