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20132015
most citedDeriving physical parameters of unresolved star clusters. I. Age, mass, and extinction degeneracies

36 citations · 84 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2015★ 8 cited

Deriving physical parameters of unresolved star clusters IV. The M33 star cluster system

P. de Meulenaer, D. Narbutis, T. Mineikis +1

Context. When trying to derive the star cluster physical parameters of the M33 galaxy using broad-band unresolved ground-based photometry, previous studies mainly made use of simpl…

astro-ph.GA2015★ 13 cited

Deriving physical parameters of unresolved star clusters III. Application to M31 PHAT clusters

Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1

This study is the third of a series that investigates the degeneracy and stochasticity problems present in the determination of physical parameters such as age, mass, extinction, a…

astro-ph.GA2014★ 2 cited

Deriving structural parameters of semi-resolved star clusters. FitClust: a program for crowded fields

D. Narbutis, D. Semionov, R. Stonkutė +4

Context. An automatic tool to derive structural parameters of semi-resolved star clusters located in crowded stellar fields in nearby galaxies is needed for homogeneous processing…

astro-ph.SR2014★ 25 cited

Deriving physical parameters of unresolved star clusters. II. The degeneracies of age, mass, extinction, and metallicity

Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1

This paper is the second of a series that investigates the stochasticity and degeneracy problems that hinder the derivation of the age, mass, extinction, and metallicity of unresol…

astro-ph.GA2013

Stochasticity effects on derivation of physical parameters of unresolved star clusters

Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1

We developed a method for a fast modeling of broad-band UBVRI integrated magnitudes of unresolved star clusters and used it to derive their physical parameters (age, mass, and exti…

astro-ph.GA2013★ 36 cited

Deriving physical parameters of unresolved star clusters. I. Age, mass, and extinction degeneracies

Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1

Context. Stochasticity and physical parameter degeneracy problems complicate the derivation of the parameters (age, mass, and extinction) of unresolved star clusters when using bro…