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The Nature of Teller Coyotes Physical Description Coyotes (Canis Latrans
The Nature of Teller Coyotes Physical Description Coyotes (Canis latrans) are members of the canine family. Of the 19 subspecies, the mountain coyote is the one you’ll encounter in Teller County. They have gray, white, tan, and brown fur. The coyote in the photograph was taken from Edlowe Road. They are about the size of a medium-size dog, weighing 20 to 50 pounds. Their long, bushy tails are helpful species identifiers. Coyotes run with their tails down while domestic dogs run with tails up and wolves run with tails straight out. Life History In many areas, coyotes are solitary outside of the breeding season; but their social organization is influenced by prey size. In populations where the majority of prey are small rodents, coyotes tend to be solitary. In populations where larger animals are available (elk and deer), large groups of coyotes (packs) may form. Like other canines, coyotes do not hibernate. A male and female will pair off and remain together for several years, although they may not be life mates. Mating occurs between January and March. They establish dens abandoned by other animals, or dig one themselves. Litters of 5-7are born sightless and hairless two months after mating. Their eyes open after 10 days, and they leave the den between 8-10 weeks of age. Movement of pups from one den to another is common. The reason is unknown, but disturbance and infestation by parasites may be factors. Coyotes in captivity may live as long as 18 years, but in wild populations few coyotes live more than 6 to 8 years. -
Glimpse of an African… Wolf? Cécile Bloch
$6.95 Glimpse of an African… Wolf ? PAGE 4 Saving the Red Wolf Through Partnerships PAGE 9 Are Gray Wolves Still Endangered? PAGE 14 Make Your Home Howl Members Save 10% Order today at shop.wolf.org or call 1-800-ELY-WOLF Your purchases help support the mission of the International Wolf Center. VOLUME 25, NO. 1 THE QUARTERLY PUBLICATION OF THE INTERNATIONAL WOLF CENTER SPRING 2015 4 Cécile Bloch 9 Jeremy Hooper 14 Don Gossett In the Long Shadow of The Red Wolf Species Survival Are Gray Wolves Still the Pyramids and Beyond: Plan: Saving the Red Wolf Endangered? Glimpse of an African…Wolf? Through Partnerships In December a federal judge ruled Geneticists have found that some In 1967 the number of red wolves that protections be reinstated for of Africa’s golden jackals are was rapidly declining, forcing those gray wolves in the Great Lakes members of the gray wolf lineage. remaining to breed with the more wolf population area, reversing Biologists are now asking: how abundant coyote or not to breed at all. the USFWS’s 2011 delisting many golden jackals across Africa The rate of hybridization between the decision that allowed states to are a subspecies known as the two species left little time to prevent manage wolves and implement African wolf? Are Africa’s golden red wolf genes from being completely harvest programs for recreational jackals, in fact, wolves? absorbed into the expanding coyote purposes. If biological security is population. The Red Wolf Recovery by Cheryl Lyn Dybas apparently not enough rationale for Program, working with many other conservation of the species, then the organizations, has created awareness challenge arises to properly express and laid a foundation for the future to the ecological value of the species. -
The Spitzer C2d Survey of Large, Nearby, Interstellar Clouds. IV
