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 [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=0.68 [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 |
SOBHB as standard sirens [4.5 yr] | None | 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 09/19/2022, 13:39:59.
Using commit: b'35befaa74739b8e5074878e77c403a8dcd365b95' of FoM repo.
Pipeline configuration is reported here: report.