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Tab to space and a vim modeline.
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@rainwoodman @kheegan
rainwoodman authored and kheegan committed Nov 21, 2017
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Expand Up @@ -85,15 +85,14 @@ <h2 id="slogan">January 10-12, 2018, Berkeley, CA</h2>
<div>
<h1>Organizing Committee
<a class="btn btn-sm float-right" href="mailto:[email protected]">Email</a>
</h1>
</h1>
<ul class="sidemenu">
<li>Marcelo Alvarez</li>
<li>Emanuele Castorina</li>
<li>Joanne Cohn</li>
<li>Emanuele Castorina</li>
<li>Joanne Cohn</li>
<li>Yu Feng</li>
<li>Uros Seljak</li>
<li>Martin White</li>

</ul>
</div>

Expand All @@ -118,71 +117,72 @@ <h1>Secretary of the Conference
</div>
<div id="main">
<div><h1><a id="overview">Overview</a></h1>
<p>
The volume probed by cosmological surveys is growing rapidly,
while the sensitivity of CMB experiments is likewise
increasing the fidelity with which secondary anisotropies can be
used as cosmological probes. Computational modeling of the sky,
in the form of mock catalogs and simulated observations, is
becoming a part of the analysis process itself, with a wide
range of techniques and approaches being developed.
</p>
<p>
The goal of the meeting is to bring together experts on modeling
large scale structure observations and discuss and compare different
approaches to determine the specific desired properties of simulated
data for a given large scale survey simulation, as well as to identify
those elements common to multiple probes for the same underlying large
scale structure.
</p>
<p>
</p>
<p>
<p>
The volume probed by cosmological surveys is growing rapidly,
while the sensitivity of CMB experiments is likewise
increasing the fidelity with which secondary anisotropies can be
used as cosmological probes. Computational modeling of the sky,
in the form of mock catalogs and simulated observations, is
becoming a part of the analysis process itself, with a wide
range of techniques and approaches being developed.
</p>
<p>
The goal of the meeting is to bring together experts on modeling
large scale structure observations and discuss and compare different
approaches to determine the specific desired properties of simulated
data for a given large scale survey simulation, as well as to identify
those elements common to multiple probes for the same underlying large
scale structure.
</p>
<p>

</p>
<p>
Please join us for a workshop on modeling the extragalactic sky at the
Berkeley Center for Cosmological Physics --
a perfect place to contemplate neutral hydrogen while enjoying Pacific views!
</p>
<p>
</p>

<p>
Where: <b> UC Berkeley </b>
<br/>
When: <b>January 10-12, 2018</b>
</p>
<p>
</p>

<p>
The format of the workshop will be aimed at facilitating informal discussions.
Topics will include computational approaches for modeling the
extragalactic sky as seen through: CMB secondary anisotropies;
clustering and redshift space distortions in spectroscopic galaxy
surveys; cosmic shear with imaging surveys; intensity mapping
techniques and the high-redshift universe.
</p>
Topics will include computational approaches for modeling the
extragalactic sky as seen through: CMB secondary anisotropies;
clustering and redshift space distortions in spectroscopic galaxy
surveys; cosmic shear with imaging surveys; intensity mapping
techniques and the high-redshift universe.
</p>
</div>
<div><h1><a id="registration"> Registration</a></h1>
<p>
<p>
Registration is limited to 50 participants.
If you are planning to attend, please register clicking the button here
</p>
<a class="btn btn-primary btn-lg center-block" role="button" href="https://goo.gl/forms/lNpEchzinpaSw96i1">Register for the workshop</a>
<p>
</p>
<a class="btn btn-primary btn-lg center-block" role="button" href="https://goo.gl/forms/lNpEchzinpaSw96i1">Register for the workshop</a>
<p>
There is no registration fee;
please contact the organizers if you require an invitation letter for visa applications.
</p>
please contact the <a href="mailto:[email protected]">organizing committee</a>
if you require an invitation letter for visa applications.
</p>
</div>

<div><h1><a id="venue">Venue</a></h1>
<p>
<p>
Registration and talks will take place in LeConte Hall on UC Berkeley Campus
(see <a href="https://goo.gl/maps/ekoUQVgfhsv">map</a>)
<br/>
Registration and talks on the first two days will happen in LeConte 375,
while on the last day they will be in LeConte 325.
The reception and dinner on Wed 22 will take place on the roof (6th floor) of New Campbell hall,
next door to LeConte.
</p>
</p>
</div>

<div><h1><a id="accomodation">Accommodation</a></h1>
<p>
Hotels in downtown Berkeley are probably most convenient.
Expand Down Expand Up @@ -276,3 +276,4 @@ <h1>Secretary of the Conference

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