How to use the drizzlepac.astrodrizzle function in drizzlepac

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github gbrammer / grizli / grizli / combine.py View on Github external
wht = 1./im['ERR'].data**2
        wht[(im['ERR'].data == 0) | (dq > 0) | (~np.isfinite(wht))] = 0
        wht[im['SCI'].data < -3*im['ERR'].data] = 0

        wht = np.cast[np.float32](wht)

        exp_wcs = pywcs.WCS(im[1].header, relax=True)
        exp_wcs.pscale = utils.get_wcs_pscale(exp_wcs)

        #pf = 0.5
        # import drizzlepac.wcs_functions as dwcs
        # xx = out_wcs.deepcopy()
        # #xx.all_pix2world = xx.wcs_world2pix
        # map = dwcs.WCSMap(exp_wcs, xx)

        astrodrizzle.adrizzle.do_driz(im['SCI'].data, exp_wcs, wht,
                                      inter_wcs, outsci, outwht, outctx,
                                      1., 'cps', 1,
                                      wcslin_pscale=exp_wcs.pscale,
                                      uniqid=1,
                                      pixfrac=pixfrac, kernel=kernel,
                                      fillval=0, stepsize=10,
                                      wcsmap=SIP_WCSMap)

        if ds9 is not None:
            ds9.view(outsci, header=outh)

    #outsci /= out_wcs.pscale**2
    rms = 1/np.sqrt(outwht)
    mask = (outwht == 0) | (rms > 100)
    rms[mask] = 0
    outsci[mask] = 0.
github gbrammer / grizli / grizli / model.py View on Github external
flt_wcs, 1, coeffs=True, interp='nearest',
                                sinscl=1.0, stepsize=1, wcsmap=None)
            
            blotted_ones = astrodrizzle.ablot.do_blot(seg_ones+1, ref_wcs,
                                flt_wcs, 1, coeffs=True, interp='nearest',
                                sinscl=1.0, stepsize=1, wcsmap=None)
            
            blotted_ones[blotted_ones == 0] = 1
            ratio = np.round(blotted_seg/blotted_ones)
            grow = nd.maximum_filter(ratio, size=3, mode='constant', cval=0)
            ratio[ratio == 0] = grow[ratio == 0]
            blotted = ratio
            
        else:
            #print '\nREFDATA\n\n', refdata.dtype, ref_wcs, flt_wcs
            blotted = astrodrizzle.ablot.do_blot(refdata, ref_wcs, flt_wcs, 1, coeffs=True, interp='poly5', sinscl=1.0, stepsize=10, wcsmap=None)
        
        return blotted

drizzlepac

HST image combination using the drizzle algorithm to combine astronomical images, to model image distortion, to remove cosmic rays, and generally to improve the fidelity of data in the final image.

BSD-3-Clause
Latest version published 1 month ago

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