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Draft:Anna Trindade Falcão

  • Comment: Well done on creating the draft, and it may potentially meet the relevant requirements (including WP:GNG, WP:ANYBIO, WP:NPROF) but presently it is not clear that it does.
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  • Comment: Has the subject held a distinguished professor or a named chair appointment? --Johannes (Talk) (Contribs) (Articles) 18:39, 28 October 2024 (UTC)
Anna Trindade Falcão
Born1995 (age 28–29)
Belo Horizonte, Brazil
Alma materThe Catholic University of America
Scientific career
FieldsAstrophysics, Astronomy
  • Supermassive Black holes
  • Active Galactic Nuclei
  • Low-redshift galaxies
  • Dual AGN
  • Galaxy formation
Institutions
  • Harvard-Smithsonian Center for Astrophysics
  • NASA Goddard Space Flight Center
Websitewww.annatrindadefalcao.com

Anna Trindade Falcão is a Brazilian astrophysicist and science educator, currently based at the Harvard-Smithsonian Center for Astrophysics..[1], in Cambridge, Massachusetts. She is best known for her contributions to the study of supermassive black holes and active galactic nuclei (AGN), with a particular focus on the interaction between active supermassive black holes and their host galaxies[2][3].

One of her major contributions is the discovery of the closest known candidate for a dual supermassive black hole pair, identified through multi-wavelength observations[4][5]. Alongside her research, Trindade Falcão actively participates in science education, regularly engaging in public talks to promote astronomy and science[6][7].

Education and Career

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Anna Trindade Falcão was born in 1995 in Belo Horizonte, a region in the southeastern part of Brazil. She earned her B.Sc. in Physics from the Universidade Federal de Minas Gerais in 2017. She later completed both her M.Sc. and Ph.D. in Physics and Astrophysics at the Catholic University of America in Washington, D.C., graduating in 2022. After completing her Ph.D., she joined the Harvard-Smithsonian Center for Astrophysics as a postdoctoral researcher[8].

Her research primarily focuses on AGN and their influence on galaxy formation and evolution. In 2023, Anna Trindade Falcão became part of the science team for NASA’s Advanced X-ray Imaging Satellite (AXIS), a high-resolution X-ray telescope under development for a 2032 launch[9]. The AXIS mission aims to provide deeper insights into AGN feedback mechanisms, dual AGNs, and the high-redshift universe[10] In July 2025, Anna Trindade Falcão will join NASA’s Goddard Space Flight Center (GSFC) as a NASA Postdoctoral Program Fellow, where she will continue her work on AGN and supermassive black holes.

Scientific Contributions

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Anna Trindade Falcão is best known for her contributions to observational astrophysics, specifically in the study of active supermassive black holes and AGN feedback mechanisms in the local Universe. Her research has explored the interplay between AGN outflows and galaxy formation, focusing on the effects of black hole activity on their surrounding environments. In 2022, she developed an innovative technique for measuring the kinematics of extended X-ray-emitting gas using optical and near-infrared emission lines[11]. Two years later, in 2024, she led a team that discovered the closest pair of active supermassive black holes in the local Universe, using data from the Hubble Space Telescope, the Chandra X-ray Observatory and the Very Large Array Telescope[12]

References

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  1. ^ "Anna Trindade Falcão". cfa.harvard.edu. Retrieved 2024-10-24.
  2. ^ Trindade Falcão, Anna; Kraemer, Steve; Fischer, Travis; Schmitt, Henrique; Feuillet, Lea; Crenshaw, Mike; Revalski, Mitchell; Maksym, Peter; Vestergaard, Marianne; Elvis, Martin; Gaskell, Martin; Ho, Luis; Netzer, Hagai; Storchi-Bergmann, Thaisa; Turner, Jane; Ward, Martin (2024-10-22). "Hubble Space Telescope Observations of Nearby Type 1 Quasars. I. Characterisation of the Extended [O III] 5007Å Emission". Monthly Notices of the Royal Astronomical Society. arXiv:2410.16053. doi:10.1093/mnras/stae2412.
  3. ^ Trindade Falcão, Anna; Kraemer, Steve; Fischer, Travis; Crenshaw, Mike; Revalski, Mitchell; Schmitt, Henrique; Vestergaard, Marianne; Elvis, Martin; Gaskell, Martin; Hamann, Fred; Ho, Luis; Hutchings, John; Mushotzky, Richard; Netzer, Hagai; Storchi-Bergmann, Thaisa; Turner, Jane; Ward, Martin (2020-10-20). "Hubble Space Telescope observations of [O iii] emission in nearby QSO2s: physical properties of the ionized outflows". Monthly Notices of the Royal Astronomical Society. 500 (1): 1491–1504. arXiv:2010.08050. doi:10.1093/mnras/staa3239.
  4. ^ Trindade Falcão, Anna (2024-09-09). "NASA's Hubble, Chandra Find Supermassive Black Hole Duo". NASA. Retrieved 2024-10-24.
  5. ^ Trindade Falcão, Anna; Turner, Jane; Kraemer, Steve; Reeves, James; Braito, Valentina; Schmitt, Henrique; Feuillet, Lea (2024-09-09). "Resolving a Candidate Dual Active Galactic Nucleus with ∼100 pc Separation in MCG-03-34-64". The Astrophysical Journal. 972 (1): 185. arXiv:2403.07717. doi:10.3847/1538-4357/ad6b91.
  6. ^ "Dr. Anna Trindade Falcão of Harvard on Active Galactic Nuclei (AGN)". YouTube. 20 September 2024.
  7. ^ "Ao vivo | Brasileira faz história no estudo de buracos negros! | 20/09/2024". YouTube. 21 September 2024.
  8. ^ "Anna Trindade Falcão". cfa.harvard.edu. Retrieved 2024-10-24.
  9. ^ Reynolds, Christopher; et al. (1 Nov 2023). "Overview of the advanced x-ray imaging satellite (AXIS)". In Siegmund, Oswald H.; Hoadley, Keri (eds.). UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXIII. p. 49. arXiv:2311.00780. doi:10.1117/12.2677468. ISBN 978-1-5106-6570-5. {{cite book}}: Unknown parameter |DUPLICATE_first38= ignored (help)
  10. ^ AXIS home page
  11. ^ Trindade Falcão, Anna; Kraemer, Steve; Crenshaw, Mike; Melendez, Marcio; Revalski, Mitchell; Fischer, Travis; Schmitt, Henrique; Turner, Jane (2022-01-27). "Tracking X-ray outflows with optical/infrared footprint lines". Monthly Notices of the Royal Astronomical Society. 511 (1): 1420–1430. arXiv:2410.16053. doi:10.1093/mnras/stac173.
  12. ^ Trindade Falcão, Anna (2024-09-09). "NASA's Hubble, Chandra Find Supermassive Black Hole Duo". NASA. Retrieved 2024-10-24.
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