Run_SKIRT9_Bands_ID.py

import os,sys,copy,re,string,time,glob,subprocess
import numpy as np
import scipy.spatial as spt
from astropy.io import fits
import h5py
import illustris_tools as it
import illustris_python as il
from astropy.cosmology import Planck15 as cosmo

def get_subhalos(basePath,snap,mstar_lower=0,mstar_upper=np.inf):
    '''
    mstar_lower and mstar_upper have log10(Mstar/Msun) units and are physical (i.e. Msun, not Msun/h).
    '''
    from astropy.cosmology import Planck15 as cosmo
    little_h = cosmo.H0.value/100.
    
    ptNumStars = il.snapshot.partTypeNum('stars') 
    fields = ['SubhaloMassType','SubhaloFlag']
    subs = il.groupcat.loadSubhalos(basePath,snap,fields=fields)

    mstar = subs['SubhaloMassType'][:,ptNumStars]
    flags = subs['SubhaloFlag']
    subs = np.arange(subs['count'],dtype=int)
    
    # convert to units used by TNG (1e10 Msun/h)
    mstar_lower = 10**(mstar_lower)/1e10*little_h
    mstar_upper = 10**(mstar_upper)/1e10*little_h
    subs = subs[(flags!=0)*(mstar>=mstar_lower)*(mstar<=mstar_upper)]
    return subs,mstar[subs]
    
def rowcount(filename):
    stdout = subprocess.check_output(f'wc -l {filename}',shell=True,text=True)
    return int(stdout.split(' ')[0])
    
def create_wl_grid(filename='Wavelength_Grid.dat'):
    wl = np.linspace(0.1,1.,181,endpoint=True)
    wl = np.append(wl,np.linspace(1.,5.,21)[1:])
    np.savetxt(filename,wl,header=str(len(wl)),comments='')
    
def nn_dist(args):
    smoothlength,point,tree = args
    return tree.query(point,k=smoothlength)[0][-1]

def RR2014_dust_density(rho_gas,Z_gas,T_gas,SFR_gas,T_thresh=75000,SFR_thresh=0.):
    '''
    Compute gas-to-dust density fraction for gas cells following Remy-Ruyer+2014 
    empirical calibrations (Figure 4 and Table 1). Use broken power law relation 
    with X_CO,Z (column 3 in Table 1). Use gas-to-dust density fraction and gas 
    density to obtain dust density, rho_dust.
    
    Assume log(Zcell/Zsun) = logOH_cell - logOH_sun and use 12+logOH_sun = 8.69
    => log(Zcell/Zsun) = 12 + logOH_cell - ( 12 + logOH_sun ) = 12 + logOH_cell - 8.69
    => logOHp12_cell is defined as 12 + logOH_cell = log(Zcell/Zsun) + 8.69 = log(Z_gas/0.014) + 8.69
    '''
    logOHp12_cell = np.log10(Z_gas/0.014) + 8.69
    # Remy-Ruyer+2014 Table 1 X_CO,Z broken power law (higher, H: 12+logOH>=8.1)
    logGtD = 2.21 + 1.00 * (8.69 - logOHp12_cell)
    # Remy-Ruyer+2014 Table 1 X_CO,Z broken power law (lower, L: 12+logOH<8.1)
    lower_mask = logOHp12_cell<8.1
    logGtD[lower_mask] = 0.96 + 3.10 * (8.69 - logOHp12_cell[lower_mask])
    rho_dust = 10**(-logGtD)*rho_gas
    # set density to zero for above/below temperature and sfr thresholds
    rho_dust[((T_gas>T_thresh) & (SFR_gas<=SFR_thresh))] = 0.
    rho_dust[np.isnan(rho_dust)]=0.
    return rho_dust

def prepare_skirt(snap,sub,sim_path,tmp_path,
                  pixelsize=100.,fovsize_hmr_dm=2.,fovsize_hmr_stars=20.,
                  smoothlength=32,fof_factor=np.sqrt(2),
                  fov_min_pc=5e4,fov_max_pc=5e5,
                  nsources_min=1e6,nsources_max=1e7,
                  correct_pdrs=True):
    '''
    pixel_size: output pixel size in [pc]
    fov_hmr: size of fov in stellar half mass radius units
    smooth_length: kernel smoothing length of stellar particles (nn distance)
    fof_factor: factor by which fovsize_hmr is multiplied to determine which FOF halo particles are used
    '''

