Prof. Dr. Marek Kowalski
Profil
Forschungsthemen8
Astrophysics Center for Multimessenger Studies in Europe (ACME)
Quelle ↗Förderer: Horizon Europe: Research and Innovation Action (RIA) Zeitraum: 09/2024 - 08/2028 Projektleitung: Dr. Jakob Nordin, Prof. Dr. Marek Kowalski
Astroteilchenphysik mit dem IceCube Neutrinoteleskop
Quelle ↗Förderer: Bundesministerium für Forschung, Technologie und Raumfahrt Zeitraum: 07/2023 - 06/2026 Projektleitung: Prof. Dr. Marek Kowalski
Astroteilchenphysik mit den Neutrinoteleskop IceCube
Quelle ↗Förderer: Bundesministerium für Forschung, Technologie und Raumfahrt Zeitraum: 07/2020 - 06/2023 Projektleitung: Prof. Dr. Marek Kowalski
HST-Beobachtungen der Wirtsgalaxie-Umgebung von Typ Ia Supernovae für Präzisionskosmologie
Quelle ↗Förderer: Bundesministerium für Wirtschaft und Energie Zeitraum: 07/2016 - 12/2018 Projektleitung: Prof. Dr. Marek Kowalski, Dr. Jakob Nordin
ICECUBE: Astroteilchenphysik mit dem IceCube-Observatorium. Teilprojekt 5
Quelle ↗Förderer: Bundesministerium für Forschung, Technologie und Raumfahrt Zeitraum: 07/2017 - 12/2020 Projektleitung: Prof. Dr. Marek Kowalski
Multimessenger School Sachmittel Kowalski
Quelle ↗Förderer: Helmholtz-Gemeinschaft Zeitraum: 09/2021 - 09/2026 Projektleitung: Prof. Dr. Marek Kowalski
NW: Opening celestial horizons: Detecting astrophysical high energy electron and tau neutrinos with IceCube
Quelle ↗Förderer: DFG Nachwuchsgruppe Zeitraum: 07/2006 - 07/2010 Projektleitung: Prof. Dr. Marek Kowalski
Verbundsproject IceCube: Astroteilchenphysik mit dem Neutrino-Teleskop IceCube
Quelle ↗Förderer: Bundesministerium für Forschung, Technologie und Raumfahrt Zeitraum: 10/2014 - 06/2017 Projektleitung: Prof. Dr. Marek Kowalski
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Publikationen25
Top 25 nach Zitationen — Quelle: OpenAlex (BAAI/bge-m3 embedded für Matching).
The Astrophysical Journal · 1700 Zitationen · DOI
Americanae nace como un proyecto conjunto que surge dentro de la Red Europea de Información y Documentación sobre América Latina (REDIAL), y que ha afrontado la Biblioteca de la Agencia Española de Cooperación Internacional para el Desarrollo (AECID). Esta nueva biblioteca virtual hace más accesibles los libros digitales de tema americanista a los investigadores y usuarios interesados de cualquier parte del mundo.
