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Church, monastery of St. Edwige - Wahlstatt, Poland
No full textChurch and Monastery of St. Edwige In Wahlstatt, Poland Drawing by Lee Govato
Line-by-line sensitivity to activity in M dwarf [Dataset]
No full textRadial velocities (RVs) measured from high-resolution stellar spectra are routinely used to detect and characterise orbiting exoplanet companions. The different lines present in stellar spectra are created by several species, which are non-uniformly affected by stellar variability features such as spots or faculae. Stellar variability distorts the shape of the spectral absorption lines from which precise RVs are measured, posing one of the main problems in the study of exoplanets. In this work we aim to study how the spectral lines present in M dwarfs are independently impacted by stellar activity. We use CARMENES optical spectra of six active early- and mid-type M dwarfs to compute line-by-line RVs and study their correlation with several well-studied proxies of stellar activity. We are able to classify spectral lines based on their sensitivity to activity in five M dwarfs displaying high levels of stellar activity. We further use this line classification to compute RVs with activity-sensitive lines and less sensitive lines, enhancing or mitigating stellar activity effects in the RV time series. For specific sets of the least activity-sensitive lines, the RV scatter decreases by ~2 to 5 times the initial one, depending on the star. Finally, we compare these lines in the different stars analysed, finding the sensitivity to activity to vary from star to star. Despite the high density of lines and blends present in M dwarf stellar spectra, we find that a line-by-line approach is able to deliver precise RVs. Line-by-line RVs are also sensitive to stellar activity effects, and allow for an accurate selection of activity- insensitive lines to mitigate activity effects in RV. However, we find stellar activity effects to vary in the same insensitive lines from star to star.Tables containing information about the sensitivity to activity of the different lines, one table for each of the six stars studied in this work. Each table includes the central wavelength of the line as measured in the spectral template used, the scatter of the line RV, and the Pearson's correlation coefficient R obtained for the correlation between the line RV and the three activity indicators considered (i.e. three different R values, one per indicator). We note that even though we use the term line, these 'lines' correspond to minima in the spectrum and are the result of blends of true atomic lines or features in molecular bands.Financial support from the Severo Ochoa grant CEX2021-001131-S funded by MCIN/AEI/ 10.13039/501100011033N
De cautione usufructuaria
No full textquam ... pro summis in utroque iure honoribus ... doctoralibus rite impetrandis publicae censurae submittit Albertus à Line Bremensis, ad diem 17. Aprilis, anni M DC LXVNicht identisch mit VD17 7:639955P (dort: körperschaftl. Widmungsempfänger auf Titelblattrückseite)Enth. 40 ThesenDiss. iur. Basel, 166
Line-by-line sensitivity to activity in M dwarfs
No full textContext. Radial velocities (RVs) measured from high-resolution stellar spectra are routinely used to detect and characterise orbiting exoplanet companions. The different lines present in stellar spectra are created by several species, which are non-uniformly affected by stellar variability features such as spots or faculae. Stellar variability distorts the shape of the spectral absorption lines from which precise RVs are measured, posing one of the main problems in the study of exoplanets. Aims. In this work we aim to study how the spectral lines present in M dwarfs are independently impacted by stellar activity. Methods. We used CARMENES optical spectra of six active early- and mid-type M dwarfs to compute line-by-line RVs and study their correlation with several well-studied proxies of stellar activity. Results. We are able to classify spectral lines based on their sensitivity to activity in five M dwarfs displaying high levels of stellar activity. We further used this line classification to compute RVs with activity-sensitive lines and less sensitive lines, enhancing or mitigating stellar activity effects in the RV time series. For specific sets of the least activity-sensitive lines, the RV scatter decreases by ~2 to 5 times the initial one, depending on the star. Finally, we compare these lines in the different stars analysed, finding the sensitivity to activity to vary from star to star. Conclusions. Despite the high density of lines and blends present in M dwarf stellar spectra, we find that a line-by-line approach is able to deliver precise RVs. Line-by-line RVs are also sensitive to stellar activity effects, and they allow for an accurate selection of activity-insensitive lines to mitigate activity effects in RV. However, we find stellar activity effects to vary in the same insensitive lines from star to star
Robert C. Line, Jr. and Ann M. Line Interview, February 10, 2005
