DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Resolving the Inner Parsec of the Blazar J1924–2914 with the Event Horizon Telescope

Journal Article · · Astrophys.J.
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [2]; ORCiD logo [4]; ORCiD logo [2]; ORCiD logo [5]; ORCiD logo [6]; ORCiD logo [7]; ORCiD logo [8]; ORCiD logo [9]; ORCiD logo [10]; ORCiD logo [11]; ORCiD logo [12]; ORCiD logo [2]; ORCiD logo [13]; ORCiD logo [2]; ORCiD logo [7]; ORCiD logo [7]; ORCiD logo [14] more »; ORCiD logo [15]; ORCiD logo [6]; ORCiD logo [2]; ORCiD logo [16]; ORCiD logo [17]; ORCiD logo [18]; ORCiD logo [19]; ORCiD logo [20]; ORCiD logo [21]; ORCiD logo [22];  [2]; ORCiD logo [23]; ORCiD logo [24]; ORCiD logo [25]; ORCiD logo [26]; ORCiD logo [2]; ORCiD logo [2];  [5]; ORCiD logo [27]; ORCiD logo [28]; ORCiD logo [29]; ORCiD logo [30];  [31]; ORCiD logo [20];  [32]; ORCiD logo [33]; ORCiD logo [34]; ORCiD logo [35];  [36]; ORCiD logo [9]; ORCiD logo [4]; ORCiD logo [2]; ORCiD logo [36]; ORCiD logo [9]; ORCiD logo [37]; ORCiD logo [38]; ORCiD logo [39]; ORCiD logo [40]; ORCiD logo [4]; ORCiD logo [41]; ORCiD logo [42]; ORCiD logo [43]; ORCiD logo [22]; ORCiD logo [44]; ORCiD logo [45]; ORCiD logo [40]; ORCiD logo [41]; ORCiD logo [46]; ORCiD logo [28]; ORCiD logo [47]; ORCiD logo [48]; ORCiD logo [49]; ORCiD logo [50]; ORCiD logo [51]; ORCiD logo [52]; ORCiD logo [53]; ORCiD logo [4]; ORCiD logo [29]; ORCiD logo [54]; ORCiD logo [55]; ORCiD logo [20]; ORCiD logo [9]; ORCiD logo [56]; ORCiD logo [28]; ORCiD logo [57]; ORCiD logo [5]; ORCiD logo [9];  [58]; ORCiD logo [31]; ORCiD logo [59]; ORCiD logo [60]; ORCiD logo [61]; ORCiD logo [36];  [36]; ORCiD logo [62]; ORCiD logo [63]; ORCiD logo [64]; ORCiD logo [65]; ORCiD logo [66]; ORCiD logo [48]; ORCiD logo [35]; ORCiD logo [28]; ORCiD logo [67]; ORCiD logo [68]; ORCiD logo [69]; ORCiD logo [70]; ORCiD logo [25]; ORCiD logo [66];  [71]; ORCiD logo [72]; ORCiD logo [73]; ORCiD logo [25]; ORCiD logo [74]; ORCiD logo [5]; ORCiD logo [25]; ORCiD logo [66]; ORCiD logo [9]; ORCiD logo [4]; ORCiD logo [29]; ORCiD logo [38]; ORCiD logo [75]; ORCiD logo [2]; ORCiD logo [76]; ORCiD logo [20]; ORCiD logo [77]; ORCiD logo [2]; ORCiD logo [78]; ORCiD logo [79]; ORCiD logo [80]; ORCiD logo [81]; ORCiD