GRAVITY+ Collaboration, Abuter, R. et al.
The GRAVITY+ Project: GRAVITY-Wide and the Beam Compressor Differential Delay Lines
Authors:
GRAVITY+ Collaboration, Abuter, R., Allouche, F., Amorim, A., Bailet, C., Berger, J., Berio, P., Bigioli, A., Boebion, O., Böttcher, R., Bolzer, M., Bonnet, H., Bourdarot, G., Bourget, P., Brandner, W., Brara, A., Clénet, Y., Courtney-Barrer, B., Davies, R., Defrère, D., Delboulbé, A., Delplancke, F., Dembet, R., Dong, S., Drescher, A., Eckart, A., Édouard, C., Eisenhauer, F., Fabricius, M., Feuchtgruber, H., Finger, G., Förster Schreiber, N., Frahm, R., Garcia, E., Garcia, P., Gendron, E., Genzel, R., Gil, J., Gillessen, S., Gomes, T., Gonté, F., Gopinath, V., Graf, J., Guajardo, P., Guieu, S., Häberle, M., Hartl, M., Haubois, X., Haußmann, F., Henning, T., Hönig, S., Horrobin, M., Hubin, N., Jochum, L., Jocou, L., Kaufer, A., Kervella, P., Kreidberg, L., Lacour, S., Lagarde, S., Lai, O., Lapeyrère, V., Laugier, R., Le Bouquin, J., Leftley, J., Léna, P., Lutz, D., Mang, F., Mérand, A., Millour, F., More, N., Mroz, P., Nowacki, H., Nowak, M., Neumayer, N., Oberti, S., Ott, T., Özdemir, H., Pallanca, L., Paumard, T., Perraut, K., Perrin, G., Petrov, R., Pfuhl, O., Pourré, N., Prowatke, H., Rabien, S., Rau, C., Rehm, C., Riquelme, M., Robbe, S., Rochat, S., Salman, M., Sauter, J., Schubert, J., Schuhler, N., Shangguan, J., Shimizu, T., Scheithauer, S., Schuppe, D., Soulez, F., Stadler, E., Straubmeier, C., Sturm, E., Subroweit, M., Sykes, C., Tacconi, L., Tristram, K., Vincent, F., Uysal, S., Wessely, P., Widmann, F., Wieprecht, E., Wiezorrek, E., Wimmer, L., Woillez, J., Yazici, S., Zins, G.
Abstract:
One of the primary goals of the GRAVITY+ upgrade is to significantly improve the sky coverage of GRAVITY and the Very Large Telescope Interferometer. With the successful commissioning and start of operations of the GRAVITY-Wide mode and the new Beam Compressor Differential Delay Lines, GRAVITY+ has opened up the sky to deep interferometric observations. These include the first dynamical black hole mass measurements at cosmic noon, vastly increased observable samples of microlensing events, and a step towards the first detection of an intermediate-mass black hole through stellar orbits.