ALBERT

Description: Hierarchical triple systems comprise a close binary and a more distant component. They are important for testing theories of star formation and of stellar evolution in the presence of nearby companions. We obtained 218 days of Kepler photometry of HD 181068 (magnitude of 7.1), supplemented by ground-based spectroscopy and interferometry, which show it to be a hierarchical triple with two types of mutual eclipses. The primary is a red giant that is in a 45-day orbit with a pair of red dwarfs in a close 0.9-day orbit. The red giant shows evidence for tidally induced oscillations that are driven by the orbital motion of the close pair. HD 181068 is an ideal target for studies of dynamical evolution and testing tidal friction theories in hierarchical triple systems.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Derekas, A -- Kiss, L L -- Borkovits, T -- Huber, D -- Lehmann, H -- Southworth, J -- Bedding, T R -- Balam, D -- Hartmann, M -- Hrudkova, M -- Ireland, M J -- Kovacs, J -- Mezo, Gy -- Moor, A -- Niemczura, E -- Sarty, G E -- Szabo, Gy M -- Szabo, R -- Telting, J H -- Tkachenko, A -- Uytterhoeven, K -- Benko, J M -- Bryson, S T -- Maestro, V -- Simon, A E -- Stello, D -- Schaefer, G -- Aerts, C -- ten Brummelaar, T A -- De Cat, P -- McAlister, H A -- Maceroni, C -- Merand, A -- Still, M -- Sturmann, J -- Sturmann, L -- Turner, N -- Tuthill, P G -- Christensen-Dalsgaard, J -- Gilliland, R L -- Kjeldsen, H -- Quintana, E V -- Tenenbaum, P -- Twicken, J D -- New York, N.Y. -- Science. 2011 Apr 8;332(6026):216-8. doi: 10.1126/science.1201762.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, Eotvos University, Budapest, Hungary. derekas@konkoly.hu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21474755" target="_blank"〉PubMed〈/a〉

Description: We report the detection of Kepler-47, a system consisting of two planets orbiting around an eclipsing pair of stars. The inner and outer planets have radii 3.0 and 4.6 times that of Earth, respectively. The binary star consists of a Sun-like star and a companion roughly one-third its size, orbiting each other every 7.45 days. With an orbital period of 49.5 days, 18 transits of the inner planet have been observed, allowing a detailed characterization of its orbit and those of the stars. The outer planet's orbital period is 303.2 days, and although the planet is not Earth-like, it resides within the classical "habitable zone," where liquid water could exist on an Earth-like planet. With its two known planets, Kepler-47 establishes that close binary stars can host complete planetary systems.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Orosz, Jerome A -- Welsh, William F -- Carter, Joshua A -- Fabrycky, Daniel C -- Cochran, William D -- Endl, Michael -- Ford, Eric B -- Haghighipour, Nader -- MacQueen, Phillip J -- Mazeh, Tsevi -- Sanchis-Ojeda, Roberto -- Short, Donald R -- Torres, Guillermo -- Agol, Eric -- Buchhave, Lars A -- Doyle, Laurance R -- Isaacson, Howard -- Lissauer, Jack J -- Marcy, Geoffrey W -- Shporer, Avi -- Windmiller, Gur -- Barclay, Thomas -- Boss, Alan P -- Clarke, Bruce D -- Fortney, Jonathan -- Geary, John C -- Holman, Matthew J -- Huber, Daniel -- Jenkins, Jon M -- Kinemuchi, Karen -- Kruse, Ethan -- Ragozzine, Darin -- Sasselov, Dimitar -- Still, Martin -- Tenenbaum, Peter -- Uddin, Kamal -- Winn, Joshua N -- Koch, David G -- Borucki, William J -- New York, N.Y. -- Science. 2012 Sep 21;337(6101):1511-4. Epub 2012 Aug 28.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Astronomy Department, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182, USA. orosz@sciences.sdsu.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22933522" target="_blank"〉PubMed〈/a〉

