4MOST Selection Functions Pipeline (4SP)
4SP consists of two parts, an object selection function (4SP-OSF) and a geometric selection function (4SP-GSF). The aim of 4SP-OSF is to provide multidimensional probability maps as a function of different parameters defined by the individual surveys. The probability maps evaluate the expected observational biases that the 4MOST instrumental setup will imprint on the spectroscopic success rate as a function of certain parameters (e.g. signal-to-noise ratio, magnitude, redshift, linewidth, temperature, metallicity etc). The principal task of 4SP-GSF is to track survey completeness as a function of position on the sky, accounting for observational effects such as fibre placement constraints and observing conditions. Additionally, using the survey simulator we will estimate for each object the probability that it is successfully observed. Combining the 4SP-GSF and 4SP-OSF will allow science users to fully model the 4MOST survey.
4MOST Galactic Pipeline (4GP)
4MOST Extragalactic Pipeline (4XP)
4XP will measure the spectral properties of all extragalactic sources observed with 4MOST. The primary, and mandatory, data products produced by 4XP will be robust spectroscopic redshifts and single-componenent emission/absorption lines measurements. Spectroscopic redshifts will be derived using both template cross-correlation and emission line pattern matching, both using photometric priors and without. In addition, 4XP will also derive higher-order galaxy properties from these measurements, such as star-formation rates, gas-phase metallicities, ionization diagnostic line ratios, etc., and fit continuum stellar population models to the spectra to estimate stellar ages and masses.