The Astrophysical Journal · 1555 Zitationen · DOI
We present a new compilation of Type Ia supernovae (SNe Ia), a new dataset of low-redshift nearby-Hubble-flow SNe and new analysis procedures to work with these heterogeneous compilations. This “Union ” compilation of 414 SN Ia, which reduces to 307 SNe after selection cuts, includes the recent large samples of SNe Ia from the Supernova Legacy Survey and ESSENCE Survey, the older datasets, as well as the recently extended dataset of distant supernovae observed with HST. A single, consistent and blind analysis procedure is used for all the various SN Ia subsamples, and a new procedure is implemented that consistently weights the heterogeneous data sets and rejects outliers. We present the latest results from this Union compilation and discuss the cosmological constraints from this new compilation and its combination with other cosmological measurements (CMB and BAO). The constraint we obtain from supernovae on the dark energy density is ΩΛ = 0.713 +0.027
Journal of Geophysical Research Atmospheres · 538 Zitationen · DOI
We have remotely mapped optical scattering and absorption in glacial ice at the South Pole for wavelengths between 313 and 560 nm and depths between 1100 and 2350 m. We used pulsed and continuous light sources embedded with the AMANDA neutrino telescope, an array of more than six hundred photomultiplier tubes buried deep in the ice. At depths greater than 1300 m, both the scattering coefficient and absorptivity follow vertical variations in concentration of dust impurities, which are seen in ice cores from other Antarctic sites and which track climatological changes. The scattering coefficient varies by a factor of seven, and absorptivity (for wavelengths less than ∼450 nm) varies by a factor of three in the depth range between 1300 and 2300 m, where four dust peaks due to stadials in the late Pleistocene have been identified. In our absorption data, we also identify a broad peak due to the Last Glacial Maximum around 1300 m. In the scattering data, this peak is partially masked by scattering on residual air bubbles, whose contribution dominates the scattering coefficient in shallower ice but vanishes at ∼1350 m where all bubbles have converted to nonscattering air hydrates. The wavelength dependence of scattering by dust is described by a power law with exponent −0.90 ± 0.03, independent of depth. The wavelength dependence of absorptivity in the studied wavelength range is described by the sum of two components: a power law due to absorption by dust, with exponent −1.08 ± 0.01 and a normalization proportional to dust concentration that varies with depth; and a rising exponential due to intrinsic ice absorption which dominates at wavelengths greater than ∼500 nm.
Astroparticle Physics · 410 Zitationen · DOI
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · 247 Zitationen · DOI
The Astrophysical Journal Letters · 228 Zitationen · DOI
The nearby supernova SN 2011fe can be observed in unprecedented detail. Therefore, it is an important test case for Type Ia supernova (SN Ia) models, which may bring us closer to understanding the physical nature of these objects. Here, we explore how available and expected future observations of SN 2011fe can be used to constrain SN Ia explosion scenarios. We base our discussion on three-dimensional simulations of a delayed detonation in a Chandrasekhar-mass white dwarf and of a violent merger of two white dwarfs (WDs) - realizations of explosion models appropriate for two of the most widely discussed progenitor channels that may give rise to SNe Ia. Although both models have their shortcomings in reproducing details of the early and near-maximum spectra of SN 2011fe obtained by the Nearby Supernova Factory (SNfactory), the overall match with the observations is reasonable. The level of agreement is slightly better for the merger, in particular around maximum, but a clear preference for one model over the other is still not justified. Observations at late epochs, however, hold promise for discriminating the explosion scenarios in a straightforward way, as a nucleosynthesis effect leads to differences in the 55Co production. SN 2011fe is close enough to be followed sufficiently long to study this effect.
HOST GALAXY PROPERTIES AND HUBBLE RESIDUALS OF TYPE Ia SUPERNOVAE FROM THE NEARBY SUPERNOVA FACTORY
2013The Astrophysical Journal · 178 Zitationen · DOI
We examine the relationship between Type Ia supernova (SN Ia) Hubble residuals and the properties of their host galaxies using a sample of 115 SNe Ia from the Nearby Supernova Factory. We use host galaxy stellar masses and specific star formation rates fi
Nature · 161 Zitationen · DOI
Astronomy and Astrophysics · 145 Zitationen · DOI
We employ 76 type Ia supernovae (SNe Ia) with optical spectrophotometry within 2.5 days of B-band maximum light obtained by the Nearby Supernova Factory to derive the impact of Si and Ca features on the supernovae intrinsic luminosity and determine a dust reddening law. We use the equivalent width of Si ii λ4131 in place of the light curve stretch to account for first-order intrinsic luminosity variability. The resulting empirical spectral reddening law exhibits strong features that are associated with Ca ii and Si ii λ6355. After applying a correction based on the Ca ii H&K equivalent width we find a reddening law consistent with a Cardelli extinction law. Using the same input data, we compare this result to synthetic rest-frame UBVRI-like photometry to mimic literature observations. After corrections for signatures correlated with Si ii λ4131 and Ca ii H&K equivalent widths and introducing an empirical correlation between colors, we determine the dust component in each band. We find a value of the total-to-selective extinction ratio, RV = 2.8 ± 0.3. This agrees with the Milky Way value, in contrast to the low RV values found in most previous analyses. This result suggests that the long-standing controversy in interpreting SN Ia colors and their compatibility with a classical extinction law, which is critical to their use as cosmological probes, can be explained by the treatment of the dispersion in colors, and by the variability of features apparent in SN Ia spectra.
