J/ApJ/927/164   Stellar population properties from LEGA-C DR2   (Borghi+, 2022)

Toward a better understanding of cosmic chronometers: stellar population properties of passive galaxies at intermediate redshift. Borghi N., Moresco M., Cimatti A., Huchet A., Quai S., Pozzetti L. <Astrophys. J., 927, 164 (2022)> =2022ApJ...927..164B 2022ApJ...927..164B
ADC_Keywords: Galaxies, spectra; Abundances; Stars, ages; Optical Keywords: Galaxy evolution ; Galaxy abundances ; Galaxy ages ; Observational cosmology Abstract: We take advantage of the publicly available LEGA-C spectroscopic survey to measure the stellar population properties of 140 individual massive and passive galaxies at z∼0.7. We develop and publicly release PyLick, a flexible Python code to measure UV to near-IR spectral indices. With PyLick we study the H/K ratio as a new diagnostic based on the pseudo-Lick CaII H and K indices and find that a cut in H/K<1.1 can be used jointly with other criteria to select (or verify the purity of) samples of passive galaxies. By combining photometric and spectroscopic criteria, we select a reliable sample of passively evolving galaxies. We constrain single-burst stellar ages, metallicities [Z/H], and [α/Fe] with an optimized set of Lick indices, exploring in detail the robustness of our measurement against different combinations. Even without imposing cosmological priors, the derived ages follow a clear trend compatible with the expected cosmological aging of the universe. We observe no significant redshift evolution for the metal abundance with respect to the values derived at z=0, with median [Z/H]=0.08±0.18 and [α/Fe]=0.13±0.11. Finally, we analyze the relations between log age, [Z/H], [α/Fe], and the stellar velocity dispersion, finding slopes of (0.5±0.1), (0.3±0.2), and (0.2±0.1), respectively; the small scatter of <0.2dex points to rather homogeneous and short star formation histories. Overall, these results confirm and extend low- redshift findings of a mass-downsizing evolution. This work further strengthens the possibility of selecting pure samples of passive galaxies to be exploited reliably as cosmic chronometers to place independent cosmological constraints. Description: The data used in this study are drawn from the second data release of LEGA-C (see Straatman+ 2018, J/ApJS/239/27), a recently completed ESO Public Spectroscopic Survey targeting ∼3000 Ks-band-selected galaxies at 0.6≲z≲1 in the COSMOS field. The observations were carried out with the Visible Multi-Object Spectrograph (VIMOS) on the VLT at Paranal Observatory. The flux-calibrated spectra span a wavelength range of 6300<λ<8800Å with a spectral resolution of R∼3500 and a median signal-to-noise ratio (S/N) of ∼15 per pixel (0.6Å). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table4.dat 80 140 *Stellar ages, metallicities [Z/H], and [α/Fe] for 140 massive and passive galaxies at z∼0.7 -------------------------------------------------------------------------------- Note on table4.dat: The work is based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under program ID 194.AF2005(A-N). See also: van der Wel+ (2016ApJS..223...29V 2016ApJS..223...29V) and Straatman+ (2018, J/ApJS/239/27). -------------------------------------------------------------------------------- See also: J/ApJS/82/197 : Mean UV Spectra of Stellar Groups (Fanelli+ 1992) J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994) J/ApJS/111/377 : Hγ & Hδ absorption features (Worthey+ 1997) J/ApJS/116/1 : Old Stellar Populations. VI. Absorption-Line (Trager+ 1998) J/ApJS/122/51 : Sp. catalog of 10 rich galaxy clusters (Dressler+ 1999) J/A+A/345/419 : Star formation in early-type galaxies (Longhetti+ 1999) J/MNRAS/326/959 : Empirical calibration of the NIR Ca triplet (Cenarro+ 2001) J/ApJ/621/673 : Line indices for 124 early-type galaxies (Thomas+, 2005) J/ApJ/633/174 : Spheroidals and bulge dominated galaxies (Treu+, 2005) J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006) J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009) J/AJ/145/77 : Imaging and sp. in 3 galaxy clusters (Jorgensen+, 2013) J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013) J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013) J/ApJ/788/72 : Observed sample of z∼0.7 massive galaxies (Gallazzi+, 2014) J/MNRAS/448/3484 : ATLAS3D Project. XXX (McDermid+, 2015) J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016) J/ApJS/239/27 : LEGA-C DR2: galaxies in the COSMOS field (Straatman+, 2018) J/MNRAS/490/417 : VANDELS massive quiescent gal. at 1.0<z<1.3 (Carnall+, 2019) Byte-by-byte Description of file: table4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- [MMS2013] [26438/259363] Object identifier (Muzzin+ 2013, J/ApJS/206/8) 8- 16 F9.5 deg RAdeg [149.7/150.8] Right Ascension (J2000) 18- 24 F7.5 deg DEdeg [1.7/2.8] Declination (J2000) 26- 30 F5.3 Gyr Age [1.2/6.1] Mean stellar age (single-burst star formation history) (1) 32- 36 F5.3 Gyr e16-Age [0.05/1.1] 16th percentile uncertainty in Age 38- 42 F5.3 Gyr e84-Age [0.05/1.4] 84th percentile uncertainty in Age 44- 49 F6.3 [-] [Z/H] [-0.24/0.6] Mean stellar metallicity [Z/H] (1) 51- 55 F5.3 [-] e16-[Z/H] [0.01/0.15] 16th percentile uncertainty in [Z/H] 57- 61 F5.3 [-] e84-[Z/H] [0.01/0.2] 84th percentile uncertainty in [Z/H] 63- 68 F6.3 [-] [a/Fe] [-0.2/0.42] Mean stellar alpha-to-iron (1) 70- 74 F5.3 [-] e16-[a/Fe] [0.007/0.11] 16th percentile uncertainty in [a/Fe] 76- 80 F5.3 [-] e84-[a/Fe] [0.009/0.12] 84th percentile uncertainty in [a/Fe] -------------------------------------------------------------------------------- Note (1): Stellar population properties age, [Z/H], [a/Fe] were derived comparing an optimized set of observed Lick indices with Thomas, Maraston & Johannson (2011MNRAS.412.2183T 2011MNRAS.412.2183T) simple stellar population models. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 17-Jan-2024
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