logo [25]; ORCiD logo [47];  [82]; ORCiD logo [25]; ORCiD logo [83]; ORCiD logo [36]; ORCiD logo [2]; ORCiD logo [84]; ORCiD logo [9]; ORCiD logo [5]; ORCiD logo [29]; ORCiD logo [79]; ORCiD logo [85]; ORCiD logo [33]; ORCiD logo [86]; ORCiD logo [87]; ORCiD logo [20]; ORCiD logo [40]; ORCiD logo [2]; ORCiD logo [88]; ORCiD logo [89]; ORCiD logo [2]; ORCiD logo [28]; ORCiD logo [90]; ORCiD logo [91]; ORCiD logo [92]; ORCiD logo [5]; ORCiD logo [3]; ORCiD logo [25]; ORCiD logo [28]; ORCiD logo [93]; ORCiD logo [2]; ORCiD logo [94]; ORCiD logo [31]; ORCiD logo [95]; ORCiD logo [4]; ORCiD logo [96]; ORCiD logo [10]; ORCiD logo [97]; ORCiD logo [98]; ORCiD logo [99]; ORCiD logo [48]; ORCiD logo [100]; ORCiD logo [101]; ORCiD logo [4]; ORCiD logo [37]; ORCiD logo [102];  [103]; ORCiD logo [104]; ORCiD logo [36]; ORCiD logo [62]; ORCiD logo [2]; ORCiD logo [105]; ORCiD logo [106]; ORCiD logo [82]; ORCiD logo [9]; ORCiD logo [2]; ORCiD logo [107]; ORCiD logo [5]; ORCiD logo [4]; ORCiD logo [2]; ORCiD logo [25]; ORCiD logo [31]; ORCiD logo [20]; ORCiD logo [108];  [36]; ORCiD logo [109];  [37]; ORCiD logo [110]; ORCiD logo [111]; ORCiD logo [29]; ORCiD logo [112]; ORCiD logo [5]; ORCiD logo [113]; ORCiD logo [42]; ORCiD logo [114]; ORCiD logo [4]; ORCiD logo [115]; ORCiD logo [6]; ORCiD logo [116]; ORCiD logo [117]; ORCiD logo [28]; ORCiD logo [2]; ORCiD logo [25]; ORCiD logo [5];  [2]; ORCiD logo [2]; ORCiD logo [98]; ORCiD logo [28]; ORCiD logo [88]; ORCiD logo [98]; ORCiD logo [65]; ORCiD logo [98]; ORCiD logo [118]; ORCiD logo [5]; ORCiD logo [119];  [37]; ORCiD logo [36]; ORCiD logo [120]; ORCiD logo [121]; ORCiD logo [77]; ORCiD logo [122]; ORCiD logo [28]; ORCiD logo [37]; ORCiD logo [33]; ORCiD logo [107]; ORCiD logo [123]; ORCiD logo [124]; ORCiD logo [28]; ORCiD logo [125];  [5]; ORCiD logo [126]; ORCiD logo [77]; ORCiD logo [127]; ORCiD logo [9]; ORCiD logo [9]; ORCiD logo [2]; ORCiD logo [128]; ORCiD logo [129]; ORCiD logo [4]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [130]; ORCiD logo [2]; ORCiD logo [9]; ORCiD logo [131]; ORCiD logo [132]; ORCiD logo [20]; ORCiD logo [92]; ORCiD logo [9]; ORCiD logo [20]; ORCiD logo [133]; ORCiD logo [134]; ORCiD logo [135]; ORCiD logo [2]; ORCiD logo [136]; ORCiD logo [66] « less
