Project title: Spectral Information Processing using Quantum Neural Networks (SIPwQNNs)
Funding basis: Contract 5304/ESA/2023/0 with the Ministry of Education and Science
Project budget:
total: PLN 855 135,00 (EUR 182 335,53)
MEiN financing: PLN 389 739,00 (89,9% of national project funding)
Description:
Quantum computing enables the application of new methods to solve challenging scientific and engineering problems. One of such problems is the classification of the ever-increasing volume of remote sensing data. The objective of the SIPwQNNs project is to investigate the potential of applying quantum machine learning techniques (QML) for the analysis and processing of spectral images obtained by Earth observation satellites. As a result of this project, we can expect new tools and methodologies that can significantly improve the process of classifying Earth observation data, which, in turn, will have a significant impact on domains such as environmental monitoring, agriculture, natural resource management, and many other areas related to Earth observations.
SIPwQNNs has the potential to bring tangible benefits to society by supporting sustainable development, environmental protection, agricultural improvement, natural resource management, and citizens' quality of life.
Project title: Hyper-Kamiokande
Funding basis: Decision 2022/WK/15 of the Ministry of Education and Science
Project budget: 67 596 799.26 PLN (total - consortium) and 8 985 964.47 PLN (CAMK)
Description:
The Hyper-Kamiokande detector will be an underground radiation detector using the Cherenkov phenomenon, so it will record the charged particles produced by neutrinos and enable determination of their energies. It will be 5 times larger (258 kt water mass) than the current Super-Kamiokande detector. An extremely attractive feature of this type of detector is its simple operating principle: a large volume filled with very pure water, surrounded by light detectors (photomultipliers). The difficulty in the construction of Hyper-K will be the huge size of the tank - it will be a cylinder 71 m high and 68 m in diameter, which requires the hollowing out of a 73 m (H) by 69 m (D) cave in the rock. The whole construction must be placed deep underground (about 650 m), for shielding the detector from cosmic radiation. This size and location present new experimental and engineering challenges, as it will be the world's largest man-made facility of its kind.
Project title: Participation in the programme „Premia na Horyzoncie 2”
Funding basis: Agreement number 568500 /PnH 2/2022
Project budget: : 30 622.00 PLN
Description:
Salary supplements for staff involved in the implementation of the grant: Integrated activities in the field of high energy astrophysics, financed by the European Union's Horizon 2020 research and innovation programme under the grant agreement number 871158.
Project title: Participation in the programme „Premia na Horyzoncie 2”
Funding basis: Agreement number 565173/PnH 2/2022
Project budget: : 30 738,00 PLN
Description:
Salary supplements for staff involved in the implementation of the grant: Probes of new physics and technological advancements from particle and gravitational wave physics experiments. A cooperative Europe - United States - Asia effort., financed by the European Union's Horizon 2020 research and innovation programme under the grant agreement number 101003460.
Project title: SST-1M Mini-array Construction and Testing as Technology Demonstrator for the Cherenkov Telescope Array
SST-1M/CTA
Funding basis: Decision DIR/WK/2017/12 of 14.12.2017 of the Ministry of Science and Higher Education
Project budget: 7 880 044,35 PLN (total - consortium) and 522 783,17 PLN (CAMK)
The aim of the current project is to check the parameters and conduct research using a mini-network of two atmospheric imaging Cherenkov telescopes SST-1M for the study of high-energy gamma radiation from space. The equipment validation and calibration carried out as part of the task will enable the implementation of a whole series of valuable, and perhaps even unique scientific research. Systematic observations of the Crab Nebula, well-studied source of gamma emissions in the energy range up to around 100 TeV which is considered to be the main calibrator for gamma astronomy, will be used to calibrate the system. The main observation program will include monitoring the variability of several known bright blazars (active nuclei of galaxies with relativistic jets facing the observer) to determine their duty cycle range and power spectra in the high energy gamma-ray range. As part of the project, we also plan to attempt to measure the stellar intensity interference SII using two Cherenkov telescopes. The implementation of this measurement technique, proposed several decades ago, would constitute a new quality in astronomy in the implementation of measurements by networks of small Cherenkov telescopes. If the planned trials were to be successful, this would be the fundamental result for instrumental astronomy obtained with our SST-1M network.
https://www.cta-observatory.org/
Project title: Polish-German Astrophysical Observatory - support for ESO space and instrumental missions
OCA/ESO
Funding basis: Decision DIR/WK/2018/09 of 21.12.2018 of the Ministry of Science and Higher Education
Project budget: 13 272 285,43 PLN
The key scientific task of the project is to performbrightness measurements of about 500 bright stars in several filters, both in the visual and near-infrared range, as well as high-resolution spectroscopy. Photometric measurements must have an uncertainty of no more than 0.008 mag, while radial velocity measurements must have an accuracy of at least 30 m/s for eclipsing systems and 200 m/s for pulsating stars. These data will be used to calibrate several key distance measurement methods, and thus serve to greatly improve the calibration of the cosmic distance scale and the determination of the Hubble constant.
