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1.
Strongly lensed supernovae, the past and the future : lecture at the University of Cambridge, 26. 6. 2024
Tanja Petrushevska, 2024, predavanje na tuji univerzi

Opis: The searches and observations of supernovae (SNe) have been motivated by the fact that they are exceptionally useful for various astrophysical and cosmological applications. Most prominently, Type Ia SNe (SNe Ia) have been used as distance indicators showing that the expansion rate of the Universe is accelerating. The strong gravitational lensing effect provides another powerful tool and occurs when a foreground mass distribution is located along the line of sight to a background source. It can happen so that galaxies and galaxy clusters can act as “gravitational telescopes”, boosting the faint signals from distant SNe and galaxies. Thanks to the magnification boost provided by the gravitational telescope, we are able to probe galaxies and SNe that otherwise would be undetectable. Therefore, the combination of the two tools, SNe and strong lensing, in the single phenomenon of strongly lensed SNe, provides a powerful simultaneous probe of several cosmological and astrophysical phenomena. By measuring the time delays of strongly lensed supernovae and having a high-quality strong lensing model of the galaxy cluster, it is possible to measure the Hubble constant with competitive precision. In this talk, I will present some of the past and recent results that have been possible due to the observations of strongly lensed supernovae and anticipate what we can expect in the future from the upcoming telescope surveys, such as the Vera C. Rubin Observatory and Nancy G. Roman Space Telescope.
Ključne besede: supernova, strong lensing, Hubble constant
Objavljeno v RUNG: 26.06.2024; Ogledov: 191; Prenosov: 4
.pdf Celotno besedilo (18,15 MB)
Gradivo ima več datotek! Več...

2.
Strongly lensed supernovae : the past and the future
Tanja Petrushevska, 2024, predavanje na tuji univerzi

Ključne besede: invited seminar, supernova, strong lensing, James Webb space telescope
Objavljeno v RUNG: 11.06.2024; Ogledov: 306; Prenosov: 2
.pdf Celotno besedilo (18,12 MB)
Gradivo ima več datotek! Več...

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What can we do with strongly lensed supernovae?
Tanja Petrushevska, 2023, objavljeni povzetek znanstvenega prispevka na konferenci

Ključne besede: cosmology, strong lensing, supernovae
Objavljeno v RUNG: 07.09.2023; Ogledov: 1032; Prenosov: 3
.pdf Celotno besedilo (18,56 MB)

6.
Contributed talk at the international conference "Cosmology in Miramare" 2023
Tanja Petrushevska, 2023, objavljeni povzetek znanstvenega prispevka na konferenci

Opis: The searches and observations of supernovae (SNe) have been motivated by the fact that they are exceptionally useful for various astrophysical and cosmological applications. Most prominently, Type Ia SNe (SNe Ia) have been used as distance indicators showing that the expansion rate of the Universe is accelerating. The strong gravitational lensing effect provides another powerful tool and occurs when a foreground mass distribution is located along the line of sight to a background source. It can happen so that galaxies and galaxy clusters can act as “gravitational telescopes”, boosting the faint signals from distant SNe and galaxies. Thanks to the magnification boost provided by the gravitational telescope, we are able to probe galaxies and SNe that otherwise would be undetectable. Therefore, the combination of the two tools, SNe and strong lensing, in the single phenomenon of strongly lensed SNe, provides a powerful simultaneous probe of several cosmological and astrophysical phenomena. By measuring the time delays of strongly lensed supernovae and having a high-quality strong lensing model of the galaxy cluster, it is possible to measure the Hubble constant with competitive precision. In this talk, I will present some of the past and recent results that have been possible due to the observations of strongly lensed supernovae and anticipate what we can expect in the future from the upcoming telescope surveys, such as the Vera C. Rubin Observatory and Nancy G. Roman Space Telescope.
Ključne besede: cosmology, supernovae, strong lensing
Objavljeno v RUNG: 07.09.2023; Ogledov: 1044; Prenosov: 2
URL Povezava na datoteko
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7.
Strong lensing as a tool to study the early universe : written report
Brankica Apostolova, 2023, raz. nal. na višji ali visoki šoli

Ključne besede: strong lensing, astrophysics, Roman Space Telescope, galaxy clustersv, galaxies
Objavljeno v RUNG: 23.08.2023; Ogledov: 960; Prenosov: 0
Gradivo ima več datotek! Več...

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Strongly lensed supernovae at high-redshifts : Invited seminar 'Strongly lensed supernovae at high-redshifts' at NCBJ, Poland
Tanja Petrushevska, predavanje na tuji univerzi

Opis: The searches and observations of supernovae (SNe) have been motivated by the fact that they are exceptionally useful for various astrophysical and cosmological applications. Most prominently, Type Ia SNe (SNe Ia) have been used as distance indicators showing that the expansion rate of the Universe is accelerating. The strong gravitational lensing effect provides another powerful tool and occurs when a foreground mass distribution is located along the line of sight to a background source. It can happen so that galaxies and galaxy clusters can act as “gravitational telescopes”, boosting the faint signals from distant SNe and galaxies. Thanks to the magnification boost provided by the gravitational telescope, we are able to probe galaxies and SNe that otherwise would be undetectable. Therefore, the combination of the two tools, SNe and strong lensing, in the single phenomenon of strongly lensed SNe, provides a powerful simultaneous probe of several cosmological and astrophysical phenomena. In this talk, I will present some of the past results that have been possible due to the observations of strongly lensed supernovae and anticipate what we can expect in the future from the upcoming telescope surveys.
Ključne besede: supernovae, strong lensing
Objavljeno v RUNG: 16.03.2023; Ogledov: 1278; Prenosov: 0
Gradivo ima več datotek! Več...

10.
Strongly Lensed Supernovae in Well-Studied Galaxy Clusters with the Vera C. Rubin Observatory
Tanja Petrushevska, 2020, izvirni znanstveni članek

Opis: Strong lensing by galaxy clusters can be used to significantly expand the survey reach, thus allowing observation of magnified high-redshift supernovae that otherwise would remain undetected. Strong lensing can also provide multiple images of the galaxies that lie behind the clusters. Detection of strongly lensed Type Ia supernovae (SNe Ia) is especially useful because of their standardizable brightness, as they can be used to improve either cluster lensing models or independent measurements of cosmological parameters. The cosmological parameter, the Hubble constant, is of particular interest given the discrepancy regarding its value from measurements with different approaches. Here, we explore the feasibility of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) of detecting strongly lensed SNe in the field of five galaxy clusters (Abell 1689 and Hubble Frontier Fields clusters) that have well-studied lensing models. Considering the 88 systems composed of 268 individual multiple images in the five cluster fields, we find that the LSST will be sensitive to SNe Ia (SNe IIP) exploding in 41 (23) galaxy images. The range of redshift of these galaxies is between 1.01 < z < 3.05. During its 10 years of operation, LSST is expected to detect 0.2 ± 0.1 SN Ia and 0.9 ± 0.3 core collapse SNe. However, as LSST will observe many more massive galaxy clusters, it is likely that the expectations are higher. We stress the importance of having an additional observing program for photometric and spectroscopic follow-up of the strongly lensed SNe detected by LSST.
Ključne besede: supernovae, strong gravitational lensing, galaxy clusters
Objavljeno v RUNG: 28.11.2020; Ogledov: 2675; Prenosov: 94
.pdf Celotno besedilo (863,97 KB)

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