<?xml version="1.0" encoding="UTF-8"?>
<rdf:RDF xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns="http://purl.org/rss/1.0/" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:taxo="http://purl.org/rss/1.0/modules/taxonomy/" xmlns:sy="http://purl.org/rss/1.0/modules/syndication/">
<channel>
<title>Mathematical Sciences</title>
<link>http://hdl.handle.net/123456789/1</link>
<description/>
<items>
<rdf:Seq>
<rdf:li resource="http://hdl.handle.net/123456789/5832"/>
<rdf:li resource="http://hdl.handle.net/123456789/5828"/>
<rdf:li resource="http://hdl.handle.net/123456789/5817"/>
<rdf:li resource="http://hdl.handle.net/123456789/5816"/>
</rdf:Seq>
</items>
</channel>
<item rdf:about="http://hdl.handle.net/123456789/5832">
<title>OPTI ˇCKA DETEKCIJA OSTATAKA SUPERNOVIH I UTICAJ NJIHOVE EMISIJE U LINIJI Hα NA ODREDIVANJE STOPE FORMIRANJA ZVEZDA</title>
<link>http://hdl.handle.net/123456789/5832</link>
<description>OPTI ˇCKA DETEKCIJA OSTATAKA SUPERNOVIH I UTICAJ NJIHOVE EMISIJE U LINIJI Hα NA ODREDIVANJE STOPE FORMIRANJA ZVEZDA

Vučetić, Milica

In this dissertation we discuss in uence of H emission from supernova remnants&#13;
(SNRs) on H derived star formation rates (SFRs). We present the detection of 16&#13;
optical SNR candidates in a part of nearby spiral galaxy IC342, and two more poten-&#13;
tial SNRs in NGC 185 galaxy. The candidates were detected by applying [S ii]/H&#13;
ratio criterion on observations made with the 2 m telescope at Rozhen National&#13;
Astronomical Observatory in Bulgaria. Also, in this dissertation we present the&#13;
most up-to-date list of nearby galaxies with optically detected SNRs. When deri-&#13;
ving H star formation rates, assumption is that the radiation is coming from the&#13;
ionized gas surrounding hot and young stars { H ii regions. In this case, emission&#13;
from SNRs contaminates H ux used to derive SFR. We found that the contribu-&#13;
tion of SNRs' ux to the total H ux, for 18 galaxies in our sample of galaxies&#13;
with optical SNRs, is 5   5%. Due to the observational selection effects, the SNR&#13;
contamination of SFRs derived herein represents only a lower limit. M83 is the&#13;
galaxy with the most detected optical SNRs and in this galaxy SNRs account for&#13;
9 per cent of the total H emission. We expect that fraction similar to this would&#13;
be close to the real contribution of SNR emission to the total H emission in spiral&#13;
galaxies.&#13;
Using two dwarf galaxies as an example, Holmberg IX and NGC 185, we show&#13;
that the contamination of H ux by SNRs, or other sources, can be much larger,&#13;
up to ten times higher than total H ux coming from H ii regions of the observed&#13;
galaxy.

</description>
</item>
<item rdf:about="http://hdl.handle.net/123456789/5828">
<title>POLINOMIJALNA ENTROPIJA INDUKAOVANIH DINAMIČKIH SISTEMA NA HIPERPROSTORIMA</title>
<link>http://hdl.handle.net/123456789/5828</link>
<description>POLINOMIJALNA ENTROPIJA INDUKAOVANIH DINAMIČKIH SISTEMA NA HIPERPROSTORIMA

Đorić, Maša

In this thesis, we applied a method for computing the polynomial entropy of&#13;
dynamical systems with a finite non-wandering set to certain hyperspaces of the interval and&#13;
the circle. We subsequently generalized these results to the case where the non-wandering&#13;
set is not finite. We proved that the polynomial entropy of the induced map C(f ) is equal&#13;
to 2, that of Fn(f ) is equal to n, and that of 2f is infinite, when f is a homeomorphism of&#13;
the interval or the circle. Furthermore, we generalized these results for the n-fold symmetric&#13;
product of the interval and the circle to an arbitrary compact metric space X and extended&#13;
them to the suspension of the space Fn(X). In addition to the results on hyperspaces, we&#13;
presented results concerning polynomial entropy on certain one-dimensional continua, such&#13;
as local dendrites and regular curves. We also constructed a family of pointwise periodic&#13;
homeomorphisms on a continuum whose polynomial entropy attains every value in [0, +∞].

