Revisiting hylomorphism: What can it contribute to our understanding of information systems?

Theorising about digital technology is core to the IS discipline. This paper presents an interpretation of technology using hylomorphism, the theory that material objects comprise both matter and form. A contemporary understanding of hylomorphism argues that the form of an object is dynamic structure, which may be actualised in the process of interacting with other objects. This paper arose out of a critical realist study on the use of technology in the classroom by senior secondary students in New Zealand. The role of theory in critical realism is outlined, and then the findings that stimulated this paper are presented. A brief history of hylomorphism is discussed before moving to the contemporary revival of Aristotelian theories. Some implications of this theory on IS research are presented, including an outline of emergence and methodological considerations

Putting it all together: intrinsic and extrinsic mechanisms governing proteasome biogenesis

Background The 26S proteasome is at the heart of the ubiquitin-proteasome system, which is the key cellular pathway for the regulated degradation of proteins and enforcement of protein quality control. The 26S proteasome is an unusually large and complicated protease comprising a 28-subunit core particle (CP) capped by one or two 19-subunit regulatory particles (RP). Multiple activities within the RP process incoming ubiquitinated substrates for eventual degradation by the barrel-shaped CP. The large size and elaborate architecture of the proteasome have made it an exceptional model for understanding mechanistic themes in macromolecular assembly. Objective In the present work, we highlight the most recent mechanistic insights into proteasome assembly, with particular emphasis on intrinsic and extrinsic factors regulating proteasome biogenesis. We also describe new and exciting questions arising about how proteasome assembly is regulated and deregulated in normal and diseased cells. Methods A comprehensive literature search using the PubMed search engine was performed, and key findings yielding mechanistic insight into proteasome assembly were included in this review. Results Key recent studies have revealed that proteasome biogenesis is dependent upon intrinsic features of the subunits themselves as well as extrinsic factors, many of which function as dedicated chaperones. Conclusion Cells rely on a diverse set of mechanistic strategies to ensure the rapid, efficient, and faithful assembly of proteasomes from their cognate subunits. Importantly, physiological as well as pathological changes to proteasome assembly are emerging as exciting paradigms to alter protein degradation in vivo

Advancing Health Policy and Advocacy Education in Medical School through a Student-run Elective

Introduction: Training medical students in the policy topics of healthcare economics, delivery systems, disparities, and reform helps to prepare them for the growing role of advocacy in medicine. We used a near-peer educational model to create an elective to advance learners’ policy knowledge and advocacy skills, while simultaneously offering student directors hands-on experience in educational program development. Methods: The 4-week elective for fourth year medical students included weekly readings, policy seminars, advocacy workshops, and journal clubs. Longitudinally, students prepared for a policy debate and prepared a research project or Op-Ed article on a healthcare disparity topic of their choice. The elective was designed, coordinated, and implemented by a team of first, second, third, and fourth-year medical students with faculty adviser oversight. Pre- and post-surveys were utilized to assess student learners’ knowledge of subject material and their perceptions of the effectiveness of the curriculum. Student directors self-assessed their confidence with the subject material and acquired skill in educational program development. Results: Student learners (n=6) noted significant improvement in their knowledge of health policy (P=0.0002) and advocacy (P=0.0064). They also reported improvement in several subtopics under policy and advocacy, with significant improvements seen in healthcare reform (P=0.0131) and writing skills (P=0.0099). Student directors (n=4) reported improved skills in curriculum development, educational evaluation, and leadership. Discussion: This novel student-run elective provided effective training in health policy and advocacy that extends beyond traditional curricula in medical school. Employing a near-peer model, the elective offers a sustainable system to educate interested students in these subjects and provide student directors unique experience in medical education. Further evaluation of future iterations will help determine the effectiveness of the curriculum in advancing individual policy and advocacy subtopics to guide future curricular modifications

Analisis dan Perancangan Sistem Akuntansi dengan Model Driven Development (MDD) Pada Konveksi Anemarie

