Combining gravitational lensing and quasars

 

A quasar is a luminous manifestation of a supermassive black hole that accretes surrounding matter, sitting at the center of a host galaxy. It is generally difficult to measure how heavy a quasar’s host galaxy is because quasars are very distant objects, and also because they are so bright that they overshine anything within its vicinity.

 

Gravitational lensing allows us to compute the mass of the lensing object. Thanks to Einstein’s theory of gravitation, we know how massive objects in the foreground of the night sky – the gravitational lens – can bend light coming from background objects. Resulting are strange rings of light, that are actually distortions of the background object’s light by the gravitational lens.

 

Courbin was cycling to the Sauverny Observatory, over a decade ago, when he realized that he could combine the two – quasars and gravitational lensing – to measure the mass of a quasar’s host galaxy. For this, he had to find a quasar in a galaxy that also acts as a gravitational lens.

 

A handful of gravitational lensing quasars observed so far

 

The Sloan Digital Sky Survey (SDSS) database was a great place to search for gravitational lensing quasars candidates, but to be sure, Courbin had to see the lensing rings. In 2010, he and colleagues commissioned time on the Hubble Space Telescope to observe 4 candidates of which 3 showed lensing. Of the three, one stood out due to its characteristic gravitational lensing rings: SDSS J0919+2720.

 

The HST image of SDSS J0919+2720 shows two bright objects in the foreground that each act as a gravitational lens, “probably two galaxies in the process of merging,” explains Courbin. The one on the left is a bright quasar, within a host galaxy too dim to be observed. The bright object on the right is another galaxy, the main gravitational lens. A faint object on the far left is a companion galaxy. The characteristic rings are deformed light coming from a background galaxy.

 

Computational lens modeling to the rescue

 

By carefully analyzing the gravitationally lensed rings in SDSS J0919+2720, it is possible to determine the mass of the two bright objects… in principle. Disentangling the masses of the various objects would have been impossible without the recent development of a wavelet-based lens modeling technique by co-author Aymeric Galan, currently at the Technical University of Münich (TUM), also on an SNF grant.

 

“One of the biggest challenges in astrophysics is to understand how a supermassive black hole forms,” explains Galan. “Knowing its mass, how it compares to its host galaxy and how it evolves through cosmic times, are what allows us to discard or validate certain formation theories.”

 

“In the local Universe, we observe that the most massive galaxies also host the most massive black holes at their center. This could suggest that the growth of galaxies is regulated by the amount of energy radiated by their central black hole and injected into the galaxy. However, to test this theory, we still need to study these interactions not only locally but also in the distant Universe”, explains Millon.

 

Gravitational lensing events are very rare, with one galaxy in a thousand unveiling the phenomenon. Since quasars are seen in about one every thousand galaxies a quasar acting as a lens is one in a million. The scientists expect to detect hundreds of these lensing quasars with the ESA-NASA mission Euclid, to be launched this summer with a Falcon-9 SpaceX rocket.

The animation depicts an artist's view of the quasar and the Einstein rings, first from the point of view of the Hubble Space Telescope, and then when the lensing galaxy is no longer in alignment with the background galaxy. Credit: EPFL / Austin Peel.