The Astrophysical Journal Letters · 131 Zitationen · DOI
Abstract The third observing run by LVC has brought the discovery of many compact binary coalescences. Following the detection of the first binary neutron star merger in this run (LIGO/Virgo S190425z), we performed a dedicated follow-up campaign with the Zwicky Transient Facility (ZTF) and Palomar Gattini-IR telescopes. The initial skymap of this single-detector gravitational wave (GW) trigger spanned most of the sky observable from Palomar Observatory. Covering 8000 deg 2 of the initial skymap over the next two nights, corresponding to 46% integrated probability, ZTF system achieved a depth of ≈21 m AB in g - and r -bands. Palomar Gattini-IR covered 2200 square degrees in J -band to a depth of 15.5 mag, including 32% integrated probability based on the initial skymap. The revised skymap issued the following day reduced these numbers to 21% for the ZTF and 19% for Palomar Gattini-IR. We narrowed 338,646 ZTF transient “alerts” over the first two nights of observations to 15 candidate counterparts. Two candidates, ZTF19aarykkb and ZTF19aarzaod, were particularly compelling given that their location, distance, and age were consistent with the GW event, and their early optical light curves were photometrically consistent with that of kilonovae. These two candidates were spectroscopically classified as young core-collapse supernovae. The remaining candidates were ruled out as supernovae. Palomar Gattini-IR did not identify any viable candidates with multiple detections only after merger time. We demonstrate that even with single-detector GW events localized to thousands of square degrees, systematic kilonova discovery is feasible.
Nuclear Physics B - Proceedings Supplements · 128 Zitationen · DOI
Computer Physics Communications · 124 Zitationen · DOI
The Astronomical Journal · 116 Zitationen · DOI
We present a measurement of the distant Type Ia supernova (SN Ia) rate derived from the first 2 yr of the Canada-France-Hawaii Telescope Supernova Legacy Survey. We observed four 1° × 1° fields with a typical temporal frequency of (Δt) ~ 4 observer-frame days over time spans of 158-211 days per season for each field, with breaks during the full Moon. We used 8-10 m class telescopes for spectroscopic follow-up to confirm our candidates and determine their redshifts. Our starting sample consists of 73 spectroscopically verified SNe Ia in the redshift range 0.2 < z < 0.6. We derive a volumetric SN Ia rate of r_V((z) = 0:47) [0:42^(+0:13)-(-0:09)(syst:) ± 0:06(stat:)]x 10^-4 yr^-1 Mpc^3, assuming h = 0:7, Ω_m = 0:3, and a flat cosmology. Using recently published galaxy luminosity functions derived in our redshift range, we derive a SN Ia rate per unit luminosity of r_L((z) = 0:47) = 0:154^(+0:048)_(-0:033)(syst:)^(+0:039)_(-0:031)(stat:) SN units. Using our rate alone, we place an upper limit on the component of SN Ia production that tracks the cosmic star \nformation history of 1 SN Ia per 10^3 M_☉ of stars formed. Our rate and other rates from surveys using spectroscopic \nsample confirmation display only a modest evolution out to z = 0:55.