  1. Harvard-Smithsonian Ctr. Astrophys.; Nijmegen U., IMAPP; Baltimore, Space Telescope Sci.
  2. Bonn, Max Planck Inst., Radioastron.
  3. Boston U.
  4. Harvard U. (main); Harvard-Smithsonian Ctr. Astrophys.
  5. Arizona U., Astron. Dept. - Steward Observ.
  6. Harvard-Smithsonian Ctr. Astrophys.; Harvard U. (main)
  7. Granada U., Theor. Phys. Astrophys.
  8. MIT; Natl. Astron. Observ. of Japan; Harvard U. (main)
  9. Nijmegen U., IMAPP
  10. Valencia U., Astro. Astrophys.; Valencia U., IFIC
  11. Princeton U., PCTS; Baltimore, Space Telescope Sci.
  12. IAA, Granada; Bologna, Ist. Radioastronomia; Bonn, Max Planck Inst., Radioastron.
  13. Concepcion U.; Turku U.; Aalto U.
  14. MIT; Natl. Astron. Observ. of Japan; Frankfurt U.
  15. Perimeter Inst. Theor. Phys.; Waterloo U.; Waterloo U., IQC
  16. Tsung-Dao Lee Inst., Shanghai; Shanghai Jiaotong U.; Frankfurt U.
  17. Granada U., Theor. Phys. Astrophys.; Bonn, Max Planck Inst., Radioastron.
  18. UNAM, Morelia, Inst. Radioastron. Astrophys.; Mexico U., ICN
  19. Columbia U., Astron. Astrophys.; Flatiron Inst., New York; Nijmegen U., IMAPP
  20. Harvard-Smithsonian Ctr. Astrophys.
  21. Shanghai, Astron. Observ.; Nanjing U. Sci. Tech.; Bonn, Max Planck Inst., Radioastron.
  22. IAA, Granada
  23. Malaya U.
  24. Harvard U. (main); Harvard-Smithsonian Ctr. Astrophys.; Texas U., San Antonio
  25. Academia Sinica, Taiwan
  26. Valencia U., Astro. Astrophys.; Valencia U., IFIC; Bonn, Max Planck Inst., Radioastron.
  27. Yale Ctr. Astron. Astrophys.
  28. MIT
  29. Illinois U., Urbana
  30. Fermilab; Chicago U., Astron. Astrophys. Ctr.
  31. Subaru Telescope
  32. Leiden Observ.
  33. Caltech
  34. East Asian Observ.; Hawaii U.
  35. McGill U.
  36. IRAM, St. Martin d'Heres
  37. Massachusetts U., Amherst
  38. KASI, DaeJeon; KAIST, Taejon
  39. Chicago U., KICP; Chicago U., Astron. Astrophys. Ctr.; Chicago U.; Chicago U., EFI
  40. Chalmers U. Tech.
  41. Cornell U., Radio. Space Res. Ctr.
  42. East Asian Observ.
  43. Shanghai, Astron. Observ.; Nanjing U. Sci. Tech.
  44. Fairfield U.
  45. Illinois U., Urbana, Astron. Dept.; Harvard-Smithsonian Ctr. Astrophys.
  46. Chicago U., Astron. Astrophys. Ctr.; Chicago U., KICP
  47. Frankfurt U.
  48. Natl. Astron. Observ. of Japan; Tokyo, Grad. U. Adv. Stud.
  49. Naples U.; Frankfurt U.; INFN, Naples
  50. U. Witwatersrand, Johannesburg, Sch. Phys.; Pretoria U.; Rhodes U.
  51. Subaru Telescope; ASTRON, Dwingeloo
  52. LESIA, Meudon
  53. Colorado U.
  54. IRAM, St. Martin d'Heres; Bonn, Max Planck Inst., Radioastron.
  55. NAOC, Beijing; Bonn, Max Planck Inst., Radioastron.
  56. Las Cumbres Observ.; UC, Santa Barbara
  57. NRAO, Charlottesville
  58. MIT; Google Inc.
  59. U. Wurzburg (main); Frankfurt U.; Bonn, Max Planck Inst., Radioastron.
  60. Harvard U. (main); Harvard U.; Harvard U., Phys. Dept.
  61. Illinois U., Urbana; Illinois U., Urbana, Astron. Dept.
  62. Waterloo U.; Waterloo U., IQC; Perimeter Inst. Theor. Phys.
  63. Cagliari U.; Cagliari Observ.
  64. Southern Denmark U., CP3-Origins; Frankfurt U.
  65. INAOE, Puebla; Conacyt, Mexico
  66. Shanghai, Astron. Observ.
  67. Kapteyn Astron. Inst., Groningen
  68. Peking U.; Peking U., Beijing, KIAA
  69. Academia Sinica, Taiwan; Subaru Telescope
  70. Natl. Astron. Observ. of Japan; Tokyo, Grad. U. Adv. Stud.; Tokyo U.
  71. INAOE, Puebla
  72. Natl. Astron. Observ. of Japan; Tokyo, Inst. Statistical Math.; Tokyo U., IPMU
  73. Leiden Observ.; NRAO, Charlottesville
  74. Unlisted, US, MA
  75. Perimeter Inst. Theor. Phys.; Waterloo U.
  76. Tokyo U., ICRR
  77. ASTRON, Dwingeloo
  78. Subaru Telescope; KASI, DaeJeon; Bonn, Max Planck Inst., Radioastron.
  79. KASI, DaeJeon
  80. Arizona U., Astron. Dept. - Steward Observ.; Caltech
  81. Natl. Astron. Observ. of Japan; Kogakuin U.
  82. Natl. Astron. Observ. of Japan; Tokyo U.
  83. Niigata U.
  84. Taiwan, Natl. Normal U.; Taiwan, Natl. Taiwan U.; Academia Sinica, Taiwan
  85. Hong Kong, Chinese U.
  86. Nanjing U., Dept. Astron.
  87. Nijmegen U., IMAPP; Harvard-Smithsonian Ctr. Astrophys.; IAA, Granada; Bologna, Ist. Radioastronomia; Bonn, Max Planck Inst., Radioastron.
