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DWD_FullPopulation_Wilhelm_Korol_Rossi_DOnghia_2020
dataset
posted on 2020-11-03, 13:53 authored by Martijn WilhelmMartijn Wilhelm, Valeriya Korol, Elena Maria Rossi, Elena D'OnghiaThese files contain the LISA observables of a full double white dwarf
(DWD) populations used in Wilhelm, Korol, Rossi & D'Onghia 2020
(MNRAS). The number in the filename corresponds to the viewing angle
(the angle between the long axis of the galactic bar and the line of
sight from the Sun to the Galactic center) in degrees. Each row
contains a single source.
These data were obtained by combining the DWD population's properties of Korol et al. 2019 (MNRAS 483) with the galaxy model of D'Onghia et al. 2020 (ApJ 890).
The columns correspond to the following quantities (units, where present, in square brackets):
Frequency [s^-1]; Time derivative of frequency [s^-2]; Ecliptic latitude [rad]; Ecliptic longitude [rad]; Wave amplitude; Binary
inclination [rad]; Wave polarization angle [rad]; Orbital phase [rad]
These data were obtained by combining the DWD population's properties of Korol et al. 2019 (MNRAS 483) with the galaxy model of D'Onghia et al. 2020 (ApJ 890).