Draft version October 24, 2018 A Preprint typeset using LTEX style emulateapj v. 08/22/09 THE SPITZER C2D SURVEY OF LARGE, NEARBY, INTERSTELLAR CLOUDS. IV. LUPUS OBSERVED WITH MIPS Nicholas L. Chapman1, Shih-Ping Lai1,2,3, Lee G. Mundy1, Neal J. Evans II4, Timothy Y. Brooke5, Lucas A. Cieza4, William J. Spiesman4, Luisa M. Rebull6, Karl R. Stapelfeldt7, Alberto Noriega-Crespo6, Lauranne Lanz1, Lori E. Allen8, Geoffrey A. Blake9, Tyler L. Bourke8, Paul M. Harvey4, Tracy L. Huard8, Jes K. Jørgensen8, David W. Koerner10, Philip C. Myers8, Deborah L. Padgett6, Annelia I. Sargent5, Peter Teuben1, Ewine F. van Dishoeck11, Zahed Wahhaj12, & Kaisa E. Young4,13 Draft version October 24, 2018 ABSTRACT We present maps of 7.78 square degrees of the Lupus molecular cloud complex at 24, 70, and 160µm. They were made with the Spitzer Space Telescope’s Multiband Imaging Photometer for Spitzer (MIPS) instrument as part of the Spitzer Legacy Program, “From Molecular Cores to Planet-Forming Disks” (c2d). The maps cover three separate regions in Lupus, denoted I, III, and IV. We discuss the c2d pipeline and how our data processing differs from it. We compare source counts in the three regions with two other data sets and predicted star counts from the Wainscoat model. This comparison shows the contribution from background galaxies in Lupus I. We also create two color magnitude diagrams using the 2MASS and MIPS data. From these results, we can identify background galaxies and distinguish them from probable young stellar objects. The sources in our catalogs are classified based on their spectral energy distribution (SED) from 2MASS and Spitzer wavelengths to create a sample of young stellar object candidates. -
Ecology of the European Badger (Meles Meles) in the Western Carpathian Mountains: a Review
Wildl. Biol. Pract., 2016 Aug 12(3): 36-50 doi:10.2461/wbp.2016.eb.4 REVIEW Ecology of the European Badger (Meles meles) in the Western Carpathian Mountains: A Review R.W. Mysłajek1,*, S. Nowak2, A. Rożen3, K. Kurek2, M. Figura2 & B. Jędrzejewska4 1 Institute of Genetics and Biotechnology, Faculty of Biology, University of Warsaw, Pawińskiego 5a, 02-106 Warszawa, Poland. 2 Association for Nature “Wolf”, Twardorzeczka 229, 34-324 Lipowa, Poland. 3 Institute of Environmental Sciences, Jagiellonian University, Gronostajowa 7, 30-387 Kraków, Poland. 4 Mammal Research Institute, Polish Academy of Sciences, Waszkiewicza 1c, 17-230 Białowieża, Poland. * Corresponding author email: [email protected]. Keywords Abstract Altitudinal Gradient; This article summarizes the results of studies on the ecology of the European Diet Composition; badger (Meles meles) conducted in the Western Carpathians (S Poland) Meles meles; from 2002 to 2010. Badgers inhabiting the Carpathians use excavated setts Mustelidae; (53%), caves and rock crevices (43%), and burrows under human-made Sett Utilization; constructions (4%) as permanent shelters. Excavated setts are located up Spatial Organization. to 640 m a.s.l., but shelters in caves and crevices can be found as high as 1,050 m a.s.l. Badger setts are mostly located on slopes with southern, eastern or western exposure. Within their territories, ranging from 3.35 to 8.45 km2 (MCP100%), badgers may possess 1-12 setts. Family groups are small (mean = 2.3 badgers), population density is low (2.2 badgers/10 km2), as is reproduction (0.57 young/year/10 km2). Hunting by humans is the main mortality factor (0.37 badger/year/10 km2). -
Sierra Nevada Red Fox (Vulpes Vulpes Necator): a Conservation Assessment
Sierra Nevada Red Fox (Vulpes vulpes necator): A Conservation Assessment John D. Perrine * Environmental Science, Policy and Management Department and Museum of Vertebrate Zoology University of California, Berkeley Lori A. Campbell** USDA Forest Service Pacific Southwest Research Station Sierra Nevada Research Center Davis, California Gregory A. Green Tetra Tech EC Bothell, Washington Current address and contact information: *Primary Author: J. Perrine, Biological Sciences Department, California Polytechnic State University, San Luis Obispo, CA 93407-0401 [email protected] **L. Campbell, School of Veterinary Medicine, University of California, Davis, One Shields Avenue, Davis, CA 95616 Perrine, Campbell and Green R5-FR-010 August 2010 NOTES IN PROOF • Genetic analyses by B. Sacks and others 2010 (Conservation Genetics 11:1523-1539) indicate that the Sacramento Valley red fox population is native to California and is closely related to the Sierra Nevada red fox. They designated the Sacramento Valley red fox as a new subspecies, V. v. patwin. • In August 2010, as this document was going to press, biologists on the Humboldt-Toiyabe National Forest detected a red fox at an automatic camera station near