Informasi Akuntansi merupakan salah satu alat untuk mengambil keputusan dalam perusahaan.Sistem Informasi Akuntansi dapat memberikan kemudahan dalam menghasilkan informasi yang akurat, tepat waktu dapat dipahami dan teruji.Selain itu, sistem informasi akuntansi dapat memudahkan siklus operasional perusahaan baik dari pembelian, produksi, sampai penjualan.Maka dari uraian itu, peneliti ingin menganalisis dan merancang sistem informasi akuntansi pada usaha yang tidak memiliki sistem informasi akuntansi dan masih melakukan pencatatan secara manual. Peneliti menggunakan data sistem akuntansi Konveksi Anemarie periode April 2017 dan Model Driven Development untuk merancang Sistem Informasi Akuntansi konveksi Anemarie. Hasil pengembangan Sistem Informasi Akuntansi dengan Model Driven Development ini ialah Desain Model Data dengan Entity Relathionship diagram baik secara keseluruhan maupun per subsistem, Desain model Proses dengan Data Flow Diagram, dan desain model output dengan pembuatan interface dari form yang dibutuhka

The Cdc48 Complex Alleviates the Cytotoxicity of Misfolded Proteins by Regulating Ubiquitin Homeostasis

The accumulation of misfolded proteins is associated with multiple neurodegenerative disorders, but it remains poorly defined how this accumulation causes cytotoxicity. Here, we demonstrate that the Cdc48/p97 segregase machinery drives the clearance of ubiquitinated model misfolded protein Huntingtin (Htt103QP) and limits its aggregation. Nuclear ubiquitin ligase San1 acts upstream of Cdc48 to ubiquitinate Htt103QP. Unexpectedly, deletion of SAN1 and/or its cytosolic counterpart UBR1 rescues the toxicity associated with Cdc48 deficiency, suggesting that ubiquitin depletion, rather than compromised proteolysis of misfolded proteins, causes the growth defect in cells with Cdc48 deficiency. Indeed, Cdc48 deficiency leads to elevated protein ubiquitination levels and decreased free ubiquitin, which depends on San1/Ubr1. Furthermore, enhancing free ubiquitin levels rescues the toxicity in various Cdc48 pathway mutants and restores normal turnover of a known Cdc48-independent substrate. Our work highlights a previously unappreciated function for Cdc48 in ensuring the regeneration of monoubiquitin that is critical for normal cellular function

Four sub-Saturns with dissimilar densities: windows into planetary cores and envelopes

We present results from a Keck/HIRES radial velocity campaign to study four sub-Saturn-sized planets, K2-27b, K2-32b, K2-39b, and K2-108b, with the goal of understanding their masses, orbits, and heavy-element enrichment. The planets have similar sizes (RP=4.5-5.5 ), but have dissimilar masses (MP=16-60 ), implying a diversity in their core and envelope masses. K2-32b is the least massive (MP = 16.5 ± 2.7 M) and orbits in close proximity to two sub-Neptunes near a 3:2:1 period commensurability. K2-27b and K2-39b are significantly more massive at MP = 30.9 ± 4.6 M and MP = 39.8 ± 4.4 M, respectively, and show no signs of additional planets. K2-108b is the most massive at MP = 59.4 ± 4.4 M, implying a large reservoir of heavy elements of about ≈50 . Sub-Saturns as a population have a large diversity in planet mass at a given size. They exhibit remarkably little correlation between mass and size; sub-Saturns range from ≈6-60 M, regardless of size. We find a strong correlation between planet mass and host star metallicity, suggesting that metal-rich disks form more massive planet cores. The most massive sub-Saturns tend to lack detected companions and have moderately eccentric orbits, perhaps as a result of a previous epoch of dynamical instability. Finally, we observe only a weak correlation between the planet envelope fraction and present-day equilibrium temperature, suggesting that photo-evaporation does not play a dominant role in determining the amount of gas sub-Saturns accrete from their protoplanetary disks

Selection on Visual Opsin Genes in Diurnal Neotropical Frogs and Loss of the SWS2 Opsin in Poison Frogs

