The Student Movement Volume 107 Issue 20: Andrews Students Spring Back from Break: Six More Weeks to Go

HUMANS Meeting Dr. McCree, Interviewed by: Grace No Interview with Dr. Luxton: Saying Goodbye, Interviewed by: Grace No Spring Break Renovations & Relaxation, Caryn Cruz ARTS & ENTERTAINMENT Currently: The Last of Us, Solana Campbell Spring Break Spotlight, Amelia Stefanescu What Happened to Wang in the Costco Bathroom?, Nora Martin NEWS Experiences Living in Lamson Hall, Abigail Kim Time is Ticking for TikTok, Brendan Oh WEAAU x CFE Service Sabbath, Terika Williams IDEAS Inequality Drags on in Tennessee, Alexander J. Hess On Value: True Crime and the Search for Meaning, Nora Martin When Winds Change: The Legacy of President Luxton, Bella Hamann PULSE A Trip to the Museo , Chris Ngugi AUSA Senates Holds Bon Appétit Forum, Neesa Richards Speaking Up With Women Press Release, Nicholas C. Gunn LAST WORD A Week of Rest and Relaxation ... Almost, Grace Nohttps://digitalcommons.andrews.edu/sm-107/1019/thumbnail.jp

Improving the normalization of complex interventions: measure development based on normalization process theory (NoMAD): study protocol

<b>Background</b> Understanding implementation processes is key to ensuring that complex interventions in healthcare are taken up in practice and thus maximize intended benefits for service provision and (ultimately) care to patients. Normalization Process Theory (NPT) provides a framework for understanding how a new intervention becomes part of normal practice. This study aims to develop and validate simple generic tools derived from NPT, to be used to improve the implementation of complex healthcare interventions.<p></p> <b>Objectives</b> The objectives of this study are to: develop a set of NPT-based measures and formatively evaluate their use for identifying implementation problems and monitoring progress; conduct preliminary evaluation of these measures across a range of interventions and contexts, and identify factors that affect this process; explore the utility of these measures for predicting outcomes; and develop an online users’ manual for the measures.<p></p> <b>Methods</b> A combination of qualitative (workshops, item development, user feedback, cognitive interviews) and quantitative (survey) methods will be used to develop NPT measures, and test the utility of the measures in six healthcare intervention settings.<p></p> <b>Discussion</b> The measures developed in the study will be available for use by those involved in planning, implementing, and evaluating complex interventions in healthcare and have the potential to enhance the chances of their implementation, leading to sustained changes in working practices

Unification of Luminous Type 1 Quasars through CIV Emission

Using a sample of 30,000 quasars from SDSS-DR7, we explore the range of properties exhibited by high-ionization, broad emission lines, such as CIV 1549. Specifically we investigate the anti-correlation between L_UV and emission line EQW (the Baldwin Effect) and the "blueshifting" of high-ionization emission lines. The blueshift of the CIV emission line is nearly ubiquitous, with a mean shift of 810 km/s for radio-quiet (RQ) quasars and 360 km/s for radio-loud (RL) quasars, and the Baldwin Effect is present in both RQ and RL samples. Composite spectra are constructed as a function of CIV emission line properties in attempt to reveal empirical relationships between different line species and the SED. Within a two-component disk+wind model of the broad emission line region (BELR), where the wind filters the continuum seen by the disk component, we find that RL quasars are consistent with being dominated by the disk component, while BALQSOs are consistent with being dominated by the wind component. Some RQ objects have emission line features similar to RL quasars; they may simply have insufficient black hole (BH) spin to form radio jets. Our results suggest that there could be significant systematic errors in the determination of L_bol and BH mass that make it difficult to place these findings in a more physical context. However, it is possible to classify quasars in a paradigm where the diversity of BELR parameters are due to differences in an accretion disk wind between quasars (and over time); these differences are underlain primarily by the SED, which ultimately must be tied to BH mass and accretion rate.Comment: 51 pages, 18 figures, accepted by AJ, revised version includes various modifications based on the referee's comment

The Student Movement Volume 107 Issue 7: Hot Drinks & Hayrides: Barn Party Comes to Campus

