Koncert ansambla ASMANGU (Ansambl studenata Muzičke akademije za novu glazbu, 27. 5. 2022.)

Prvi dio snimke koncerta održanog na Muzičkoj akademiji u Koncertnoj dvorani "Blagoje Bersa" 27. 5. 2022. Izvođači: Ansambl studenata Muzičke akademije za novu glazbu, Petra Akrap (klavir), Petar Krokar (klavir), Nadir Hošić (klavir), Maria Garcia Vera (klavir), Maja Primorac (klavir), Maria Babić (klavir), Božidar Vlašić (klavir), Katarina Nera Biondić (klavir). Dirigent: red. prof. art. Berislav Šipuš. Program: 1. Sara Jakopović: Impromptu (izvođač: Petra Akrap); 2. Vigo Kovačić: I. River Breeze, II. Baby Spiders’Night Out (izvođač: Petar Krokar); 3. Claude Debussy: Le Prélude à l’Après-midi d’un faune (izvođač: ansambl ASMANGU); 4. Tin Ujević: Klavir-19 (izvođač: Nadir Hošić); 5. Pierre Boulez: Dérive 1, za šest instrumenata (izvođač: ansambl ASMANGU); 6. Sara Jakopović: Sedam klavirskih preludija (izvođači: Maria Garcia Vera, Maja Primorac); 7. Danijela Bošnjak: Veni Creator Spiritus (izvođač: Maria Babić); 8. Olivier Messiaen: Pièce pour piano et quatuor à cordes (izvođač: ansambl ASMANGU); 9. Tomislav Krobot: Klavirske minijature (izvođač: Božidar Vlašić); 10. Vigo Kovačić: Za lijeve ruke (Mono Mano) (izvođači: Nadir Hošić, Petar Krokar, Katarina Nera Biondić, Maja Primorac, Maria Garcia Vera); 11. Iannis Xenakis: O-mega, za solo udaraljke i 13 instrumenata (izvođač: ansambl ASMANGU)

Koncert ansambla ASMANGU (Ansambl studenata Muzičke akademije za novu glazbu, 27. 5. 2022.)

Drugi dio snimke koncerta održanog na Muzičkoj akademiji u Koncertnoj dvorani "Blagoje Bersa" 27. 5. 2022. Izvođači: Ansambl studenata Muzičke akademije za novu glazbu, Petra Akrap (klavir), Petar Krokar (klavir), Nadir Hošić (klavir), Maria Garcia Vera (klavir), Maja Primorac (klavir), Maria Babić (klavir), Božidar Vlašić (klavir), Katarina Nera Biondić (klavir). Dirigent: red. prof. art. Berislav Šipuš. Program: 1. Sara Jakopović: Impromptu (izvođač: Petra Akrap); 2. Vigo Kovačić: I. River Breeze, II. Baby Spiders’Night Out (izvođač: Petar Krokar); 3. Claude Debussy: Le Prélude à l’Après-midi d’un faune (izvođač: ansambl ASMANGU); 4. Tin Ujević: Klavir-19 (izvođač: Nadir Hošić); 5. Pierre Boulez: Dérive 1, za šest instrumenata (izvođač: ansambl ASMANGU); 6. Sara Jakopović: Sedam klavirskih preludija (izvođači: Maria Garcia Vera, Maja Primorac); 7. Danijela Bošnjak: Veni Creator Spiritus (izvođač: Maria Babić); 8. Olivier Messiaen: Pièce pour piano et quatuor à cordes (izvođač: ansambl ASMANGU); 9. Tomislav Krobot: Klavirske minijature (izvođač: Božidar Vlašić); 10. Vigo Kovačić: Za lijeve ruke (Mono Mano) (izvođači: Nadir Hošić, Petar Krokar, Katarina Nera Biondić, Maja Primorac, Maria Garcia Vera); 11. Iannis Xenakis: O-mega, za solo udaraljke i 13 instrumenata (izvođač: ansambl ASMANGU)

Koncert ansambla ASMANGU (Ansambl studenata Muzičke akademije za novu glazbu, 27. 5. 2022.)

Prvi dio snimke koncerta održanog na Muzičkoj akademiji u Koncertnoj dvorani "Blagoje Bersa" 27. 5. 2022. Izvođači: Ansambl studenata Muzičke akademije za novu glazbu, Petra Akrap (klavir), Petar Krokar (klavir), Nadir Hošić (klavir), Maria Garcia Vera (klavir), Maja Primorac (klavir), Maria Babić (klavir), Božidar Vlašić (klavir), Katarina Nera Biondić (klavir). Dirigent: red. prof. art. Berislav Šipuš. Program: 1. Sara Jakopović: Impromptu (izvođač: Petra Akrap); 2. Vigo Kovačić: I. River Breeze, II. Baby Spiders’Night Out (izvođač: Petar Krokar); 3. Claude Debussy: Le Prélude à l’Après-midi d’un faune (izvođač: ansambl ASMANGU); 4. Tin Ujević: Klavir-19 (izvođač: Nadir Hošić); 5. Pierre Boulez: Dérive 1, za šest instrumenata (izvođač: ansambl ASMANGU); 6. Sara Jakopović: Sedam klavirskih preludija (izvođači: Maria Garcia Vera, Maja Primorac); 7. Danijela Bošnjak: Veni Creator Spiritus (izvođač: Maria Babić); 8. Olivier Messiaen: Pièce pour piano et quatuor à cordes (izvođač: ansambl ASMANGU); 9. Tomislav Krobot: Klavirske minijature (izvođač: Božidar Vlašić); 10. Vigo Kovačić: Za lijeve ruke (Mono Mano) (izvođači: Nadir Hošić, Petar Krokar, Katarina Nera Biondić, Maja Primorac, Maria Garcia Vera); 11. Iannis Xenakis: O-mega, za solo udaraljke i 13 instrumenata (izvođač: ansambl ASMANGU)

Koncert ansambla ASMANGU (Ansambl studenata Muzičke akademije za novu glazbu, 27. 5. 2022.)