    #load current scale factor
    header = dict(h5py.File(f'{sim_path}/snapdir_{snap:03d}/snap_{snap:03d}.0.hdf5',"r")["Header"].attrs.items())
    a2 = header["Time"]

    sub_cat = il.groupcat.loadSingle(sim_path,snap,subhaloID=sub)
    # GPM position and parent FOF halo of subhalo
    group_idx = sub_cat['SubhaloGrNr']
    centerGal = sub_cat['SubhaloPos']
    
    # use DM half-mass radius
    fovsize_ckpch_dm = fovsize_hmr_dm*sub_cat["SubhaloHalfmassRadType"][1] # ckpc/h
    fovsize_ckpch_stars = fovsize_hmr_stars*sub_cat["SubhaloHalfmassRadType"][4] # ckpc/h
    fovsize_ckpch = max(fovsize_ckpch_stars,fovsize_ckpch_dm)
    fovsize = it.convertlength(fovsize_ckpch)*a2*1000 # pc
    fovsize = max(fovsize,fov_min_pc) # set minimum fov to 50 pkpc
    fovsize = min(fovsize,fov_max_pc) # set maximum fov to 0.5 pMpc
    npix = np.ceil(fovsize/pixelsize).astype(int)

    if fovsize == 0:
        print("Not a valid subhalo, I will stop now and running SKIRT makes no sense")
        raise SystemExit
    
    # save f_stars,f_mappings,f_gas to file
    f_stars = f'shalo_{snap:03d}-{sub}_stars.dat'
    f_mappings = f'shalo_{snap:03d}-{sub}_mappings.dat'
    f_gas = f'shalo_{snap:03d}-{sub}_gas.dat'
    
    #############
    ### Stars ###
    #############
    if not (os.access(f'{tmp_path}/{f_stars}',0) or os.access(f'{tmp_path}/{f_mappings}',0)):
        fields = ["Coordinates","GFM_StellarFormationTime","GFM_InitialMass",
                  "GFM_Metallicity", "Velocities", "Masses"]
        #load star particles
        stars = il.snapshot.loadHalo(sim_path,snap,group_idx,4,fields)
        coords,cntr = it.periodicfix(stars['Coordinates'],centerGal) # ckpc/h
        coords = it.convertlength(coords)*a2*1000 # pc
        cntr = it.convertlength(cntr)*a2*1000 # pc

        #ignore all wind particles 
        star_idx = stars['GFM_StellarFormationTime'] > 0
        #include only particles within certain distance of target galaxy
        star_idx *= np.prod(np.abs(coords-cntr)<=fovsize*fof_factor/2,axis=1,dtype=bool)
        #coords of fof stars within fovsize*fof_factor from SubhaloPos
        coords = coords[star_idx]-cntr

        #smoothing length in proper pc (distance to smoothlength closest neighbour)
        #create array with locations
        #setup KDTree
        tree = spt.cKDTree(coords,leafsize = 100)
        environ = os.environ
        nthreads = int(environ['SKIRT_CPUS_PER_TASK']) if 'SKIRT_CPUS_PER_TASK' in environ else 1
        if nthreads>1:
            from multiprocessing import Pool
            argList = [(smoothlength,point,tree) for point in coords]
            with Pool(nthreads) as pool:
                h = np.asarray(pool.map(nn_dist,argList))
        else:
            h = np.zeros(len(coords))
            for i,point in enumerate(coords):
                dist = tree.query(point,k=smoothlength)[0][-1]
                h[i] = dist
            h = np.asarray(h)

        #initial mass in solar masses
        M = it.convertmass(stars["GFM_InitialMass"][star_idx])
        #metallicity (actual metallicity, not in solar units)
        Z = stars["GFM_Metallicity"][star_idx]
        #age of the stars in years
        if nthreads>1:
            from multiprocessing import Pool
            argList = [(a1,a2) for a1 in stars["GFM_StellarFormationTime"][star_idx]]
            with Pool(nthreads) as pool:
                t = np.asarray(pool.starmap(it.age,argList))
        else:
            t = it.age(stars["GFM_StellarFormationTime"][star_idx],a2)
        #parameters for all stars
        total_stars = np.column_stack((coords,h,M,Z,t))
        nsources = total_stars.shape[0]
        nsources = max(nsources,nsources_min)
        nsources = min(nsources,nsources_max)

        ### Old stars ####
        age_idx = t>1e7 #only consider stars older than 10Myr for bruzual charlot spectra
        np.savetxt(f'{tmp_path}/{f_stars}',total_stars[age_idx],delimiter = " ")