115 Zitationen · DOI
LiveScan3D is a free, open source system for live, 3D data acquisition using multiple Kinect v2 sensors. It allows the user to place any number of sensors in any physical configuration and start gathering data at real time speed. The freedom of placing the sensors in any configuration allows for many possible acquisition scenarios such as: capturing a single object from many viewpoints or creating 3D panoramas with multiple devices located close to each other. Thanks to the off-the-shelf Kinect v2 sensor the system is both accurate and inexpensive, opening 3D acquisition up to more recipients. In the paper we describe our system with the algorithms it is using and show its effectiveness in multiple scenarios including head shape reconstruction and 3D reconstruction of dynamic scenes.
Astronomy and Astrophysics · 110 Zitationen · DOI
We present a new atmospheric extinction curve for Mauna Kea spanning 3200–9700 Å. It is the most comprehensive to date, being based on some 4285 standard star spectra obtained on 478 nights spread over a period of 7 years obtained by the Nearby SuperNova Factory using the SuperNova Integral Field Spectrograph. This mean curve and its dispersion can be used as an aid in calibrating spectroscopic or imaging data from Mauna Kea, and in estimating the calibration uncertainty associated with the use of a mean extinction curve. Our method for decomposing the extinction curve into physical components, and the ability to determine the chromatic portion of the extinction even on cloudy nights, is described and verified over the wide range of conditions sampled by our large dataset. We demonstrate good agreement with atmospheric science data obtain at nearby Mauna Loa Observatory, and with previously published measurements of the extinction above Mauna Kea.
Journal of High Energy Astrophysics · 104 Zitationen · DOI
Observation of high energy atmospheric neutrinos with the Antarctic muon and neutrino detector array
2002Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · 90 Zitationen · DOI
The Antarctic muon and neutrino detector array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified by secondary muons moving upward through the array. Cosmic rays in the atmosphere generate a background of downward moving muons, which are about ${10}^{6}$ times more abundant than the upward moving muons. Over 130 days of exposure, we observed a total of about 300 neutrino events. In the same period, a background of $1.05\ifmmode\times\else\texttimes\fi{}{10}^{9}$ cosmic ray muon events was recorded. The observed neutrino flux is consistent with atmospheric neutrino predictions. Monte Carlo simulations indicate that 90% of these events lie in the energy range 66 GeV to 3.4 TeV. The observation of atmospheric neutrinos consistent with expectations establishes AMANDA-B10 as a working neutrino telescope.
Blood · 83 Zitationen · DOI
Tumor necrosis factor (TNF) production and non-Hodgkin lymphoma (NHL) outcome was found to be related to the TNF(-308) polymorphism. To explore whether this could be linked to neighboring polymorphisms, we genotyped the TNF(-376,-308,-238,-163), lymphotoxin alpha (LTalpha)(+252), and HLA DRB1 alleles in 204 patients with NHL and 120 controls. TNF(-308A) was the only allele associated with higher TNF and its p55 and p75 receptors' levels (P =.009, P =.03, and P =.007) and lower complete remission rates (P =.006). Freedom from progression (FFP) and overall survival (OS) were shorter in patients with TNF(-308A) (P =.009 and P =.02), null HLA DRB1*02 allele (P =.007 and P =.14), or both genetic markers (P =.004 and P =.005). Multivariate analysis incorporating International Prognostic Index (IPI) identified TNF(-308A) (P <.0001, relative risk [RR] = 1.63; P <.0001, RR = 1.51) and null HLA DRB1*02 alleles (P =.015, RR = 1.18; P <.0001, RR = 1.25) as independent factors for FFP and OS. These results indicate the existence of at least 2 inherited factors involved in NHL outcome.
Physical Review Letters · 82 Zitationen · DOI
We present the results of a search for point sources of high-energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several active-galactic-nuclei blazars, microquasars, magnetars, and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.
