Issue |
A&A
Volume 629, September 2019
|
|
---|---|---|
Article Number | A97 | |
Number of page(s) | 13 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201935921 | |
Published online | 11 September 2019 |
COSMOGRAIL
XVIII. time delays of the quadruply lensed quasar WFI2033−4723⋆
1
Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
e-mail: vivien.bonvin@epfl.ch
2
Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85740 Garching, Germany
3
Physik-Department, Technische Universität München, James-Franck-Straße 1, 85748 Garching, Germany
4
Institute of Astronomy and Astrophysics, Academia Sinica, 11F of ASMAB, No. 1, Section 4, Roosevelt Road, Taipei 10617, Taiwan
5
Subaru Telescope, National Astronomical Observatory of Japan, 650 N Aohoku Pl, Hilo 96720, Japan
6
Department of Physics, University of California, Davis, CA 95616, USA
7
STAR Institute, Quartier Agora – Allée du six Août 19c, 4000 Liège, Belgium
8
Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
9
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
10
Department of Physics and Astronomy, PAB, 430 Portola Plaza, Box 951547 Los Angeles, CA 90095, USA
11
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94035, USA
12
Fermi National Accelerator Laboratory, PO Box 500 Batavia, IL 60510, USA
13
Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, USA
14
Departamento de Ciencias Físicas, Universidad Andres Bello Fernandez Concha 700, Las Condes, Santiago, Chile
15
Centro de Astroingeniería, Facultad de Física, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Macul 7820436 Santiago, Chile
16
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
17
Las Cumbres Observatory Global Telescope, 6740 Cortona Dr., Suite 102, Goleta, CA 93111, USA
18
Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA
19
Instituto de Física y Astronomía, Universidad de Valparaíso, Avda. Gran Bretaña 1111, Playa Ancha, Valparaíso 2360102, Chile
20
Millennium Institute of Astrophysics, Chile
21
Department of Physics, United States Naval Academy, 572C Holloway Rd., Annapolis, MD 21402, USA
22
Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany
23
Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210, USA
24
Center for Cosmology and Astroparticle Physics, The Ohio State University, 191 W. Woodruff Avenue, Columbus, OH 43210, USA
Received:
20
May
2019
Accepted:
11
June
2019
We present new measurements of the time delays of WFI2033−4723. The data sets used in this work include 14 years of data taken at the 1.2 m Leonhard Euler Swiss telescope, 13 years of data from the SMARTS 1.3 m telescope at Las Campanas Observatory and a single year of high-cadence and high-precision monitoring at the MPIA 2.2 m telescope. The time delays measured from these different data sets, all taken in the R-band, are in good agreement with each other and with previous measurements from the literature. Combining all the time-delay estimates from our data sets results in ΔtAB = 36.2+0.7−0.8 days (2.1% precision), ΔtAC = −23.3+1.2−1.4 days (5.6%) and ΔtBC = −59.4+1.3−1.3 days (2.2%). In addition, the close image pair A1-A2 of the lensed quasars can be resolved in the MPIA 2.2 m data. We measure a time delay consistent with zero in this pair of images. We also explore the prior distributions of microlensing time-delay potentially affecting the cosmological time-delay measurements of WFI2033−4723. Our time-delay measurements are not precise enough to conclude that microlensing time delay is present or absent from the data. This work is part of a H0LiCOW series focusing on measuring the Hubble constant from WFI2033−4723.
Key words: gravitational lensing: strong / galaxies: individual: WFI2033−4723 / cosmological parameters
Full light curves of the four data sets are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/629/A97
© ESO 2019
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