Library Tools for Connecting with the Curriculum

Serving as liaison librarians at the department level, the authors discuss strategies for integrating library and online resources with the curriculum. Examples of technology-based capabilities range from current awareness services, e-reserves, and journal finding applications to smart linking functions that can be built into library catalogs, licensed databases, course syllabi, and tailored research guides. Attendees will be able to increase student engagement with learning resources by using their institution’s library tools more effectively, and by requesting librarian assistance to employ these functions in online research guides and course syllabi

Library Tools for Connecting With the Curriculum: How To Create a Professional Development Workshop for Teaching Faculty

The article focuses on ways taken by librarians in linking library tools with the faculty curriculum in Georgia. It states that librarians Sonya Shepherd, Debra Skinner and Bob Fernekes from Zach S. Henderson Library have formed a team that would push students into library resources required by their faculty. It also mentions the creation of linking tools tutorials to improve student and faculty use of the resources

Information Literacy Instruction and Assessment: College of Business Administration and College of Education, Georgia Southern University

This presentation was given during the Georgia International Conference on Information Literacy

Assessing Information Literacy with Knowledge Surveys: Interim Report from Two Computer-Based Trials

This presentation was given during the Georgia International Conference on Information Literacy

Direct Observations of the Ionizing Star in the UC HII Region G29.96-0.02: A Strong Constraint on the Stellar Birth Line for Massive Stars

We have observed the ultracompact HII region G29.96-0.02 in the near infrared J, H, and K bands and in the Br-gamma line. By comparison with radio observations, we determine that the extinction to the nebula is AK = 2.14 with a 3 sigma uncertainty of 0.25. We identify the ionizing star and determine its intrinsic K magnitude. The star does not have an infrared excess and so appears to be no longer accreting. The K magnitude and the bolometric luminosity allow us to place limits on the location of the ionizing star in the HR diagram. The 3 sigma upper limit on the effective temperature of the ionizing star is 42500 K. We favor a luminosity appropriate for star with a mass in excess of about 60 solar masses. The limit on the temperature and luminosity exclude stars on the ZAMS and stars within 10^6 yr of the ZAMS. Since the age of the UC HII region is estimated to be only about 10^5 yr, we suggest that this is direct evidence that the stellar birth line for massive stars at twice solar metallicity must be significantly redder than the ZAMS.Comment: 42 pages; LaTex; 11 Postscript figures; accepted for publication in Ap

Ionized Gas Towards Molecular Clumps: Physical Properties of Massive Star Forming Regions

We have conducted a search for ionized gas at 3.6 cm, using the Very Large Array, toward 31 Galactic intermediate- and high-mass clumps detected in previous millimeter continuum observations. In the 10 observed fields, 35 H II regions are identified, of which 20 are newly discovered. Many of the H II regions are multiply peaked indicating the presence of a cluster of massive stars. We find that the ionized gas tends to be associated toward the millimeter clumps; of the 31 millimeter clumps observed, nine of these appear to be physically related to ionized gas, and a further six have ionized gas emission within 1'. For clumps with associated ionized gas, the combined mass of the ionizing massive stars is compared to the clump masses to provide an estimate of the instantaneous star formation efficiency. These values range from a few percent to 25%, and have an average of 7% ± 8%. We also find a correlation between the clump mass and the mass of the ionizing massive stars within it, which is consistent with a power law. This result is comparable to the prediction of star formation by competitive accretion that a power-law relationship exists between the mass of the most massive star in a cluster and the total mass of the remaining stars

Spitzer IRAC and MIPS Imaging of Clusters and Outflows in 9 High-mass Star Forming Regions

We present Spitzer Space Telescope IRAC and MIPS observations toward a sample of nine high-mass star forming regions at a distance of around 2 kpc. Based on IRAC and MIPS 24 $\mu$m photometric results and 2MASS JHKs data, we carry out a census of young stellar objects (YSOs) in a 5' by 5' field toward each region. Toward seven out of the nine regions, we detect parsec sized clusters with around 20 YSOs surrounded by a more extended and sparse distribution of young stars and protostars. For the other two regions, IRAS 20126+4104 and IRAS 22172+5549, the former has the lowest number of YSOs in the sample and shows no obvious cluster, and the latter appears to be part of a larger, potentially more evolved cluster. The deep IRAC imaging reveals at least twelve outflows in eight out of the nine regions, with nine outflows prominent in the 4.5 $\mu$m band most probably attributed to shocked H$_2$ emission, two outflows dominated by scattered light in the 3.6 and 4.5 $\mu$m bands, and one outflow standing out from its hydrocarbon emission in the 8.0 $\mu$m band. In comparison with previous ground-based observations, our IRAC observations reveal new outflow structures in five regions. The dramatically different morphologies of detected outflows can be tentatively interpreted in terms of possible evolution of massive outflows. The driving sources of these outflows are deeply embedded in dense dusty cores revealed by previous millimeter interferometric observations. We detect infrared counterparts of these dusty cores in the IRAC or MIPS 24 $\mu$m bands. Reflection nebulae dominated by the emission from UV heated hydrocarbons in the 8 $\mu$m band can be found in most regions and they may imply the presence of young B stars.Comment: 76 pages, 25 figures and 5 tables, ApJ in press, a full resolution version available at http://www.cfa.harvard.edu/~kqiu/spitzer.pd

