196,538 research outputs found

    Sciurus pucheranii (Rodentia: Sciuridae)

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    Leonard, Katherine M., Pasch, Bret, Koprowski, John L. (2009): Sciurus pucheranii (Rodentia: Sciuridae). Mammalian Species 841 (4): 1-4, DOI: 10.1644/841.1, URL: http://dx.doi.org/10.1644/841.

    Fig. 4 in Sciurus pucheranii (Rodentia: Sciuridae)

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    Fig. 4.—Lateral view of a baculum of Sciurus pucheranii from Acevedo, Huila, Colombia (drawing modified from Didier [1955]).Published as part of Leonard, Katherine M., Pasch, Bret & Koprowski, John L., 2009, Sciurus pucheranii (Rodentia: Sciuridae), pp. 1-4 in Mammalian Species 841 (4) on page 3, DOI: 10.1644/841.1, http://zenodo.org/record/503374

    Fig. 2 in Sciurus sanborni (Rodentia: Sciuridae)

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    Fig. 2.—Geographic distribution of Sciurus sanborni modified from Thorington et al. (2012). Created by M. J. Merrick.Published as part of Palmer, Rosa R & Koprowski, John L, 2017, Sciurus sanborni (Rodentia: Sciuridae), pp. 93-96 in Mammalian Species 49 (952) on page 94, DOI: 10.1093/mspecies/sex010, http://zenodo.org/record/716855

    FIGURE 22 in Mammals of Korea: a review of their taxonomy, distribution and conservation status

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    FIGURE 22. Blood vessel on uropatigium of M. ikonnikovi and M. brandtii.Published as part of Jo, Yeong-Seok, Baccus, John T. & Koprowski, John L., 2018, Mammals of Korea: a review of their taxonomy, distribution and conservation status, pp. 1-216 in Zootaxa 4522 (1) on page 41, DOI: 10.11646/zootaxa.4522.1.1, http://zenodo.org/record/261019

    (Sub)millimetre-selected galaxies and the cosmic star-formation history

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    Understanding the time evolution of the star formation in the Universe is one of the main aims of observational astronomy. Since a significant portion of the UV starlight is being absorbed by dust and re-emitted in the IR, we need to understand both of those regimes to properly describe the cosmic star formation history. In UV, the depth and the resolution of the data permits calculations of the star formation rate densities out to very high redshifts (z ∼ 8 − 9). In IR however, the large beam sizes and the relatively shallow data limits these calculations to z ∼ 2. In this thesis, I explore the SMA and PdBI high-resolution follow-up of 30 bright sources originally selected by AzTEC and LABOCA instruments at 1.1 mm and 870 μm respectively in conjunction with the SCUBA-2 Cosmology Legacy Survey (S2CLS) deep COSMOS and wide UDS maps, where 106 and 283 sources were detected, with the signal-to-noise ratio of > 5 and > 3.5 at 850 μm respectively. I find that the (sub)mm-selected galaxies reside and the mean redshifts of ¯z ≃ 2.5±0.05 with the exception of the brightest sources which seem to lie at higher redshifts (¯z ≃ 3.5 ± 0.2), most likely due to the apparent correlation of the (sub)mm flux with redshift, where brighter sources tend to lie at higher redshifts. Stellar masses, M⋆, and star formation rates, SFRs, were found (M⋆ & 1010M⊙ and SFR & 100M⊙ yr−1) and used to calculate the specific SFRs. I determine that the (sub)mm-selected sources mostly lie on the high-mass end of the star formation ‘main-sequence’ which makes them a high-mass extension of normal star forming galaxies. I also find that the specific SFR slightly evolves at redshifts 2−4, suggesting that the efficiency of the star formation seems to be increasing at these redshifts. Using the S2CLS data, the bolometric IR luminosity functions (IR LFs) were found for a range of redshifts z = 1.2 − 4.2 and the contribution of the SMGs to the total star formation rate density (SFRD) was calculated. The IR LFs were found to evolve out to redshift ∼ 2.5. The star formation activity in the Universe was found to peak at z ≃ 2 followed by a slight decline. Assuming the IR to total SFRD correction found in the literature the SFRD found in this work closely follows the best-fitting function of Madau & Dickinson (2014)

    Meles Brisson 1762

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    Genus Meles Brisson, 1762 Meles, formerly known as a monotypic genus, is currently composed of three species, M. anakuma in Japan, M. leucurus in continental Asia and M. meles in Europe.Published as part of Jo, Yeong-Seok, Baccus, John T. & Koprowski, John L., 2018, Mammals of Korea: a review of their taxonomy, distribution and conservation status, pp. 1-216 in Zootaxa 4522 (1) on page 72, DOI: 10.11646/zootaxa.4522.1.1, http://zenodo.org/record/261019

    Moschus Linnaeus 1758

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    Genus Moschus Linnaeus, 1758 Moschus was previously regarded as a monospecific genus, but seven species have been recently recognized in this genus (Grubb 2005). Only one species, M. moschiferus, occurs in Korea.Published as part of Jo, Yeong-Seok, Baccus, John T. & Koprowski, John L., 2018, Mammals of Korea: a review of their taxonomy, distribution and conservation status, pp. 1-216 in Zootaxa 4522 (1) on page 103, DOI: 10.11646/zootaxa.4522.1.1, http://zenodo.org/record/261019

    Talpidae G. Fischer 1814

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    Family TALPIDAE G. Fischer, 1814 In Korea, the Family Talpidae contains the single species Mogera robusta. Here, M. wogura coreana is regarded as synonym of M. robusta whereas, M. wogura is considered endemic in Japan (Corbet 1978; Kawada & Yokohata 2009).Published as part of Jo, Yeong-Seok, Baccus, John T. & Koprowski, John L., 2018, Mammals of Korea: a review of their taxonomy, distribution and conservation status, pp. 1-216 in Zootaxa 4522 (1) on page 29, DOI: 10.11646/zootaxa.4522.1.1, http://zenodo.org/record/261019

    Fig. 4 in Caracal caracal (Carnivora: Felidae)

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    Fig. 4.—Typical Caracal caracal habitat on sheep farmland in the Central Karoo, Western Cape Province, South Africa (top). Typical C. caracal habitat in the Cederberg mountains, Western Cape Province, South Africa (bottom). Photographs by Marine Drouilly.Published as part of Veals, Amanda M, Burnett, Alexandra D, Morandini, Marina, Drouilly, Marine & Koprowski, John L, 2020, Caracal caracal (Carnivora: Felidae), pp. 71-85 in Mammalian Species 52 (993) on page 77, DOI: 10.1093/mspecies/seaa006, http://zenodo.org/record/716895

    Fig. 2 in Sciurus ignitus (Rodentia: Sciuridae)

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    Fig. 2.—Subadult Sciurus ignitus taken at Hotel Esmeralda, Coroico, Bolivia (16811 021 00S, 67843011 00 W, altitude: 1,660 m above sea level), October 2012. Photograph by Clayton Burne used with permission.Published as part of Merrick, Melissa J., Ketcham, Shari L. & Koprowski Abstract, John L., 2014, Sciurus ignitus (Rodentia: Sciuridae), pp. 93-100 in Mammalian Species 46 (915) on page 96, DOI: 10.1644/915.1, http://zenodo.org/record/503325
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