We present a pipeline based on a random forest classifier for the identification of high column density clouds of neutral hydrogen (i.e. the Lyman limit systems, LLSs) in absorption within large spectroscopic surveys of z ≳ 3 quasars. We test the performance of this method on mock quasar spectra that reproduce the expected data quality of the Dark Energy Spectroscopic Instrument and the WHT (William Herschel Telescope) Enhanced Area Velocity Explorer surveys, finding ≳90 per cent completeness and purity for NHI≳1017.2 cm−2 LLSs against quasars of g < 23 mag at z ≈ 3.5–3.7. After training and applying our method on 10 000 quasar spectra at z ≈ 3.5–4.0 from the Sloan Digital Sky Survey (Data Release 16), we identify ≈6600 LLSs with NHI≳1017.5 cm−2 between z ≈ 3.1 and 4.0 with a completeness and purity of ≳90 per cent for the classification of LLSs. Using this sample, we measure a number of LLSs per unit redshift of ℓ(z) = 2.32 ± 0.08 at z = [3.3, 3.6]. We also present results on the performance of random forest for the measurement of the LLS redshifts and H I column densities, and for the identification of broad absorption line quasars.

Fumagalli, M., Fotopoulou, S., Thomson, L. (2020). Detecting neutral hydrogen at z ≳ 3 in large spectroscopic surveys of quasars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 498(2), 1951-1962 [10.1093/mnras/staa2388].

Detecting neutral hydrogen at z ≳ 3 in large spectroscopic surveys of quasars

Fumagalli, Michele
;
2020

Abstract

We present a pipeline based on a random forest classifier for the identification of high column density clouds of neutral hydrogen (i.e. the Lyman limit systems, LLSs) in absorption within large spectroscopic surveys of z ≳ 3 quasars. We test the performance of this method on mock quasar spectra that reproduce the expected data quality of the Dark Energy Spectroscopic Instrument and the WHT (William Herschel Telescope) Enhanced Area Velocity Explorer surveys, finding ≳90 per cent completeness and purity for NHI≳1017.2 cm−2 LLSs against quasars of g < 23 mag at z ≈ 3.5–3.7. After training and applying our method on 10 000 quasar spectra at z ≈ 3.5–4.0 from the Sloan Digital Sky Survey (Data Release 16), we identify ≈6600 LLSs with NHI≳1017.5 cm−2 between z ≈ 3.1 and 4.0 with a completeness and purity of ≳90 per cent for the classification of LLSs. Using this sample, we measure a number of LLSs per unit redshift of ℓ(z) = 2.32 ± 0.08 at z = [3.3, 3.6]. We also present results on the performance of random forest for the measurement of the LLS redshifts and H I column densities, and for the identification of broad absorption line quasars.
Articolo in rivista - Articolo scientifico
methods: data analysis; galaxies: haloes; intergalactic medium; quasars: absorption lines; Astrophysics - Astrophysics of Galaxies; Astrophysics - Instrumentation and Methods for Astrophysics
English
31-ago-2020
2020
498
2
1951
1962
reserved
Fumagalli, M., Fotopoulou, S., Thomson, L. (2020). Detecting neutral hydrogen at z ≳ 3 in large spectroscopic surveys of quasars. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 498(2), 1951-1962 [10.1093/mnras/staa2388].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/294031
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