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    <title>Centre for Exoplanets and Habitability &#187; News (tag [MNRAS])</title>
    <link>https://warwick.ac.uk/fac/sci/physics/research/astro/ceh/news/</link>
    <description>The latest from Centre for Exoplanets and Habitability &#187; News (tag [MNRAS])</description>
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    <category>Untagged</category>
    <item>
      <title>NGTS-4b: A sub-Neptune transiting in the desert</title>
      <link>https://academic.oup.com/mnras/article/486/4/5094/5475662</link>
      <description>&lt;div class="news-thumbnail" style="float: left; margin-right: 10px; margin-bottom: 5px;"&gt;&lt;img class="thumbnail" width="100" height="100" src="https://warwick.ac.uk/sitebuilder2/file/fac/sci/physics/research/astro/ceh/news?sbrPage=%2Ffac%2Fsci%2Fphysics%2Fresearch%2Fastro%2Fceh%2Fnews&amp;newsItem=8a1785d86b0d349a016b0dc5cd161264" alt="image"&gt;&lt;/div&gt;&lt;p&gt;CEH member Richard West leads the fascinating discovery of an exoplanet that falls in the middle of what has been termed the 'Neptunian desert'. This refers to a region close-in to the parent star where previously no Neptune-sized exoplanets had been found. NGTS-4b has a mass 20 times that of the Earth and orbits its star (a 13th mag K dwarf) once every 1.34 days! What's more, it's the smallest planet discovered by a wide-field ground-based photometric survey to date - excellent work!&lt;/p&gt;

&lt;p&gt;This study was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 486, Issue 4, July 2019, Pages 5094&amp;ndash;5103&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link: &lt;/strong&gt;&lt;a href="https://arxiv.org/pdf/1809.00678.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved:&lt;/strong&gt; Richard West (lead), Daniel Bayliss, James Jackman, George King, James McCormac, Peter Wheatley, David Armstrong, Paul Chote, Ben Cooke, Emma Foxell, Boris G&#228;nsicke, Tom Louden &amp;amp; Don Pollacco&lt;/p&gt;</description>
      <category>Habitability</category>
      <category>publication</category>
      <category>CEH</category>
      <category>University of Warwick</category>
      <category>Exoplanets</category>
      <category>CEHpublication</category>
      <category>NGTS</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <pubDate>Fri, 31 May 2019 12:03:00 GMT</pubDate>
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    <item>
      <title>Ground-based detection of G star superflares with NGTS</title>
      <link>https://academic.oup.com/mnras/article-abstract/477/4/4655/4967002</link>
      <description>&lt;p&gt;CEH member James Jackman leads a recent study of flares in G-type stars, as observed using NGTS. The study shows that G-stars can have flares many times the energy of the Carrington event, and the primary detection is one of the largest amplitude superflares detected from a bright G star. &lt;/p&gt;

&lt;p&gt;This work was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 477, Issue 4, p.4655-4664&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link: &lt;/strong&gt;&lt;a href="https://arxiv.org/pdf/1804.03377.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved: &lt;/strong&gt;James Jackman (lead), Peter Wheatley, Chloe Pugh, Boris G&#228;nsicke, Anne-Marie Broomhall, David Armstrong &amp;amp; James McCormac&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>University of Warwick</category>
      <category>Exoplanets</category>
      <category>CEHpublication</category>
      <category>NGTS</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <category>astrophysics</category>
      <pubDate>Mon, 04 Jun 2018 11:43:00 GMT</pubDate>
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    </item>
    <item>
      <title>Cool DZ white dwarfs II: compositions and evolution of old remnant planetary systems</title>
      <link>https://academic.oup.com/mnras/article-abstract/477/1/93/4923092</link>
      <description>&lt;p&gt;CEH member Mark Hollands leads a new study which examines pollution of cool DZ white dwarfs.&lt;/p&gt;

&lt;p&gt;This work was published in&lt;strong&gt; Monthly Notices of the Royal Astronomical Society, Volume 477, Issue 1, p.93-111&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link: &lt;a href="https://arxiv.org/pdf/1801.07714.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved:&lt;/strong&gt; Mark Hollands (lead), Boris G&#228;nsicke&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>University of Warwick</category>
      <category>CEHpublication</category>
      <category>NGTS</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <category>astrophysics</category>
      <category>White Dwarf</category>
      <pubDate>Mon, 04 Jun 2018 11:39:00 GMT</pubDate>
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    </item>
    <item>
      <title>Automatic vetting of planet candidates from ground based surveys: Machine learning with NGTS</title>
      <link>https://academic.oup.com/mnras/article-abstract/478/3/4225/4999921</link>
      <description>&lt;p&gt;CEH member David Armstrong has published a new study on automatic vetting of exoplanet candidates using machine learning techniques. In this work he applies it to candidates from NGTS, but the technique is extendable to other transiting exoplanet surveys.&lt;/p&gt;

&lt;p&gt;This work was published in&lt;strong&gt; Monthly Notices of the Royal Astronomical Society, Volume 478, Issue 3, August 2018, Pages 4225&amp;ndash;4237&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link:&lt;/strong&gt; &lt;a href="https://arxiv.org/pdf/1805.07089.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved: &lt;/strong&gt;David Armstrong (lead), James McCormac, Daniel Bayliss, Tom Louden, Don Pollacco, Richard West &amp;amp; Peter Wheatley&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>University of Warwick</category>
      <category>Exoplanets</category>
      <category>CEHpublication</category>
      <category>NGTS</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astrophysics</category>
      <pubDate>Mon, 04 Jun 2018 11:37:00 GMT</pubDate>
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    </item>
    <item>
      <title>Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system</title>
      <link>https://academic.oup.com/mnras/article-abstract/478/4/4720/4993331</link>
      <description>&lt;p&gt;The Next Generation Transit Survey, which is led by CEH member Peter Wheatley, has publised its third planet discovery. NGTS-3Ab is in an unresolved binary system, and vetting the planet was a challenging task that produced new insights in BIS correlations in exoplanet observations.&lt;/p&gt;