The Astrophysical Journal · 79 Zitationen · DOI
We present optical photometry and spectroscopy of five Type Ia supernovae discovered by the Nearby Supernova Factory selected to be spectroscopic analogs of the candidate super-Chandrasekhar-mass events SN2003fg and SN2007if. Their spectra are characterized by hot, highly ionized photospheres near maximum light, for which SN1991T supplies the best phase coverage among available close spectral templates. Like SN2007if, these supernovae are overluminous (-19.5 < M V < -20) and the velocity of the Si II λ6355 absorption minimum is consistent with being constant in time from phases as early as a week before, and up to two weeks after, B-band maximum light. We interpret the velocity plateaus as evidence for a reverse-shock shell in the ejecta formed by interaction at early times with a compact envelope of surrounding material, as might be expected for SNe resulting from the mergers of two white dwarfs. We use the bolometric light curves and line velocity evolution of these SNe to estimate important parameters of the progenitor systems, including 56Ni mass, total progenitor mass, and masses of shells and surrounding carbon/oxygen envelopes. We find that the reconstructed total progenitor mass distribution of the events (including SN2007if) is bounded from below by the Chandrasekhar mass, with SN2007if being the most massive. We discuss the relationship of these events to the emerging class of super-Chandrasekhar-mass SNeIa, estimate the relative rates, compare the mass distribution to that expected for double-degenerate SNIa progenitors from population synthesis, and consider implications for future cosmological Hubble diagrams.
Physical Review Letters · 77 Zitationen · DOI
Data from the AMANDA-B10 detector taken during the austral winter of 1997 have been searched for a diffuse flux of high energy extraterrestrial muon neutrinos. This search yielded no excess events above those expected from background atmospheric neutrinos, leading to upper limits on the extraterrestrial neutrino flux measured at the earth. For an assumed E-2 spectrum, a 90% classical confidence level upper limit has been placed at a level E2Phi(E)=8.4 x 10(-7) cm(-2) s(-1) sr(-1) GeV (for a predominant neutrino energy range 6-1000 TeV), which is the most restrictive bound placed by any neutrino detector. Some specific predicted model spectra are excluded. Interpreting these limits in terms of the flux from a cosmological distributions of sources requires the incorporation of neutrino oscillations, typically weakening the limits by a factor of 2.
The Astronomical Journal · 74 Zitationen · DOI
Americanae nace como un proyecto conjunto que surge dentro de la Red Europea de Información y Documentación sobre América Latina (REDIAL), y que ha afrontado la Biblioteca de la Agencia Española de Cooperación Internacional para el Desarrollo (AECID). Esta nueva biblioteca virtual hace más accesibles los libros digitales de tema americanista a los investigadores y usuarios interesados de cualquier parte del mundo.
2022 IEEE/CVF Conference on Computer Vision and Pattern Recognition (CVPR) · 73 Zitationen · DOI
We extend neural 3D representations to allow for intu-itive and interpretable user control beyond novel view ren-dering (i. e. camera control). We allow the user to annotate which part of the scene one wishes to control with just a small number of mask annotations in the training images. Our key idea is to treat the attributes as latent variables that are regressed by the neural network given the scene en-coding. This leads to afew-shot learning framework, where attributes are discovered automatically by the framework, when annotations are not provided. We apply our method to various scenes with different types of controllable attributes (e.g. expression control on human faces, or state control in movement of inanimate objects). Overall, we demonstrate, to the best of our knowledge, for the first time novel view and novel attribute re-rendering of scenes from a single video.
The Astrophysical Journal · 73 Zitationen · DOI
53 pages, 15 figures, published in the Astrophysical Journal. Minor (spelling and grammatical) changes to bring in line with published version
Astroparticle Physics · 72 Zitationen · DOI
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
university
Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Astroteilchenphysik mit dem IceCube Neutrinoteleskop
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Stammdaten
Identität, Organisation und Kontakt aus HU-FIS.
- Name
- Prof. Dr. Marek Kowalski
- Titel
- Prof. Dr.
- Fakultät
- Mathematisch-Naturwissenschaftliche Fakultät
- Institut
- Institut für Physik
- Arbeitsgruppe
- Experimentelle Physik, Experimentelle Astroteilchenphysik - DESY (S)
- Telefon
- +49 30 2093-7635
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