the Sonora Pass along the border of Tuolomne and Mono Counties. Preliminary genetic analyses conducted at UC Davis indicate that the fox was a Sierra Nevada red fox. Further surveys and analyses are planned. • The California Department of Fish and Game Region 1 Timber Harvest Program has established a Sierra Nevada red fox information portal, where many management-relevant documents can be downloaded as PDFs. See: https://r1.dfg.ca.gov/Portal/SierraNevadaRedFox/tabid/618/Default.aspx Sierra Nevada Red Fox Conservation Assessment EXECUTIVE SUMMARY This conservation assessment provides a science-based, comprehensive assessment of the status of the Sierra Nevada red fox (Vulpes vulpes necator) and its habitat. -
I. G E O G RAP H IC PA T T E RNS in DIV E RS IT Y a . D Iversity And
I. GEOGRAPHIC PATTERNS IN DIVERSITY A. Diversity and Endemicty B. Patterns in Mammalian Richness 1 – latitude 2 – area 3 – isolation 4 – elevation C. Hotspots of Mammalian Biodiversity 1 – relevance 2 – optimal characteristics of hotspots 3 – empirical patterns for mammals II. CONSERVATION STATUS OF MAMMALS A. Prehistoric Extinctions B. Historic Extinctions 1 – summary (totals) 2 – taxonomic, morphologic bias 3 – Geographic bias C. Geography of Extinctions 1 – prehistory and human colonization 2 – geographic questions 3 – range collapse in mammals Hotspots of Mammalian Endemicity Endemic Mammals Species Richness (fig. 1) Schipper et al 2009 – Science 322:226. (color pdf distributed to lab sections) Fig. 2. Global patterns of threat, for land (brown) and marine (blue) mammals. (A) Number of globally threatened species (Vulnerable, Endangered or Critically Fig. 4. Global patterns of knowledge, for land Endangered). Number of species affected by: (B) habitat loss; (C) harvesting; (D) (terrestrial and freshwater, brown) and marine (blue) accidental mortality; and (E) pollution. Same color scale employed in (B), (C), (D) species. (A) Number of species newly described since and (E) (hence, directly comparable). 1992. (B) Data-Deficient species. Mammal Extinctions 1500 to 2000 (151 species or subspecies; ~ 83 species) COMMON NAME LATIN NAME DATE RANGE PRIMARY CAUSE Lesser Hispanolan Ground Sloth Acratocnus comes 1550 Hispanola introduction of rats and pigs Greater Puerto Rican Ground Sloth Acratocnus major 1500 Puerto Rico introduction of rats -
Federal Trade Commission § 301.0
Federal Trade Commission § 301.0 NAME GUIDE § 301.0 Fur products name guide. NAME GUIDE Name Order Family Genus-species Alpaca ...................................... Ungulata ................ Camelidae ............. Lama pacos. Antelope ................................... ......do .................... Bovidae ................. Hippotragus niger and Antilope cervicapra. Badger ..................................... Carnivora ............... Mustelidae ............. Taxida sp. and Meles sp. Bassarisk ................................. ......do .................... Procyonidae .......... Bassariscus astutus. Bear ......................................... ......do .................... Ursidae .................. Ursus sp. Bear, Polar ............................... ......do .................... ......do .................... Thalarctos sp. Beaver ..................................... Rodentia ................ Castoridae ............. Castor canadensis. Burunduk ................................. ......do .................... Sciuridae ............... Eutamias asiaticus. Calf .......................................... Ungulata ................ Bovidae ................. Bos taurus. Cat, Caracal ............................. Carnivora ............... Felidae .................. Caracal caracal. Cat, Domestic .......................... ......do .................... ......do .................... Felis catus. Cat, Lynx ................................. ......do .................... ......do .................... Lynx refus. Cat, Manul .............................. -
Using Herschel and Planck Observations to Delineate the Role of Magnetic Fields in Molecular Cloud Structure
