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SUMMARY:Small grains - big impact on the LSST discoveries?
DTSTART;VALUE=DATE-TIME:20261020T083000Z
DTEND;VALUE=DATE-TIME:20261020T084500Z
DTSTAMP;VALUE=DATE-TIME:20261112T103450Z
UID:indico-contribution-2258@events.ncbj.gov.pl
DESCRIPTION:Speakers: Patryk Matera (Narodowe Centrum Badań Jądrowych)\n
 The Vera C. Rubin Observatory is currently conducting the largest sky surv
 ey in human history: the LSST. It will observe the entire sky every three 
 days for ten years. It will collect astronomical amounts of data and obser
 ve nearly 20 billion galaxies. Despite these advantages\, LSST observation
 s will range from 338 to 1010 nm\, thus leaving us without infrared measur
 ements\, which are crucial for correctly estimating the physical propertie
 s of galaxies\, such as mass and star formation rate (SFR). This raises th
 e question: can we approximate dust attenuation using only six Rubin filte
 rs? In this talk\, I will attempt to answer this question.\n\nhttps://even
 ts.ncbj.gov.pl/event/502/contributions/2258/
LOCATION:
URL:https://events.ncbj.gov.pl/event/502/contributions/2258/
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