Index
| FoM | OR | Link |
|---|---|---|
| Background | ||
| Estimating the galactic background noise [1.0 yr] | SI1.1 1.1c | report |
| Estimating the galactic background noise [4.5 yr] | SI1.1 1.1c | report |
| SO1 : Study the formation and evolution of compact binary stars in the Milky Way Galaxy. | ||
| Horizon distance of stellar-mass source 4.5 yr | SI1.1, SI1.2, SI4.1, SI4.2 1.1.a, 1.2.b, 4.1, 4.2 | report |
| Capability to detect and characterise a significantly large population of resolved detached stellar-mass binaries [4.5 yr] | SI1.1 1.1a | report |
| Capability to detect mass-transferring binaries [4.5 yr] | SI1.1, SI1.2 1.1a, 1.2c | report |
| Capability to detect and characterise a significantly large population of resolved stellar mass-binaries with accurate chirp masses. [4.5 yr] | SI1.1 1.1b | report |
| Capability to detect and characterise a significantly large population of resolved stellar mass-binaries with accurate position. [4.5 yr] | SI1.1 1.1b | report |
| Capability to characterize mass-transferring binaries [4.5 yr] | SI1.2 1.2c | report |
| Detectability of verification binaries and measurement of the their frequency evolution [1.0 yr] | SI1.2 1.2a | report |
| Detectability of verification binaries and measurement of the their frequency evolution [4.5 yr] | SI1.2 1.2a | report |
| SO2 : Trace the origin, growth and merger history of massive black holes across cosmic ages | ||
| Disentangling seed formation mechanisms [4.5 yr] | SI 3.2.1 | report |
| Reconstructing the cosmic history (mass measurements) [4.5 yr] | SI 3.2.2a | report |
| Reconstructing the cosmic history (spin measurements) [4.5 yr] | SI 3.2.2b | report |
| Discovering nearly equal mass IMBHs in the local universe [4.5 yr] | SI 3.2.4a | report |
| Discovering unequal mass IMBHs [4.5 yr] | SI 3.2.4b | report |
| Multimessenger astronomy, enabling pre-localization of platinum binaries [4.5 yr] | SI 3.2.3a | report |
| Multimessenger astronomy, post merger [4.5 yr] | SI 3.2.3b | report |
| SO3 : Probe the dynamics of dense nuclear clusters using EMRIs | ||
| Detectability of \(10^5-10 M_{\odot}\) 2 years EMRI at redshift z=3 with eccentricity e_plunge=0.68 [1.0 yr] | SI3.1 3.1 | report |
| Detectability of \(10^6-10 M_{\odot}\) 2 years EMRI at redshift z=3 with eccentricity e_plunge=0.25 [1.0 yr] | SI3.1 3.1 | report |
| Detectability of EMRI catalog [4.5 yr] | WP SI.3 | report |
| SO4 : Understand the astrophysics of stellar origin black holes | ||
| Ability to detect GW150914-like events using optimal sky position [4.5 yr] | SI4.1 4.1 | report |
| Capability to detect a 10-10 \(M_{\odot}\) BH-BH source out to specific horizon distances [4.5 yr] | SI4.2 | report |
| Capability to detect a GW150914 like source out to specific horizon distances [4.5 yr] | SI4.1 SI4.2 4.2 | report |
| Capability to detect a GW190521 like source out to specific horizon distances [4.5 yr] | SI4.2 4.2 | report |
| Number of detectable sources based on the LVC astrophysical model of BBH population [4.5 yr] | SI4.1, SI4.2 | report |
| SO5 : Explore the fundamental nature of gravity and black holes | ||
| Detectability of ringdown for high mass SMBH [1.0 yr] | SI5.1 5.1 | report |
| Probing near-horizon structures: GW echoes from exotic compact objects [1.0 yr] | 5.1 | report |
| Detectability of GWs from ultralight scalar clouds [4.5 yr] | SI5.5 | report |
| SO6 : Probe the rate of expansion of the Universe | ||
| MBHB as standard sirens [1.0 yr] | SI6.2 6.2 | report |
| SO7 : Understand stochastic GW backgrounds | ||
| Unresolved stellar origin black holes [4.5 yr] | SI7.1 7.1 | report |
| Cosmic strings beyond SKA [4.5 yr] | iSI7.2 7.2 | report |
| SGWB from PBH dark matter [4.5 yr] | SR7.2 | report |
| Characterise representative template for SGWB power-law with n=0 [4.5 yr] | 7.2 SI7.2 | report |
| Characterise representative template for SGWB power-law with n=2/3 [4.5 yr] | SI7.2, 7.2 | report |
| Characterise representative template for SGWB power-law with n=-3 [4.5 yr] | 7.2 SI7.2 | report |
About
Those results have been obtained on the 11/04/2022, 18:12:06.
Using commit: b'289219549752bd88f7fe4e0b43208f45b5a42e4b' of FoM repo.
Pipeline configuration is reported here: report.