On the viability of determining galaxy properties from observations - I. Star formation rates and kinematics

We explore how observations relate to the physical properties of the emitting galaxies by post-processing a pair of merging z similar to 2 galaxies from the cosmological, hydrodynamical simulation NewHorizon, using lcars (Light from Cloudy Added to RAMSES) to encode the physical properties of the simulated galaxy into H alpha emission line. By carrying out mock observations and analysis on these data cubes, we ascertain which physical properties of the galaxy will be recoverable with the HARMONI spectrograph on the European Extremely Large Telescope (ELT). We are able to estimate the galaxy's star formation rate and dynamical mass to a reasonable degree of accuracy, with values within a factor of 1.81 and 1.38 of the true value. The kinematic structure of the galaxy is also recovered in mock observations. Furthermore, we are able to recover radial profiles of the velocity dispersion and are therefore able to calculate how the dynamical ratio varies as a function of distance from the galaxy centre. Finally, we show that when calculated on galaxy scales the dynamical ratio does not always provide a reliable measure of a galaxy's stability against gravity or act as an indicator of a minor merger.

Automated summary

By conducting mock observations and analysis, researchers have determined that the HARMONI spectrograph can recover certain physical properties of galaxies, such as star formation rate, dynamical mass, and kinematic structure. They have also found that calculating the dynamical ratio on galaxy scales does not always provide a reliable measure of a galaxy's stability against gravity or act as an indicator of a minor merger.