  88. Bologna Observ.
  89. Academia Sinica, Taiwan; Taiwan, Natl. Taiwan U.
  90. Subaru Telescope; Yunnan Observ.; NAOC, Beijing
  91. Bologna Observ.; Bonn, Max Planck Inst., Radioastron.
  92. U. Amsterdam, GRAPPA
  93. Princeton, Inst. Advanced Study; Arizona U., Astron. Dept. - Steward Observ.
  94. ESTEC, Noordwijk; Chicago U., Astron. Astrophys. Ctr.
  95. Nijmegen U., IMAPP; Harvard-Smithsonian Ctr. Astrophys.; Tsung-Dao Lee Inst., Shanghai; Shanghai Jiaotong U.; Frankfurt U.
  96. Bonn, Max Planck Inst., Radioastron.; Nijmegen U., IMAPP
  97. U. Amsterdam, GRAPPA; Nijmegen U., IMAPP
  98. IRAM, Granada
  99. Illinois U., Urbana, Astron. Dept.
  100. Concepcion U.
  101. Hachinohe Inst. Tech.; Academia Sinica, Taiwan
  102. U. Witwatersrand, Johannesburg, Sch. Phys.; South African Astron. Observ.
  103. Frankfurt U.; Athens U.
  104. Villanova U.
  105. Washington U., St. Louis
  106. Sejong U.
  107. Natl. Astron. Observ. of Japan
  108. Academia Sinica, Taiwan; Perimeter Inst. Theor. Phys.; Canadian Inst. Theor. Astrophys.; Toronto U., Astron. Dept.; Canadian Inst. Advanced Res.
  109. UC, Berkeley
  110. U. Amsterdam, GRAPPA; Frankfurt U.
  111. University Coll., Cork; Bonn, Max Planck Inst., Radioastron.
  112. Perimeter Inst. Theor. Phys.
  113. Taiwan, Natl. Normal U.; Academia Sinica, Taiwan
  114. Gemini Observ., Hilo; Subaru Telescope
  115. Frankfurt U.; Frankfurt U., FIAS; Trinity Coll., Dublin
  116. Princeton U., Astrophys. Sci. Dept.; Flatiron Inst., New York
  117. Harvard-Smithsonian Ctr. Astrophys.; Harvard U. (main); Nijmegen U., IMAPP
  118. Natl. Astron. Observ. of Japan; Hiroshima U.
  119. Aalto U.; Bonn, Max Planck Inst., Radioastron.
  120. Peking U., Beijing, KIAA; Bonn, Max Planck Inst., Radioastron.
  121. Subaru Telescope; Shanghai, Astron. Observ.; Nanjing U. Sci. Tech.
  122. Subaru Telescope; KASI, DaeJeon; KAIST, Taejon; Yonsei U.
  123. Texas Tech. U., Lubbock; Baltimore, Space Telescope Sci.
  124. Nijmegen U., IMAPP; Leiden Observ.; NWO, The Hague; Arizona U., Astron. Dept. - Steward Observ.
  125. Bonn, Max Planck Inst., Radioastron.; IRAM, Granada
  126. Seoul Natl. U.; Subaru Telescope
  127. ASTRON, Dwingeloo; Leiden Observ.; New Mexico U.
  128. Central Lancashire U.
  129. Brandeis U.
  130. Tuorla Observ.
  131. Princeton, Inst. Advanced Study; Princeton U.
  132. Subaru Telescope; Hua-Zhong U. Sci. Tech.
  133. Mullard Space Sci. Lab.; Frankfurt U.
  134. Subaru Telescope; Shanghai, Astron. Observ.; Beijing, GUCAS
  135. Subaru Telescope; Hefei, CUST
  136. Bard Coll.

The blazar J1924–2914 is a primary Event Horizon Telescope (EHT) calibrator for the Galactic center’s black hole Sagittarius A*. Here we present the first total and linearly polarized intensity images of this source obtained with the unprecedented 20 μas resolution of the EHT. J1924–2914 is a very compact flat-spectrum radio source with strong optical variability and polarization. In April 2017 the source was observed quasi-simultaneously with the EHT (April 5–11), the Global Millimeter VLBI Array (April 3), and the Very Long Baseline Array (April 28), giving a novel view of the source at four observing frequencies, 230, 86, 8.7, and 2.3 GHz. These observations probe jet properties from the subparsec to 100 pc scales. We combine the multifrequency images of J1924–2914 to study the source morphology. We find that the jet exhibits a characteristic bending, with a gradual clockwise rotation of the jet projected position angle of about 90° between 2.3 and 230 GHz. Linearly polarized intensity images of J1924–2914 with the extremely fine resolution of the EHT provide evidence for ordered toroidal magnetic fields in the blazar compact core.

