Gravitationally Lensed Quasar SDSS J1442+4055: Redshifts of Lensing Galaxies, Time Delay, Microlensing Variability, and Intervening Metal System at z ~ 2
| Autor: | Luis J. Goicoechea, Vyacheslav N. Shalyapin |
|---|---|
| Přispěvatelé: | Universidad de Cantabria |
| Jazyk: | angličtina |
| Rok vydání: | 2019 |
| Předmět: |
010504 meteorology & atmospheric sciences
Dark matter FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics Gravitational microlensing 01 natural sciences Gravitation 0103 physical sciences 010303 astronomy & astrophysics Astrophysics::Galaxy Astrophysics 0105 earth and related environmental sciences Physics Astrophysics::Instrumentation and Methods for Astrophysics gravitational lensing: strong Astronomy Astronomy and Astrophysics Quasar individual ( SDSS J1442 + 4055 ) [Quasars] High-redshift (galaxies) Astrophysics - Astrophysics of Galaxies Galaxy Redshift Quasars: individual ( SDSS J1442 + 4055 ) Space and Planetary Science strong [gravitational lensing] Astrophysics of Galaxies (astro-ph.GA) Astrophysics::Earth and Planetary Astrophysics |
| Zdroj: | Apj 873 117 (2019) UCrea Repositorio Abierto de la Universidad de Cantabria instname |
| Popis: | We present an $r$--band photometric monitoring of the two images A and B of the gravitationally lensed quasar SDSS J1442+4055 using the Liverpool Telescope (LT). From the LT light curves between 2015 December and 2018 August, we derive at once a time delay of 25.0 $\pm$ 1.5 days (1$\sigma$ confidence interval; A is leading) and microlensing magnification gradients below 10$^{-4}$ mag day$^{-1}$. The delay interval is not expected to be affected by an appreciable microlensing--induced bias, so it can be used to estimate cosmological parameters. This paper also focuses on new Gran Telescopio Canarias (GTC) and LT spectroscopic observations of the lens system. We determine the redshift of two bright galaxies around the doubly imaged quasar using LT spectroscopy, while GTC data lead to low--noise individual spectra of A, B, and the main lensing galaxy G1. The G1 spectral shape is accurately matched to an early--type galaxy template at $z$ = 0.284, and it has potential for further relevant studies. Additionally, the quasar spectra show absorption by metal--rich gas at $z \sim$ 2. This dusty absorber is responsible for an extinction bump at a rest--frame wavelength of 2209 $\pm$ 2 \AA, which has strengths of $\sim$ 0.47 and 0.76 mag $\mu$m$^{-1}$ for A and B, respectively. In such intervening system, the dust--to--gas ratio, gas--phase metallicity indicator [Zn/H], and dust depletion level [Fe/Zn] are relatively high. Comment: 21 pages, 9 figures, 9 tables. The long Tables 1-4 are available at https://grupos.unican.es/glendama/q1442.htm |
| Databáze: | OpenAIRE |
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