        ### Young stars ###
        age_idx = t<=1e7 #only consider stars younger than 10Myr for MappingsIII spectra
        #calculate SFR (assuming SFR has been constant in the last 10Myr)
        SFRm = total_stars[age_idx,4]/1e7
        #for compactness, take typical value of 5:
        logC = np.full(len(SFRm),5)
        #for ISM pressure, take typical value log(P/kB / cm^-3K) = 5, P = 1.38e-12 N/m2
        pISM = np.full(len(SFRm),1.38e-12)
        #for PDR covering fraction, take f = 0.2
        fPDR = np.full(len(SFRm),0.0)
        #create 2D-array and write into data file
        young_stars = np.column_stack((coords[age_idx],h[age_idx],
                                       SFRm,Z[age_idx],logC,pISM,fPDR))
        np.savetxt(f'{tmp_path}/{f_mappings}',young_stars,delimiter = " ")
        del total_stars,young_stars
    else:
        nsources = rowcount(f'{tmp_path}/{f_stars}')
        nsources+= rowcount(f'{tmp_path}/{f_mappings}')
        nsources = max(nsources,nsources_min)
        nsources = min(nsources,nsources_max)

    #############
    #### Gas ####
    #############
    if not os.access(f'{tmp_path}/{f_gas}',0):
        fields = ["Coordinates","Density","GFM_Metallicity","InternalEnergy",
                  "ElectronAbundance","StarFormationRate","Masses"]
        #load gas particles
        gas = il.snapshot.loadHalo(sim_path,snap,group_idx,0,fields)
        # allow possibility of no gas
        if gas["count"] != 0:
            coords,cntr = it.periodicfix(gas['Coordinates'],centerGal) # ckpc/h
            coords = it.convertlength(coords)*a2*1000 # pc
            cntr = it.convertlength(cntr)*a2*1000 # pc
            #include only particles within certain distance of target galaxy
            gas_idx = np.prod(np.abs(coords-cntr)<=fovsize*fof_factor/2,axis=1,dtype=bool)
            # coords of fof gas within fovsize*fof_factor from SubhaloPos
            coords = coords[gas_idx]-cntr
            # density
            rhog = it.convertdensity(gas["Density"][gas_idx])/((1000*a2)**3)
            #gas particle metallicity (not in solar units)
            #This will actually become the dust abundance
            Zg = gas["GFM_Metallicity"][gas_idx]
            #gas temperature in K
            T = it.temp(gas["InternalEnergy"][gas_idx],gas["ElectronAbundance"][gas_idx])
            #SFR of gas cell
            SFRg = gas["StarFormationRate"][gas_idx]
            #metal mass of each gas cells
            metal_mass = Zg*it.convertmass(gas["Masses"][gas_idx])
            
            if correct_pdrs:
                #load young star properties for gas/dust calculations
                young_stars = np.loadtxt(f'{tmp_path}/{f_mappings}')
                #Correct for double accounting of dust in PDR regions
                #Calculate mass of metals in the PDR and take this from the stellar particles within the smoothing length
                for young_star in young_stars:
                    #assume metallicity of star equals metallicity of parent PDR
                    #factor of 10 assumes Mpdr = 10 x Mstar
                    metal_mass_PDR = 10 * young_star[5] * young_star[4]*1e7                  
                    metal_mass_excess, n_grow = -1, 1.
                    #grow N until the enclosed dust mass in h*N exceeds PDR mass
                    while metal_mass_excess < 0:
                        loc_idx = ( np.sum((coords-young_star[:3])**2,axis=1) < (n_grow*young_star[3])**2 )
                        #Metal mass in the gas cells within that smoothing length
                        loc_metal_mass = np.sum(metal_mass[loc_idx])
                        #Metal mass left over in the gas cells after subtracting pdr contribution
                        metal_mass_excess = loc_metal_mass - metal_mass_PDR
                        n_grow *= 2.
                    norm = loc_metal_mass/metal_mass_excess
                    Zg[loc_idx] = Zg[loc_idx]/norm
                del young_stars
                
