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HTTP/1.1 200 OKx-amz-id-2: 3qksJR+arRRjDm0JOEZ6oijuTmrbp5suizcnd8Q0MjXsmISWljU3/gjlaUX38qOmAqHVuuGssQcx-amz-request-id: Y5AREPN9NKRJR7AADate: Wed, 03 Dec 2025 01:02:09 GMTLast-Modified: Wed, 14 May 2025 21:23:18 GMTETag: 2611bc8e39c71f62356891e0f23dde5cContent-Type: text/htmlContent-Length: 23373Server: AmazonS3 !-- ////////////////////////////////////////////////////////////////Author: Free-Template.coAuthor URL: http://free-template.co.License: https://creativecommons.org/licenses/by/3.0/License URL: https://creativecommons.org/licenses/by/3.0/Site License URL: https://free-template.co/template-license/ Website: https://free-template.coFacebook: https://www.facebook.com/FreeDashTemplate.coTwitter: https://twitter.com/Free_TemplatecoRSS Feed: https://feeds.feedburner.com/Free-templateco////////////////////////////////////////////////////////////////-->!DOCTYPE html>html langen> head> title>Magnetic Fields in Galaxies — (SALSA Legacy Program)/title> meta charsetutf-8> meta nameviewport contentwidthdevice-width, initial-scale1, shrink-to-fitno> meta namedescription content /> meta namekeywords content /> meta nameauthor content /> link hrefhttps://fonts.googleapis.com/css?familyRoboto:300,400,900|Oswald:300,400,700 relstylesheet> link relstylesheet hreffonts/icomoon/style.css> link relstylesheet hrefcss/bootstrap.min.css> link relstylesheet hrefcss/jquery-ui.css> link relstylesheet hrefcss/owl.carousel.min.css> link relstylesheet hrefcss/owl.theme.default.min.css> link relstylesheet hrefcss/owl.theme.default.min.css> link relstylesheet hrefcss/jquery.fancybox.min.css> link relstylesheet hrefcss/bootstrap-datepicker.css> link relstylesheet hreffonts/flaticon/font/flaticon.css> link relstylesheet hrefcss/aos.css> link relstylesheet hrefcss/style.css> !-- Other head elements --> style> .image-link { display: block; width: 100%; } .publication-image { width: 100%; height: auto; object-fit: cover; } /style> /head> body data-spyscroll data-target.site-navbar-target data-offset300> div classsite-wrap> div classsite-mobile-menu site-navbar-target> div classsite-mobile-menu-header> div classsite-mobile-menu-close mt-3> span classicon-close2 js-menu-toggle>/span> /div> /div> div classsite-mobile-menu-body>/div> /div> header classsite-navbar py-1 js-sticky-header site-navbar-target rolebanner> div classcontainer> div classrow align-items-center> div classcol-5 col-xl-2> h1 classmb-0 site-logo m-0 p-0>a hrefindex.html classmb-0>/a>/h1> /div> div classcol-12 col-md-10 d-none d-xl-block> nav classsite-navigation position-relative text-right rolenavigation> ul classsite-menu main-menu js-clone-nav mr-auto d-none d-lg-block> li>a href#home-section classnav-link>Home/a>/li> li>a href#about-section classnav-link>About/a>/li> li>a href#team-section classnav-link>Team/a>/li> li>a href#data-section classnav-link >Data/a>/li> li>a href#tools-section classnav-link>Tools/a>/li> li>a href#publications-section classnav-link >Publications/a>/li> /ul> /nav> /div> div classcol-6 d-inline-block d-xl-none ml-md-0 py-3>a href# classsite-menu-toggle js-menu-toggle text-white float-right>span classicon-menu h3>/span>/a>/div> /div> /div> /header> div classsite-block-wrap> div classowl-carousel with-dots> div classsite-blocks-cover overlay overlay-2 stylebackground-image: url(images/cenA.png); data-aosfade idhome-section> div classcontainer> div classrow align-items-center justify-content-center> div classcol-md-10 mt-lg-5 text-center> h1 classtext-shadow>Survey of Extragalactic Magnetism with SOFIA/h1> p classmb-5 text-shadow>(SALSA: SOFIA Legacy Program)/p> /div> /div> /div> /div> /div> /div> section classsite-section idabout-section> div classcontainer> div classrow mb-5> div classcol-md-12 text-left> h2 classsection-title mb-3>About/h2> p classlead>This Joint Legacy Program aims to construct a comprehensive empirical picture of the magnetic field strength and structure in the multiphase ISM of galaxies. For the first time, we will construst a FIR polarimetric survey of nearby galaxies. We will combine these results with radio polarimetric and optical spectroscopic observations to obtain magnetic field strength/structure and gas dynamics as a function of host galaxy properties and kpc-scale galactic