Astronomy & Astrophysics manuscript no. 35779arxiv c ESO 2019 September 12, 2019 Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structure Juan D. Soler1 1. Max Planck Institute for Astronomy, Konigstuhl¨ 17, 69117, Heidelberg, Germany. [email protected] Received 26 APR 2019 / Accepted 07 AUG 2019 ABSTRACT We present a study of the relative orientation between the magnetic field projected onto the plane of sky (B?) on scales down to 0.4 pc, inferred from the polarized thermal emission of Galactic dust observed by Planck at 353 GHz, and the distribution of gas column density (NH) structures on scales down to 0.026 pc, derived from the observations by Herschel in submillimeter wavelengths, toward ten nearby (d < 450 pc) molecular clouds. Using the histogram of relative orientation technique in combination with tools from circular statistics, we found that the mean relative orientation between NH and B? toward these regions increases progressively ◦ ◦ from 0 , where the NH structures lie mostly parallel to B?, with increasing NH, in many cases reaching 90 , where the NH structures lie mostly perpendicular to B?. We also compared the relative orientation between NH and B? and the distribution of NH, which is characterized by the slope of the tail of the NH probability density functions (PDFs). We found that the slopes of the NH PDF tail are steepest in regions where NH and B? are close to perpendicular. This coupling between the NH distribution and the magnetic field suggests that the magnetic fields play a significant role in structuring the interstellar medium in and around molecular clouds. -
These Sky Maps Were Made Using the Freeware UNIX Program "Starchart", from Alan Paeth and Craig Counterman, with Some Postprocessing by Stuart Levy
These sky maps were made using the freeware UNIX program "starchart", from Alan Paeth and Craig Counterman, with some postprocessing by Stuart Levy. You’re free to use them however you wish. There are five equatorial maps: three covering the equatorial strip from declination −60 to +60 degrees, corresponding roughly to the evening sky in northern winter (eq1), spring (eq2), and summer/autumn (eq3), plus maps covering the north and south polar areas to declination about +/− 25 degrees. Grid lines are drawn at every 15 degrees of declination, and every hour (= 15 degrees at the equator) of right ascension. The equatorial−strip maps use a simple rectangular projection; this shows constellations near the equator with their true shape, but those at declination +/− 30 degrees are stretched horizontally by about 15%, and those at the extreme 60−degree edge are plotted twice as wide as you’ll see them on the sky. The sinusoidal curve spanning the equatorial strip is, of course, the Ecliptic −− the path of the Sun (and approximately that of the planets) through the sky. The polar maps are plotted with stereographic projection. This preserves shapes of small constellations, but enlarges them as they get farther from the pole; at declination 45 degrees they’re about 17% oversized, and at the extreme 25−degree edge about 40% too large. These charts plot stars down to magnitude 5, along with a few of the brighter deep−sky objects −− mostly star clusters and nebulae. Many stars are labelled with their Bayer Greek−letter names. Also here are similarly−plotted maps, based on galactic coordinates. -
American Black Bear Ecology in Southeastern Oklahoma: Population Status and Capture Methodology
AMERICAN BLACK BEAR ECOLOGY IN SOUTHEASTERN OKLAHOMA: POPULATION STATUS AND CAPTURE METHODOLOGY By MORGAN A. PFANDER Bachelor of Science in Natural Resource Management University of Arizona Tucson, Arizona 2011 Submitted to the Faculty of the Graduate College of the Oklahoma State University in partial fulfillment of the requirements for the Degree of MASTER OF SCIENCE May, 2016 AMERICAN BLACK BEAR ECOLOGY IN SOUTHEASTERN OKLAHOMA: POPULATION STATUS AND CAPTURE METHODOLOGY Thesis Approved: Dr. W. Sue Fairbanks Thesis Adviser Dr. David M. Leslie, Jr. Dr. Barney Luttbeg ii ACKNOWLEDGEMENTS Thank you to all of the people who have made this research project possible. It has been a wonderful experience working with all of the graduate students, faculty, and staff