rubin_sim.maf.maf_contrib.get_outdir_name(band, nside, pixel_radius, yr_cutoff, zbin, mag_cut_i, run_name, poisson_noise, zero_pt)

Return the output directory name where the cls for deltaN/N would be, given the input parameters. We assume that dust extinction is always added and counts are always normalized.

Returns: [outdir, yr_tag, zbin_tag, poisson_tag, zero_pt_tag]

* band: str: band to get the output directory name for.

Options: ‘u’, ‘g’, ‘r’, ‘i’

* nside: int: HEALpix resolution parameter.
* pixel_radius: int: number of pixels to mask along the shallow border
* yr_cutoff: int: year cut to restrict analysis to only a subset of the survey.

Must range from 1 to 9, or None for the full survey analysis (10 yrs).

* zbin: str: options include ‘0.<z<0.15’, ‘0.15<z<0.37’, ‘0.37<z<0.66, ‘0.66<z<1.0’,

‘1.0<z<1.5’, ‘1.5<z<2.0’, ‘2.0<z<2.5’, ‘2.5<z<3.0’,’3.0<z<3.5’, ‘3.5<z<4.0’, ‘all’ for no redshift restriction (i.e. 0.<z<4.0)

* mag_cut_i: float: upper limit on i-band magnitude when calculating the galaxy counts. will deal

with color correction automatically (for u,g,r bands ..) depending on the band

* run_name: str: run name tag to identify the output of specified OpSim output.

Since new OpSim outputs have different columns, the run_name for enigma_1189 must be ‘enigma1189’; can be anything for other outputs, e.g. ‘minion1016’

* poisson_noise: bool: set to True to consider the case where poisson noise is added to galaxy

counts after border masking (and the incorporation of calibration errors).

* zero_pt: bool: set to True to consider the case where photometric calibration errors were incorporated.