The case against gravitational millilensing in the multiply-imaged quasar B1152+199
Artikel i vetenskaplig tidskrift, 2020

Previous very long baseline interferometry (VLBI) observations of the quasar B1152+199 at 5 GHz has revealed two images of a strongly lensed jet with seemingly discordant morphologies. Whereas the jet appears straight in one of the images, the other exhibits slight curvature on milliarcsecond scales. This is unexpected from the lensing solution and has been interpreted as possible evidence for secondary, small-scale lensing (millilensing) by a compact object with a mass of 10(5)-10(7) M-circle dot located close to the curved image. The probability for such a superposition is extremely low unless the millilens population has very high surface number density. Here, we revisit the case for millilensing in B1152+199 by combining new global-VLBI data at 8.4 GHz with two data sets from the European VLBI Network (EVN) at 5 GHz (archival), and the previously published 5 GHz Very Long Baseline Array (VLBA) data. We find that the new data with a more circular synthesized beam, exhibits no apparent milliarcsecond-scale curvature in image B. Various observations of the object spanning similar to 15 yr apart enable us to improve the constraints on lens system to the point that the only plausible explanation left for the apparent curvature is the artefact due to the shape of the synthesized beam.

dark matter

galaxies: jets

gravitational lensing: strong

Författare

Saghar Asadi

AlbaNova

Stockholms universitet

Erik Zackrisson

Uppsala universitet

Eskil Varenius

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Rymdgeodesi och geodynamik

Emily Freeland

AlbaNova

Stockholms universitet

John Conway

Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium

Kaj Wiik

Turun Yliopisto

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 492 1 742-748

Ämneskategorier

Fjärranalysteknik

Geofysik

Datorseende och robotik (autonoma system)

DOI

10.1093/mnras/stz3450

Mer information

Senast uppdaterat

2020-04-23