# An extensive VLT/X-Shooter library of photospheric templates of pre-main sequence stars

## TL;DR

This paper presents a comprehensive library of VLT/X-Shooter spectra of pre-main sequence stars, providing essential templates for stellar parameter estimation and assessing chromospheric effects on accretion measurements.

## Contribution

It offers a new extensive set of flux-calibrated, telluric-corrected spectra of young stars, along with derived stellar parameters and calibration of colors, aiding studies of star formation and disk evolution.

## Key findings

- Spectral types range from G5 to M8 with negligible extinction.
- Chromospheric emission impacts accretion rate measurements, setting a detection limit of ~3x10^-10 Msun/yr.
- Calibrated stellar colors as a function of spectral type for young stars.

## Abstract

Studies of the formation and evolution of young stars and their disks rely on the knowledge of the stellar parameters of the young stars. The derivation of these parameters is commonly based on comparison with photospheric template spectra. Furthermore, chromospheric emission in young active stars impacts the measurement of mass accretion rates, a key quantity to study disk evolution. Here we derive stellar properties of low-mass pre-main sequence stars without disks, which represent ideal photospheric templates for studies of young stars. We also use these spectra to constrain the impact of chromospheric emission on the measurements of mass accretion rates. The spectra in reduced, flux-calibrated, and corrected for telluric absorption form are made available to the community. We derive the spectral type for our targets by analyzing the photospheric molecular features present in their VLT/X-Shooter spectra by means of spectral indices and comparison of the relative strength of photospheric absorption features. We also measure effective temperature, gravity, projected rotational velocity, and radial velocity from our spectra by fitting them with synthetic spectra with the ROTFIT tool. The targets have negligible extinction and spectral type from G5 to M8. We perform synthetic photometry on the spectra to derive the typical colors of young stars in different filters. We measure the luminosity of the emission lines present in the spectra and estimate the noise due to chromospheric emission in the measurements of accretion luminosity in accreting stars. We provide a calibration of the photospheric colors of young PMS stars as a function of their spectral type in a set of standard broad-band optical and near-infrared filters. For stars with masses of ~ 1.5Msun and ages of ~1-5 Myr, the chromospheric noise converts to a limit of measurable mass accretion rates of ~ 3x10^-10 Msun/yr.