Software Open Access
<?xml version='1.0' encoding='UTF-8'?> <record xmlns="http://www.loc.gov/MARC21/slim"> <leader>00000nmm##2200000uu#4500</leader> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">H0LiCOW</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">Cosmology</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">Hubble constant</subfield> </datafield> <controlfield tag="005">20200206072052.0</controlfield> <controlfield tag="001">3633035</controlfield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Ecole Polytechnique Fédérale de Lausanne</subfield> <subfield code="0">(orcid)0000-0003-1471-3952</subfield> <subfield code="a">Vivien Bonvin</subfield> </datafield> <datafield tag="856" ind1="4" ind2=" "> <subfield code="s">517178</subfield> <subfield code="z">md5:37520f3f6bb9a9038250761d746033aa</subfield> <subfield code="u">https://zenodo.org/record/3633035/files/H0_inference_code.zip</subfield> </datafield> <datafield tag="542" ind1=" " ind2=" "> <subfield code="l">open</subfield> </datafield> <datafield tag="260" ind1=" " ind2=" "> <subfield code="c">2020-02-05</subfield> </datafield> <datafield tag="909" ind1="C" ind2="O"> <subfield code="p">software</subfield> <subfield code="o">oai:zenodo.org:3633035</subfield> </datafield> <datafield tag="100" ind1=" " ind2=" "> <subfield code="u">Ecole Polytechnique Fédérale de Lausanne</subfield> <subfield code="0">(orcid)0000-0001-7051-497X</subfield> <subfield code="a">Martin Millon</subfield> </datafield> <datafield tag="245" ind1=" " ind2=" "> <subfield code="a">H0LiCOW cosmological parameter sampling software</subfield> </datafield> <datafield tag="536" ind1=" " ind2=" "> <subfield code="c">200020_172712</subfield> <subfield code="a">COSMOGRAIL: Cosmology with Time Delays in Gravitationally Lensed Quasars</subfield> </datafield> <datafield tag="536" ind1=" " ind2=" "> <subfield code="c">787886</subfield> <subfield code="a">Cosmology with Strong Gravitational Lensing</subfield> </datafield> <datafield tag="540" ind1=" " ind2=" "> <subfield code="u">https://creativecommons.org/licenses/by/4.0/legalcode</subfield> <subfield code="a">Creative Commons Attribution 4.0 International</subfield> </datafield> <datafield tag="650" ind1="1" ind2="7"> <subfield code="a">cc-by</subfield> <subfield code="2">opendefinition.org</subfield> </datafield> <datafield tag="520" ind1=" " ind2=" "> <subfield code="a"><p>Python notebook for H<sub>0</sub> inference using H0LiCOW collaboration&#39;s 6-lens distance measurements.&nbsp; The python notebook is also available here:<br> https://github.com/shsuyu/H0LiCOW-public/tree/master/H0_inference_code<br> <br> The posterior distributions of the time-delay distances and angular diameter distances for five of the six lens systems can be downloaded here:<br> https://github.com/shsuyu/H0LiCOW-public/tree/master/h0licow_distance_chains<br> The remaining lens (B1608+656) has an analytical fit to the PDF.</p> <p>If you make use of the distance measurements (time-delay distance and/or lens angular diameter distance) to the 6 lens systems from H0LiCOW, please cite the relevant publications:</p> <ul> <li><a href="https://ui.adsabs.harvard.edu/abs/2010ApJ...711..201S/abstract">Suyu et al. 2010</a> (B1608+656 time-delay distance fit)</li> <li><a href="https://ui.adsabs.harvard.edu/abs/2019Sci...365.1134J/abstract">Jee et al. 2019</a> (B1608+656 angular diameter distance fit)</li> <li><a href="https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.1743C/abstract">Chen et al. 2019</a>, <a href="https://ui.adsabs.harvard.edu/abs/2017MNRAS.465.4895W/abstract">Wong et al. 2017</a> (HE0435-1223 distance posterior)</li> <li><a href="https://ui.adsabs.harvard.edu/abs/2019MNRAS.484.4726B/abstract">Birrer et al. 2019</a> (J1206+4332 distance posterior)</li> <li><a href="https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.1743C/abstract">Chen et al. 2019</a>, <a href="https://ui.adsabs.harvard.edu/abs/2014ApJ...788L..35S/abstract">Suyu et al. 2014</a> (RXJ1131-1231 distance posterior)</li> <li><a href="https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.1743C/abstract">Chen et al. 2019</a> (PG1115+080 distance posterior)</li> <li><a href="https://arxiv.org/abs/1905.09338">Rusu et al. 2019</a> (WFI2033-4723 distance posterior)</li> <li><a href="https://arxiv.org/abs/1907.04869">Wong et al. 2019</a> (combined inference)</li> </ul> <p>The H<sub>0</sub> inference from these posteriors can be obtained following the python notebook.&nbsp; The cosmological parameter chains from running the python notebook are available here:<br> https://github.com/shsuyu/H0LiCOW-public/tree/master/cosmo_parameter_chains</p></subfield> </datafield> <datafield tag="773" ind1=" " ind2=" "> <subfield code="n">url</subfield> <subfield code="i">isDerivedFrom</subfield> <subfield code="a">https://github.com/shsuyu/H0LiCOW-public/tree/master/H0_inference_code</subfield> </datafield> <datafield tag="773" ind1=" " ind2=" "> <subfield code="n">doi</subfield> <subfield code="i">isVersionOf</subfield> <subfield code="a">10.5281/zenodo.3633034</subfield> </datafield> <datafield tag="024" ind1=" " ind2=" "> <subfield code="a">10.5281/zenodo.3633035</subfield> <subfield code="2">doi</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">software</subfield> </datafield> </record>
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