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The transit method is the most successful tool for exoplanet discovery to date. With more than half of all known exoplanets discovered by \\emph{Kepler} using this method, the mission also revealed a number of objects with dimming events that defy the common explanations, the most prominent being KIC 8462852 aka ``Tabby's star''. I embarked on a search for objects with such irregular transit signatures in the data of K2, the two-wheeled successor mission of \\emph{Kepler}. My method is a combination of automated pre-selection of targets showing downward flux excursions and visual light curve inspection of the selected subset comprising about \\SI{1.5}{\\percent} of the initial sample. In addition, I developed a tool to constrain the effective temperature of a planet-hosting star from photometry alone. This software finds broad application in any science case where a photometric spectral type estimate is necessary. I used existing transit models and Bayesian inference to perform a Markov Chain Monte Carlo (MCMC) analysis of a planetary candidate I discovered. This putative gas giant is in a \\SI{1.32}{\\day} circular orbit with an exceptionally tight orbital radius of $a \\approx 0.012\\,\\mathrm{AU}$. My analysis revealed a scaled planetary radius of $R_\\mathrm{p}/R_\\star = 0.0927\\pm0.0026$ and an edge-on orientation with an inclination $i=89.8\\substack{+3.0 \\\\ -3.4}$. EPIC 217393088.01 is one of the closest-orbiting exoplanets ever detected and the first giant planet with such a small orbital radius. An additional major finding of my search is EPIC 220262993, which exhibits aperiodic, asymmetric dips in flux with rapid dimming rates and up to \\SI{\\sim 25}{\\percent} depth, lasting for \\SIrange{2}{4}{\\day}. In previous works based on optical and mid-infrared photometry, this object was inconsistently classified as a possible quasar or a white dwarf. We conducted follow-up observations both photometrically with GROND on the MPI/ESO \\SI{2.2}{\\meter} telescope in La Silla (Chile) and spectroscopically with FIRE on the Magellan/Baade \\SI{6.5}{\\meter} telescope. With additional spectroscopy using ESI on the Keck \\rom{2} \\SI{10}{\\meter} telescope we were able to distinguish between these cases: EPIC 220262993 is a quasar with redshift $z=1.42$. This is the only known exemplar showing deep dips in flux on such a short time scale.
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Materials can include software, code or scripts, raw or processed data, simulation results, documents, conference posters", "page": "", "title": "Astronomy-General" }, "revision_id": 0, "slug": "astronomy-general", "updated": "2017-05-12T15:04:32.585605+00:00" }, { "access": { "member_policy": "open", "members_visibility": "public", "record_policy": "open", "review_policy": "open", "visibility": "public" }, "children": { "allow": false }, "created": "2015-04-01T20:29:36+00:00", "custom_fields": {}, "deletion_status": { "is_deleted": false, "status": "P" }, "id": "b5023520-b14a-4f06-8085-b5af82c2e0da", "links": {}, "metadata": { "curation_policy": "This collection includes theses and dissertations written to complete Masters or PhD requirements on topics in the fields of astronomy and astrophysics. Other publication types and topics will not be accepted; however, documents that supplement your thesis, such as data sets or videos, are welcome. Although Zenodo accepts all file formats, PDF is strongly preferred for publication submissions. Theses and dissertations written in any language will be accepted, but the metadata record should be created in English. If the NASA ADS has already indexed your thesis, provide us the Bibcode in the Alternate Identifier field before submitting the document.
\r\n", "page": "This community, curated by astronomy librarians, aims to bring together astronomy and astrophysics theses and dissertations. Share the full-text of your cumulative, graduate or PhD level, research with the world by uploading it as open-access to this subject based community. Once added to the community, it can be indexed by ADS, searched for on Zenodo, and browsed to in the community page. The ADS indexes this community once a month.
\r\n\r\nThis thematic, community-wide repository – curated by astronomy librarians and indexed by the NASA ADS – collocates theses and dissertations on astronomy and astrophysics.
\r\n\r\nEven if the ADS already lists your dissertation, you can provide open access to a free, full-text, online version of your own work.
\r\n
\r\nBrowse the collection | Upload your thesis
For detailed instructions on contributing see: our short video walk-through or our written walk-through.
\r\n\r\nPoints to Remember!
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