No full textRobert Line discusses his family history, including his father’s move from Nebraska to Columbus, Montana and his paternal grandfather’s work as a rural doctor, drugstore owner, and community leader. He describes his father’s World War II service, including his time stationed in Germany, the changes made to the family drugstore after the war, and the summer camp his parents started to host children displaced by war. Line also discusses his maternal grandmother’s involvement in the University Church Women and the Cosmos Club in Missoula, Montana, and his mother’s relationship with Jeannette Rankin and the peace movement. Both Robert and Ann describe the personal and business content of their letter collection.https://scholarworks.umt.edu/linefamily_interviews/1000/thumbnail.jp
The construction of Karen Karnak: The multi-author-function
No full textThis thesis is situated within the comparatively recent developments of Web 2.0 and the emergence of interactive WikiMedia, and explores the mode of authorship within a Read/Write culture compared to that of a Read/Only tradition. The hypothesis of this study is that the role of the audience has become merged with the author, and as such, represents new functions and attributes, distinct from a more conventional concept of authorship, in which the roles of audience and author are more separate. Read/Write and participatory culture, as defined by this study, is focused on collaboration, and includes the influences of D.I.Y. culture, Open-Source practices and the production of text by multiple authors. Multi-authorship presents a re-thinking of several concepts which support the notion of the individual author, since the focus of multi-authorship is not on attribution and ownership of a finished text, but on the continued malleability of a text. Modes of multi-authorship, demonstrated in the use of the pseudonyms Alan Smithee and Karen Eliot, represent declarative authors whose names signify multiple origins, whilst concurrently indicating a distinct body of work. The function of these names form an important context to this study, since primary research involves the construction of an experimental mode of multi-authorship utilising WikiMedia technology and the interaction of thirty nine participants, who are invited to create a body of work under the collective pseudonym Karen Karnak. The data generated by this experiment is analysed using aspects of Michel Foucault's author-function to identify and determine power structures inherent in the WikiMedia context. The interplay of power structures, including concepts such as identity, ownership and the body of work, affect the resulting mode of authorship and contribute to the construction of Karen Karnak, suggesting further areas of research into the emerging multi-author
Oregon Short Line Railroad ; Installation of "D&M" Cleaning Machine for Cleaning Locomotives ; Pocatello, Idaho
No full textblack and white and colored drawing of Oregon Short Line Railroad Installation of "D&M" Cleaning Machine for Cleaning Locomotives ; Pocatello, Idah
Inbred sorghum line 'R07007'
No full textAn inbred sorghum line, designated R07007, is disclosed. The invention relates to the seeds of inbred sorghum line R07007, to the plants of inbred sorghum line R07007 and to methods for producing a sorghum plant by crossing the inbred line R07007 with itself or another sorghum line. The invention further relates to hybrid sorghum seeds and plants produced by crossing the inbred line R07007 with another sorghum line. The invention further relates to methods for producing a sorghum plant containing in its genetic material one or more transgenes and to the transgenic plants produced by that method and to methods for producing other inbred sorghum lines derived from the inbred R07007.U
Dr. Jo Line: Redefining Leadership in Sports Through Co-Action
No full textRuntime 36:10Join Dr. Nicole M. LaVoi as she discusses with Dr. Jo Line their transformative concept of co-action in sports teams. This episode covers how Dr. Line’s research and practical applications challenge traditional leadership models, aiming to cultivate equity and collaboration within sports teams. Dr. Jo Line Website (https://jolinephd.com/) & Hiram College Profile (https://www.hiram.edu/faculty-and-staff/joanna-line). Athlete Ally (https://www.athleteally.org/)
Line-start permanent-magnet motor: single-phase starting performance analysis
No full textThis paper presents a detailed quasi-steady-state approach to different torque components (average and pulsating) for a single-phase capacitor-run permanent-magnet (PM) motor. By employing average electromagnetic torque, and the expected envelope of the pulsating torque, an accurate prediction of starting torque components behavior is made. The quasi-steady-state analysis of the asynchronous performance of the single-phase capacitor-start capacitor-run PM motor is realized through a combination of symmetrical components and d-q axes theory. The developed approach is valid for any m-phase AC motor-induction, synchronous reluctance, or synchronous PM
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