ISO 9001 - AS 9100 - ITAR Standard & Custom Optical Filters and Coatings

The MATTISE was launched in 2019

Our optical filters continue to generate new discoveries through the years,

in Feb 2022 MATISSE helped uncover a hidden supermassive black hole

Matisse - Update 

This illustration shows what the core of Messier 77 might look like. As other active galactic nuclei, the central region of Messier 77 is powered by a black hole that is surrounded by a thin accretion disc, which itself is surrounded by a thick ring or torus of gas and dust. In the case of Messier 77, this thick ring completely obscures our view of the supermassive black hole.
This active galactic nucleus is also believed to have jets, as well as dusty winds, that flow out of the region around the black hole perpendicularly to the accretion disc around it.
ESO/M. Kornmesser and L. Calçada

An international team of astronomers led by Violeta Gámez Rosas (Leiden University) has observed a supermassive black hole hidden in a ring of dust. This discovery fits the idea that the so-called active centers of galaxies are much more similar than observations show, because the viewing angle from Earth causes distortions. The research was done with the MATISSE instrument, co-developed in the Netherlands, which combines infrared light from four European Very Large Telescopes (VLT) in Chile.

MATISSE is the acronym for Multi AperTure mid-Infrared SpectroScopic Experiment. MATISSE not only couples the light from the VLT, but also analyzes it. MATISSE was created specifically for infrared light with wavelengths between 3 micrometers and 13 micrometers. Infrared light is also created when something gives off heat. Therefore, MATISSE is cooled to minus 241 degrees Celsius so the instrument itself does not interfere with the measurements.

Nanometer precision

Netherlands Research School for Astronomy (NOVA) built all the lenses and mirrors in the cooled part of MATISSE together with the Dutch space industry. The Netherlands had gained experience while developing its forerunner MIDI, which could link two telescopes instead of four.

The heart where the beams of the four VLT telescopes converge, consists of two aluminum boxes that are almost a meter in size. These boxes are filled to the brim with hundreds of optical components, dozens of sensors and dozens of tiny motors. Most of the components work with nanometer precision or even higher.

For more on this discovery, see Supermassive Black Hole Caught Hiding in an Immense Ring of Cosmic Dust.

Reference: “Thermal imaging of dust hiding the black hole in the Active Galaxy NGC 1068”by Violeta Gámez Rosas, Jacob W. Isbell, Walter Jaffe, Romain G. Petrov, James H. Leftley, Karl-Heinz Hofmann, Florentin Millour, Leonard Burtscher, Klaus Meisenheimer, Anthony Meilland, Laurens B. F. M. Waters, Bruno Lopez, Stéphane Lagarde, Gerd Weigelt, Philippe Berio, Fatme Allouche, Sylvie Robbe-Dubois, Pierre Cruzalèbes, Felix Bettonvil, Thomas Henning, Jean-Charles Augereau, Pierre Antonelli, Udo Beckmann, Roy van Boekel, Philippe Bendjoya, William C. Danchi, Carsten Dominik, Julien Drevon, Jack F. Gallimore, Uwe Graser, Matthias Heininger, Vincent Hocdé, Michiel Hogerheijde, Josef Hron, Caterina M. V. Impellizzeri, Lucia Klarmann, Elena Kokoulina, Lucas Labadie, Michael Lehmitz, Alexis Matter, Claudia Paladini, Eric Pantin, Jörg-Uwe Pott, Dieter Schertl, Anthony Soulain, Philippe Stee, Konrad Tristram, Jozsef Varga, Julien Woillez, Sebastian Wolf, Gideon Yoffe and Gerard Zins, 16 February 2022, Nature.
DOI: 10.1038/s41586-021-04311-7