J/MNRAS/528/2790  Age resolution in stellar population synthesis (Zibetti+ 2024)

On the maximum age resolution achievable through stellar population synthesis models. Zibetti S., Rossi E., Gallazzi A.R. <Mon. Not. R. Astron. Soc. 528, 2790-2804 (2024)> =2024MNRAS.528.2790Z 2024MNRAS.528.2790Z (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, spectra ; Galaxies, optical ; Populations, stellar ; Stars, ages Keywords: galaxies: evolution - galaxies: fundamental parameters - galaxies: stellar content Abstract: As the reconstruction of the star-formation histories (SFH) of galaxies from spectroscopic data becomes increasingly popular, we explore the best age resolution achievable with stellar population synthesis (SPS) models, relying on different constraints: broad-band colours, absorption indices, a combination of the two, and the full spectrum. We perform idealized experiments on SPS models and show that the minimum resolvable relative duration of a star-formation episode (time difference between 10% and 90% of the stellar mass formed divided by the median age) is never better than 0.4, even when using spectra with signal-to-noise ratio (SNR) larger than 100 per Å. Typically, the best relative age resolution ranges between 0.4 and 0.7 over most of the age-metallicity plane, corresponding to minimum bin sizes for SFH sampling between 0.15 and 0.25dex. This resolution makes the spectroscopic exploration of distant galaxies mandatory in order to reconstruct the early phases of galaxies' SFHs. We show that spectroscopy with SNR≳20Å-1 is essential for good age resolution. Remarkably, using the full spectrum does not prove significantly more effective than relying on absorption indices, especially at SNR≲20Å-1. We discuss the physical origins of the age resolution trends as a function of age and metallicity, and identify the presence of maxima in age resolution (i.e. minima in measurable relative time duration) at the characteristic ages that correspond to quick time variations in spectral absorption features. We connect these maxima to bumps commonly observed in reconstructed SFHs. Description: The minimum measurable relative duration of idealized star-formation histories are reported for different constraints and different signal-to-noise ratio regimes, as a function of the median age of the stellar population (age50). The relative duration is expressed in terms of {DELTA}age10-90/age50=dagen (dagen={DELTA}agen), where {DELTA}age10-90 is the time span between the epoch at which 10% and and 90% of the stellar mass have been already formed (see Sec. 2.1 in the paper). All quantities represented in Figures 2, 3, 4, and A1 are provided in log10. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig2.dat 111 83 Fig.2 min dagen(age50,Z), different constraints fig3z002.dat 62 83 Fig.3.1 min dagen(age50), Z=0.02 Zsun for different spectroscopic SNR (indices) fig3z020.dat 62 83 Fig.3.2 min dagen(age50), Z=0.20 Zsun for different spectroscopic SNR (indices) fig3z040.dat 62 83 Fig.3.3 min dagen(age50), Z=0.40 Zsun for different spectroscopic SNR (indices) fig3z100.dat 62 83 Fig.3.4 min dagen(age50), Z=1.00 Zsun for different spectroscopic SNR (indices) fig3z250.dat 62 83 Fig.3.5 min dagen(age50), Z=2.50 Zsun for different spectroscopic SNR (indices) fig4.dat 146 83 Fig.4 min dagen(age50), Z=1.00 Zsun for different spectroscopic constraints at different SNR (different panels) figa1.dat 146 83 Fig.A1 min dagen(age50), Z=0.20 Zsun for different spectroscopic constraints at different SNR (different panels) -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.3 [yr] logage50 Median age of the stellar population 8- 13 F6.3 --- logdagen-col-Z002 ? Minimum dagen, colours only, Z=0.02 Zsun 15- 20 F6.3 --- logdagen-col-Z020 ? Minimum dagen, colours only, Z=0.20 Zsun 22- 27 F6.3 --- logdagen-col-Z040 ? Minimum dagen, colours only, Z=0.40 Zsun 29- 34 F6.3 --- logdagen-col-Z100 ? Minimum dagen, colours only, Z=1.00 Zsun 36- 41 F6.3 --- logdagen-col-Z250 ? Minimum dagen, colours only, Z=2.50 Zsun 43- 48 F6.3 --- logdagen-idx-Z002 ? Minimum dagen, indices only, Z=0.02 Zsun 50- 55 F6.3 --- logdagen-idx-Z020 ? Minimum dagen, indices only, Z=0.20 Zsun 57- 62 F6.3 --- logdagen-idx-Z040 ? Minimum dagen, indices only, Z=0.40 Zsun 64- 69 F6.3 --- logdagen-idx-Z100 ? Minimum dagen, indices only, Z=1.00 Zsun 71- 76 F6.3 --- logdagen-idx-Z250 ? Minimum dagen, indices only, Z=2.50 Zsun 78- 83 F6.3 --- logdagen-all-Z002 ? Minimum dagen, colours+indx, Z=0.02 Zsun 85- 90 F6.3 --- logdagen-all-Z020 ? Minimum dagen, colours+indx, Z=0.20 Zsun 92- 97 F6.3 --- logdagen-all-Z040 ? Minimum dagen, colours+indx, Z=0.40 Zsun 99-104 F6.3 --- logdagen-all-Z100 ? Minimum dagen, colours+indx, Z=1.00 Zsun 106-111 F6.3 --- logdagen-all-Z250 ? Minimum dagen, colours+indx, Z=2.50 Zsun -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig3z???.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.3 [yr] logage50 Median age of the stellar population 8- 13 F6.3 --- logdagen-col ? Minimum dagen, colours only 15- 20 F6.3 --- logdagen-SNR5 ? Minimum dagen, colours+indices SNR=5 22- 27 F6.3 --- logdagen-SNR10 ? Minimum dagen, colours+indices SNR=10 29- 34 F6.3 --- logdagen-SNR20 ? Minimum dagen, colours+indices SNR=20 36- 41 F6.3 --- logdagen-SNR50 ? Minimum dagen, colours+indices SNR=50 43- 48 F6.3 --- logdagen-SNR100 ? Minimum dagen, colours+indices SNR=100 50- 55 F6.3 --- logdagen-SNR200 ? Minimum dagen, colours+indices SNR=200 57- 62 F6.3 --- logdagen-SNR500 ? Minimum dagen, colours+indices SNR=500 -------------------------------------------------------------------------------- Byte-by-byte Description of file: fig4.dat figa1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.3 [yr] logage50 Median age of the stellar population 8- 13 F6.3 --- logdagenIdxcol-5 ? Minimum dagen, SNR=5 colours+indices (logdagen-idxcol-SNR5) 15- 20 F6.3 --- logdagen-FS-n-5 ? Minimum dagen, SNR=5 full spectrum [3800-5600Å] (logdagen-FS-narrow-SNR5) 22- 27 F6.3 --- logdagenFS-w-5 ? Minimum dagen, SNR=5 full spectrum [3500-7000Å] (logdagen-FS-wide-SNR5) 29- 34 F6.3 --- logdagenFS-r-n-5 ? Minimum dagen, SNR=5 full spectrum rectified [3800-5600Å] (logdagen-FS-rect-narrow-SNR5) 36- 41 F6.3 --- logdagenFS-r-w-5 ? Minimum dagen, SNR=5 full spectrum rectified [3500-7000Å] (logdagen-FS-rect-wide-SNR5) 43- 48 F6.3 --- logdagenIdxcol-10 ? Minimum dagen, SNR=10 colours+indices (logdagen-idxcol-SNR10) 50- 55 F6.3 --- logdagenFS-n-10 ? Minimum dagen, SNR=10 full spectrum [3800-5600Å] (logdagen-FS-narrow-SNR10) 57- 62 F6.3 --- logdagenFS-w-10 ? Minimum dagen, SNR=10 full spectrum [3500-7000Å] (logdagen-FS-wide-SNR10) 64- 69 F6.3 --- logdagenFS-r-n-10 ? Minimum dagen, SNR=10 full spectrum rectified [3800-5600Å] (logdagen-FS-rect-narrow-SNR10) 71- 76 F6.3 --- logdagenFS-r-w-10 ? Minimum dagen, SNR=10 full spectrum rectified [3500-7000Å] (logdagen-FS-rect-wide-SNR10) 78- 83 F6.3 --- logdagenIdxcol-20 ? Minimum dagen, SNR=20 colours+indices (logdagen-idxcol-SNR20) 85- 90 F6.3 --- logdagenFS-n-20 ? Minimum dagen, SNR=20 full spectrum [3800-5600Å] (logdagen-FS-narrow-SNR20) 92- 97 F6.3 --- logdagenFS-w-20 ? Minimum dagen, SNR=20 full spectrum [3500-7000Å] (logdagen-FS-wide-SNR20) 99-104 F6.3 --- logdagenFS-r-n-20 ? Minimum dagen, SNR=20 full spectrum rectified [3800-5600Å] (logdagen-FS-rect-narrow-SNR20) 106-111 F6.3 --- logdagenFS-r-w-20 ? Minimum dagen, SNR=20 full spectrum rectified [3500-7000Å] (logdagen-FS-rect-wide-SNR20) 113-118 F6.3 --- logdagenIdxcol-100 ? Minimum dagen, SNR=100 colours+indices (logdagen-idxcol-SNR100) 120-125 F6.3 --- logdagenFS-n-100 ? Minimum dagen, SNR=100 full spectrum [3800-5600Å] (logdagen-FS-narrow-SNR100) 127-132 F6.3 --- logdagenFS-w-100 ? Minimum dagen, SNR=100 full spectrum [3500-7000Å] (logdagen-FS-wide-SNR100) 134-139 F6.3 --- logdagenFS-r-n-100 ? Minimum dagen, SNR=100 full spectrum rectified [3800-5600Å] (logdagen-FS-rect-narrow-SNR100) 141-146 F6.3 --- logdagenFS-r-w-100 ? Minimum dagen, SNR=100 full spectrum rectified [3500-7000Å] (logdagen-FS-rect-wide-SNR100) -------------------------------------------------------------------------------- Acknowledgements: Stefano Zibetti, stefano.zibetti(at)inaf.it
(End) Patricia Vannier [CDS] 06-Feb-2024
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