A software to simulate RR Lyrae light curves undergoing the Blazhko effect.
Building on RR Lyrae (RRab, RRc) templates from Sesar et al. (2010), the Blazhko effect is simulated by using a combination of amplitude and frequency modulation.
To simulate light curves from the LSST survey, the light curves are calculated on the appropriate cadences.
Photometric uncertainties are calculated according to the photometric error model of LSST (Ivezic et al. 2019)
where
is the photometric error where
with
Finally, the observed light curve is obtained as
where l is the simulated light curve without uncertainties.
A similar approach is used in Kovačević et al. (2021) for AGN light curves.
plot_flag flag indicates if plots should be generated
cadence_u_filename, path to cadence input file cadence_g_filename, cadence_r_filename, cadence_i_filename, cadence_z_filename
rHJD0 phase offset; if set to -1: randomize; good parameters: 0 to 1
period_blazhko Blazhko effect amplitude modulation; ifset to -1: randomize; good parameters: 10 - 100
fac_fm period for the Blazhko effect frequency modulation; if set to -1: randomize; good parameters: 3.0 to 7.0 b modulation index describes the factor by which the period is stretched at maximum; if set to -1: randomize; good parameters: 1.0 to 6.0
Sesar, B., Ivezić, Z., Grammer, S. H., et al. 2010, ApJ, 708, 7 https://ui.adsabs.harvard.edu/abs/2010ApJ...708..717S/abstract
Ivezic, Z., Kahn, S. M., Tyson, A., Abel, b., Acosta, E., et al. 2019, ApJ, 873, 44 https://iopscience.iop.org/article/10.3847/1538-4357/ab042c
Kovačević, A., Ilić, D., Popović, L. C., et al. 2021 https://arxiv.org/pdf/2105.14889.pdf