&lt;p&gt;This work was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 478, Issue 4, August 2018, Pages 4720&amp;ndash;4737&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link:&lt;/strong&gt; &lt;a href="https://arxiv.org/pdf/1805.01378.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved: &lt;/strong&gt;James McCormac, David Armstrong, Benjamin Cooke, Boris G&#228;nsicke, Tom Louden, Don Pollacco &amp;amp; Peter Wheatley&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>University of Warwick</category>
      <category>CEHpublication</category>
      <category>NGTS</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <category>astrophysics</category>
      <pubDate>Mon, 04 Jun 2018 11:33:00 GMT</pubDate>
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    <item>
      <title>The XUV environments of exoplanets from Jupiter-size to super-Earth</title>
      <link>https://academic.oup.com/mnras/article-abstract/478/1/1193/4990663</link>
      <description>&lt;p&gt;CEH member George King has published an exciting study looking at the extreme UV environment of several exoplanets, including a detection of the transit of WASP-80b in the NUV using XMM Newton.&lt;/p&gt;

&lt;p&gt;The study was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 478, Issue 1, July 2018, Pages 1193&amp;ndash;1208&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link:&lt;/strong&gt; &lt;a href="https://arxiv.org/pdf/1804.11124.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved: &lt;/strong&gt;George King, Peter Wheatley &amp;amp; Tom Louden&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>Exoplanets</category>
      <category>CEHpublication</category>
      <category>MNRAS</category>
      <category>X-rays</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <category>astrophysics</category>
      <category>UV</category>
      <pubDate>Mon, 04 Jun 2018 11:29:00 GMT</pubDate>
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    </item>
    <item>
      <title>Unstable low-mass planetary systems as drivers of white dwarf pollution</title>
      <link>https://academic.oup.com/mnras/article-abstract/476/3/3939/4893726</link>
      <description>&lt;p&gt;A new study examining white dwarf pollution, and featuring contributions from CEH members Dimitri Veras and Boris G&#228;nsicke, concludes that if planet-planet scattering is responsible for the phenomenon then many such objects can be expected to host (currently undetectable) super-Earth planets on orbits of several au and beyond.&lt;/p&gt;

&lt;p&gt;This work was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 476, Issue 3, p.3939-3955&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;Open access link: &lt;/strong&gt;&lt;a href="https://arxiv.org/pdf/1711.02940.pdf" target="_blank" rel="noopener"&gt;arXiv&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved:&lt;/strong&gt; Dimitri Veras &amp;amp; Boris G&#228;nsicke&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>University of Warwick</category>
      <category>Exoplanets</category>
      <category>CEHpublication</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <category>astrophysics</category>
      <category>White Dwarf</category>
      <category>scattering</category>
      <pubDate>Mon, 04 Jun 2018 11:22:00 GMT</pubDate>
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    </item>
    <item>
      <title>Implications of the interstellar object 1I/'Oumuamua for planetary dynamics and planetesimal formation</title>
      <link>https://academic.oup.com/mnras/article/476/3/3031/4909830</link>
      <description>&lt;p&gt;A new study, involving CEH member Dimitri Veras, examines the implications fo newly discovered solar system interloper 'Oumuamua for hypotheses of planetary dynamics.&lt;/p&gt;

&lt;p&gt;This work was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 476, Issue 3, p.3031-3038&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved:&lt;/strong&gt; Dimitri Veras&lt;/p&gt;</description>
      <category>publication</category>
      <category>CEH</category>
      <category>CEHpublication</category>
      <category>asteroids</category>
      <category>planetesimals</category>
      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <pubDate>Mon, 04 Jun 2018 11:17:00 GMT</pubDate>
      <guid isPermaLink="false">8a17841b63b1a2bb0163ca84145119aa</guid>
    </item>
    <item>
      <title>The Next Generation Transit Survey (NGTS)</title>
      <link>https://academic.oup.com/mnras/article/475/4/4476/4597999</link>
      <description>&lt;div class="news-thumbnail" style="float: left; margin-right: 10px; margin-bottom: 5px;"&gt;&lt;img class="thumbnail" width="100" height="100" src="https://warwick.ac.uk/sitebuilder2/file/fac/sci/physics/research/astro/ceh/news?sbrPage=%2Ffac%2Fsci%2Fphysics%2Fresearch%2Fastro%2Fceh%2Fnews&amp;newsItem=8a17841a63b1a45a0163ca7a33950d10" alt="image"&gt;&lt;/div&gt;&lt;p&gt;CEH member Peter Wheatley, PI of the NGTS transiting exoplanet survey, has published a paper describing the project.&lt;/p&gt;

&lt;p&gt;This work was published in &lt;strong&gt;Monthly Notices of the Royal Astronomical Society, Volume 475, Issue 4, p.4476-4493&lt;/strong&gt;&lt;/p&gt;

&lt;p&gt;&lt;strong&gt;CEH members involved: &lt;/strong&gt;Peter Wheatley (lead), Richard West, Don Pollacco, James McCormac, David Armstrong, Emma Foxell, Boris G&#228;nsicke, James Jackman &amp;amp; Tom Louden&lt;/p&gt;</description>
      <category>publication</category>
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      <category>MNRAS</category>
      <category>Centre for Exoplanets and Habitability</category>
      <category>astronomy</category>
      <category>astrophysics</category>
      <pubDate>Mon, 04 Jun 2018 11:06:00 GMT</pubDate>
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