{"id":2227,"date":"2024-09-16T06:32:06","date_gmt":"2024-09-16T05:32:06","guid":{"rendered":"https:\/\/pepsi.aip.de\/?p=2227"},"modified":"2024-09-16T06:32:06","modified_gmt":"2024-09-16T05:32:06","slug":"retrieving-young-cloudy-l-dwarfs-a-nearby-planetary-mass-companion-bd60-1417b-and-its-isolated-red-twin-w0047","status":"publish","type":"post","link":"https:\/\/pepsi.aip.de\/?p=2227","title":{"rendered":"Retrieving Young Cloudy L Dwarfs: A Nearby Planetary-mass Companion BD+60 1417B and its Isolated Red Twin W0047"},"content":{"rendered":"\n\n\n<p>We present an atmospheric retrieval analysis on a set of young, cloudy, red L dwarfs\u2014CWISER J124332.12+600126.2 (BD+60 1417B) and WISEP J004701.06+680352.1 (W0047)\u2014using the Brewster retrieval framework. We also present the first elemental abundance measurements of the young K-dwarf (K0) host star, BD+60 1417, using high-resolution (R = 50,000) spectra taken with the Potsdam Echelle Polarimetric and Spectroscopic Instrument on the Large Binocular Telescope. In the complex cloudy L-dwarf regime the emergence of condensate cloud species complicates retrieval analysis when only near-infrared data are available. We find that for both L dwarfs in this work, despite testing three different thermal profile parameterizations we are unable to constrain reliable abundance measurements and thus the carbon-to-oxygen ratio. While we cannot conclude what the abundances are, we can conclude that the data strongly favor a cloud model over a cloudless model. We note that the difficulty in retrieval constraints persists regardless of the signal-to-noise ratio of the data examined (S\/N \u223c 10 for CWISER BD+60 1417B and 40 for WISEP W0047). The results presented in this work provide valuable lessons about retrieving young, low-surface-gravity cloudy L dwarfs. This work provides continued evidence of missing information in models and the crucial need for JWST to guide and inform retrieval analysis in this regime.<\/p>\n\n\n\n<figure id=\"attachment_2226\" aria-describedby=\"caption-attachment-2226\" style=\"width: 2002px\" class=\"wp-caption alignnone\"><a href=\"https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-2226\" src=\"https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr.jpg\" alt=\"\" width=\"2002\" height=\"517\" srcset=\"https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr.jpg 2002w, https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr-300x77.jpg 300w, https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr-1024x264.jpg 1024w, https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr-768x198.jpg 768w, https:\/\/pepsi.aip.de\/wp-content\/uploads\/2024\/09\/apjad5d57f1_hr-1536x397.jpg 1536w\" sizes=\"auto, (max-width: 2002px) 100vw, 2002px\" \/><\/a><figcaption id=\"caption-attachment-2226\" class=\"wp-caption-text\">PEPSI spectra of BD+60 1417 in selected wavelength regions of 7687\u20137695 \u00c5 (left), 7770\u20137778 \u00c5 (center), and 8770\u20138777 \u00c5 (right). Line features used in the abundance analysis have been labeled.<\/figcaption><\/figure>\n\n\n\n<p>Read more:\u00a0 <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2024ApJ...972..172P\/abstract\">Phillips et al. 2024, ApJ, 972, 172 <\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>We present an atmospheric retrieval analysis on a set of young, cloudy, red L dwarfs\u2014CWISER J124332.12+600126.2 (BD+60 1417B) and WISEP J004701.06+680352.1 (W0047)\u2014using the Brewster retrieval framework. We also present the first elemental abundance measurements of the young K-dwarf (K0) host star, BD+60 1417, using high-resolution (R = 50,000) spectra taken with the Potsdam Echelle Polarimetric &hellip; <a href=\"https:\/\/pepsi.aip.de\/?p=2227\" class=\"more-link\">Continue reading <span class=\"screen-reader-text\">Retrieving Young Cloudy L Dwarfs: A Nearby Planetary-mass Companion BD+60 1417B and its Isolated Red Twin W0047<\/span> <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":5,"featured_media":0,"comment_status":"closed","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[11],"tags":[],"class_list":["post-2227","post","type-post","status-publish","format-standard","hentry","category-publications"],"_links":{"self":[{"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=\/wp\/v2\/posts\/2227","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=\/wp\/v2\/users\/5"}],"replies":[{"embeddable":true,"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=2227"}],"version-history":[{"count":1,"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=\/wp\/v2\/posts\/2227\/revisions"}],"predecessor-version":[{"id":2228,"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=\/wp\/v2\/posts\/2227\/revisions\/2228"}],"wp:attachment":[{"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2227"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=2227"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/pepsi.aip.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=2227"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}