Research Organization:
INFN, Naples; LESIA, Meudon; IRAM, Granada; Chicago U., EFI; UNAM, Morelia, Inst. Radioastron. Astrophys.; Peking U.; Yale Ctr. Astron. Astrophys.; ASTRON, Dwingeloo; University Coll., Cork; Harvard-Smithsonian Ctr. Astrophys.; Hefei, CUST; U. Wurzburg (main); ESTEC, Noordwijk; Nijmegen U., IMAPP; Canadian Inst. Theor. Astrophys.; Naples U.; Fairfield U.; Hachinohe Inst. Tech.; Mullard Space Sci. Lab.; NAOC, Beijing; NWO, The Hague; Princeton, Inst. Advanced Study; KAIST, Taejon; Baltimore, Space Telescope Sci.; INAOE, Puebla; Gemini Observ., Hilo; Granada U., Theor. Phys. Astrophys.; Natl. Astron. Observ. of Japan; Colorado U.; Flatiron Inst., New York; Princeton U., PCTS; Canadian Inst. Advanced Res.; South African Astron. Observ.; Central Lancashire U.; Toronto U., Astron. Dept.; Seoul Natl. U.; Peking U., Beijing, KIAA; Sejong U.; Niigata U.; Athens U.; Illinois U., Urbana, Astron. Dept.; Texas U., San Antonio; Frankfurt U., FIAS; Harvard U. (main); Valencia U., Astro. Astrophys.; Academia Sinica, Taiwan; Hong Kong, Chinese U.; Tokyo, Inst. Statistical Math.; Taiwan, Natl. Normal U.; Chicago U.; Illinois U., Urbana; Turku U.; Boston U.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Princeton U., Astrophys. Sci. Dept.; Mexico U., ICN; Kapteyn Astron. Inst., Groningen; Hua-Zhong U. Sci. Tech.; Perimeter Inst. Theor. Phys.; NRAO, Charlottesville; Cagliari Observ.; McGill U.; Texas Tech. U., Lubbock; Tsung-Dao Lee Inst., Shanghai; Las Cumbres Observ.; Massachusetts U., Amherst; Kogakuin U.; Brandeis U.; Waterloo U.; Tokyo, Grad. U. Adv. Stud.; Trinity Coll., Dublin; Bonn, Max Planck Inst., Radioastron.; Valencia U., IFIC; Southern Denmark U., CP3-Origins; Princeton U.; Shanghai Jiaotong U.; Washington U., St. Louis; Leiden Observ.; UC, Santa Barbara; Chalmers U. Tech.; U. Witwatersrand, Johannesburg, Sch. Phys.; Yonsei U.; IRAM, St. Martin d'Heres; Bologna, Ist. Radioastronomia; Pretoria U.; MIT; U. Amsterdam, GRAPPA; Nanjing U. Sci. Tech.; Waterloo U., IQC; Beijing, GUCAS; Chicago U., Astron. Astrophys. Ctr.; UC, Berkeley; Tuorla Observ.; Yunnan Observ.; New Mexico U.; Malaya U.; Hiroshima U.; Nanjing U., Dept. Astron.; Villanova U.; Taiwan, Natl. Taiwan U.; Caltech; Rhodes U.; Bard Coll.; Hawaii U.; Conacyt, Mexico; Chicago U., KICP; Tokyo U.; Google Inc.; Bologna Observ.; Subaru Telescope; KASI, DaeJeon; Aalto U.; IAA, Granada; Harvard U.; Concepcion U.; Columbia U., Astron. Astrophys.; Cornell U., Radio. Space Res. Ctr.; Unlisted, US, MA; East Asian Observ.; Tokyo U., IPMU; Shanghai, Astron. Observ.; Tokyo U., ICRR; Harvard U., Phys. Dept.; Cagliari U.; Frankfurt U.; Arizona U., Astron. Dept. - Steward Observ.
Sponsoring Organization:
US Department of Energy
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1885020
Report Number(s):
FERMILAB-PUB-22-653-PPD; oai:inspirehep.net:2132004; arXiv:2208.01662
Journal Information:
Astrophys.J., Journal Name: Astrophys.J. Vol. 934
Country of Publication:
United States
Language:
English