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); Institute for Research in Fundamental Sciences (2019–2026); University of Florence (2019–2024)
Postdoc Researcher
Research Areas
Links
Biography and Research Information
OverviewAI-generated summary
Amirnezam Amiri investigates the physical and chemical processes within the early Universe and the characteristics of active galactic nuclei (AGN). His work utilizes observational data from instruments like the James Webb Space Telescope (JWST) to measure metallicity in distant galaxies and to understand the diffuse ionized gas in star-forming regions. Amiri also studies multiple AGN systems with small angular separations, confirming candidates selected through novel methods and analyzing feedback and ionized gas outflows in low-radio power AGN. He has contributed to the development of new computational tools for photoionization modeling (HOMERUN) and 3D gas kinematic modeling (MOKA3D). Amiri's research network includes collaborations with Rafael T. Eufrasio, with whom he has co-authored four publications.
Metrics
- h-index: 10
- Publications: 80
- Citations: 594
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
- 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
- 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
Showing 5 of 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
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
Showing 5 of 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
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
Showing 5 of 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
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
Showing 5 of 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
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
Showing 5 of 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
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
Showing 5 of 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
- 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
- MIRACLE
Showing 5 of 8 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
- MIRACLE
Showing 5 of 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
- 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
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
- MUSE adaptive-optics spectroscopy confirms dual active galactic nuclei and strongly lensed systems at sub-arcsec separation
Showing 5 of 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
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
- MIRACLE
Showing 5 of 7 shared publications
- Feedback and ionized gas outflows in four low-radio power AGN at <i>z</i> ∼ 0.15
- MOKA<sup>3D</sup>: An innovative approach to 3D gas kinematic modelling
- 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
- MIRACLE
Showing 5 of 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
- HOMERUN a new approach to photoionization modelling. I -- reproducing observed emission lines with percent accuracy and obtaining accurate physical properties of the ionized gas
- Stripped and enriched: the role of ram–pressure in shaping chemical enrichment of galaxies at intermediate redshift
Showing 5 of 6 shared publications
- HOMERUN: A new approach to photoionization modeling
- 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
- 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