Amphibians are ideal for studying visual system evolution because their biphasic (aquatic and terrestrial) life history and ecological diversity expose them to a broad range of visual conditions. Here, we evaluate signatures of selection on visual opsin genes across Neotropical anurans and focus on three diurnal clades that are well-known for the concurrence of conspicuous colors and chemical defense (i.e., aposematism): poison frogs (Dendrobatidae), Harlequin toads (Bufonidae: Atelopus), and pumpkin toadlets (Brachycephalidae: Brachycephalus). We found evidence of positive selection on 44 amino acid sites in LWS, SWS1, SWS2, and RH1 opsin genes, of which one in LWS and two in RH1 have been previously identified as spectral tuning sites in other vertebrates. Given that anurans have mostly nocturnal habits, the patterns of selection revealed new sites that might be important in spectral tuning for frogs, potentially for adaptation to diurnal habits and for color-based intraspecific communication. Furthermore, we provide evidence that SWS2, normally expressed in rod cells in frogs and some salamanders, has likely been lost in the ancestor of Dendrobatidae, suggesting that under low-light levels, dendrobatids have inferior wavelength discrimination compared to other frogs. This loss might follow the origin of diurnal activity in dendrobatids and could have implications for their behavior. Our analyses show that assessments of opsin diversification in across taxa could expand our understanding of the role of sensory system evolution in ecological adaptation.</p

Three temperate Neptunes orbiting nearby stars

We present the discovery of three modestly irradiated, roughly Neptune-mass planets orbiting three nearby Solartype stars. HD 42618 b has a minimum mass of 15.4±2.4 M⊕, a semimajor axis of 0.55 au, an equilibrium temperature of 337 K, and is the first planet discovered to orbit the solar analogue host star, HD 42618. We also discover new planets orbiting the known exoplanet host stars HD 164922 and HD 143761 (p CrB). The new planet orbiting HD 164922 has a minimum mass of 12.9±1.6 M⊕ and orbits interior to the previously known Jovian mass planet orbiting at 2.1 au. HD 164922 c has a semimajor axis of 0.34 au and an equilibrium temperature of 418 K. HD 143761 c orbits with a semimajor axis of 0.44 au, has a minimum mass of 25±2 M⊕, and is the warmest of the three new planets with an equilibrium temperature of 445 K. It orbits exterior to the previously known warm Jupiter in the system. A transit search using space-based CoRoT data and ground-based photometry from the Automated Photometric Telescopes (APTs) at Fairborn Observatory failed to detect any transits, but the precise, high-cadence APT photometry helped to disentangle planetary-reflex motion from stellar activity. These planets were discovered as part of an ongoing radial velocity survey of bright, nearby, chromospherically inactive stars using the Automated Planet Finder (APF) telescope at Lick Observatory. The high-cadence APF data combined with nearly two decades of radial velocity data from Keck Observatory and gives unprecedented sensitivity to both short-period low-mass, and long-period intermediate-mass planets

Masses, radii, and orbits of small Kepler planets : The transition from gaseous to rocky planets

We report on the masses, sizes, and orbits of the planets orbiting 22 Kepler stars. There are 49 planet candidates around these stars, including 42 detected through transits and 7 revealed by precise Doppler measurements of the host stars. Based on an analysis of the Kepler brightness measurements, along with high-resolution imaging and spectroscopy, Doppler spectroscopy, and (for 11 stars) asteroseismology, we establish low false-positive probabilities (FPPs) for all of the transiting planets (41 of 42 have an FPP under 1%), and we constrain their sizes and masses. Most of the transiting planets are smaller than three times the size of Earth. For 16 planets, the Doppler signal was securely detected, providing a direct measurement of the planet's mass. For the other 26 planets we provide either marginal mass measurements or upper limits to their masses and densities; in many cases we can rule out a rocky composition. We identify six planets with densities above 5 g cm-3, suggesting a mostly rocky interior for them. Indeed, the only planets that are compatible with a purely rocky composition are smaller than 2 R ⊕. Larger planets evidently contain a larger fraction of low-density material (H, He, and H2O).Peer reviewedFinal Accepted Versio