Tuesday, December 03, 2024
03:30 AM - 05:00 PM
ASD Colloquium (Hybrid)
QUVIK - Quick Ultra-Violet Kilonova surveyor
Norbert Werner (Masaryk University)
After summarizing the results of the GRBAlpha, GRBBeta, and VZLUSAT-2 nanosatellites that are detecting gamma-ray bursts, I will present the status and the science case of the Quick Ultra-Violet Kilonova surveyor—QUVIK mission. QUVIK is an ultra-violet (UV) space telescope on an approximately 130 kg small satellite with a moderately fast re-pointing capability and a real-time alert communication system, approved for a Czech national space mission. The satellite, which is expected to launch in five years, will provide key follow-up capabilities to increase the discovery potential of gravitational wave observatories and future wide-field multi-wavelength surveys. The primary objective of the mission is the measurement of the UV brightness evolution of kilonovae, resulting from mergers of neutron stars, to distinguish between different explosion scenarios. The mission, which is designed to be complementary to the Ultraviolet Transient Astronomy Satellite—ULTRASAT, will also provide unique follow-up capabilities for other transients both in the near- and far-UV bands. Between the observations of transient sources, the satellite will perform observations of other targets of interest for the scientific community, such as stars, stellar systems, and galactic nuclei.
Read more about this event Norbert Werner (Masaryk University)
After summarizing the results of the GRBAlpha, GRBBeta, and VZLUSAT-2 nanosatellites that are detecting gamma-ray bursts, I will present the status and the science case of the Quick Ultra-Violet Kilonova surveyor—QUVIK mission. QUVIK is an ultra-violet (UV) space telescope on an approximately 130 kg small satellite with a moderately fast re-pointing capability and a real-time alert communication system, approved for a Czech national space mission. The satellite, which is expected to launch in five years, will provide key follow-up capabilities to increase the discovery potential of gravitational wave observatories and future wide-field multi-wavelength surveys. The primary objective of the mission is the measurement of the UV brightness evolution of kilonovae, resulting from mergers of neutron stars, to distinguish between different explosion scenarios. The mission, which is designed to be complementary to the Ultraviolet Transient Astronomy Satellite—ULTRASAT, will also provide unique follow-up capabilities for other transients both in the near- and far-UV bands. Between the observations of transient sources, the satellite will perform observations of other targets of interest for the scientific community, such as stars, stellar systems, and galactic nuclei.
Tuesday, December 03, 2024
10:00 AM - 11:00 AM
Virtual Chat with the Code 600 Director
Everyone is Welcome!
ACTUAL TIME: 10:10–10:55 a.m.
Read more about this event ACTUAL TIME: 10:10–10:55 a.m.
Friday, December 06, 2024
12:00 PM - 01:00 PM
Agencywide All-Hands
Join us for an agencywide all-hands meeting to celebrate 2024 accomplishments and the individuals who make NASA the best agency to work for in the federal government. We will hear from Administrator Bill Nelson, Deputy Administrator Pam Melroy, and Associate Administrator Jim Free.
Read more about this event Tuesday, December 10, 2024
03:30 AM - 05:00 PM
ASD Colloquium (Hybrid)
David Chuss (Villanova)
Read more about this event Thursday, December 12, 2024
12:00 PM - 01:00 PM
SED Director’s Seminar
Please join us for the SED Director’s Seminar hosted by the Observational Cosmology Laboratory, Code 665!
More information to come!
Read more about this event More information to come!
Tuesday, December 17, 2024
03:30 AM - 05:00 PM
ASD Colloquium (Hybrid)
Congratulations to the ASD Winners of 2024 Robert H. Goddard Awards 665/Jonathan Gardner, 662/Michale Loewenstein (Univ of...
Thursday, August 01, 2024