            #Calculate the dust density
            rho_dust = RR2014_dust_density(rhog,Zg,T,SFRg)

        else:
            coords,rho_dust= np.array([[],[],[]]).T,[]
        #create 2D-array and write into data file
        total_gas = np.column_stack((coords,rho_dust))
        np.savetxt(f'{tmp_path}/{f_gas}',total_gas,delimiter = " ")
        ncells = len(total_gas)
        del total_gas
    else:
        ncells = rowcount(f'{tmp_path}/{f_gas}')
        
    return fovsize,npix,ncells,nsources,fof_factor,f_stars,f_mappings,f_gas

def run_skirt(snap,sub,cam,sim_tag,sim_path,tmp_path,skirt_path,out_path,
              wl_min=0.1,wl_max=5,wl_probe=0.55,packet_factor=200,
              bands = ['CFHT_MegaCam.u','CFHT_MegaCam.r',
                       'Subaru_HSC.g','Subaru_HSC.r','Subaru_HSC.i','Subaru_HSC.z','Subaru_HSC.Y',
                       'UKIRT_UKIDSS.J','UKIRT_UKIDSS.H','UKIRT_UKIDSS.K',
                       'Spitzer_IRAC.I1','Spitzer_IRAC.I2','Spitzer_IRAC.I3','Spitzer_IRAC.I4']
             ):
    '''
    sim_path: base path to simulation snapshot data
    tmp_path: working directory for job 
    skirt_path: path to skirt template files (like shalo.ski, wavelength file)
    
    Paths default to working directory if not specified.
    '''
    
    snap,sub = int(snap),int(sub)
    
    fovsize,npix,ncells,nsources,fof_factor,f_stars,f_mappings,f_gas = prepare_skirt(snap,sub,sim_path,tmp_path,correct_pdrs=False)
    
    redshift = il.groupcat.loadHeader(sim_path,snap)['Redshift']
    little_h = cosmo.H0.value/100
    omega_m = cosmo.Om0
    speed_of_light = 2.998e14 # [micron/s]
    # nsources*=200
    nsources*=packet_factor
    ski_in = f'{skirt_path}/shalo_bands.ski'

    if not os.access(tmp_path,0):
        os.system(f'mkdir -p {tmp_path}')
    os.chdir(tmp_path)        
    # prepare skirt output and place in tmpdir
    ski_out = f'shalo_{snap:03d}-{sub}.ski'
    
    cams = np.array(['v0','v1','v2','v3'])
    incls = [109.5,109.5,109.5,0.]
    azims = [0.,120.,-120.,0.]
    idx = np.argwhere(cams==cam)[0][0]
    incl = incls[idx]
    azim = azims[idx]
    
    environ = os.environ
    if 'SKIRT_NTASKS' in environ:
        nprocesses = int(environ['SKIRT_NTASKS'])
        nthreads = int(environ['SKIRT_CPUS_PER_TASK'])
    else:
        nprocesses = 1
        nthreads = 1
    with open(ski_in,'r') as f:
        filedata = f.read()
        
    # order bandpasses by pivot wl (skirt output default) and write to .ski
    band_dir = f'{skirt_path}/Photometry/SKIRT9/Filters'
    wl_pivot = []
    for band in copy.copy(bands):
        wl_band,transmission = np.loadtxt(f'{band_dir}/{band}.dat',unpack=True)
        if (wl_max*(1+redshift) < wl_band[-1]) or (wl_min*(1+redshift) > wl_band[0]):
            # band is removed if it source spectrum does not cover its entire range
            bands.remove(band)
        else:
            # band stays and its pivot wavelenght is computed and appended
            wl_pivot.append(np.sqrt(np.trapz(transmission,wl_band)/np.trapz(transmission/wl_band**2,wl_band)))
    sort_idx = np.argsort(wl_pivot)
    bands = np.array(bands)[sort_idx]
    bandtxt = ''.join([' '*28+f'<FileBand filename="{band_dir}/{band}.dat"/>\n' for band in bands])
    bandtxt = bandtxt.strip('\n') # drop last return carriage