here at Oklahoma State University and I feel blessed to have had the opportunity to spend a couple of years in the bear woods of Oklahoma. Thank you especially to my thesis advisor, Dr. W. Sue Fairbanks, for the opportunity to be a part of such an amazing project and for all of the encouragement and advice throughout the research process. I am also grateful to my committee members, Dr. Chip Leslie and Dr. Barney Luttbeg, for their invaluable contributions to the development and analysis of this study. Thank you to Sara Lyda for introducing me to the bear woods and for all of her help with training and project logistics. I would also like to thank all of the Oklahoma Department of Wildlife Conservation officials, especially Jeff Ford and Joe Hemphill, and my summer technicians and volunteers for all of their help in the field. -
Supernova Star Maps
Supernova Star Maps Which Stars in the Night Sky Will Go Su pernova? About the Activity Allow visitors to experience finding stars in the night sky that will eventually go supernova. Topics Covered Observation of stars that will one day go supernova Materials Needed • Copies of this month's Star Map for your visitors- print the Supernova Information Sheet on the back. • (Optional) Telescopes A S A Participants N t i d Activities are appropriate for families Cre with children over the age of 9, the general public, and school groups ages 9 and up. Any number of visitors may participate. Location and Timing This activity is perfect for a star party outdoors and can take a few minutes, up to 20 minutes, depending on the Included in This Packet Page length of the discussion about the Detailed Activity Description 2 questions on the Supernova Helpful Hints 5 Information Sheet. Discussion can start Supernova Information Sheet 6 while it is still light. Star Maps handouts 7 Background Information There is an Excel spreadsheet on the Supernova Star Maps Resource Page that lists all these stars with all their particulars. Search for Supernova Star Maps here: http://nightsky.jpl.nasa.gov/download-search.cfm © 2008 Astronomical Society of the Pacific www.astrosociety.org Copies for educational purposes are permitted. Additional astronomy activities can be found here: http://nightsky.jpl.nasa.gov Star Maps: Stars likely to go Supernova! Leader’s Role Participants’ Role (Anticipated) Materials: Star Map with Supernova Information sheet on back Objective: Allow visitors to experience finding stars in the night sky that will eventually go supernova. -
(2019) Old World Canis Spp. with Taxonomic Ambiguity: Workshop Conclusions
Old World Canis spp. with taxonomic ambiguity: Workshop conclusions and recommendations Vairão, Portugal, 28th - 30th May 2019 Francisco Alvares1*, Wieslaw Bogdanowicz2, Liz A.D. Campbell3, Raquel Godinho1, Jennifer Hatlauf4, Yadvendradev V. Jhala5, Andrew C. Kitchener6, Klaus-Peter Koepfli7, Miha Krofel8, Helen Senn9, Claudio Sillero-Zubiri3,10, Suvi Viranta11, and Geraldine Werhahn3,10 1 CIBIO-InBIO, Research Center in Biodiversity and Genetic Resources from Porto University, Vairão, Portugal. Email: [email protected] 2 Polish Academy of Sciences Poland. 3 Wildlife Conservation Research Unit (WildCRU), Department of Zoology, University of Oxford, UK 4 Institute of Wildlife Biology and Game Management, University of Natural Resources and Life Sciences (BOKU), Vienna, Austria. 5 Wildlife Institute of India, India 6 National Museums Scotland, Department of Natural Sciences, Chambers Street, Edinburgh, EH1 1JF, UK 7 Smithsonian Conservation Biology Institute, Center for Species Survival, Washington, D.C. USA 8 Biotechnical Faculty, University of Ljubljana, Slovenia 9 Royal Zoological Society of Scotland, Edinburgh, UK 10 IUCN SSC Canid specialist Group, Oxford, UK 11 University of Helsinki, Finland * Convener Introduction In response to a need for answers to questions regarding the taxonomy of several Old World Canis taxa, a work- shop of experts in taxonomy, evolution, biology and conservation of the Canidae took place in Vairão, Portugal, on 28th-30th May 2019, organised by CIBIO-InBIO and the IUCN SSC Canid Specialist Group. See appendix