The Event Horizon Telescope Image of the Quasar NRAO 530

DOI: 
10.3847/1538-4357/acaea8
Publication date: 
15/02/2023
Main author: 
Jorstad, Svetlana
IAA authors: 
Lico, Rocco;Zhao, Guang-Yao;Alberdi, Antxon;Cho, Ilje;Fuentes, Antonio;Gómez, José L.;Traianou, Efthalia
Authors: 
Jorstad, Svetlana;Wielgus, Maciek;Lico, Rocco;Issaoun, Sara;Broderick, Avery E.;Pesce, Dominic W.;Liu, Jun;Zhao, Guang-Yao;Krichbaum, Thomas P.;Blackburn, Lindy;Chan, Chi-kwan;Janssen, Michael;Ramakrishnan, Venkatessh;Akiyama, Kazunori;Alberdi, Antxon;Algaba, Juan Carlos;Bouman, Katherine L.;Cho, Ilje;Fuentes, Antonio;Gómez, José L.;Gurwell, Mark;Johnson, Michael D.;Kim, Jae-Young;Lu, Ru-Sen;Martí-Vidal, Iván;Moscibrodzka, Monika;Pötzl, Felix M.;Traianou, Efthalia;van Bemmel, Ilse;Alef, Walter;Anantua, Richard;Asada, Keiichi;Azulay, Rebecca;Bach, Uwe;Baczko, Anne-Kathrin;Ball, David;Baloković, Mislav;Barrett, John;Bauböck, Michi;Benson, Bradford A.;Bintley, Dan;Blundell, Raymond;Bower, Geoffrey C.;Boyce, Hope;Bremer, Michael;Brinkerink, Christiaan D.;Brissenden, Roger;Britzen, Silke;Broguiere, Dominique;Bronzwaer, Thomas;Bustamante, Sandra;Byun, Do-Young;Carlstrom, John E.;Ceccobello, Chiara;Chael, Andrew;Chatterjee, Koushik;Chatterjee, Shami;Chen, Ming-Tang;Chen, Yongjun;Cheng, Xiaopeng;Christian, Pierre;Conroy, Nicholas S.;Conway, John E.;Cordes, James M.;Crawford, Thomas M.;Crew, Geoffrey B.;Cruz-Osorio, Alejandro;Cui, Yuzhu;Davelaar, Jordy;De Laurentis, Mariafelicia;Deane, Roger;Dempsey, Jessica;Desvignes, Gregory;Dexter, Jason;Dhruv, Vedant;Doeleman, Sheperd S.;Dougal, Sean;Dzib, Sergio A.;Eatough, Ralph P.;Emami, Razieh;Falcke, Heino;Farah, Joseph;Fish, Vincent L.;Fomalont, Ed;Ford, H. Alyson;Fraga-Encinas, Raquel;Freeman, William T.;Friberg, Per;Fromm, Christian M.;Galison, Peter;Gammie, Charles F.;García, Roberto;Gentaz, Olivier;Georgiev, Boris;Goddi, Ciriaco;Gold, Roman;Gómez-Ruiz, Arturo I.;Gu, Minfeng;Hada, Kazuhiro;Haggard, Daryl;Haworth, Kari;Hecht, Michael H.;Hesper, Ronald;Heumann, Dirk;Ho, Luis C.;Ho, Paul;Honma, Mareki;Huang, Chih-Wei L.;Huang, Lei;Hughes, David H.;Ikeda, Shiro;Impellizzeri, C. M. Violette;Inoue, Makoto;James, David J.;Jannuzi, Buell T.;Jeter, Britton;Jiang, Wu;Jiménez-Rosales, Alejandra;Joshi, Abhishek V.;Jung, Taehyun;Karami, Mansour;Karuppusamy, Ramesh;Kawashima, Tomohisa;Keating, Garrett K.;Kettenis, Mark;Kim, Dong-Jin;Kim, Jongsoo;Kim, Junhan;Kino, Motoki;Koay, Jun Yi;Kocherlakota, Prashant;Kofuji, Yutaro;Koyama, Shoko;Kramer, Carsten;Kramer, Michael;Kuo, Cheng-Yu;La Bella, Noemi;Lauer, Tod R.;Lee, Daeyoung;Lee, Sang-Sung;Leung, Po Kin;Levis, Aviad;Li, Zhiyuan;Lindahl, Greg;Lindqvist, Michael;Lisakov, Mikhail;Liu, Kuo;Liuzzo, Elisabetta;Lo, Wen-Ping;Lobanov, Andrei P.;Loinard, Laurent;Lonsdale, Colin J.;MacDonald, Nicholas R.;Mao, Jirong;Marchili, Nicola;Markoff, Sera;Marrone, Daniel P.;Marscher, Alan P.;Matsushita, Satoki;Matthews, Lynn D.;Medeiros, Lia;Menten, Karl M.;Michalik, Daniel;Mizuno, Izumi;Mizuno, Yosuke;Moran, James M.;Moriyama, Kotaro;Müller, Cornelia;Mus, Alejandro;Musoke, Gibwa;Myserlis, Ioannis;Nadolski, Andrew;Nagai, Hiroshi;Nagar, Neil M.;Nakamura, Masanori;Narayan, Ramesh;Narayanan, Gopal;Natarajan, Iniyan;Nathanail, Antonios;Fuentes, Santiago