The project tasks include:
The work envisaged in the project will be carried out in a unique astronomical observatory located at the foot of Cerro Armazones in northern Chile, called Observatory Cerro Armazones (OCA). The Cerro Armazones mountain was chosen by the European Southern Observatory (ESO) to host the world's largest telescope, the Extremely Large Telescope (ELT), due to its stable weather conditions, with more than 340 clear nights per year and record low humidity, therefore the telescopes being built and installed within this project will be in close proximity to the ELT.
https://araucaria.camk.edu.pl/
Project title: National Center for Quantum Satellite Communications (NCSatKom)
Funding basis: Agreement Nr 7016/IA/SP/2019 of 19.07.2019 of the Ministry of Science and Higher Education
Project budget: 9 646 000,00 PLN
The project is based on the construction of a robotic telescope and a quantum communication system.
Robotic ground-based telescopes are becoming one of the most important branches of instrumental astronomy. These devices are capable of carrying out at least one night of observation on their own based on general guidelines set by their users, but usually such devices work independently for months and collect huge amounts of data. Robotic telescopes are now also used as sensors in the area of satellitesand space debris tracking. As part of the Polish Space Strategy, Poland indicated this segment, called SST (Space Surveillance and Tracking), as one of the three basic pillars of the Polish space industry. The aim is to develop the current system for monitoring and tracking of Earth artificial satellites and to assess current and future space threats, such as satellite collisions or their parts. In order to achieve this goal in practice, it is necessary to develop efficient algorithms for the reduction and analysis of data from satellites and terrestrial telescopes, and to ensure confidential communication between the terrestrial and satellite systems. Robotic telescopes can be used as an element of the terrestrial system of communication with satellites through links based on encrypted quantum communication.
Task title: Computational infrastructure for Polish gravitational wave astrophysics
Virgo
Funding basis: Agreement Nr 6931/II-LAN/SP/2019 of 19.07.2019
Co-financing: 360 000,00 PLN
Total value of the task: 398 769,00 PLN
Funding by the Ministry of Science and Higher Education grant for the development of IT infrastructure
Data analysis in the field of gravitational waves requires access to enormous computing power in the shortest possible time after the end of the observation campaign, calibration and data release (this is also important because the periods between collecting and calibrating data and making it public are gradually shortened). In addition, the astrophysicists at CAMK are actively developing new data analysis methods based on machine learning. Therefore, CAMK PAN applied on behalf of the Polish consortium Virgo for the necessary computing resources.
The grant was awarded for the expansion of a large IT infrastructure at CAMK serving the Virgo-Polgraw group (https://polgraw.camk.edu.pl/pl/), which operates within the European Virgo consortium (https: //www.virgo-gw. eu /).
Thanks to the grant, a GPU supercomputer for deep machine learning was purchased. Please, find more information here.
Project title: Very high energy astrophysics with H.E.S.S.
Funding basis: Decision 2021/WK/06 of the Ministry of Education and Science
Project budget: : 412 847,37 PLN (total - consortium) and 338 097,37 PLN (CAMK)
Description:
The overriding goal of the project is to provide Polish scientists with the opportunity to continue research in the field of very high energy gamma-ray astrophysics using the international High Energy Stereoscopic System (H.E.S.S.) observatory in Namibia. These telescopes are designed to observe the Universe in the very high energies, between several dozen GeV and about 100 TeV (the so-called VHE range). Telescopes of the H.E.S.S. Observatory record the Cherenkov radiation produced by the particles of the atmospheric shower resulting from the interaction of high-energy gamma photons with the Earth's atmosphere. The images of the shower make it possible to reconstruct the energy of the original gamma photon and to determine its incoming direction.
Scientific objectives of the H.E.S.S. belong to three main thematic groups:
1) searching for sources of cosmic rays (cosmic particle accelerators) and studying their properties and role in the Universe, with particular emphasis on the study of remnants of supernova explosions, pulsar nebulae, pulsars, micro-quasars, binary star systems, star formation regions, galaxies, blazars, radio galaxies, and gamma ray bursts;
2) study of the extragalactic background light (EBL) and the properties and structure of the intergalactic magnetic field;
3) testing fundamental physical theories by looking for traces of dark matter particle annihilation and studying Lorentz invariance. These studies are supplemented by cooperation with observatories operating in other energy ranges, the development of new data analysis methods and the use of modern computer methods for simulation and data acquisition.
Project title: Participation in the programme „Premia na Horyzoncie 2”
Funding basis: Agreement number 526845 /PnH 2/2021
Project budget: : 16 862 839,00 PLN
Description:
Salary supplements for staff involved in the implementation of the grant: Sub-percent calibration of the extragalactic distance scale in the era of big surveys – UniverScale, financed by the European Union's Horizon 2020 research and innovation programme under the grant agreement number 951549
