<html>
<head>
<meta http-equiv="Content-Type" content="text/html; charset=iso-8859-1">
</head>
<body>
Dear everyone, <br>
<br>
Reminder of today's seminar. We in A5:1003 at 13:15. You can also join by zoom<br>
https://stockholmuniversity.zoom.us/j/3575421837<br>
<br>
Speaker: Priscila J. Pessi<br>
Title: Characteristics of the ZTF sample of hydrogen rich Type II Superluminous Supernova<br>
Abstract:<br>
Hydrogen rich superluminous supernovae (SLSNe II) is a puzzling class of extremely intrinsically bright events. Their exact powering mechanism is not yet understood. Most SLSNe II show interaction with circumstellar material (CSM). The mechanism that dictates
which is the dominant mass loss event (e.g: winds, outbursts, mass ejections) producing CSM in different progenitors is unknown. Systematic analysis of large samples of SLSNe II light curve features could aid to constrain their possible progenitors. In this
talk I will present results from the analysis of a sample of SLSNe II light curves from the ZTF survey, focusing on extreme events that may indicate differences in the powering mechanism of this class.<br>
<br>
Best,<br>
Haakon (on behalf of the organisers)
</body>
</html>