Drugi dio snimke koncerta održanog na Muzičkoj akademiji u Koncertnoj dvorani "Blagoje Bersa" 27. 5. 2022. Izvođači: Ansambl studenata Muzičke akademije za novu glazbu, Petra Akrap (klavir), Petar Krokar (klavir), Nadir Hošić (klavir), Maria Garcia Vera (klavir), Maja Primorac (klavir), Maria Babić (klavir), Božidar Vlašić (klavir), Katarina Nera Biondić (klavir). Dirigent: red. prof. art. Berislav Šipuš. Program: 1. Sara Jakopović: Impromptu (izvođač: Petra Akrap); 2. Vigo Kovačić: I. River Breeze, II. Baby Spiders’Night Out (izvođač: Petar Krokar); 3. Claude Debussy: Le Prélude à l’Après-midi d’un faune (izvođač: ansambl ASMANGU); 4. Tin Ujević: Klavir-19 (izvođač: Nadir Hošić); 5. Pierre Boulez: Dérive 1, za šest instrumenata (izvođač: ansambl ASMANGU); 6. Sara Jakopović: Sedam klavirskih preludija (izvođači: Maria Garcia Vera, Maja Primorac); 7. Danijela Bošnjak: Veni Creator Spiritus (izvođač: Maria Babić); 8. Olivier Messiaen: Pièce pour piano et quatuor à cordes (izvođač: ansambl ASMANGU); 9. Tomislav Krobot: Klavirske minijature (izvođač: Božidar Vlašić); 10. Vigo Kovačić: Za lijeve ruke (Mono Mano) (izvođači: Nadir Hošić, Petar Krokar, Katarina Nera Biondić, Maja Primorac, Maria Garcia Vera); 11. Iannis Xenakis: O-mega, za solo udaraljke i 13 instrumenata (izvođač: ansambl ASMANGU)

Euclid. IV. The NISP Calibration Unit

International audienceThe near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (<12% variations) and temporally stable illumination (0.1%-0.2% over 1200s) over the NISP detector plane, with minimal power consumption and energy dissipation. NI-CU is covers the spectral range ~[900,1900] nm - at cryo-operating temperature - at 5 fixed independent wavelengths to capture wavelength-dependent behaviour of the detectors, with fluence over a dynamic range of >=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations

Euclid. IV. The NISP Calibration Unit

The near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations

Euclid. IV. The NISP Calibration Unit

International audienceThe near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations

Euclid. IV. The NISP Calibration Unit

International audienceThe near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (<12% variations) and temporally stable illumination (0.1%-0.2% over 1200s) over the NISP detector plane, with minimal power consumption and energy dissipation. NI-CU is covers the spectral range ~[900,1900] nm - at cryo-operating temperature - at 5 fixed independent wavelengths to capture wavelength-dependent behaviour of the detectors, with fluence over a dynamic range of >=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations

Euclid. IV. The NISP Calibration Unit

International audienceThe near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (<12% variations) and temporally stable illumination (0.1%-0.2% over 1200s) over the NISP detector plane, with minimal power consumption and energy dissipation. NI-CU is covers the spectral range ~[900,1900] nm - at cryo-operating temperature - at 5 fixed independent wavelengths to capture wavelength-dependent behaviour of the detectors, with fluence over a dynamic range of >=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations

Euclid. IV. The NISP Calibration Unit

International audienceThe near-infrared calibration unit (NI-CU) onboard Euclid's Near-Infrared Spectrometer and Photometer (NISP) is the first astronomical calibration lamp based on light-emitting diodes (LEDs) to be operated in space. Euclid is a mission in ESA's 'Cosmic Vision 2015-2025' framework, to explore the dark universe and provide a next-level characterisation of the nature of gravitation, dark matter, and dark energy. Calibrating photometric and spectrometric measurements of galaxies to better than 1.5% accuracy in a survey homogeneously mapping ~14000 deg^2 of extragalactic sky requires a very detailed characterisation of near-infrared (NIR) detector properties, as well their constant monitoring in flight. To cover two of the main contributions - relative pixel-to-pixel sensitivity and non-linearity characteristics - as well as support other calibration activities, NI-CU was designed to provide spatially approximately homogeneous (<12% variations) and temporally stable illumination (0.1%-0.2% over 1200s) over the NISP detector plane, with minimal power consumption and energy dissipation. NI-CU is covers the spectral range ~[900,1900] nm - at cryo-operating temperature - at 5 fixed independent wavelengths to capture wavelength-dependent behaviour of the detectors, with fluence over a dynamic range of >=100 from ~15 ph s^-1 pixel^-1 to >1500 ph s^-1 pixel^-1. For this functionality, NI-CU is based on LEDs. We describe the rationale behind the decision and design process, describe the challenges in sourcing the right LEDs, as well as the qualification process and lessons learned. We also provide a description of the completed NI-CU, its capabilities and performance as well as its limits. NI-CU has been integrated into NISP and the Euclid satellite, and since Euclid's launch in July 2023 has started supporting survey operations