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modules: | ||
- galsim.des | ||
- galsim_extra | ||
- montara | ||
- numpy | ||
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pipeline: | ||
steps: | ||
- galsim_montara | ||
# - coadd_nwgint | ||
# - swarp | ||
# - src_extractor | ||
# - desdm_meds | ||
- pizza_cutter | ||
- metadetect | ||
# - fitvd | ||
- delete_images | ||
- delete_sources | ||
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fitvd: | ||
conda_prefix: "/global/common/software/des/mambaforge/envs/des-y6-fitvd" | ||
n_jobs: 128 | ||
det_band: "r" | ||
bands: ["g", "r", "i", "z"] | ||
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galsim_montara: {} | ||
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delete_images: | ||
delete_coadd: True | ||
delete_se: True | ||
delete_se_nwgint: True | ||
delete_seg: True | ||
save_tilenames: [DES0131-2458] | ||
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delete_sources: | ||
save_tilenames: [DES0131-2458] | ||
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swarp: | ||
coadd_bands: ["r", "i", "z"] | ||
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src_extractor: {} | ||
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coadd_nwgint: | ||
n_jobs: 128 | ||
run_on_inputs: False | ||
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desdm_meds: | ||
n_jobs: 128 | ||
use_nwgint: False | ||
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pizza_cutter: | ||
n_jobs: 32 # more jobs leads to OOM errors | ||
use_nwgint: False | ||
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metadetect: | ||
n_jobs: 128 # don't hyperthread | ||
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eval_variables: | ||
sstar_mag_col: &star_mag_col | ||
type: FormattedStr | ||
format: "%smag" | ||
items: | ||
- "$band" | ||
sgal_mag_col: &gal_mag_col | ||
type: FormattedStr | ||
format: "mag_%s_dered" | ||
items: | ||
- "$band" | ||
sz_col: &z_col "photoz" | ||
ftruth_g: | ||
type: List | ||
items: | ||
- 0. | ||
- '$float((@gal.ellip).g)' | ||
index: '@current_obj_type_index' | ||
ftruth_beta: | ||
type: List | ||
items: | ||
- 0. | ||
- '$float((@gal.ellip).beta.rad)' | ||
index: '@current_obj_type_index' | ||
ftruth_rotate: | ||
type: List | ||
items: | ||
- 0. | ||
- '$float((@gal.rotate).rad)' | ||
index: '@current_obj_type_index' | ||
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input: | ||
# Use analytic galaxies with size and flux parameters that match the distribution seen | ||
# in the COSMOS galaxies. | ||
catalog_sampler: | ||
file_name: /dvs_ro/cfs/cdirs/des/y3-image-sims/input_cosmos_v4.fits | ||
cuts: | ||
mag_i: [15., 25.] # use only 15<mag_i<25. for now. | ||
isgal: [1,] # select galaxies only since we're simulating stars separately. | ||
mask_flags: [0,] # apply mask flags | ||
bdf_hlr: [0., 5.] | ||
desstar: | ||
file_name: | ||
type: FormattedStr | ||
format: /dvs_ro/cfs/projectdirs/des/atong/y6kp-shear/starsim/catalogs/merged_y6/%s.fits | ||
items: | ||
- "@output.tilename" | ||
mag_i_max: 25. | ||
mag_i_col: imag | ||
des_piff: | ||
file_name: "$piff_path" | ||
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image: | ||
type: WideScattered | ||
border: 15 | ||
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# The number of objects across the full focal plane. | ||
nobjects: | ||
type: MixedNObjects | ||
ngalaxies: | ||
type: RandomPoisson | ||
mean: "$170000 * (((@coadd_wcs).toWorld(galsim.PositionD(9750, 0)).ra.deg - (@coadd_wcs).toWorld(galsim.PositionD(250, 0)).ra.deg) * (math.cos((@coadd_wcs).toWorld(galsim.PositionD(0, 250)).dec.rad) - math.cos((@coadd_wcs).toWorld(galsim.PositionD(0, 9750)).dec.rad))) / ((ra_max_deg - ra_min_deg) * (math.cos(math.radians(dec_max_deg)) - math.cos(math.radians(dec_min_deg))))" | ||
use_all_stars: True | ||
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#could read this from the image headers, but let's set them explicitly for now | ||
xsize: 2048 | ||
ysize: 4096 | ||
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world_pos: | ||
type: RADec | ||
ra: | ||
type: Degrees | ||
theta: | ||
type: Eval | ||
str: "ra_star if object_type_list[@obj_num-start_obj_num]=='star' else ra_gal" | ||
