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Compute rest-frame line luminosity.
lineLum(intInt, z, f.rest = 115.27, omega.m = 0.27, omega.lambda = 0.73, H.0 = 71)
Integrated intensity in Jy km/s
Redshift
Line rest frequency in GHz
Omega matter parameter
Omega lambda parameter
Hubble constant in km/s/Mpc
Rest-frame line luminosity in solar luminosities.
Solomon, Downes & Radford (1992), ApJ 398, L29, equation (1)
Lprime
# NOT RUN { snu <- 1.e-3 # 1 mJy peak wid <- 400 # 400 km/s wide intInt <- 1.06*snu*wid # Gaussian line z <- 2.3 lineLum(intInt, z) # }
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