Navarro;Neilsen, Joey;Neri, Roberto;Ni, Chunchong;Noutsos, Aristeidis;Nowak, Michael A.;Oh, Junghwan;Okino, Hiroki;Olivares, Héctor;Ortiz-León, Gisela N.;Oyama, Tomoaki;Özel, Feryal;Palumbo, Daniel C. M.;Paraschos, Georgios Filippos;Park, Jongho;Parsons, Harriet;Patel, Nimesh;Pen, Ue-Li;Piétu, Vincent;Plambeck, Richard;PopStefanija, Aleksandar;Porth, Oliver;Prather, Ben;Preciado-López, Jorge A.;Psaltis, Dimitrios;Pu, Hung-Yi;Rao, Ramprasad;Rawlings, Mark G.;Raymond, Alexander W.;Rezzolla, Luciano;Ricarte, Angelo;Ripperda, Bart;Roelofs, Freek;Rogers, Alan;Ros, Eduardo;Romero-Cañizales, Cristina;Roshanineshat, Arash;Rottmann, Helge;Roy, Alan L.;Ruiz, Ignacio;Ruszczyk, Chet;Rygl, Kazi L. J.;Sánchez, Salvador;Sánchez-Argüelles, David;Sánchez-Portal, Miguel;Sasada, Mahito;Satapathy, Kaushik;Savolainen, Tuomas;Schloerb, F. Peter;Schonfeld, Jonathan;Schuster, Karl-Friedrich;Shao, Lijing;Shen, Zhiqiang;Small, Des;Sohn, Bong Won;SooHoo, Jason;Souccar, Kamal;Sun, He;Tazaki, Fumie;Tetarenko, Alexandra J.;Tiede, Paul;Tilanus, Remo P. J.;Titus, Michael;Torne, Pablo;Trent, Tyler;Trippe, Sascha;Turk, Matthew;van Langevelde, Huib Jan;van Rossum, Daniel R.;Vos, Jesse;Wagner, Jan;Ward-Thompson, Derek;Wardle, John;Weintroub, Jonathan;Wex, Norbert;Wharton, Robert;Wiik, Kaj;Witzel, Gunther;Wondrak, Michael F.;Wong, George N.;Wu, Qingwen;Yamaguchi, Paul;Yoon, Doosoo;Young, André;Young, Ken;Younsi, Ziri;Yuan, Feng;Yuan, Ye-Fei;Zensus, J. Anton;Zhang, Shuo;Zhao, Shan-Shan
Journal: 
The Astrophysical Journal
Publication type: 
Article
Volume: 
943
Pages: 
170
Abstract: 
We report on the observations of the quasar NRAO 530 with the Event Horizon Telescope (EHT) on 2017 April 5-7, when NRAO 530 was used as a calibrator for the EHT observations of Sagittarius A*. At z = 0.902, this is the most distant object imaged by the EHT so far. We reconstruct the first images of the source at 230 GHz, at an unprecedented angular resolution of ~20 μas, both in total intensity and in linear polarization (LP). We do not detect source variability, allowing us to represent the whole data set with static images. The images reveal a bright feature located on the southern end of the jet, which we associate with the core. The feature is linearly polarized, with a fractional polarization of ~5%-8%, and it has a substructure consisting of two components. Their observed brightness temperature suggests that the energy density of the jet is dominated by the magnetic field. The jet extends over 60 μas along a position angle ~ -28°. It includes two features with orthogonal directions of polarization (electric vector position angle), parallel and perpendicular to the jet axis, consistent with a helical structure of the magnetic field in the jet. The outermost feature has a particularly high degree of LP, suggestive of a nearly uniform magnetic field. Future EHT observations will probe the variability of the jet structure on microarcsecond scales, while simultaneous multiwavelength monitoring will provide insight into the high-energy emission origin.
Database: 
ADS
SCOPUS
URL: 
https://ui.adsabs.harvard.edu/#abs/2023ApJ...943..170J/abstract
ADS Bibcode: 
2023ApJ...943..170J
Keywords: 
Extragalactic astronomy;506;Astrophysics - High Energy Astrophysical Phenomena;Astrophysics - Astrophysics of Galaxies