Description: Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple coplanar planets have been seen to have low obliquities. This has been interpreted as evidence that hot-Jupiter formation is linked to dynamical disruption, as opposed to planet migration through a protoplanetary disk. We used asteroseismology to measure a large obliquity for Kepler-56, a red giant star hosting two transiting coplanar planets. These observations show that spin-orbit misalignments are not confined to hot-Jupiter systems. Misalignments in a broader class of systems had been predicted as a consequence of torques from wide-orbiting companions, and indeed radial velocity measurements revealed a third companion in a wide orbit in the Kepler-56 system.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Huber, Daniel -- Carter, Joshua A -- Barbieri, Mauro -- Miglio, Andrea -- Deck, Katherine M -- Fabrycky, Daniel C -- Montet, Benjamin T -- Buchhave, Lars A -- Chaplin, William J -- Hekker, Saskia -- Montalban, Josefina -- Sanchis-Ojeda, Roberto -- Basu, Sarbani -- Bedding, Timothy R -- Campante, Tiago L -- Christensen-Dalsgaard, Jorgen -- Elsworth, Yvonne P -- Stello, Dennis -- Arentoft, Torben -- Ford, Eric B -- Gilliland, Ronald L -- Handberg, Rasmus -- Howard, Andrew W -- Isaacson, Howard -- Johnson, John Asher -- Karoff, Christoffer -- Kawaler, Steven D -- Kjeldsen, Hans -- Latham, David W -- Lund, Mikkel N -- Lundkvist, Mia -- Marcy, Geoffrey W -- Metcalfe, Travis S -- Silva Aguirre, Victor -- Winn, Joshua N -- New York, N.Y. -- Science. 2013 Oct 18;342(6156):331-4. doi: 10.1126/science.1242066.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉NASA Ames Research Center, MS 244-30, Moffett Field, CA 94035, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24136961" target="_blank"〉PubMed〈/a〉

Description: We present the detection of five planets--Kepler-62b, c, d, e, and f--of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii (R plus sign in circle), orbiting a K2V star at periods of 5.7, 12.4, 18.2, 122.4, and 267.3 days, respectively. The outermost planets, Kepler-62e and -62f, are super-Earth-size (1.25 R plus sign in circle 〈 planet radius 〈/= 2.0 R plus sign in circle) planets in the habitable zone of their host star, respectively receiving 1.2 +/- 0.2 times and 0.41 +/- 0.05 times the solar flux at Earth's orbit. Theoretical models of Kepler-62e and -62f for a stellar age of ~7 billion years suggest that both planets could be solid, either with a rocky composition or composed of mostly solid water in their bulk.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Borucki, William J -- Agol, Eric -- Fressin, Francois -- Kaltenegger, Lisa -- Rowe, Jason -- Isaacson, Howard -- Fischer, Debra -- Batalha, Natalie -- Lissauer, Jack J -- Marcy, Geoffrey W -- Fabrycky, Daniel -- Desert, Jean-Michel -- Bryson, Stephen T -- Barclay, Thomas -- Bastien, Fabienne -- Boss, Alan -- Brugamyer, Erik -- Buchhave, Lars A -- Burke, Chris -- Caldwell, Douglas A -- Carter, Josh -- Charbonneau, David -- Crepp, Justin R -- Christensen-Dalsgaard, Jorgen -- Christiansen, Jessie L -- Ciardi, David -- Cochran, William D -- DeVore, Edna -- Doyle, Laurance -- Dupree, Andrea K -- Endl, Michael -- Everett, Mark E -- Ford, Eric B -- Fortney, Jonathan -- Gautier, Thomas N 3rd -- Geary, John C -- Gould, Alan -- Haas, Michael -- Henze, Christopher -- Howard, Andrew W -- Howell, Steve B -- Huber, Daniel -- Jenkins, Jon M -- Kjeldsen, Hans -- Kolbl, Rea -- Kolodziejczak, Jeffery -- Latham, David W -- Lee, Brian L -- Lopez, Eric -- Mullally, Fergal -- Orosz, Jerome A -- Prsa, Andrej -- Quintana, Elisa V -- Sanchis-Ojeda, Roberto -- Sasselov, Dimitar -- Seader, Shawn -- Shporer, Avi -- Steffen, Jason H -- Still, Martin -- Tenenbaum, Peter -- Thompson, Susan E -- Torres, Guillermo -- Twicken, Joseph D -- Welsh, William F -- Winn, Joshua N -- New York, N.Y. -- Science. 2013 May 3;340(6132):587-90. doi: 10.1126/science.1234702. Epub 2013 Apr 18.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉NASA Ames Research Center, Moffett Field, CA 94035, USA. william.j.borucki@nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23599262" target="_blank"〉PubMed〈/a〉

