Cite

Papers describing the method and the data, from the most recent to the oldest. Open a card to see its details, the BibTeX and the first page.

CiteDevelopment paper: cite this if you mention results from its content.
#1 · Journal article

Extinction by non-spherical particles with the Nanoparticle Transition Matrix Code: Perspectives for interstellar medium and exoplanetary atmospheres

Extinction by non-spherical particles with the Nanoparticle Transition Matrix Code: Perspectives for interstellar medium and exoplanetary atmospheres

G. La Mura, G. Mulas, M. A. Iatì, C. Cecchi-Pestellini, G. Aresu, S. Rezaei, R. Saija

Journal of Quantitative Spectroscopy and Radiative Transfer · vol. 367, article 110167 · February 2027
Also on arXiv: arXiv:2610.17081

DOI arXiv ADS

BibTeX
@article{LaMura2027,
  author = {La Mura, G. and Mulas, G. and Iatì, M. A. and Cecchi-Pestellini, C. and Aresu, G. and Rezaei, S. and Saija, R.},
  title = {{Extinction by non-spherical particles with the Nanoparticle Transition Matrix Code: Perspectives for interstellar medium and exoplanetary atmospheres}},
  journal = {Journal of Quantitative Spectroscopy and Radiative Transfer},
  volume = {367},
  pages = {110167},
  year = {2027},
  doi = {10.1016/j.jqsrt.2026.110167},
  eprint = {2610.17081},
  archivePrefix = {arXiv},
}
First page of: Extinction by non-spherical particles with the Nanoparticle Transition Matrix Code: Perspectives for interstellar medium and exoplanetary atmospheres First page · arXiv version
CiteCite this paper if you use the data for forsterite, spinel and/or silicon monoxide (SiO).
#2 · Preprint

The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres

The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres

G. Aresu, G. La Mura, G. Mulas, C. Cecchi-Pestellini, M. A. Iatì, S. Rezaei, A. Petralia, D. Locci, G. Micela, F. Saija, R. Saija

arXiv preprint · arXiv:2610.28117 · 20 October 2026

Accepted for publication in ApJ

arXiv ADS

BibTeX
@misc{Aresu2026,
  author = {Aresu, G. and La Mura, G. and Mulas, G. and Cecchi-Pestellini, C. and Iatì, M. A. and Rezaei, S. and Petralia, A. and Locci, D. and Micela, G. and Saija, F. and Saija, R.},
  title = {{The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres}},
  year = {2026},
  eprint = {2610.28117},
  archivePrefix = {arXiv},
  note = {Accepted for publication in ApJ},
}
Why

It presents the absorption and scattering cross sections of these three species for particles of different sizes and shapes, from compact ensembles of spheres to porous aggregates, and it is the reference for the data deposited on Zenodo.

First page of: The T-matrix method for modeling the optical properties of grains in exoplanetary atmospheres First page · arXiv version
CiteCite this paper whenever you use any data from this database.
#3 · Journal article

Nano-particle Transition Matrix code implementation

Nano-particle Transition Matrix code implementation

G. La Mura, G. Mulas, G. Aresu, M. A. Iatì, C. Cecchi-Pestellini, S. Rezaei, R. Saija

Astronomy and Computing · vol. 55, article 101077 · April 2026
Also on arXiv: arXiv:2602.05520

DOI arXiv ADS

BibTeX
@article{LaMura2026,
  author = {La Mura, G. and Mulas, G. and Aresu, G. and Iatì, M. A. and Cecchi-Pestellini, C. and Rezaei, S. and Saija, R.},
  title = {{Nano-particle Transition Matrix code implementation}},
  journal = {Astronomy and Computing},
  volume = {55},
  pages = {101077},
  year = {2026},
  doi = {10.1016/j.ascom.2026.101077},
  eprint = {2602.05520},
  archivePrefix = {arXiv},
}
Why

It presents NP_TMcode, the T-matrix code that computed every cross section in the database, so it credits the method behind all of the data.

First page of: Nano-particle Transition Matrix code implementation First page · arXiv version