LG MS 36 Michael Rossetti Collection Finding Aid

Description: Michael Rossetti was chiefly responsible for creating and running Southern Maine Pride, and was the grandmaster at the 2006 Pride festival. The Papers contain records and artifacts documenting Southern Maine Pride and other Gay and Lesbian events from the 1980s to 2000. Date Range: 1980s-2000 Size of Collection: 4 ft

GEN MS 30 Thurston/Corthell Collection Finding Aid

Description: W.J. Corthell was the first principal of the Western State Normal School in Gorham, founded in 1878. The other collector may have been Marjorie Thurston, class of 1907. The Memorabilia consists of artifacts and photographs found in Special Collections. Date Range: 1870s-1907 Size of Collection: 1 ft

LG MS 34 GAYLA Archives Finding Aid

Description: GAYLA is a brotherhood of gay and bisexual men, “expressly designed to provide mutual support, nurturance, friendship, loving, and mentoring of one another,” in order to maximize personal and collective growth. It meets annually for a week in the summer at Ferry Beach in Saco, Maine. The brothers sustain their spirit through the year by organizing periodic winter reunions, area social events and pot-lucks; publishing a newsletter; and establishing a virtual network through email and a GAYLA brothers only Yahoo group. The Archives contains documents and artifacts from the annual conferences, including photographs, audio cassettes, video cassettes, schedules, planning and evaluation papers. Date Range: 1980-2005 Size of Collection: 2 ft

GEN MS 31 Thomas Carper Papers Finding Aid

Description: This collection contains poems, writing logs and published works of poet Thomas Carper. Originally from Cornish, Maine, Carper is a Professor Emeritus who taught poetry and creative writing at USM from 1967 to 1997 and currently divides his time between Maine and France. The Papers include multiple drafts showing revisions of the poem along with the final version. Date Range: 1982-2007 Size of Collection: 2 f

Ligand Substitution of Ruthenium (II) Complexes that Elicit Physical and Chemical Changes

Over the last few years the exploration into ruthenium compounds and the field of coordination chemistry have grown. Ruthenium (II) and ruthenium (III) carry oxidation states that accommodate six-coordinated octahedral configurations in which axial attached ligands can determine chemical and steric properties. UV/Vis spectrometry, H1 NMR, and electrochemical voltammetry will be used to gather data from previously synthesized ruthenium (II) coordination complexes. We hope that by substituting various R groups on three different locations of our ruthenium (II) complex we will be able to control for many physical and chemical changes. After collecting the data from all three complimentary techniques we hope to directly compare E1/2 values, MLCT energies and NMR chemical shifts. Based on the literature we know that there will be a direct relationship between these results based on our chosen substituents

Factors Influencing Physician Treatment Strategies in Crotaline Snake Envenomation

BACKGROUND: Crotaline snake envenomation is a potentially serious medical condition that affects thousands of Americans each year. There continues to be variation in treatment practices by physicians in the United States despite guidelines establishing the use of antivenom and supportive care as the mainstays for treating crotaline snake envenomation. METHODS: This study sought to determine associations between physician treatment strategies, snake identification (ID), venom effects, bite location and patient presentation. A cross-sectional review of electronic medical records (EMR) for patients diagnosed with venomous snake bites from July 1, 2014 to August 31, 2019 was completed. Data collected from the EMR included: patient demographics, transfer information, length of hospital and ICU stays, snake ID, bite site, progression of local tissue effects, additional clinical and lab results, patient comorbidities and complications, and provider treatment strategy. RESULTS: Of the 83 patients who met inclusion criteria, 68 patients (81.9%) received antivenom. None of the 15 patients who were under observation (no antivenom) for treatment went to the ICU. These patients experienced the shortest hospital stays (H(2)=16.76, p<0.001). Hospital stays were longest for patients envenomated by an identified rattlesnake or cottonmouth compared to patients envenomated by an unknown snake or copperhead (H(2)=14.32, p<0.05). Rattlesnake envenomations used more vials of antivenom than copperhead envenomations (H(2)=8.76, p=0.01). In a regression model of treatment strategy, progression of local tissue effects was the only statistically significant predictor of receiving antivenom while other independent variables including snake ID, patient age, hemotoxicity, systemic symptoms, site of the snakebite, and patient comorbidities were not significant predictors. Lastly, there was a statistically significant association between treatment strategy and opioid prescription, with 77.9% of patients who received antivenom also receiving an opioid for pain management vs. 33.3% of patients under observation (no antivenom) who received opioids (Fisher Exact Probability Test, p=0.001). CONCLUSION: Envenomated patients are likely to be treated with antivenom if there was progression of local tissue effects. For patients in this study who were bitten by copperheads and unknown snakes, close observation without antivenom administration had favorable outcomes including shorter hospital stays and likely decreased hospital costs.N

