In our model, we assume that the production rates, p X,i, can vary in time.
In the first model we assume that the GHZ extends over the entire galactic thin disk16,17.
In our model we assume that only 82% of cases are symptomatic and only 54% of symptomatic cases are notified29.
In this model, we assume that treatment influences parameters of both frailty distribution and baseline hazard.
In the first model we assume the vendor has complete information about the buyer's cost structure.
In the model we assume that is a fixed parameter, and g, e are random parameters with and, where G denotes the n × n genomic relationship matrix.
For the thermal plasma model, we assume the solar abundances contained in Grevesse, N. & Sauval, A.J. (1998, Space Science Reviews 85, 161).
For this model we assume a certain emission pattern of the accretion column, based on physical modeling of the in-falling material in a strong magnetic field.
Different from the standard model, we assume that the firm's compensation decisions are taken by the board of directors and not by the firm's shareholders.
In this model, we assume an attack by unauthorized users.
For the class-AB model we assume CF=5.3.
