| Parameters . | Description . | Unit . |
|---|---|---|
| GALPARAMS: | Observation parameters of the mock galaxy | |
| distance | Distance of the galaxy centre to the observer | kpc |
| |$\theta _{zx}$| | Angles that the galaxy rotates along the Y-axis in the direction from z to x | deg |
| |$\theta _{yz}$| | Angles that the galaxy rotates along the X-axis in the direction from y to z | deg |
| l | Galactic longitude of the centre of the galaxy | deg |
| b | Galactic latitude of the centre of the galaxy | deg |
| SSPPARAMS: | Parameters of the SSP templates | |
| model | The SSP model to be used for the spectrum (MILES or PEGASE-HR) | |
| isochrone | Isochrones used to generate the SSP templates | |
| IMF | Initial-mass function used to generate the SSP templates | |
| single_alpha | If use single |$[\mathrm{\alpha /Fe}]$| or |$\alpha$|-variable templates for the spectrum | bool |
| factor | Oversampling factor of the templates | |
| FWHM_gal | Spectral resolution in FWHM of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| dlam | Bin width of the wavelength sampling of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| age_range | Optional age range (inclusive) in for the SSP models | Gyr |
| metal_range | Optional metallicity range (inclusive) in for the SSP models | dex |
| wave_range | Optional wavelength range (inclusive) in for the SSP models | |$\, {\rm \mathring{\rm A}}$| |
| spec_interpolator | Interpolation method to assign the spectrum to the particle given its (age, metallicity, |$[\mathrm{\alpha /Fe}]$|) | |
| INSPARAMS: | Instrument properties | |
| instrument | Instrument name, when using this parameter, the other parameters will be automatically set | |
| spatial_resolution | Spatial resolution of the data cube | arcsec |
| spatial_nbin | Number of spatial bins (spaxels) in two coordinates, in the format of [|$n_x$|, |$n_y$|] | |
| FWHM_spatial | Full width half-maximum of the PSF function to model the atmosphere | arcsec |
| Parameters . | Description . | Unit . |
|---|---|---|
| GALPARAMS: | Observation parameters of the mock galaxy | |
| distance | Distance of the galaxy centre to the observer | kpc |
| |$\theta _{zx}$| | Angles that the galaxy rotates along the Y-axis in the direction from z to x | deg |
| |$\theta _{yz}$| | Angles that the galaxy rotates along the X-axis in the direction from y to z | deg |
| l | Galactic longitude of the centre of the galaxy | deg |
| b | Galactic latitude of the centre of the galaxy | deg |
| SSPPARAMS: | Parameters of the SSP templates | |
| model | The SSP model to be used for the spectrum (MILES or PEGASE-HR) | |
| isochrone | Isochrones used to generate the SSP templates | |
| IMF | Initial-mass function used to generate the SSP templates | |
| single_alpha | If use single |$[\mathrm{\alpha /Fe}]$| or |$\alpha$|-variable templates for the spectrum | bool |
| factor | Oversampling factor of the templates | |
| FWHM_gal | Spectral resolution in FWHM of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| dlam | Bin width of the wavelength sampling of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| age_range | Optional age range (inclusive) in for the SSP models | Gyr |
| metal_range | Optional metallicity range (inclusive) in for the SSP models | dex |
| wave_range | Optional wavelength range (inclusive) in for the SSP models | |$\, {\rm \mathring{\rm A}}$| |
| spec_interpolator | Interpolation method to assign the spectrum to the particle given its (age, metallicity, |$[\mathrm{\alpha /Fe}]$|) | |
| INSPARAMS: | Instrument properties | |
| instrument | Instrument name, when using this parameter, the other parameters will be automatically set | |
| spatial_resolution | Spatial resolution of the data cube | arcsec |
| spatial_nbin | Number of spatial bins (spaxels) in two coordinates, in the format of [|$n_x$|, |$n_y$|] | |
| FWHM_spatial | Full width half-maximum of the PSF function to model the atmosphere | arcsec |
| Parameters . | Description . | Unit . |