environment. The wide-field, multi-wavelength polarimetric observations from this Legacy Program will be a transformative leap that will establish the foundational framework of the kpc-scale magnetic field structure in the molecular gas disks of nearby galaxies./p> /div> /div> /div> hr> /section> section classsite-section idteam-section> div classcontainer> div classrow mb-5> div classcol-md-12 text-left> h2 classsection-title mb-3>Team/h2> p classlead>Our team is comprised of an international group of recognized experts in the field of magnetic fields of galaxies, IR and radio polarimetric observations, and Herschel and HAWC+ instrumentation. The primary aim of this team is to maximize the science output of the FIR and radio polarimetric data to understand the magnetic fields in the multi-phase interstellar medium of galaxies. Secondary to the science is a strong commitment to ensuring as appropriate the best possible balance in demographics, including gender, career position, and nationality./p> p classlead>The overall responsibility of this program resides with the two co-PIs, Dr. Enrique Lopez-Rodriguez in the USA and Dr. Sui Ann Mao in Germany, and their Science Working Group./p> div classrow> div classcontainer-fluid> table idtotal votes classtable table-hover text-centered> thead> tr> th>Enrique Lopez-Rodriguez (co-PI)/a>/th> th> Sui Ann Mao (co-PI) /th> /tr> /thead> tbody> tr> td>a hrefhttps://enloro.github.io/website/> img srcimages/ELR.jpg classimg-fluid>/a> /td> td>a hrefhttps://www.mpifr-bonn.mpg.de/person/35556/2169> img srcimages/SAM.jpg classimg-fluid>/a> /td> /tr> tr> td>University of South Carolina/td> td>Max Planck Institute for Radio Astronomy/td> /tr> tr> td>Dr. Lopez-Rodriguez is leading the efforts on the FIR observations, data analysis, and interpretation./td> td>Dr. Mao is leading the efforts on the radio polarimetric observations, data analysis, and interpretation./td> /tr> /tbody> /table>/div> p classlead>The project’s work is structured into several teams, and each team lead reports to the co-PIs. The Science Working Group oversees the efforts to achieve the science goals of this project, and their members inspire and motivate the rest of the team to build linkages between the SOFIA Legacy project and other aspects of the astronomical community. In particular, this includes collaborations with teams from large projects on other observatories (like the nearby galaxy surveys on Spitzer and Herschel) and ongoing closely related work (like ground-based and balloon observations of sub-mm polarization)./p> /div> /div> h3 classlead>Science Working Group/h3> table classtable> thead classthead-light> tr> th scopecol>Member/th> th scopecol>Institution/th> /tr> /thead> tbody> tr> td>Rainer Beck/td> td>Max Planck Institute for Radio Astronomy, Germany/td> /tr> tr> td>John Beckman/td> td>Instituto de Astrofisica de Canarias, Spain/td> /tr> tr> td>Susan Clark/td> td>KIPAC/Stanford University, USA/td> /tr> tr> td>Daniel Dale/td> td>University of Wyoming, USA/td> /tr> tr> td>Tanio Diaz-Santos/td> td>University of Crete, Greece/td> /tr> tr> td>Darren C. Dowell/td> td>JPL, USA/td> /tr> tr> td>Doyal A. Harper/td> td>University of Chicago, USA/td> /tr> tr> td>Annie Hughes/td> td>IRAP, Toulouse, France/td> /tr> tr> td>Pamela Marcum/td> td>NASA Ames Research Center, USA/td> /tr> tr> td>Ignacio Moral Castillo/td> td>Instituto de Astrofisica de Canarias, Spain/td> /tr> tr> td>Sergio Martin Alvarez/td> td>KIPAC/Stanford University, USA/td> /tr> tr> td>Evangelia Ntormousi/td> td>University of Crete, Greece/td> /tr> tr> td>Gina Panopoulou/td> td>Chalmers University/td> /tr> tr> td>William T. Reach/td> td>SOFIA Science Center, USA/td> /tr> tr> td>Julia Roman-Duval/td> td>Space Telescope Science Institute (STScI), USA/td> /tr> tr> td>Kandaswamy Subramanian/td> td>Inter-University Centre for Astronomy and Astrophysics, India/td> /tr> tr> td>Mehrnoosh Tahani/td> td>KIPAC/Stanford University, USA/td> /tr> tr> td>Konstantinos Tassis/td> td>University of Crete, Greece/td> /tr> tr> td>Ngoc Tram Le/td> td>Leiden university, Netherlands/td> /tr> tr> td>Ellen Zweibel/td> td>University of Wisconsin, USA/td> /tr> /tbody>/table> /div> hr> /section> section classsite-section iddata-section> div classcontainer> div classrow mb-2> div