Description: Vasopressin and oxytocin strongly modulate autonomic fear responses, through mechanisms that are still unclear. We describe how these neuropeptides excite distinct neuronal populations in the central amygdala, which provides the major output of the amygdaloid complex to the autonomic nervous system. We identified these two neuronal populations as part of an inhibitory network, through which vasopressin and oxytocin modulate the integration of excitatory information from the basolateral amygdala and cerebral cortex in opposite manners. Through this network, the expression and endogenous activation of vasopressin and oxytocin receptors may regulate the autonomic expression of fear.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Huber, Daniel -- Veinante, Pierre -- Stoop, Ron -- New York, N.Y. -- Science. 2005 Apr 8;308(5719):245-8.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Cellular Biology and Morphology, Centre Hospitalier Universitaire Vaudois, University of Lausanne, Switzerland.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15821089" target="_blank"〉PubMed〈/a〉

Description: In addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of oscillations in 500 solar-type stars in the Kepler field of view, an ensemble that is large enough to allow statistical studies of intrinsic stellar properties (such as mass, radius, and age) and to test theories of stellar evolution. We find that the distribution of observed masses of these stars shows intriguing differences to predictions from models of synthetic stellar populations in the Galaxy.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Chaplin, W J -- Kjeldsen, H -- Christensen-Dalsgaard, J -- Basu, S -- Miglio, A -- Appourchaux, T -- Bedding, T R -- Elsworth, Y -- Garcia, R A -- Gilliland, R L -- Girardi, L -- Houdek, G -- Karoff, C -- Kawaler, S D -- Metcalfe, T S -- Molenda-Zakowicz, J -- Monteiro, M J P F G -- Thompson, M J -- Verner, G A -- Ballot, J -- Bonanno, A -- Brandao, I M -- Broomhall, A-M -- Bruntt, H -- Campante, T L -- Corsaro, E -- Creevey, O L -- Dogan, G -- Esch, L -- Gai, N -- Gaulme, P -- Hale, S J -- Handberg, R -- Hekker, S -- Huber, D -- Jimenez, A -- Mathur, S -- Mazumdar, A -- Mosser, B -- New, R -- Pinsonneault, M H -- Pricopi, D -- Quirion, P-O -- Regulo, C -- Salabert, D -- Serenelli, A M -- Silva Aguirre, V -- Sousa, S G -- Stello, D -- Stevens, I R -- Suran, M D -- Uytterhoeven, K -- White, T R -- Borucki, W J -- Brown, T M -- Jenkins, J M -- Kinemuchi, K -- Van Cleve, J -- Klaus, T C -- New York, N.Y. -- Science. 2011 Apr 8;332(6026):213-6. doi: 10.1126/science.1201827.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK. w.j.chaplin@bham.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21474754" target="_blank"〉PubMed〈/a〉

Description: Stellar interiors are inaccessible through direct observations. For this reason, helioseismologists made use of the Sun's acoustic oscillation modes to tune models of its structure. The quest to detect modes that probe the solar core has been ongoing for decades. We report the detection of mixed modes penetrating all the way to the core of an evolved star from 320 days of observations with the Kepler satellite. The period spacings of these mixed modes are directly dependent on the density gradient between the core region and the convective envelope.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Beck, P G -- Bedding, T R -- Mosser, B -- Stello, D -- Garcia, R A -- Kallinger, T -- Hekker, S -- Elsworth, Y -- Frandsen, S -- Carrier, F -- De Ridder, J -- Aerts, C -- White, T R -- Huber, D -- Dupret, M-A -- Montalban, J -- Miglio, A -- Noels, A -- Chaplin, W J -- Kjeldsen, H -- Christensen-Dalsgaard, J -- Gilliland, R L -- Brown, T M -- Kawaler, S D -- Mathur, S -- Jenkins, J M -- New York, N.Y. -- Science. 2011 Apr 8;332(6026):205. doi: 10.1126/science.1201939. Epub 2011 Mar 17.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, 3001 Leuven, Belgium. paul.beck@ster.kuleuven.be〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21415318" target="_blank"〉PubMed〈/a〉

