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Na voljo sta dva načina iskanja: enostavno in napredno. Enostavno iskanje išče po naslovu, opisu, ključnih besedah in celotnem besedilu in ne omogoča operatorjev iskanja. Pri naprednem iskanju lahko izbirate med množico atributov, po katerih naj išče in omogoča operatorje iskanja. V zadetkih iskanja so nekatere vrednosti izpisane v obliki povezav. Povezava na naslovu gradiva izpiše več o gradivu, ostale povezave sprožijo novo iskanje.

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21.
Performance of the Cherenkov Telescope Array
Ulisses Barres de Almeida, Christopher Eckner, Gašper Kukec Mezek, Samo Stanič, Serguei Vorobiov, Lili Yang, Gabrijela Zaharijas, Danilo Zavrtanik, Marko Zavrtanik, Lukas Zehrer, 2019, objavljeni znanstveni prispevek na konferenci

Opis: The Cherenkov Telescope Array (CTA) is expected to become the by far largest and most sensitive observatory for very-high-energy gamma rays in the energy range from 20 GeV to more than 300 TeV. CTA will be capable of detecting gamma rays from extremely faint sources with unprecedented precision on energy and direction. The performance of the future observatory derived from detailed Monte Carlo simulations is presented in this contribution for the two CTA sites located on the island of La Palma (Spain) and near Paranal (Chile). This includes the evaluation of CTA sensitivity over observations pointing towards different elevations and for operations at higher night-sky background light levels.
Ključne besede: very-high-energy gamma rays, the Cherenkov Telescope Array (CTA) Observatory, detector performances
Objavljeno v RUNG: 07.11.2024; Ogledov: 162; Prenosov: 4
.pdf Celotno besedilo (452,81 KB)
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22.
Massive stars exploding in a He-rich circumstellar medium - X : flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt
Z.-Y. Wang, A. Pastorello, K. Maeda, A. Reguitti, Y.-Z. Cai, D. Andrew Howell, S. Benetti, Mateusz Bronikowski, E. Concepcion, Tanja Petrushevska, 2024, izvirni znanstveni članek

Opis: We present optical and near-infrared observations of two Type Ibn supernovae (SNe), SN\,2018jmt and SN\,2019cj. Their light curves have rise times of about ten days, reaching an absolute peak magnitude of $M_g$(SN\,2018jmt) = $-$19.07 pm 0.37 and $M_V$(SN\,2019cj) = $-$18.94 pm 0.19 mag, respectively. The early-time spectra of SN\,2018jmt are dominated by a blue continuum, accompanied by narrow (600$-$1000 km $) He i lines with the P-Cygni profile. At later epochs, the spectra become more similar to those of the prototypical SN Ibn 2006jc. At early phases, the spectra of SN\,2019cj show flash ionisation emission lines of C iii N iii and He ii superposed on a blue continuum. These features disappear after a few days, and then the spectra of SN\,2019cj evolve similarly to those of SN\,2018jmt. The spectra indicate that the two SNe exploded within a He-rich circumstellar medium (CSM) lost by the progenitors a short time before the explosion. We modelled the light curves of the two SNe Ibn to constrain the progenitor and the explosion parameters. The ejecta masses are consistent with either what is expected for a canonical SN Ib (sim 2 odot $) or for a massive Wolf Rayet star ($>$ sim 4 M$_ odot $), with the kinetic energy on the order of $10^ $ erg. The lower limit on the ejecta mass ($>$ sim 2 M odot $) argues against a scenario involving a relatively low-mass progenitor (e.g. $M_ ZAMS $ sim 10 M$_ odot $). We set a conservative upper limit of sim 0.1 M$_ odot $ for the 56Ni masses in both SNe. From the light curve modelling, we determined a two-zone CSM distribution, with an inner, flat CSM component and an outer CSM with a steeper density profile. The physical properties of SN\,2018jmt and SN\,2019cj are consistent with those expected from the core collapse of relatively massive envelope-stripped stars.
Ključne besede: supernovae
Objavljeno v RUNG: 06.11.2024; Ogledov: 156; Prenosov: 3
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23.
Orientacijski dan Univerze v Novi Gorici v Vipavo privabil številne mlade
Veronika Piccinini, 2024, poljudni članek

Ključne besede: študij, univerze, visoko šolstvo
Objavljeno v RUNG: 05.11.2024; Ogledov: 167; Prenosov: 1
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Uvajanje novega izdelka na izbrani ciljni trg, primer teranov liker Srdelin : diplomsko delo
Rok Frančeškin, 2024, diplomsko delo