classcol-12 text-center> h2 classsection-title mb-1>Data/h2> /div> /div> table classtable> thead classthead-light> tr> th scopecol>Galaxy Sample/th> /tr> /thead> tbody> tr> td>a hrefsingleobjects/antennae.html>Antennae/a>/td> td>a hrefsingleobjects/centaurusA.html>Centaurus A/a>/td> td>a hrefsingleobjects/circinus.html>Circinus/a>/td> td>a hrefsingleobjects/m51.html>M51/a>/td> td>a hrefsingleobjects/m82.html>M82/a>/td> /tr> tr> td>a hrefsingleobjects/m83.html>M83/a>/td> td>a hrefsingleobjects/ngc253.html>NGC 253/a> td>a hrefsingleobjects/ngc1068.html>NGC 1068/a>/td> td>a hrefsingleobjects/ngc1097.html>NGC 1097/a>/td> td>a hrefsingleobjects/ngc2146.html>NGC 2146/a>/td> /tr> tr> td>a hrefsingleobjects/ngc3627.html>NGC 3627/a>/td> td>a hrefsingleobjects/ngc4736.html>NGC 4736/a>/td> td>a hrefsingleobjects/ngc4826.html>NGC 4826/a>/td> td>a hrefsingleobjects/ngc6946.html>NGC 6946/a>/td> td>a hrefsingleobjects/ngc7331.html>NGC 7331/a>/td> /tr> tr> td>a hrefData/Zetas.zip classbtn btn-primary>Zetas (angular dispersion analysis)/a>/td> td>a hrefData/PitchAngles.zip classbtn btn-primary>Pitch Angles (models and radial profiles)/a>/td> /tr> /tbody> /table> /div> hr> /section> section classsite-section idpublications-section> div classcontainer> div classrow mb-2> div classcol-12 text-center> h2 classsection-title mb-3>Publications/h2> /div> /div> div classrow> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a href#data-section classimage-link>img srcimages/SALSAVII/SALSAVII.jpg alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>SALSA VII: A Tomographic View of Far-infrared and Radio Polarimetric Observations through MHD Simulations of Galaxies/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2024ApJ...966...43M/abstract>Martin-Alvarez et al. (2024) /div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a href#data-section classimage-link>img srcimages/Antennae/NGC4038.jpg alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>SALSA VI: The Magnetic Fields in the Multiphase Interstellar Medium of the Antennae Galaxies/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2023ApJ...942L..13L/abstract>Lopez-Rodriguez et al. (2023) /div> div classmeta mb-2>a hrefsingleobjects/antennae.html>Data Available/div> /div> /div> /div> div classrow> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a href#data-section classimage-link>img srcimages/SALSAV/fig1.png alt classimg-fluid publication-image>/a> h2 classfont-size-regular>a classtext-dark>SALSA V: First results on the magnetic field orientation of galaxies/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2023arXiv230313586B/abstract>Borlaff et al. (2023) /div> div classmeta mb-2>a href#data-section>Data Available/div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a href#data-section classimage-link>img srcimages/SALSAIV/fig1.jpg alt classimg-fluid publication-image>/a> h2 classfont-size-regular>a classtext-dark>SALSA IV: Program overview and first results on the polarization fraction/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2022arXiv220501105L/abstract>Lopez-Rodriguez et al. (2022b) /div> div classmeta mb-2>a href#data-section>Data Available/div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a href#data-section >img srcimages/SALSAIII/fig1.jpg alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>SALSA III: First data release and on-the-fly polarization mapping characterization/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2022arXiv220413611L/abstract>Lopez-Rodriguez et al. (2022a) /div> div classmeta mb-2>a href#data-section>Data Available/div> /div> /div> /div> div classrow> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a hrefsingleobjects/ngc1097.html>img srcimages/NGC1097/fig0.gif alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>SALSA II: NGC1097/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2021arXiv210709063L/abstract>Lopez-Rodriguez et al. (2021b) /div> div classmeta mb-2>a hrefsingleobjects/ngc1097.html>Data Available/div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a hrefsingleobjects/m51.html>img srcimages/M51/M51_FIR.png alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>SALSA I: M51/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2021arXiv210509315B/abstract>Borlaff et al. (2021) /div> div