Mass of first object in binary (in solar masses)

Mass of second object in binary (in solar masses)

Enter the following angular values in degrees. Binary location should be entered in J2000 ecliptic (coordinate transformations from other systems can be found here). The default location is for a source at the galactic center.

Latitude (θ) of the binary.

Azimuthal location (φ) of the binary.

Inclination angle (ι) of the binary.

Polarization angle (ψ) of the binary.

Initial gravitational phase (φ_o) of the binary

Initial azimuthal offset of LISA (κ)

Initial rotational offset of LISA (λ)

Choose either time to coalescence or initial frequency input

Use time to coalescence (in years)

Use initial frequency (in mHz)

Choose either luminosity distance or redshift input

Use luminosity distance (in kpc)

Use redshift

Observation time (in years)

No galactic binary noise

Include galactic binary noise using the a fit to HB (see below).

Include galactic binary noise using the TRC analysis of HBW (see below).

Use standard LISA values for arm length, number of detector vertices, shot and acceleration noise levels.

Use the values entered for a non-standard LISA type detector.

Arm length, in meters, of the detector (standard LISA arm length = 5.0e+09 m).

Use two vertices (for two Michelson detectors).

Use one vertex (for one Michelson detector).

Position noise of the detector (standard LISA laser position noise = 2.0E-11 m/sqrt(Hz)).

Acceleration noise of the detector (standard LISA acceleration noise = 3.0e-15 m/s²/sqrt(Hz)).