Decolonizing climate change–heritage research

Climate change poses a threat to heritage globally. Decolonial approaches to climate change–heritage research and practice can begin to address systemic inequities, recognize the breadth of heritage and strengthen adaptation action globally.DATA AVAILABILITY STATEMENT: The underlying dataset for Fig. 1a is available open access from the supplemental material in ref. 5, and datasets for Fig. 1b,c from the UNESCO World Heritage List 2021 in ref. 32.The UK government’s Foreign, Commonwealth & Development Office and the International Development Research Centre, Ottawa, Canada; the FLAIR Fellowship Programme: a partnership between the African Academy of Sciences and the Royal Society funded by the UK government’s Global Challenges Research Fund; the Mapping Africa’s Endangered Archaeological Sites and Monuments project funded by Arcadia — a charitable fund of Lisbet Rausing and Peter Baldwin; the Leverhulme Trust Doctoral Training Scheme, hosted by Southampton Marine and Maritime Institute at the University of Southampton.https://www.nature.com/nclimatehj2023Historical and Heritage Studie

Randomized, Phase II Trial of Pemetrexed and Carboplatin with or without Enzastaurin versus Docetaxel and Carboplatin as First-Line Treatment of Patients with Stage IIIB/IV Non-small Cell Lung Cancer

Enzastaurin is an oral serine/threonine kinase inhibitor that targets protein kinase C-beta (PKC-β) and the phosphatidylinositol-3-kinase/AKT pathway. This trial assessed pemetrexed-carboplatin ± enzastaurin to docetaxel-carboplatin in advanced non-small cell lung cancer.Patients with stage IIIB (with pleural effusion) or IV non-small cell lung cancer and performance status 0 or 1 were randomized to one of the three arms: (A) pemetrexed 500 mg/m and carboplatin area under the curve 6 once every 3 weeks for up to 6 cycles with a loading dose of enzastaurin 1125 or 1200 mg followed by 500 mg daily until disease progression, (B) the same regimen of pemetrexed-carboplatin without enzastaurin, or (C) docetaxel 75 mg/m and carboplatin area under the curve 6 once every 3 weeks for up to six cycles. The primary end point was time to disease progression (TTP).Between March 2006 and May 2008, 218 patients were randomized. Median TTP was 4.6 months for pemetrexed-carboplatin-enzastaurin, 6.0 months for pemetrexed-carboplatin, and 4.1 months for docetaxel-carboplatin (differences not significant). Median survival was 7.2 months for pemetrexed-carboplatin-enzastaurin, 12.7 months for pemetrexed-carboplatin, and 9.2 months for docetaxel-carboplatin (log-rank = 0.05). Compared with the other arms, docetaxel-carboplatin was associated with lower rates of grade 3 thrombocytopenia and anemia but a higher rate of grade 3 or 4 febrile neutropenia.There was no difference in TTP between the three arms, but survival was longer with pemetrexed-carboplatin compared with docetaxel-carboplatin. Enzastaurin did not add to the activity of pemetrexed-carboplatin

Evaluating the Effects of SARS-CoV-2 Spike Mutation D614G on Transmissibility and Pathogenicity.

Global dispersal and increasing frequency of the SARS-CoV-2 spike protein variant D614G are suggestive of a selective advantage but may also be due to a random founder effect. We investigate the hypothesis for positive selection of spike D614G in the United Kingdom using more than 25,000 whole genome SARS-CoV-2 sequences. Despite the availability of a large dataset, well represented by both spike 614 variants, not all approaches showed a conclusive signal of positive selection. Population genetic analysis indicates that 614G increases in frequency relative to 614D in a manner consistent with a selective advantage. We do not find any indication that patients infected with the spike 614G variant have higher COVID-19 mortality or clinical severity, but 614G is associated with higher viral load and younger age of patients. Significant differences in growth and size of 614G phylogenetic clusters indicate a need for continued study of this variant