    # Replace the target string
    filedata = re.sub('_REDSHIFT_',str(redshift),filedata)
    filedata = re.sub('_LITTLEH_',str(little_h),filedata)
    filedata = re.sub('_OMEGAM_',str(omega_m),filedata)
    filedata = re.sub('_WLMIN_',str(wl_min),filedata)
    filedata = re.sub('_WLMAX_',str(wl_max),filedata)
    filedata = re.sub('_WLPROBE_',str(wl_probe),filedata)
    filedata = re.sub('_BANDTEXT_',bandtxt,filedata)
    filedata = re.sub('_FILENAME_STARS_',f_stars,filedata)
    filedata = re.sub('_FILENAME_MAPPINGS_',f_mappings,filedata)
    filedata = re.sub('_FILENAME_GAS_',f_gas,filedata)
    filedata = re.sub('_FOVSIZE_',str(fovsize),filedata)
    filedata = re.sub('_PIXELNUM_',str(npix),filedata)
    filedata = re.sub('_SIZE_',str(fovsize*fof_factor/2.),filedata)
    filedata = re.sub('_NUMCELLS_',str(ncells),filedata)
    filedata = re.sub('_INSTRUMENT_NAME_',cam,filedata)
    filedata = re.sub('_INCLINATION_',str(incl),filedata)
    filedata = re.sub('_AZIMUTH_',str(azim),filedata)
    filedata = re.sub('_NUMPACKAGES_',str(nsources),filedata)
    filedata = re.sub('_DISTANCE_','0',filedata)
    with open(ski_out, 'w') as f:
        f.write(filedata)
        
    skirt_total = f'shalo_{snap:03}-{sub}_{cam}_total.fits'
    if not os.access(skirt_total,0):
        os.system(f'mpirun -n {nprocesses} skirt -t {nthreads} {ski_out}')

    hdu = fits.open(skirt_total)
    images = hdu[0].data*1e26 # [Jy*Hz/micron/arcsec2]
    header = hdu[0].header
    wl_pivot2 = np.array([wl_pivot[0]**2 for wl_pivot in hdu[1].data]) # microns2
    
    # calibrated images in maggies
    images = images*wl_pivot2.reshape(-1,1,1)/speed_of_light/3631.
    # convert to mag/arcsec2 surface brightness for numerical ease
    with np.errstate(divide='ignore'):
        images = -2.5*np.log10(images) # [mag/arcsec2] AB system
        images[images==np.inf]=99.
        
    hdu_list = fits.HDUList()
    for i in range(len(bands)):
        hdu = fits.ImageHDU(images[i].astype('float32'),name=bands[i])
        hdr = hdu.header
        hdr['ORIGIN'] = ('SKIRT 9 Simulation','Image origin')
        hdr['SIMTAG'] = (sim_tag,'Simulation name')
        hdr['SNAPNUM'] = (snap,'Simulation snapshot')
        hdr['SUBHALO'] = (sub,'Subhalo ID')
        hdr['CAMERA'] = (cam,'Camera ID')
        hdr['INCL'] = (incl,'Camera inclination')
        hdr['AZIM'] = (azim,'Camera azimuth')
        hdr['ROLL'] = (0.,'Camera roll')
        hdr['COSMO'] = (cosmo.name,'Cosmology')
        hdr['REDSHIFT'] = (float(f'{redshift:.4f}'),'Redshift')
        hdr['FILTER'] = (bands[i],'Filter name')
        hdr['NPACKET'] = (nsources,'Number of photon packets')
        hdr['WLPIVOT'] = (np.sqrt(wl_pivot2[i]),'Pivot wavelength (micron)')
        hdr['BUNIT'] = ('AB mag/arcsec2','Image units')
        hdr['FOVSIZE'] = (fovsize/1e3,'Field of view [kpc]')
        hdr['CRPIX1'] = (npix/2, 'X-axis coordinate system reference pixel')
        hdr['CRVAL1'] = (0., 'Coordinate system value at X-axis reference pix')
        hdr['CDELT1'] = (fovsize/1e3/npix, 'Coordinate increment along X-axis')
        hdr['CTYPE1'] = ('kpc', 'Physical units of the X-axis increment')
        hdr['CRPIX2'] = (npix/2, 'Y-axis coordinate system reference pixel')
        hdr['CRVAL2'] = (0., 'Coordinate system value at Y-axis reference pix')
        hdr['CDELT2'] = (fovsize/1e3/npix, 'Coordinate increment along Y-axis')
        hdr['CTYPE2'] = ('kpc', 'Physical units of the Y-axis increment')
        hdu_list.append(hdu)
        
    # output directory
    if not os.access(out_path,0):
        os.system(f'mkdir -p {out_path}')
        
    photo_name = f'{out_path}/shalo_{snap:03}-{sub}_{cam}_photo.fits'
    hdu_list.writeto(photo_name,overwrite=True) 
    
def prepare_only(args):
    
    snap,sub_idx = int(args[1]),int(args[2])
    sim_tag = 'TNG50-1'
    