classmeta mb-2>a hrefsingleobjects/m51.html>Data Available/div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a hrefsingleobjects/m82.html>img srcimages/M82/M82_ELR.png alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>M82/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2021ApJ...914...24L/abstract> Lopez-Rodriguez et al. (2021a) /a>/div> div classmeta mb-2>a hrefsingleobjects/m82.html>Data Available/div> /div> /div> /div> div classrow> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a hrefsingleobjects/centaurusA.html>img srcimages/CentaurusA/CenA_LIC.png alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>Centaurus A/a>/h2> div classmeta mb-1>a hrefhttps://www.nature.com/articles/s41550-021-01329-9>Lopez-Rodriguez 2021 (Nature Astronomy) /div> div classmeta mb-2>a hrefsingleobjects/centaurusA.html>Data Available/div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a hrefsingleobjects/ngc1068.html>img srcimages/NGC1068/ngc1068_apod.png alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>NGC 1068/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2020ApJ...888...66L/abstract>Lopez-Rodriguez et al. (2020)/a> /div> div classmeta mb-2>a hrefsingleobjects/ngc1068.html>Data Available/a>/div> /div> /div> div classcol-md-6 col-lg-4 mb-4 mb-lg-4> div classh-entry> a hrefsingleobjects/m82.html>img srcimages/m82_apod.jpg alt classimg-fluid>/a> h2 classfont-size-regular>a classtext-dark>M82/a>/h2> div classmeta mb-1>a hrefhttps://ui.adsabs.harvard.edu/abs/2019ApJ...870L...9J/abstract>Jones et al. (2019)/a> /div> div classmeta mb-2>a hrefsingleobjects/m82.html>Data Available/a>/div> /div> /div> /div> /div> hr> /section> section classsite-section bg-light idtools-section> div classcontainer> div classrow mb-5> div classcol-12 text-center> h2 classsection-title mb-3>Tools/h2> /div> p>Python scripts will be available soon./p> table classtable> thead classthead-light> tr> th scopecol>Description/th> th scopecol>Link/th> /tr> /thead> tbody> tr> td>GitHub repository of the Legacy Program/td> td>a hrefhttps://github.com/galmagfields>galmagfields in GitHub/a>/td> /tr> tr> td>Python code used for the analysis of M51/td> td>a hrefhttps://zenodo.org/record/5116134#.YQDfsFNKhTZ>Borlaff et al. (2021; Zenodo link)/a>/td> /tr> tr> td>White paper describing the data format of HAWC+/td> td>a hrefhttps://ui.adsabs.harvard.edu/abs/2018arXiv181103100G/abstract>Gordon et al. (2018)/a>/td> /tr> /table> /div> /div> hr> /section> footer classsite-footer> div classcontainer> div classrow> div classcol-sm-5> div classfooter-widget> h3>Stay in touch/h3> div classfooter-widget-content> a hrefmailto:elopezrodriguez@sc.edu classcontact-link>Enrique Lopez-Rodriguez (elopezrodriguez at sc.edu)/a> a hrefmailto:mao@mpifr-bonn.mpg.de classcontact-link red> Ann Mao (mao at mpifr-bonn.mpg.de)/a> /div> /div> /div> div classcol-sm-6> div classfooter-widget> h3>/h3> div classfooter-widget-content> div classmedia> div classmedia-left> a hrefhttps://www.nasa.gov/>img srcimages/footer/nasa_logo.png alt classimg-thumbnail>/a> /div> div classmedia-left> a hrefhttps://www.sofia.usra.edu/>img srcimages/footer/sofia_logo.png alt classimg-thumbnail>/a> /div> div classmedia-left> a hrefhttps://www.mpifr-bonn.mpg.de/2169/en>img srcimages/footer/mpifr-logo.png alt classimg-thumbnail>/a> /div> /div> /div> /div> /div> /div> /div> !-- Copyright --> div classfooter-copyright text-center py-3>small>© script>document.write(new Date().getFullYear());/script> Magnetic Fields in Galaxies. All Rights Reserved. Design by a hrefhttps://free-template.co target_blank>Free-Template.co/a>/small> /div> !-- Copyright -->/footer>!-- Footer --> !-- .site-wrap --> a href#top classgototop>span classicon-angle-double-up>/span>/a> script srcjs/jquery-3.3.1.min.js>/script> script srcjs/jquery-ui.js>/script> script srcjs/popper.min.js>/script> script srcjs/bootstrap.min.js>/script> script srcjs/owl.carousel.min.js>/script> script srcjs/jquery.countdown.min.js>/script> script srcjs/bootstrap-datepicker.min.js>/script> script srcjs/jquery.easing.1.3.js>/script> script srcjs/aos.js>/script> script srcjs/jquery.fancybox.min.js>/script> script srcjs/jquery.sticky.js>/script> script srcjs/main.js>/script> /body>/html>
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