HUMANS Meet David Springer: AUGSA President, Interviewed by: Kavya Mohanram Meet Rock Choi: AUSA Presidential Assistant, Interviewed by: Anna Pak Women in Stem: Minseo Kang, Interviewed by: Anna Pak ARTS & ENTERTAINMENT Creatives on Campus: Passion Through A New Lens, Amelia Stefanescu Currently..., Solana Campbell Fatphobic or Sensitive?, Lily Rodriguez Take 3: Is Love Truly Blind?, Hannah Cruse NEWS AUSA & AFIA End Filipino American History Month On A High Note, Nicholas C. Gunn AUSA Hosts Barn Party, Alannah Tjhatra Honors Outing to Chicago Shakespeare Theater, Nora Martin IDEAS Reader\u27s Digest: Midterm Election, Terika Willliams The Death of the Rom-Com, Grace No When Art and Activism Collide, Valerie Akinyi PULSE Cafe Cutlery: What\u27s the Deal with the Dishwasher?, Ralph Gifford Dress Code?, Abraham Bravo Homesick, Gloria Oh How to Have a Devotional Life as a College Student, Melissa Moore LAST WORD Andrews University: Diverse But Divided?, Alannah Tjhatrahttps://digitalcommons.andrews.edu/sm-107/1006/thumbnail.jp

The Student Movement Volume 107 Issue 8: Cuffing Season, Co-Curriculars, and CTC Telehealth: The Student Movement Highlights Important Issues on Campus

HUMANS CTC Prevention Coordinator/Staff Counselor Interview: Nycole Goldberg, Interviewed by: Lauren Kim Meet Ellie Dovich: Cast/Cardinal Lead Editor, Interviewed by: Nora Martin Women in Stem: A Peek into Physics, Interviewed by: Caryn Cruz ARTS & ENTERTAINMENT Creatives on Campus: Art via Insta, Ceiry Flores Currently..., Solana Campbell Spotlight: The Parent Trap, Skyler Campbell NEWS AUSA Senate News Update, November 2022, Neesa Richards, AUSA Senate Public Relations Officer Governor Whitmer Takes A Stop In Benton Harbor, Nicholas C. Gunn Home Season Opener, Solana Campbell Hopes and Plans Behind the Seminary Center of Community Change, Interviewed by: Gloria Oh The Days Speak on Veterans Day, Andrew Francis IDEAS T Spills the Tea on Co-Curriculars, T Bruggemann To Bee or not to Bee: The Importance, Causes, and Impact of Bee Disappearance, Alexander Navarro Ye Being an Issue Once Again!, Jonathon Woolford-Hunt PULSE A Dive into Lamson Hall Maintenance, Scott Moncrieff Condemned: Horror Stories from Lamson Hall, Joseph Keough Marriage From Our Point of View, Gloria Oh Reflections on the Soccer Season, Brendan Syto LAST WORD Reflection on Writing Poetry, Alannah Tjhatrahttps://digitalcommons.andrews.edu/sm-107/1007/thumbnail.jp

Acoustic scale from the angular power spectra of SDSS-III DR8 photometric luminous galaxies

We measure the acoustic scale from the angular power spectra of the Sloan Digital Sky Survey III (SDSS-III) Data Release 8 imaging catalog that includes 872,921 galaxies over ~ 10,000 deg^2 between 0.45<z<0.65. The extensive spectroscopic training set of the Baryon Oscillation Spectroscopic Survey (BOSS) luminous galaxies allows precise estimates of the true redshift distributions of galaxies in our imaging catalog. Utilizing the redshift distribution information, we build templates and fit to the power spectra of the data, which are measured in our companion paper, Ho et al. 2011, to derive the location of Baryon acoustic oscillations (BAO) while marginalizing over many free parameters to exclude nearly all of the non-BAO signal. We derive the ratio of the angular diameter distance to the sound horizon scale D_A/r_s= 9.212 + 0.416 -0.404 at z=0.54, and therefore, D_A= 1411+- 65 Mpc at z=0.54; the result is fairly independent of assumptions on the underlying cosmology. Our measurement of angular diameter distance D_A is 1.4 \sigma higher than what is expected for the concordance LCDM (Komatsu et al. 2011), in accordance to the trend of other spectroscopic BAO measurements for z >~ 0.35. We report constraints on cosmological parameters from our measurement in combination with the WMAP7 data and the previous spectroscopic BAO measurements of SDSS (Percival et al. 2010) and WiggleZ (Blake et al. 2011). We refer to our companion papers (Ho et al. 2011; de Putter et al. 2011) for investigations on information of the full power spectrum.Comment: 16 pages, 14 figures, 3 tables, submitted to Ap

