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Current · Arkansas
Last published
2026
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OpenAlex · ORCID
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2026-10-05
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Amirnezam Amiri
Affiliation confirmed via AI analysis of OpenAlex, ORCID, and web sources.
Postdoctoral Associate Reasearcher
Also affiliated: Universidad de La Laguna (2023); Kharazmi University (2019–2021); Arcetri Astrophysical Observatory (2019–2024); Instituto de Astrofísica de Canarias (2023–2025); Istituto Nazionale di Fisica Nucleare, Sezione di Firenze (2023); Institute for Research in Fundamental Sciences (2019–2026); University of Florence (2019–2024); National Institute for Astrophysics (2019–2023)
10 h-index
68 pubs
608 cited
Research Areas
Links
Biography and Research Information
OverviewAI-generated summary
Amirnezam Amiri's research primarily focuses on the study of active galactic nuclei (AGN) and the chemical enrichment of the early universe, utilizing data from instruments such as the James Webb Space Telescope (JWST). His work investigates phenomena like galaxy-scale ionized winds driven by ultra-fast outflows in nearby quasars, and the diffuse ionized gas (DIG) in star-forming galaxies. Amiri has also explored new methods for identifying and confirming multiple AGN systems with small separations, including dual and lensed AGNs, through techniques like the GMP method and advanced spectroscopic analysis. His publications include research on feedback mechanisms and ionized gas outflows in low-radio power AGN, as well as the development of new approaches to photoionization modeling, such as HOMERUN. Amiri has a publication record of 83 papers with 606 citations and an h-index of 10. He has collaborated with Rafael T. Eufrasio and Ali Amiri on multiple publications.
Metrics
- h-index: 10
- Publications: 68
- Citations: 608
Positions
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Postdoctoral Associate Reasearcher 2023–presentUniversity of Arkansas Physics ORCID
Selected Publications
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Uncovering the multi-scale structure of dust distribution in nearby galaxies (2026)
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MAUVE–MUSE: Ionization and Kinematic Signatures of Environmental Effects on Virgo Cluster Disks (2026)
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MAUVE–MUSE: when metallicity follows or fights star formation – a mass-dependent inversion in Virgo galaxies (2026)
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The PHANGS-H <i>α</i> survey (2026)
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Dyson Spheres on H–R Diagram (2026)
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Surveying the Whirlpool at Arcseconds with NOEMA (SWAN) (2026)
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Tracing nitrogen enrichment across cosmic time with JWST (2026)
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MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at <i>z</i> ∼ 2 (2026)
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MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at <i>z</i> ∼ 2 (2026)
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lightning.py: Python SED Fitting Code (2025)
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lightning.py: Python SED Fitting Code (2025)
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M <sup>3</sup> D: Mosaicking M33 with MUSE datacubes (2025)
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Duration and properties of the embedded phase of star formation in 37 nearby galaxies from PHANGS-JWST (2025)
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PHANGS-JWST: The largest extragalactic molecular cloud catalog traced by polycyclic aromatic hydrocarbon emission (2025)
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PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies (2025)
Collaboration Network
Top Collaborators
Francesco Belfiore
Arcetri Astrophysical Observatory (IT)
13 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
Showing 5 of 13 shared publications
A. Marconi
Arcetri Astrophysical Observatory (IT)
12 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
Showing 5 of 12 shared publications
F. Mannucci
Arcetri Astrophysical Observatory (IT)
10 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
Showing 5 of 10 shared publications
G. Cresci
Arcetri Astrophysical Observatory (IT)
10 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
Showing 5 of 10 shared publications
M. Scialpi
University of Trento (IT)
9 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
Showing 5 of 9 shared publications
C. Marconcini
University of Zagreb (HR)
9 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
Showing 5 of 9 shared publications
M. Ginolfi
Arcetri Astrophysical Observatory (IT)
8 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- MIRACLE
Showing 5 of 8 shared publications
Giacomo Venturi
Scuola Normale Superiore (IT)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- MIRACLE
Showing 5 of 7 shared publications
E. Bertola
Arcetri Astrophysical Observatory (IT)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MIRACLE
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
Showing 5 of 7 shared publications
Stefano Carniani
Scuola Normale Superiore (IT)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
Showing 5 of 7 shared publications
Q. D’Amato
Arcetri Astrophysical Observatory (IT)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MIRACLE
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
Showing 5 of 7 shared publications
G. Tozzi
Max Planck Institute for Extraterrestrial Physics (DE)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- MIRACLE
Showing 5 of 7 shared publications
L. Ulivi
University of Trento (IT)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- GMP-selected dual and lensed AGNs: Selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, Keck/OSIRIS, and LBT/LUCI
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- MIRACLE
Showing 5 of 7 shared publications
Neven Tomičić
University of Zagreb (HR)
7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- HOMERUN: A new approach to photoionization modeling
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- Stripped and enriched: the role of ram–pressure in shaping chemical enrichment of galaxies at intermediate redshift
- HOMERUN a new approach to photoionization modelling. I -- reproducing observed emission lines with percent accuracy and obtaining accurate physical properties of the ionized gas
Showing 5 of 7 shared publications
Antonino Marasco
Osservatorio Astronomico di Padova (IT)
5 shared publications
- HOMERUN: A new approach to photoionization modeling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- HOMERUN a new approach to photoionization modelling. I -- reproducing observed emission lines with percent accuracy and obtaining accurate physical properties of the ionized gas