Description: In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbit-composition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky "super-Earth," whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Carter, Joshua A -- Agol, Eric -- Chaplin, William J -- Basu, Sarbani -- Bedding, Timothy R -- Buchhave, Lars A -- Christensen-Dalsgaard, Jorgen -- Deck, Katherine M -- Elsworth, Yvonne -- Fabrycky, Daniel C -- Ford, Eric B -- Fortney, Jonathan J -- Hale, Steven J -- Handberg, Rasmus -- Hekker, Saskia -- Holman, Matthew J -- Huber, Daniel -- Karoff, Christopher -- Kawaler, Steven D -- Kjeldsen, Hans -- Lissauer, Jack J -- Lopez, Eric D -- Lund, Mikkel N -- Lundkvist, Mia -- Metcalfe, Travis S -- Miglio, Andrea -- Rogers, Leslie A -- Stello, Dennis -- Borucki, William J -- Bryson, Steve -- Christiansen, Jessie L -- Cochran, William D -- Geary, John C -- Gilliland, Ronald L -- Haas, Michael R -- Hall, Jennifer -- Howard, Andrew W -- Jenkins, Jon M -- Klaus, Todd -- Koch, David G -- Latham, David W -- MacQueen, Phillip J -- Sasselov, Dimitar -- Steffen, Jason H -- Twicken, Joseph D -- Winn, Joshua N -- New York, N.Y. -- Science. 2012 Aug 3;337(6094):556-9. doi: 10.1126/science.1223269. Epub 2012 Jun 21.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. jacarter@cfa.harvard.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22722249" target="_blank"〉PubMed〈/a〉

Description: The quest for Earth-like planets is a major focus of current exoplanet research. Although planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on their surfaces. We present the detection of Kepler-186f, a 1.11 +/- 0.14 Earth-radius planet that is the outermost of five planets, all roughly Earth-sized, that transit a 0.47 +/- 0.05 solar-radius star. The intensity and spectrum of the star's radiation place Kepler-186f in the stellar habitable zone, implying that if Kepler-186f has an Earth-like atmosphere and water at its surface, then some of this water is likely to be in liquid form.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Quintana, Elisa V -- Barclay, Thomas -- Raymond, Sean N -- Rowe, Jason F -- Bolmont, Emeline -- Caldwell, Douglas A -- Howell, Steve B -- Kane, Stephen R -- Huber, Daniel -- Crepp, Justin R -- Lissauer, Jack J -- Ciardi, David R -- Coughlin, Jeffrey L -- Everett, Mark E -- Henze, Christopher E -- Horch, Elliott -- Isaacson, Howard -- Ford, Eric B -- Adams, Fred C -- Still, Martin -- Hunter, Roger C -- Quarles, Billy -- Selsis, Franck -- New York, N.Y. -- Science. 2014 Apr 18;344(6181):277-80. doi: 10.1126/science.1249403.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24744370" target="_blank"〉PubMed〈/a〉

Description: The conservation of large carnivores is a formidable challenge for biodiversity conservation. Using a data set on the past and current status of brown bears (Ursus arctos), Eurasian lynx (Lynx lynx), gray wolves (Canis lupus), and wolverines (Gulo gulo) in European countries, we show that roughly one-third of mainland Europe hosts at least one large carnivore species, with stable or increasing abundance in most cases in 21st-century records. The reasons for this overall conservation success include protective legislation, supportive public opinion, and a variety of practices making coexistence between large carnivores and people possible. The European situation reveals that large carnivores and people can share the same landscape.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Chapron, Guillaume -- Kaczensky, Petra -- Linnell, John D C -- von Arx, Manuela -- Huber, Djuro -- Andren, Henrik -- Lopez-Bao, Jose Vicente -- Adamec, Michal -- Alvares, Francisco -- Anders, Ole -- Balciauskas, Linas -- Balys, Vaidas -- Bedo, Peter -- Bego, Ferdinand -- Blanco, Juan Carlos -- Breitenmoser, Urs -- Broseth, Henrik -- Bufka, Ludek -- Bunikyte, Raimonda -- Ciucci, Paolo -- Dutsov, Alexander -- Engleder, Thomas -- Fuxjager, Christian -- Groff, Claudio -- Holmala, Katja -- Hoxha, Bledi -- Iliopoulos, Yorgos -- Ionescu, Ovidiu -- Jeremic, Jasna -- Jerina, Klemen -- Kluth, Gesa -- Knauer, Felix -- Kojola, Ilpo -- Kos, Ivan -- Krofel, Miha -- Kubala, Jakub -- Kunovac, Sasa -- Kusak, Josip -- Kutal, Miroslav -- