A Northward Range Extension of the Hispid Cotton Rat (\u3ci\u3eSigmodon hispidus\u3c/i\u3e) in Missouri

The hispid cotton rat (Sigmodon hispidus) is a widely distributed rodent with a geographic range extending from north-central Mexico to southern Nebraska and central Virginia and from southeastern Arizona east to Florida (Carleton et al. 1999, Peppers and Bradley 2000, Wilson and Reeder 2005) with isolated populations in Arizona (Bradley et al. 2012) and California (Clark 1972). Range expansions for the species have been well documented (Clark 1972, Farney 1975, Benedict et al. 2000, Wright et al. 2010, Wills et al. 2011). The majority of these range expansions have occurred across the Central Plains during the 20th century and have been attributed to climate change (e.g., Benedict et al. 2000, Hoffman 2008). Bailey (1902) was the first to document movement of S. hispidus into the Central Plains by documenting individuals for the first time in Kansas that most likely moved northward from Oklahoma. By 1947, the species had reached the Kansas/Nebraska border (Cockrum 1948). Just over 10 years later, Jones (1960) reported 12 individuals near the Nemaha River in southeastern Nebraska, and by the late 1960s (Choate and Genoways 1967, Genoways and Schlitter 1967) and mid-1970s (Farney 1975), the species had been documented in several parts of the state

NOTES: RANGE EXTENSION OF THE VIRGINIA OPOSSUM (DIDELPHIS VIRGINIANA) IN NORTH DAKOTA

The Virginia opossum (Didelphis virginiana) is broadly distributed across North America from Costa Rica in the south to southern Ontario in the north and from the southern Great Plains in the west to the eastern United States. The Virginia opossum also was introduced multiple times to thePacific Coast beginning in the late 1800s and has established populations in that region (Gardner and Sunquist 2003). This species is a habitat generalist known to frequent wetland and hardwood habitats but also can be found in grasslands, along forest edges, and in agricultural and suburban settings throughout its range (Gardner and Sunquist 2003, Beatty et al. 2014). However, the Virginia opossum is adapted poorly to winter, limiting its northern distribution to more tolerable warmer climates. It does not hibernate or exhibit torpor, and it will remain in its den rather than forage on nights when temperatures are below freezing or when there is deep snow, risking starvation if more than 54 days of winter are too harsh to forage (Brocke 1970). Despite these limitations, the Virginia opossum has expanded north in recent decades (Myers et al. 2009) and has been documented in novel areas of the Upper Midwest and New England (e.g., Dice 1927, Goodwin 1935, Jackson 1961). Both climate change and human land use alteration have been identified as contributing factors to their current range expansion. A recent study conducted across Michigan and Wisconsin identified reduced days of snow on the ground and increased agricultural land as two key factors facilitating the opossum’s expansion in the Midwest (Walsh and Tucker 2017). As generalist omnivores, opossums benefit from increased road kill and resources provided by agricultural practices (Beatty et al. 2014). Humans are further ameliorating winter conditions by providing shelter and easily accessible food, as evidenced by opossums in urban areas weighing more than individuals in adjacent natural habitats (Kanda 2005, Wright et al. 2012)

A Prolegomenon to the Systematics of South American Cottontail Rabbits (Mammalia, Lagomorpha, Leporidae: Sylvilagus): Designation of a Neotype for S. brasiliensis (Linnaeus, 1758), and Restoration of S. andinus (Thomas, 1897) and S. tapetillus Thomas, 1913.

A critical issue with species names derived from Linnaeus’ 10th edition of the Systema Naturae is the lack of holotypes, which in many instances has led to taxonomic confusion and uncertainty, as well as an unstable taxonomy. In the particular case of the South American cottontail, currently known as Sylvilagus brasiliensis, Linnaeus listed the type locality as “America Meridionali,” or South America. As a result, S. brasiliensis was ascribed a widespread distribution in North and South America, over an area estimated as approximately 1.09 × 107 Km2, and containing upwards of 37 named subspecies.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/136089/1/MP205.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/136089/2/MP205_SupplementaryFigs.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/136089/3/MP205_Appendix1.pdfhttp://deepblue.lib.umich.edu/bitstream/2027.42/136089/4/MP205_Appendix 2.xlsxDescription of MP205.pdf : Main ArticleDescription of MP205_SupplementaryFigs.pdf : Additional FiguresDescription of MP205_Appendix1.pdf : Dataset - MapsDescription of MP205_Appendix 2.xlsx : Datase

Hysteresis in mesoscopic superconducting disks: the Bean-Livingston barrier

The magnetization behavior of mesoscopic superconducting disks can show hysteretic behavior which we explain by using the Ginzburg-Landau (GL) theory and properly taking into account the de-magnetization effects due to geometrical form factors. In large disks the Bean-Livingston surface barrier is responsible for the hysteresis. While in small disks a volume barrier is responsible for this hysteresis. It is shown that although the sample magnetization is diamagnetic (negative), the measured magnetization can be positive at certain fields as observed experimentally, which is a consequence of the de-magnetization effects and the experimental set up.Comment: Latex file, 4 ps file

Singlet and Triplet Excitation Management in a Bichromophoric Near-Infrared-Phosphorescent BODIPY-Benzoporphyrin Platinum Complex

Multichromophoric arrays provide one strategy for assembling molecules with intense absorptions across the visible spectrum but are generally focused on systems that efficiently produce and manipulate singlet excitations and therefore are burdened by the restrictions of (a) unidirectional energy transfer and (b) limited tunability of the lowest molecular excited state. In contrast, we present here a multichromophoric array based on four boron dipyrrins (BODIPY) bound to a platinum benzoporphyrin scaffold that exhibits intense panchromatic absorption and efficiently generates triplets. The spectral complementarity of the BODIPY and porphryin units allows the direct observation of fast bidirectional singlet and triplet energy transfer processes (k_(ST)(^1BDP→^1Por) = 7.8 × 10^(11) s^(−1), k_(TT)(^3Por→^3BDP) = 1.0 × 10^(10) s^(−1), k_(TT)(^3BDP→^3Por) = 1.6 × 10^(10) s^(−1)), leading to a long-lived equilibrated [^3BDP][Por]⇔[BDP][^3Por] state. This equilibrated state contains approximately isoenergetic porphyrin and BODIPY triplets and exhibits efficient near-infrared phosphorescence (λ_(em) = 772 nm, Φ = 0.26). Taken together, these studies show that appropriately designed triplet-utilizing arrays may overcome fundamental limitations typically associated with core−shell chromophores by tunable redistribution of energy from the core back onto the antennae

Leveraging natural history biorepositories as a global, decentralized, pathogen surveillance network

The Severe Acute Respiratory Syndrome Coronavirus 2 (SARS-CoV-2) pandemic reveals a major gap in global biosecurity infrastructure: a lack of publicly available biological samples representative across space, time, and taxonomic diversity. The shortfall, in this case for vertebrates, prevents accurate and rapid identification and monitoring of emerging pathogens and their reservoir host(s) and precludes extended investigation of ecological, evolutionary, and environmental associations that lead to human infection or spillover. Natural history museum biorepositories form the backbone of a critically needed, decentralized, global network for zoonotic pathogen surveillance, yet this infrastructure remains marginally developed, underutilized, underfunded, and disconnected from public health initiatives. Proactive detection and mitigation for emerging infectious diseases (EIDs) requires expanded biodiversity infrastructure and training (particularly in biodiverse and lower income countries) and new communication pipelines that connect biorepositories and biomedical communities. To this end, we highlight a novel adaptation of Project ECHO’s virtual community of practice model: Museums and Emerging Pathogens in the Americas (MEPA). MEPA is a virtual network aimed at fostering communication, coordination, and collaborative problem-solving among pathogen researchers, public health officials, and biorepositories in the Americas. MEPA now acts as a model of effective international, interdisciplinary collaboration that can and should be replicated in other biodiversity hotspots. We encourage deposition of wildlife specimens and associated data with public biorepositories, regardless of original collection purpose, and urge biorepositories to embrace new specimen sources, types, and uses to maximize strategic growth and utility for EID research. Taxonomically, geographically, and temporally deep biorepository archives serve as the foundation of a proactive and increasingly predictive approach to zoonotic spillover, risk assessment, and threat mitigation

The SPIRITS Sample of Luminous Infrared Transients: Uncovering Hidden Supernovae and Dusty Stellar Outbursts in Nearby Galaxies

We present a systematic study of the most luminous (M IR [Vega magnitudes] brighter than −14) infrared (IR) transients discovered by the SPitzer InfraRed Intensive Transients Survey (SPIRITS) between 2014 and 2018 in nearby galaxies (D 12) show multiple, luminous IR outbursts over several years and have directly detected, massive progenitors in archival imaging. With analyses of extensive, multiwavelength follow-up, we suggest the following possible classifications: five obscured core-collapse supernovae (CCSNe), two erupting massive stars, one luminous red nova, and one intermediate-luminosity red transient. We define a control sample of all optically discovered transients recovered in SPIRITS galaxies and satisfying the same selection criteria. The control sample consists of eight CCSNe and one Type Iax SN. We find that 7 of the 13 CCSNe in the SPIRITS sample have lower bounds on their extinction of 2 < A V < 8. We estimate a nominal fraction of CCSNe in nearby galaxies that are missed by optical surveys as high as ${38.5}_{-21.9}^{+26.0} \%$ (90% confidence). This study suggests that a significant fraction of CCSNe may be heavily obscured by dust and therefore undercounted in the census of nearby CCSNe from optical searches

Mammal collections of the Western Hemisphere: A survey and directory of collections

As a periodic assessment of the mammal collection resource, the Systematic Collections Committee (SCC) of the American Society of Mammalogists undertakes decadal surveys of the collections held in the Western Hemisphere. The SCC surveyed 429 collections and compiled a directory of 395 active collections containing 5,275,155 catalogued specimens. Over the past decade, 43 collections have been lost or transferred and 38 new or unsurveyed collections were added. Growth in number of total specimens, expansion of genomic resource collections, and substantial gains in digitization and web accessibility were documented, as well as slight shifts in proportional representation of taxonomic groups owing to increasingly balanced geographic representation of collections relative to previous surveys. While we find the overall health of Western Hemisphere collections to be adequate in some areas, gaps in spatial and temporal coverage and clear threats to long-term growth and vitality of these resources have also been identified. Major expansion of the collective mammal collection resource along with a recommitment to appropriate levels of funding will be required to meet the challenges ahead for mammalogists and other users, and to ensure samples are broad and varied enough that unanticipated future needs can be powerfully addressed. © 2018 The Author(s)