Some scene examples
Below are some examples of ‘scene’ files as well as the resulting simulated images.
Example 1: selected number of slices
Let’s start with a simple example, simulating a flat illumination of slices 1
through 15 in the IFU field of view. Here we are using the file
scene01.yaml.
scene_block_name: constant flux
spectrum:
type: constant-flux
geometry:
type: slices 1-15
nphotons: 1.5E7
wavelength_sampling: random # optional: default=random
apply_seeing: False # optional: default=True
apply_atmosphere_transmission: False # optional: default=True
render: True # optional: default=True
Execute fridadrp-ifu_simulator:
(venv_frida) $ fridadrp-ifu_simulator \
--scene scene01.yaml \
--flux_factor 10 \
--grating medium-K \
--scale fine \
--bias 0 \
--rnoise 0 \
--flatpix2pix none \
--seed 1234 \
--output_dir work \
--record
(venv_frida) $ numina-ximshow work/test_ifu_white2D_method0_os1.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_ifu_white2D_method0_os10.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_rss_2D_method0.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_detector_2D_method0.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_rss_2D_method1.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-extract_2d_slice_from_3d_cube work/test_ifu_3D_method0.fits
(venv_frida) $ numina-extract_2d_slice_from_3d_cube work/test_ifu_3D_method1.fits
Example 2: collection of Gaussian objects
Here we are using the file scene02.yaml.
scene_block_name: Gaussian center
spectrum:
type: constant-flux
geometry:
type: gaussian
fwhm_ra_arcsec: 0.04
fwhm_dec_arcsec: 0.04
position_angle_deg: 0.0
delta_ra_arcsec: 0.0
delta_dec_arcsec: 0.0
nphotons: 1E4
wavelength_sampling: random
apply_seeing: False
apply_atmosphere_transmission: False
render: True
---
scene_block_name: Gaussian top left
spectrum:
type: constant-flux
geometry:
type: gaussian
fwhm_ra_arcsec: 0.08
fwhm_dec_arcsec: 0.16
position_angle_deg: 0.0
delta_ra_arcsec: 0.18
delta_dec_arcsec: 0.15
nphotons: 1E5
wavelength_sampling: random
apply_seeing: False
apply_atmosphere_transmission: False
render: True
---
scene_block_name: Gaussian bottom left
spectrum:
type: constant-flux
geometry:
type: gaussian
fwhm_ra_arcsec: 0.08
fwhm_dec_arcsec: 0.08
position_angle_deg: 0.0
delta_ra_arcsec: 0.18
delta_dec_arcsec: -0.15
nphotons: 5E4
wavelength_sampling: random
apply_seeing: False
apply_atmosphere_transmission: False
render: True
---
scene_block_name: Gaussian top right
spectrum:
type: constant-flux
geometry:
type: gaussian
fwhm_ra_arcsec: 0.04
fwhm_dec_arcsec: 0.08
position_angle_deg: 0.0
delta_ra_arcsec: -0.18
delta_dec_arcsec: 0.15
nphotons: 3E4
wavelength_sampling: random
apply_seeing: False
apply_atmosphere_transmission: False
render: True
---
scene_block_name: Gaussian bottom right
spectrum:
type: constant-flux
geometry:
type: gaussian
fwhm_ra_arcsec: 0.32
fwhm_dec_arcsec: 0.04
position_angle_deg: 45
delta_ra_arcsec: -0.18
delta_dec_arcsec: -0.15
nphotons: 1E5
wavelength_sampling: random
apply_seeing: False
apply_atmosphere_transmission: False
render: True
Execute fridadrp-ifu_simulator:
(venv_frida) $ fridadrp-ifu_simulator \
--scene scene02.yaml \
--flux_factor 10 \
--grating medium-K \
--scale fine \
--bias 0 \
--rnoise 0 \
--flatpix2pix none \
--seed 1234 \
--output_dir work \
--record
(venv_frida) $ numina-ximshow work/test_ifu_white2D_method0_os1.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_ifu_white2D_method0_os10.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_rss_2D_method0.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_detector_2D_method0.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_rss_2D_method1.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-extract_2d_slice_from_3d_cube work/test_ifu_3D_method0.fits
(venv_frida) $ numina-extract_2d_slice_from_3d_cube work/test_ifu_3D_method1.fits
Example 3: M51-like galaxy
Here we are using the file scene03.yaml.
scene_block_name: M51 DSS1
spectrum:
type: constant-flux
geometry:
type: from-FITS-image
filename: m51_dss1.fits
diagonal_fov_arcsec: 0.80
background_to_subtract: mode
nphotons: 1E6
apply_atmosphere_transmission: True
render: True
---
scene_block_name: skycalc radiance
spectrum:
type: skycalc-radiance
geometry:
type: flatfield
nphotons: 1E6
apply_seeing: False
apply_atmosphere_transmission: False
render: True
We aim to simulate a galaxy resembling the morphology of Messier 51. To achieve this, we generated a \({15 \times 15}~{\rm arcmin}^2\) image using the ESO Online Digitized Sky Survey. The corresponding file is m51_dss1.fits.
Execute fridadrp-ifu_simulator:
(venv_frida) $ fridadrp-ifu_simulator \
--scene scene03.yaml \
--flux_factor 1 \
--grating medium-K \
--scale fine \
--bias 0 \
--rnoise 0 \
--flatpix2pix none \
--seed 1234 \
--output_dir work \
--record
(venv_frida) $ numina-ximshow work/test_ifu_white2D_method0_os1.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_ifu_white2D_method0_os10.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_rss_2D_method0.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_detector_2D_method0.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-ximshow work/test_rss_2D_method1.fits \
--cbar_orientation vertical --z1z2 minmax --aspect equal
(venv_frida) $ numina-extract_2d_slice_from_3d_cube work/test_ifu_3D_method0.fits
(venv_frida) $ numina-extract_2d_slice_from_3d_cube work/test_ifu_3D_method1.fits