Astro2020 Science White Paper: Triggered High-Priority Observations of Dynamic Solar System Phenomena

Unexpected dynamic phenomena have surprised solar system observers in the past and have led to important discoveries about solar system workings. Observations at the initial stages of these events provide crucial information on the physical processes at work. We advocate for long-term/permanent programs on ground-based and space-based telescopes of all sizes - including Extremely Large Telescopes (ELTs) - to conduct observations of high-priority dynamic phenomena, based on a predefined set of triggering conditions. These programs will ensure that the best initial dataset of the triggering event are taken; separate additional observing programs will be required to study the temporal evolution of these phenomena. While not a comprehensive list, the following are notional examples of phenomena that are rare, that cannot be anticipated, and that provide high-impact advances to our understandings of planetary processes. Examples include: new cryovolcanic eruptions or plumes on ocean worlds; impacts on Jupiter, Saturn, Uranus, or Neptune; extreme eruptions on Io; convective superstorms on Saturn, Uranus, or Neptune; collisions within the asteroid belt or other small-body populations; discovery of an interstellar object passing through our solar system (e.g. 'Oumuamua); and responses of planetary atmospheres to major solar flares or coronal mass ejections.Comment: Astro2020 white pape

Astro2020 Science White Paper: Triggered High-Priority Observations of Dynamic Solar System Phenomena

Unexpected dynamic phenomena have surprised solar system observers in the past and have led to important discoveries about solar system workings. Observations at the initial stages of these events provide crucial information on the physical processes at work. We advocate for long-term/permanent programs on ground-based and space-based telescopes of all sizes - including Extremely Large Telescopes (ELTs) - to conduct observations of high-priority dynamic phenomena, based on a predefined set of triggering conditions. These programs will ensure that the best initial dataset of the triggering event are taken; separate additional observing programs will be required to study the temporal evolution of these phenomena. While not a comprehensive list, the following are notional examples of phenomena that are rare, that cannot be anticipated, and that provide high-impact advances to our understandings of planetary processes. Examples include: new cryovolcanic eruptions or plumes on ocean worlds; impacts on Jupiter, Saturn, Uranus, or Neptune; extreme eruptions on Io; convective superstorms on Saturn, Uranus, or Neptune; collisions within the asteroid belt or other small-body populations; discovery of an interstellar object passing through our solar system (e.g. 'Oumuamua); and responses of planetary atmospheres to major solar flares or coronal mass ejections

Finishing the euchromatic sequence of the human genome

The sequence of the human genome encodes the genetic instructions for human physiology, as well as rich information about human evolution. In 2001, the International Human Genome Sequencing Consortium reported a draft sequence of the euchromatic portion of the human genome. Since then, the international collaboration has worked to convert this draft into a genome sequence with high accuracy and nearly complete coverage. Here, we report the result of this finishing process. The current genome sequence (Build 35) contains 2.85 billion nucleotides interrupted by only 341 gaps. It covers ∼99% of the euchromatic genome and is accurate to an error rate of ∼1 event per 100,000 bases. Many of the remaining euchromatic gaps are associated with segmental duplications and will require focused work with new methods. The near-complete sequence, the first for a vertebrate, greatly improves the precision of biological analyses of the human genome including studies of gene number, birth and death. Notably, the human enome seems to encode only 20,000-25,000 protein-coding genes. The genome sequence reported here should serve as a firm foundation for biomedical research in the decades ahead