# fra_gal: { type: Random, min: "$ra_min_deg", max: "$ra_max_deg" } | ||
fra_gal: | ||
type: Random | ||
min: "$(@coadd_wcs).toWorld(galsim.PositionD(250, 0)).ra.deg" | ||
max: "$(@coadd_wcs).toWorld(galsim.PositionD(9750, 0)).ra.deg" | ||
fra_star: { type: DESStarValue, col: "ra" } | ||
dec: | ||
type: Degrees | ||
theta: | ||
type: Eval | ||
str: "dec_star if object_type_list[@obj_num-start_obj_num]=='star' else math.degrees(dec_gal_radians)" | ||
fdec_gal_radians: | ||
type: RandomDistribution | ||
function: "math.cos(x)" # Uniform on the sky means P(delta) ~ cos(delta) | ||
# x_min: "$math.radians(dec_min_deg)" | ||
# x_max: "$math.radians(dec_max_deg)" | ||
x_min: "$(@coadd_wcs).toWorld(galsim.PositionD(0, 250)).dec.rad" | ||
x_max: "$(@coadd_wcs).toWorld(galsim.PositionD(0, 9750)).dec.rad" | ||
fdec_star: { type: DESStarValue, col: "dec" } | ||
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psf: | ||
type: Gaussian | ||
fwhm: 0.9 | ||
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#No knots | ||
gal: | ||
type: Sum | ||
items: | ||
- type: Exponential | ||
half_light_radius: { type: catalog_sampler_value, col: bdf_hlr } | ||
flux: { type: Eval, str: "1-fracdev", ffracdev: { type: catalog_sampler_value, col: bdf_fracdev } } | ||
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- type: DeVaucouleurs | ||
half_light_radius: '@gal.items.0.half_light_radius' | ||
flux: "[email protected]" | ||
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ellip: | ||
type: GBeta | ||
g: { type: Eval, str: "np.sqrt(g1**2 + g2**2)", fg1: { type: catalog_sampler_value, col: bdf_g1 }, fg2: { type: catalog_sampler_value, col: bdf_g2 } } | ||
beta: { type: Random } | ||
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rotate: {type: Random} | ||
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flux: | ||
type: Eval | ||
str: "10**(0.4*(mag_zp-mag))" | ||
fmag: { type: catalog_sampler_value, col: *gal_mag_col } | ||
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gsparams: | ||
folding_threshold: 1.0e-4 | ||
kvalue_accuracy: 1.0e-8 | ||
maxk_threshold: 1.0e-5 | ||
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star: | ||
type: Gaussian # Basically a delta function. | ||
sigma: 1.e-6 | ||
flux: | ||
type: Eval | ||
str: "10**( 0.4 * (mag_zp - mag))" | ||
fmag: { type: DESStarValue, col: *star_mag_col } | ||
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stamp: | ||
type: CoaddMixedScene | ||
objects: | ||
# obj_type is specified, so these numbers aren't used | ||
star: 1 | ||
gal: 1 | ||
obj_type: {type: Eval, | ||
str: "object_type_list[i]", | ||
ii: "$obj_num-start_obj_num" | ||
} | ||
draw_method: auto | ||
shear_scene: {type: Eval, | ||
str: "False if object_type_list[@obj_num-start_obj_num]=='star' else True" | ||
} | ||
shear: | ||
type: G1G2 | ||
g1: 0.00 | ||
g2: -0.02 | ||
gsparams: | ||
maximum_fft_size: 32768 # 4 x default=8192 | ||
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output: | ||
type: DESTile | ||
tilename: DES0433-2332 | ||
bands: ["g", "r", "i", "z"] | ||
desrun: "des-pizza-slices-y6" | ||
imsim_data: "$os.environ['IMSIM_DATA']" | ||
noise_mode: from_weight | ||
add_bkg: False | ||
grid_objects: False | ||
nproc: 128 | ||
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#Save weight and badpix extensions too | ||
badpixfromfits: | ||
hdu: 1 | ||
mask_hdu: 2 | ||
mask_file: "$orig_image_path" | ||
weight: | ||
hdu: 2 | ||
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truth: | ||
columns: | ||
num: obj_num | ||
half_light_radius: | ||
type: Eval | ||
str: "0.0 if @current_obj_type=='star' else hlr" | ||
fhlr: "@gal.items.0.half_light_radius" | ||
g1: "$(@stamp.shear).g1" | ||
g2: "$(@stamp.shear).g2" | ||
g: "$truth_g" | ||
beta: "$truth_beta" | ||
rotate: "$truth_rotate" | ||
obj_type: "@current_obj_type" | ||
obj_type_index: "@current_obj_type_index" | ||
band: "band" | ||
mag_zp: "$mag_zp" | ||
laigle_number: | ||
type: Eval | ||
str: "-1 if @current_obj_type=='star' else int(laigle_number)" | ||
flaigle_number: { type: catalog_sampler_value, col: laigle_number } | ||
z: | ||
type: Eval | ||
str: "-1. if @current_obj_type=='star' else z_gal" | ||
fz_gal: { type: catalog_sampler_value, col: "$z_col" } |