Common Book Selection: Game of Thrones Edition

Citation: Coleman, T. and Vaughan, M. (201). Common Book Selection: Game of Thrones Edition. 37th Annual Conference on the First-Year Experience, San Antonio, TX.Selecting a common book can feel like a battle for the Iron Throne. To ensure that our book isn't chosen by the faction with the biggest dragon (power) or biggest cache of gold (resources), we employ various strategies to ensure the rightful heir is crowned the ruler of Westeros (K-State). This session provides an insight into the committee selection, data collection processes, and qualitative coding used to determine the final book. We'll share specific strategies that have helped us keep our selection process equitable while validating our claim to the throne and avoiding tyrant kings

Your Journey to First-Year Success: A K-State First Companion Textbook

This textbook companion is a resource to help students successfully navigate through their first year at Kansas State University. It serves as part of the K-State First mission to create an outstanding university experience for every first-year student by helping with the transition to college-level learning and college life. The textbook helps improve chances for student success by focusing on fostering campus community, offering resources for diverse activities, highlighting academic expectations, and empowering students with personal responsibility and social agency. Instructors are encouraged to use the textbook in their K-State First classes, and it is also offered as a direct resource for students. In any university setting there are often unwritten rules that students are expected to understand, and this guide addresses and answers those questions directly. Ultimately, this guide encourages students to be engaged learners and to enjoy all facets of education, both inside and outside the classroom.https://newprairiepress.org/ebooks/1019/thumbnail.jp

Integrated photonic-based coronagraphic systems for future space telescopes

The detection and characterization of Earth-like exoplanets around Sun-like stars is a primary science motivation for the Habitable Worlds Observatory. However, the current best technology is not yet advanced enough to reach the 10^-10 contrasts at close angular separations and at the same time remain insensitive to low-order aberrations, as would be required to achieve high-contrast imaging of exo-Earths. Photonic technologies could fill this gap, potentially doubling exo-Earth yield. We review current work on photonic coronagraphs and investigate the potential of hybridized designs which combine both classical coronagraph designs and photonic technologies into a single optical system. We present two possible systems. First, a hybrid solution which splits the field of view spatially such that the photonics handle light within the inner working angle and a conventional coronagraph that suppresses starlight outside it. Second, a hybrid solution where the conventional coronagraph and photonics operate in series, complementing each other and thereby loosening requirements on each subsystem. As photonic technologies continue to advance, a hybrid or fully photonic coronagraph holds great potential for future exoplanet imaging from space.Comment: Conference Proceedings of SPIE: Techniques and Instrumentation for Detection of Exoplanets XI, vol. 12680 (2023

Visible extreme adaptive optics on extremely large telescopes: Towards detecting oxygen in Proxima Centauri b and analogs

Looking to the future of exo-Earth imaging from the ground, core technology developments are required in visible extreme adaptive optics (ExAO) to enable the observation of atmospheric features such as oxygen on rocky planets in visible light. UNDERGROUND (Ultra-fast AO techNology Determination for Exoplanet imageRs from the GROUND), a collaboration built in Feb. 2023 at the Optimal Exoplanet Imagers Lorentz Workshop, aims to (1) motivate oxygen detection in Proxima Centauri b and analogs as an informative science case for high-contrast imaging and direct spectroscopy, (2) overview the state of the field with respect to visible exoplanet imagers, and (3) set the instrumental requirements to achieve this goal and identify what key technologies require further development.Comment: SPIE Proceeding: 2023 / 12680-6

I Have Many Skills: Becoming the Xena of Teaching Modalities

While COVID-19 cases rose throughout the spring and summer months, faculty were expected to create flexible and engaging online learning environments, as many understood that courses would not represent the common classroom experience that students hope for as they begin college. Much like the titular warrior princess Xena, who faced overwhelming challenges and honed her impressive multitude of skills, faculty quickly learned and integrated new online teaching strategies and created varying new course modalities. Together we’ll explore the skills we’ve built and challenges we’ve faced that can be integrated into first-year courses moving forward through pandemic teaching and beyond

Archiving (for) the Future: Creating First-Year Experience Programs Digital Archives

Citation: Coleman, T. L., Eiselein, G., Vaughan, M. (2017). Archiving (for) the Future: Creating First-Year Experience Programs Digital Archives. 36th Annual Conference on the First-Year Experience, Atlanta, GA.K-State First is often contacted by schools interested in creating a first-year experience program. Between outside requests and internal needs, we decided to establish an archive in Kansas State University's institutional repository. We store, preserve, and showcase our work creating and maintaining our program in this archive. This session will provide an overview of how FYE programs can create their own digital archives documenting their programs' histories and successes. We will share concrete examples of K-State's decisions, the process of creating our Digital FYE archive, and we will provide recommendations for programs wanting to create their own archives

Visible extreme adaptive optics on extremely large telescopes: towards detecting oxygen in Proxima Centauri b and analogs

International audienceLooking to the future of exo-Earth imaging from the ground, core technology developments are required in visible Extreme Adaptive Optics (ExAO) to enable the observation of atmospheric features such as oxygen on rocky planets in visible light. UNDERGROUND (Ultra-fast AO techNology Determination for Exoplanet imageRs from the GROUND), a collaboration built in Feb. 2023 at the Optimal Exoplanet Imagers Lorentz Workshop, aims to (1) motivate oxygen detection in Proxima Centauri b and analogs as an informative science case for high-contrast imaging and direct spectroscopy, (2) overview the state of the field with respect to visible exoplanet imagers, and (3) set the instrumental requirements to achieve this goal and identify what key technologies require further development

Chasing rainbows and ocean glints: Inner working angle constraints for the Habitable Worlds Observatory

International audienceNASA is engaged in planning for a Habitable Worlds Observatory (HabWorlds ), a coronagraphic space mission to detect rocky planets in habitable zones and establish their habitability. Surface liquid water is central to the definition of planetary habitability. Photometric and polarimetric phase curves of starlight reflected by an exoplanet can reveal ocean glint, rainbows, and other phenomena caused by scattering by clouds or atmospheric gas. Direct imaging missions are optimized for planets near quadrature, but HabWorlds ' coronagraph may obscure the phase angles where such optical features are strongest. The range of accessible phase angles for a given exoplanet will depend on the planet's orbital inclination and/or the coronagraph's inner working angle (IWA). We use a recently created catalog relevant to HabWorlds of 164 stars to estimate the number of exo-Earths that could be searched for ocean glint, rainbows, and polarization effects due to Rayleigh scattering. We find that the polarimetric Rayleigh scattering peak is accessible in most of the exo-Earth planetary systems. The rainbow due to water clouds at phase angles of ~20○ - 60○ would be accessible with HabWorlds for a planet with an Earth equivalent instellation in ~46 systems, while the ocean glint signature at phase angles of ~130○ - 170○ would be accessible in ~16 systems, assuming an IWA = 62 mas (3λ/D). Improving the IWA = 41 mas (2λ/D) increases accessibility to rainbows and glints by factors of approximately 2 and 3, respectively. By observing these scattering features, HabWorlds could detect a surface ocean and water cycle, key indicators of habitability