|---|---|---|
| GALPARAMS: | Observation parameters of the mock galaxy | |
| distance | Distance of the galaxy centre to the observer | kpc |
| |$\theta _{zx}$| | Angles that the galaxy rotates along the Y-axis in the direction from z to x | deg |
| |$\theta _{yz}$| | Angles that the galaxy rotates along the X-axis in the direction from y to z | deg |
| l | Galactic longitude of the centre of the galaxy | deg |
| b | Galactic latitude of the centre of the galaxy | deg |
| SSPPARAMS: | Parameters of the SSP templates | |
| model | The SSP model to be used for the spectrum (MILES or PEGASE-HR) | |
| isochrone | Isochrones used to generate the SSP templates | |
| IMF | Initial-mass function used to generate the SSP templates | |
| single_alpha | If use single |$[\mathrm{\alpha /Fe}]$| or |$\alpha$|-variable templates for the spectrum | bool |
| factor | Oversampling factor of the templates | |
| FWHM_gal | Spectral resolution in FWHM of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| dlam | Bin width of the wavelength sampling of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| age_range | Optional age range (inclusive) in for the SSP models | Gyr |
| metal_range | Optional metallicity range (inclusive) in for the SSP models | dex |
| wave_range | Optional wavelength range (inclusive) in for the SSP models | |$\, {\rm \mathring{\rm A}}$| |
| spec_interpolator | Interpolation method to assign the spectrum to the particle given its (age, metallicity, |$[\mathrm{\alpha /Fe}]$|) | |
| INSPARAMS: | Instrument properties | |
| instrument | Instrument name, when using this parameter, the other parameters will be automatically set | |
| spatial_resolution | Spatial resolution of the data cube | arcsec |
| spatial_nbin | Number of spatial bins (spaxels) in two coordinates, in the format of [|$n_x$|, |$n_y$|] | |
| FWHM_spatial | Full width half-maximum of the PSF function to model the atmosphere | arcsec |
| Parameters . | Description . | Unit . |
|---|---|---|
| GALPARAMS: | Observation parameters of the mock galaxy | |
| distance | Distance of the galaxy centre to the observer | kpc |
| |$\theta _{zx}$| | Angles that the galaxy rotates along the Y-axis in the direction from z to x | deg |
| |$\theta _{yz}$| | Angles that the galaxy rotates along the X-axis in the direction from y to z | deg |
| l | Galactic longitude of the centre of the galaxy | deg |
| b | Galactic latitude of the centre of the galaxy | deg |
| SSPPARAMS: | Parameters of the SSP templates | |
| model | The SSP model to be used for the spectrum (MILES or PEGASE-HR) | |
| isochrone | Isochrones used to generate the SSP templates | |
| IMF | Initial-mass function used to generate the SSP templates | |
| single_alpha | If use single |$[\mathrm{\alpha /Fe}]$| or |$\alpha$|-variable templates for the spectrum | bool |
| factor | Oversampling factor of the templates | |
| FWHM_gal | Spectral resolution in FWHM of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| dlam | Bin width of the wavelength sampling of the output data cube | |$\, {\rm \mathring{\rm A}}$| |
| age_range | Optional age range (inclusive) in for the SSP models | Gyr |
| metal_range | Optional metallicity range (inclusive) in for the SSP models | dex |
| wave_range | Optional wavelength range (inclusive) in for the SSP models | |$\, {\rm \mathring{\rm A}}$| |
| spec_interpolator | Interpolation method to assign the spectrum to the particle given its (age, metallicity, |$[\mathrm{\alpha /Fe}]$|) | |
| INSPARAMS: | Instrument properties | |
| instrument | Instrument name, when using this parameter, the other parameters will be automatically set | |
| spatial_resolution | Spatial resolution of the data cube | arcsec |
| spatial_nbin | Number of spatial bins (spaxels) in two coordinates, in the format of [|$n_x$|, |$n_y$|] | |
| FWHM_spatial | Full width half-maximum of the PSF function to model the atmosphere | arcsec |
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