The Student Movement Volume 107, Issue 9: Power (Outage) to the People: Students Frolic in Winter Wonderland

HUMANS Interview with the Speech Pathology Club, Interviewed by: Gloria Oh Meet The Chiefs of The Twin Cities, Nicholas C. Gunn Meet the Student Graduate Liaison of AUGSA, Natasha Richards, Interviewed by: Kavya Mohanram What Are AU Students Thankful For?, Interviewed by: Grace No ARTS & ENTERTAINMENT Anthony León Wins Placido Domingo\u27s Operailia 2022, Aiko J. Ayala Rios Currently..., Solana Campbell Thanks for Making Me Laugh: My Top Ten Thanksgiving Sitcom Episodes, Bella Hamann Top Gun Maverick: A SuperSonic Sequel, Leo Martins NEWS Honors Church: Lessons and Carols, Terika Williams Prime Minister after Prime Minister, Abigail Kim The Seatless Delegate: An Unfulfilled Promise to the Cherokee Nation, Julia Randall Innovation & Entrepreneurship: The Sole Full Winner of the Shark Tank Competition, Yoel Kim IDEAS A Reflect ion on Body Image, Elizabeth Getahun The Frenzy of Fast Fashion, Abby Shim The Scoop on Introverts: What Extroverts Need to Know, Isabelle Martinez To Bee or not to Bee: The Importance, Causes, and Impact of Bee Disappearance, Alexander Navarro PULSE All About AU Engage, Lexie Dunham Thoughts on Daylight Savings, Gloria Oh Thanksgiving and Our Heritage, Zothile Sibanda LAST WORD Romanticizing the Past, Alannah Tjhatrahttps://digitalcommons.andrews.edu/sm-107/1008/thumbnail.jp

The Morphology of Galaxies in the Baryon Oscillation Spectroscopic Survey

We study the morphology of luminous and massive galaxies at 0.3<z<0.7 targeted in the Baryon Oscillation Spectroscopic Survey (BOSS) using publicly available Hubble Space Telescope imaging from COSMOS. Our sample (240 objects) provides a unique opportunity to check the visual morphology of these galaxies which were targeted based solely on stellar population modelling. We find that the majority (74+/-6%) possess an early-type morphology (elliptical or S0), while the remainder have a late-type morphology. This is as expected from the goals of the BOSS target selection which aimed to predominantly select slowly evolving galaxies, for use as cosmological probes, while still obtaining a fair fraction of actively star forming galaxies for galaxy evolution studies. We show that a colour cut of (g-i)>2.35 selects a sub-sample of BOSS galaxies with 90% early-type morphology - more comparable to the earlier Luminous Red Galaxy (LRG) samples of SDSS-I/II. The remaining 10% of galaxies above this cut have a late-type morphology and may be analogous to the "passive spirals" found at lower redshift. We find that 23+/-4% of the early-type galaxies are unresolved multiple systems in the SDSS imaging. We estimate that at least 50% of these are real associations (not projection effects) and may represent a significant "dry merger" fraction. We study the SDSS pipeline sizes of BOSS galaxies which we find to be systematically larger (by 40%) than those measured from HST images, and provide a statistical correction for the difference. These details of the BOSS galaxies will help users of the data fine-tune their selection criteria, dependent on their science applications. For example, the main goal of BOSS is to measure the cosmic distance scale and expansion rate of the Universe to percent-level precision - a point where systematic effects due to the details of target selection may become important.Comment: 18 pages, 11 figures; v2 as accepted by MNRA