</description>
</item>
<item rdf:about="http://hdl.handle.net/123456789/5817">
<title>XI SERBIAN CONFERENCE ON SPECTRAL LINE SHAPES IN ASTROPHYSICS, Book of abstracts</title>
<link>http://hdl.handle.net/123456789/5817</link>
<description>XI SERBIAN CONFERENCE ON SPECTRAL LINE SHAPES IN ASTROPHYSICS, Book of abstracts

Kovačević, Anđelka

Simić, Saša

</description>
</item>
<item rdf:about="http://hdl.handle.net/123456789/5816">
<title>Novel goodness-of-fit tests based on independence-type characterizations</title>
<link>http://hdl.handle.net/123456789/5816</link>
<description>Novel goodness-of-fit tests based on independence-type characterizations

Halaj Mileusnić, Katarina

The main objective of this dissertation is to develop novel goodness-of-&#13;
fit tests based on independence characterizations and to investigate their proper-&#13;
ties. The starting point is the fact that certain distributions can be uniquely char-&#13;
acterized by the independence of suitable functions of random variables. This&#13;
observation makes it possible to reduce goodness-of-fit testing for a hypothe-&#13;
sized model to the problem of detecting departures from the corresponding in-&#13;
dependence condition. Accordingly, the proposed test statistics are constructed&#13;
by comparing empirical versions of joint functionals with the product of the cor-&#13;
responding marginal functionals, where the resulting discrepancy serves as the&#13;
basis for new goodness-of-fit tests for different classes of distributions.&#13;
One of the contributions of the dissertation is the development of goodness-&#13;
of-fit tests for the geometric distribution based on Ferguson’s independence char-&#13;
acterization. In this setting, the general framework of comparing joint and&#13;
marginal empirical functionals is implemented through V-empirical probability&#13;
generating functions. Furthermore, a novel approach to goodness-of-fit testing&#13;
for absolutely continuous distributions is proposed, relying on the discrepancy&#13;
between the joint U-empirical distribution function of an appropriately defined&#13;
random vector and the product of its marginal U-empirical distribution func-&#13;
tions. Another part of the research focuses on circular data. A goodness-of-fit test&#13;
for the wrapped normal distribution is proposed, where the general methodology&#13;
is adapted to the periodic structure of observations on the circle.&#13;
The theoretical part of the dissertation is devoted to the derivation of the&#13;
asymptotic properties of the proposed test statistics, drawing on the theory of&#13;
U- and V- statistics as well as on the theory of U-empirical processes. An addi-&#13;
tional contribution is the establishment of new asymptotic results for finite linear&#13;
combinations of weakly degenerate V-statistics, both in settings with known pa-&#13;
rameters and in settings involving parameter estimation. These findings provide&#13;
the theoretical foundation for a class of combined tests in which appropriately&#13;
chosen weights regulate the contribution of individual components and can be&#13;
used to enhance the overall efficiency of the testing procedure.&#13;
The practical performance of the proposed methods will be assessed through&#13;
extensive simulation studies and the analysis of several real data sets. The sim-&#13;
ulation study will investigate the finite-sample properties of the tests under the&#13;
null hypothesis and a range of relevant alternatives, while the real-data applica-&#13;
tions will demonstrate their usefulness in practical statistical problems. In this&#13;
way, the empirical part of the dissertation will complement the theoretical de-&#13;
velopments and provide evidence of the practical applicability of the proposed&#13;
methodologies.

</description>
</item>
</rdf:RDF>
