Created
May 1, 2015 22:32
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Loop over orbital elements
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# Create grids for periods, masses, ecc, mean anomaly, and longitude of pericenter | |
periods <- ... | |
masses <- ... | |
eccentricities <- c(0, 0.1, 0.2) | |
mas <- seq(0, 360, length.out=(N/2))[-1] | |
lops <- seq(0, 360, length.out=(N/2))[-1] | |
# Create a list of detection matrices; each element corresponds to the recovery rate matrix | |
# in (P, M) for the eccentricity. | |
detection.list <- list() | |
for e in eccentricities { | |
# If eccentricity is circular, then only one grid point is needed for the l.o.p. (0), | |
# otherwise use the one defined at the top of the file | |
if (e == 0) | |
loop.lops <- 0 | |
else | |
loop.lops <- lops | |
# Create the (P, M) matrix | |
f <- matrix(nrow = N, ncol = N) | |
# loop over periods and masses, as | |
for P in periods { | |
# ... skip if P > detectable.P, as usual ... | |
for M in masses { | |
detections <- 0 | |
# loop over mas and loop.lops (which is either 0 or the lop vector) | |
for MA in mas { | |
for w in loop.lops { | |
# [ create dataset corresponding to signal due to planet with (P, M, MA, e, w) ] | |
if (detectable) | |
detections <- detections + 1 | |
} | |
} | |
... | |
f[i, j] <- detections / (length(mas) * length(loop.lops)) | |
} | |
} | |
# append the matrix to the list | |
detection.list[[length(detection.list)+1]] <- f | |
} |
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