Index
| FoM | OR | Link |
|---|---|---|
| Background | ||
| Estimating the galactic background noise [1.0 yr] | SI1.1 1.1c | report |
| Estimating the galactic background noise [6.0 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 6.0 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 [6.0 yr] | SI1.1 1.1a | report |
| Capability to detect mass-transferring binaries [6.0 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. [6.0 yr] | SI1.1 1.1b | report |
| Capability to detect and characterise a significantly large population of resolved stellar mass-binaries with accurate position. [6.0 yr] | SI1.1 1.1b | report |
| Capability to characterize mass-transferring binaries [6.0 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 [6.0 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 [1.0 yr] | SI2.1 2.1 | report |
| Constraining the progenitors of luminous quasars at the peak of quasar activity (new OR low freq) [1.0 yr] | new | report |
| Reconstructing the cosmic history of the most common MBHs populating galaxies today [1.0 yr] | SI2.2 2.2a | report |
| Understanding MBH spin growth [1.0 yr] | SI2.2 2.2b | report |
| Multimessenger astronomy, enabling follow-ups [1.0 yr] | SI2.3 2.3b | report |
| Discovering IMBHs in the local universe [1.0 yr] | SI2.4 2.4a | report |
| Detecting intermediate mass ratio inspirals [1.0 yr] | SI2.4 2.4b | report |
| Multimessenger astronomy, enabling pre-localization [1.0 yr] | SI2.3 2.3a | report |
| Multimessenger astronomy, enabling pre-localization of platinum binaries [1.0 yr] | SI2.3 2.3a | report |
| Disentangling seed formation mechanisms [1.0 yr] | SI2.1 2.1 | report |
| Disentangling seed formation mechanisms [1.0 yr] | SI2.1 2.1 | 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}=0.25 [1.0 yr] | SI3.1 3.1 | report |
| Detectability of \(10^6-10 M_{\odot}\) 2 years EMRI at redshift z=3 with eccentricity e0=0.25 [1.0 yr] | SI3.1 3.1 | report |
| Detectability of EMRI catalog [6.0 yr] | WP SI.3 | report |
| SO4 : Understand the astrophysics of stellar origin black holes | ||
| Ability to detect GW150914-like events using optimal sky position [6.0 yr] | SI4.1 4.1 | report |
| Capability to detect a 10-10 \(M_{\odot}\) BH-BH source out to specific horizon distances [6.0 yr] | SI4.2 | report |
| Capability to detect a GW150914 like source out to specific horizon distances [6.0 yr] | SI4.1 SI4.2 4.2 | report |
| Capability to detect a GW190521 like source out to specific horizon distances [6.0 yr] | SI4.2 4.2 | report |
| Number of detectable sources based on the LVC astrophysical model of BBH population [6.0 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 [6.0 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 |
| SOBHB as standard sirens [6.0 yr] | None | report |
| SO7 : Understand stochastic GW backgrounds | ||
| Unresolved stellar origin black holes [6.0 yr] | SI7.1 7.1 | report |
| Cosmic strings beyond SKA [6.0 yr] | iSI7.2 7.2 | report |
| SGWB from PBH dark matter [6.0 yr] | SR7.2 | report |
| Characterise representative template for SGWB power-law with n=0 [6.0 yr] | 7.2 SI7.2 | report |
| Characterise representative template for SGWB power-law with n=2/3 [6.0 yr] | SI7.2, 7.2 | report |
| Characterise representative template for SGWB power-law with n=-3 [6.0 yr] | 7.2 SI7.2 | report |
About
Those results have been obtained on the 09/08/2022, 07:39:52.
Using commit: b'31259e5b9b03271101d3c1c47a4bbca62e54f565' of FoM repo.
Pipeline configuration is reported here: report.