Opis: Domačija Srdelin iz Tomaja na Krasu ima bogato tradicijo v pridelovanju vinske sorte refošk, vina teran ter teranovega likerja. Bogato znanje v pridelavi se je uspešno prenašalo in nadgrajevalo iz generacije v generacijo, vse do današnjega časa, ko je domači pridelek teranov liker dosegel stopnjo dovršenosti v okusu in tehnologiji pridelave, da ga je mogoče ponuditi širši javnosti. Domačija Srdelin že prodaja svoje izdelke v obliki dopolnilne dejavnosti in jih v omejenih količinah že trži. Srdelinov liker se na trgu razlikuje po svoji dolgi tradiciji pridelave in inovativnosti okusov in postopka staranja. S posebnimi tehnikami proizvodnje se lahko pohvali z gladkejšo teksturo in intenzivnejšimi okusi. Diplomsko delo vsebuje strategijo prodaje teranovega likerja Srdelin za izbrani ciljni trg. Metodološki del diplomskega dela vsebuje podrobno opredelitev osnovnih pojmov. Podrobneje je opisan razvoj in uvajanje novih izdelkov na trg, predstavljen pa je tudi model razvojnega procesa po Kotlerju. V eksperimentalnem delu je podrobneje predstavljen izdelek in njegova pridelava. V tem delu je predstavljena analiza trga z obstoječimi izdelki in konkurenti domačije. Predstavljeni so ključni uporabniki teranovega likerja. Na tem področju je bila izvedena SWOT analiza, predstavljeni so profili ciljnega kupca (buyer persona) predstavljeni pa so še glavni elementi diverzifikacije izdelka.
Ključne besede: diplomske naloge, teranov liker, alkoholne pijače, kras, teran, likerji, domačija Srdelin
Objavljeno v RUNG: 05.11.2024; Ogledov: 149; Prenosov: 0
.pdf Celotno besedilo (570,12 KB)

26.
Harnessing in vitro selection opportunities for obtaining epitope-specific binders : lecture at the CDKL5 Forum 2024, Cambridge, MA, USA, 27 October 2024
Ario De Marco, 2024, prispevek na konferenci brez natisa

Ključne besede: CDKL5, nanobodies, biopanning
Objavljeno v RUNG: 05.11.2024; Ogledov: 149; Prenosov: 0
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27.
Łukasiewicz anti fuzzy subalgebras of BCK/BCI-algebras
Jeong Gi Kang, Hashem Bordbar, 2025, izvirni znanstveni članek

Opis: The subalgebra of BCK/BCI-algebra using Łukasiewicz anti fuzzy set introduced by Jun is studied in this article. The concept of Łukasiewicz anti fuzzy subalgebra of a BCK/BCI-algebra is introduced, and several properties are investigated. The relationship between anti fuzzy subalgebra and Łukasiewicz anti fuzzy subalgebra is given, and characterization of a Łukasiewicz anti fuzzy subalgebra is discussed. Conditions are found in which a Lukasiewicz anti fuzzy set is a Lukasiewicz anti fuzzy subalgebra Finally, conditions under which ⋖-subset, Υsubset, and anti-subset become subalgebra are explored.
Ključne besede: anti fuzzy subalgebra, Łukasiewicz anti fuzzy set, Łukasiewicz anti fuzzy, subalgebra, Υ-subset, anti subset
Objavljeno v RUNG: 30.10.2024; Ogledov: 283; Prenosov: 0
.pdf Celotno besedilo (406,85 KB)

28.
Spectroscopic analysis of the strongly lensed SN Encore : constraints on cosmic evolution of Type Ia supernovae
S. Dhawan, Justin Pierel, M. Gu, A. B. Newman, C. Larison, M. Siebert, Tanja Petrushevska, F. Poidevin, S. W. Jha, W. Chen, 2024, izvirni znanstveni članek

Opis: Abstract Strong gravitational lensing magnifies the light from a background source, allowing us to study these sources in detail. Here, we study the spectra of a z = 1.95 lensed Type Ia supernova SN Encore for its brightest Image A, taken 39 days apart. We infer the spectral age with template matching using the supernova identification (SNID) software and find the spectra to be at 29.0 ±5.0 and 37.4 ±2.8 rest-frame days post maximum respectively, consistent with separation in the observer frame after accounting for time-dilation. Since SNe Ia measure dark energy properties by providing relative distances between low- and high-z SNe, it is important to test for evolution of spectroscopic properties. Comparing the spectra to composite low-z SN Ia spectra, we find strong evidence for similarity between the local sample and SN Encore. The line velocities of common SN Ia spectral lines, Si II 6355 and Ca II NIR triplet are consistent with the distribution for the low-z sample as well as other lensed SNe Ia, e.g. iPTF16geu (z = 0.409)and SN H0pe (z = 1.78). The consistency between the low-z sample and lensed SNe at high-z suggests no obvious cosmic evolution demonstrating their using as high-z distance indicators, though this needs to be confirmed/refuted via a larger sample. We also find that the spectra of SN Encore match the predictions for explosion models very well. With future large samples of lensed SNe Ia e.g. with the Vera C. Rubin Observatory, spectra at such late phases will be important to distinguish between different explosion scenarios.
Ključne besede: Encore
Objavljeno v RUNG: 29.10.2024; Ogledov: 239; Prenosov: 1
.pdf Celotno besedilo (6,45 MB)
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30.
Analiza hitrosti sproščanja antibiotikov iz biokompozitnih materialov za uporabo v medicin
Matevž Može Davidović, 2023, objavljeni povzetek znanstvenega prispevka na konferenci

Ključne besede: biokompozitni materiali, spektrometrija, toplotne leče, protibakterijske lastnost
Objavljeno v RUNG: 29.10.2024; Ogledov: 205; Prenosov: 0
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