    # base path where TNG data is stored
    sim_path = f'/lustre/work/connor.bottrell/Simulations/IllustrisTNG/{sim_tag}/output'
    # base path of output directory
    project_path = '/lustre/work/connor.bottrell/Simulations/IllustrisTNG'
    # photometry path
    phot_path = f'{project_path}/{sim_tag}/postprocessing/SKIRT9/Photometry/{snap:03}'
    # spectroscopy path
    spec_path = f'{project_path}/{sim_tag}/postprocessing/SKIRT9/Spectroscopy/{snap:03}'
    
    subs,mstar = get_subhalos(sim_path,snap=snap,mstar_lower=9)
    sub = subs[sub_idx]

    # Check if output already exists. If so, skip.
    cams = ['v0','v1','v2','v3']
    outfiles = glob.glob(f'{phot_path}/shalo_{snap:03}-{sub}_*_photo.fits')
    if len(outfiles)==len(cams):
        sys.exit(f'All output images already exist for {sim_tag}-{snap:03}-{sub}.')
    
    # working directory for job
    tmp_path=f'/lustre/work/connor.bottrell/tmpdir/tmp_{snap:03}-{sub}'
    if not os.access(tmp_path,0):
        os.system(f'mkdir -p {tmp_path}')
    os.chdir(tmp_path)
    
    fovsize,npix,ncells,nsources,fof_factor,f_stars,f_mappings,f_gas = prepare_skirt(snap,sub,sim_path,tmp_path,correct_pdrs=False)
    
def run_only(args):
    
    snap,sub_idx = int(args[1]),int(args[2])
    sim_tag = 'TNG50-1'
    
    # base path where TNG data is stored
    sim_path = f'/lustre/work/connor.bottrell/Simulations/IllustrisTNG/{sim_tag}/output'
    # base path of output directory
    project_path = '/lustre/work/connor.bottrell/Simulations/IllustrisTNG'
    # photometry path
    phot_path = f'{project_path}/{sim_tag}/postprocessing/SKIRT9/Photometry/{snap:03}'
    # spectroscopy path
    spec_path = f'{project_path}/{sim_tag}/postprocessing/SKIRT9/Spectroscopy/{snap:03}'
    
    subs,mstar = get_subhalos(sim_path,snap=snap,mstar_lower=9)
    sub = subs[sub_idx]

    cams = ['v0','v1','v2','v3']
        
    # working directory for job
    tmp_path=f'/lustre/work/connor.bottrell/tmpdir/tmp_{snap:03d}-{sub}'
    skirt_path = f'{project_path}/Scripts/SKIRT'
    
    f_stars = f'{tmp_path}/shalo_{snap:03d}-{sub}_stars.dat'
    f_mappings = f'{tmp_path}/shalo_{snap:03d}-{sub}_mappings.dat'
    f_gas = f'{tmp_path}/shalo_{snap:03d}-{sub}_gas.dat'
    
    for skirt_file in [f_stars,f_mappings,f_gas]:
        if not os.access(skirt_file,0):
            sys.exit(f'Missing SKIRT input files for {snap:03}-{sub}. Quitting...')
    
    for cam in cams:
        if not os.access(f'{phot_path}/shalo_{snap:03}-{sub}_{cam}_photo.fits',0):
            run_skirt(snap,sub,cam,sim_tag,
                     sim_path=sim_path,
                     tmp_path=tmp_path,
                     skirt_path=skirt_path,
                     out_path=phot_path)

    files_exist = True
    for cam in cams:
        if not os.access(f'{phot_path}/shalo_{snap:03}-{sub}_{cam}_photo.fits',0):
            files_exist=False

    # clean up
    if files_exist:
        os.system(f'rm -rf {tmp_path}')
        
if __name__=='__main__':
    
    args = sys.argv
    snap,sub,cam = int(args[1]),int(args[2]),args[3]
    sim_tag = 'TNG50-1'
    sim_path = f'/lustre/work/connor.bottrell/Simulations/IllustrisTNG/{sim_tag}/output'
    tmp_path = f'/lustre/work/connor.bottrell/tmpdir/tmp_{snap:03}-{sub}/'
    project_path = '/lustre/work/connor.bottrell/Simulations/IllustrisTNG'
    skirt_path = f'{project_path}/Scripts/SKIRT'
    out_path = f'{project_path}/{sim_tag}/postprocessing/SKIRT9/Photometry/{snap:03}'
        
    # working directory for job
    if not os.access(tmp_path,0):
        os.system(f'mkdir -p {tmp_path}')   
    os.chdir(tmp_path)
    
    run_skirt(snap,sub,cam,sim_tag,sim_path,tmp_path,skirt_path,out_path)