1. INSPIRE: INvestigating Stellar Population in RElics: I. Survey presentation and pilot study
- Author
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Oxford Hintze Centre for Astrophysical Surveys (UK), La Caixa, Bonn-Cologne Graduate School of Physics and Astronomy, Sun Yat-sen University, International Max Planck Research Schools, Spiniello, C., Tortora, C., D'Ago, G., Coccato, Lodovico, Barbera, F. la, Ferré-Mateu, Anna, Napolitano, N. R., Spavone, M., Scognamiglio, D., Arnaboldi, M., Gallazzi, A., Hunt, L., Moehler, S., Radovich, Milan, Zibetti, Stefano, Oxford Hintze Centre for Astrophysical Surveys (UK), La Caixa, Bonn-Cologne Graduate School of Physics and Astronomy, Sun Yat-sen University, International Max Planck Research Schools, Spiniello, C., Tortora, C., D'Ago, G., Coccato, Lodovico, Barbera, F. la, Ferré-Mateu, Anna, Napolitano, N. R., Spavone, M., Scognamiglio, D., Arnaboldi, M., Gallazzi, A., Hunt, L., Moehler, S., Radovich, Milan, and Zibetti, Stefano
- Abstract
[Context] Massive elliptical galaxies are thought to form through a two-phase process. At early times (z > 2), an intense and fast starburst forms blue and disk-dominated galaxies. After quenching, the remaining structures become red, compact, and massive (i.e. red nuggets). Then, a time-extended second phase, which is dominated by mergers, causes structural evolution and size growth. Given the stochastic nature of mergers, a small fraction of red nuggets survive, without any interaction, massive and compact until today: these are relic galaxies. Since this fraction depends on the processes dominating the size growth, counting relics at low-z is a valuable way of disentangling between different galaxy evolution models. [Aims] In this paper, we introduce the INvestigating Stellar Population In RElics (INSPIRE) Project, which aims to spectroscopically confirm and fully characterise a large number of relics at 0:1z0:5. We focus here on the first results based on a pilot study targeting three systems, representative of the whole sample. [Methods] For these three candidates, we extracted 1D optical spectra over an aperture of r = 0:4000, which comprises 30% of the galaxies’ light, and we obtained the line-of-sight integrated stellar velocity and velocity dispersion. We also inferred the stellar [/Fe] abundance from line-index measurements and mass-weighted age and metallicity from full-spectral fitting with single stellar population models. [Results] Two galaxies have large integrated stellar velocity dispersion values (250 km s), confirming their massive nature. They are populated by stars with super-solar metallicity and [/Fe]. Both objects have formed 80% of their stellar mass within a short (0:5:0 Gyr) initial star formation episode occurred only 1 Gyr after the Big Bang. The third galaxy has a more extendedstar formation history and a lower velocity dispersion. Thus we confirm two out of three candidates as relics. [Conclusions] This paper is the first step towards
- Published
- 2021