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<p>Dear colleagues, <br>
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<div>our next EO meeting will take place this Thursday Nov 5 at 13:15 via Zoom. <br>
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<div>The meeting will be online. To join access <font size="3" face="Calibri,Helvetica,sans-serif,serif,EmojiFont" color="black">
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<div><font size="3" face="Calibri,Helvetica,sans-serif,serif,EmojiFont" color="black"><span style="font-size:12pt;" id="divtagdefaultwrapper">You will be able to enter the meeting room from 13:00.</span></font><font size="3" face="Calibri,Helvetica,sans-serif,serif,EmojiFont" color="black"><span style="font-size:12pt;" id="divtagdefaultwrapper">
See below for other methods to participate. </span></font></div>
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<p><span>This week <b>Ana Sagués Carracedo</b> from Stockholm University will present</span><br>
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<div style="background-color:transparent;margin-top:0;margin-bottom:0;"><font color="#0E101A"><span style="background-color:transparent;"><span style="background-color:transparent;"><b>Titl</b></span><span style="background-color:transparent;"><b>e:
</b></span><span style="background-color:transparent;">Constraints on detection rate and properties of kilonovae with the Zwicky Transient Facility</span></span></font></div>
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<div style="background-color:transparent;margin-top:0;margin-bottom:0;"><font color="#0E101A"><span style="background-color:transparent;"><span style="background-color:transparent;"><b>Abstract:</b></span><span style="background-color:transparent;"> LIGO and
VIRGO's third observing run concluded, and 13 merger candidates involving at least one neutron star were followed-up by optical wide-field surveys like the Zwicky Transient Facility (ZTF). The observations and kilonova identification have proven to be challenging.
Some of the difficulties rase from poor localization maps together with the lack of knowledge of a kilonovae population that is intrinsically fainter than common supernovae and with rapid evolution. After an extraordinary effort from the multimessenger astronomy
community, no electromagnetic source has been identified as a confident counterpart of gravitational waves signals. During my talk, I am going to show you the scientific implications of non-detections recently published using ZTF data. We are able to competitively
constraint the detection rate of kilonovae (https://arxiv.org/pdf/2008.00008.pdf) as well as its luminosity function (https://arxiv.org/pdf/2006.11306.pdf). With deep enough observations and assuming theoretical models, we are able to put strong constraints
on the ejecta parameters for the first neutron star-black hole (NSBH) merger candidates in gravitational waves (https://arxiv.org/pdf/2009.07210.pdf). </span></span></font></div>
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<p>See you then! <br>
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<div>Andre da Silva Schneider is inviting you to a scheduled Zoom meeting.<br>
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Topic: EO Meeting<br>
Time: Nov 5, 2020 01:00 PM Stockholm<br>
Every 2 weeks on Thu, 4 occurrence(s)<br>
Nov 5, 2020 01:00 PM<br>
Nov 19, 2020 01:00 PM<br>
Dec 3, 2020 01:00 PM<br>
Dec 17, 2020 01:00 PM<br>
Please download and import the following iCalendar (.ics) files to your calendar system.<br>
Weekly: https://stockholmuniversity.zoom.us/meeting/u5EkdeGtqj4oHdR8xLPfgh3x0S0IUQWMfTFX/ics?icsToken=98tyKu-tpzkiH9CQsh6HR_MMHYjoWe_wiCVBgqdvxAfJMyZUalDuZtESG4dOJ_XW<br>
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https://stockholmuniversity.zoom.us/j/65928545270<br>
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Meeting ID: 659 2854 5270<br>
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<p style="font-size:16px; font-family:Calibri,Helvetica,sans-serif">---------------------------------</p>
<p style="font-size:16px; font-family:Calibri,Helvetica,sans-serif">André da Silva Schneider<br>
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<p style="font-size:16px; font-family:Calibri,Helvetica,sans-serif"><span style="font-size:10pt; font-family:Calibri,Helvetica,sans-serif,serif,EmojiFont">Department of Astronomy</span><br>
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<p style="font-size:16px; font-family:Calibri,Helvetica,sans-serif"><span style="font-family:Calibri,Helvetica,sans-serif,serif,EmojiFont"><span style="font-size:10pt">Stockholm University</span></span></p>
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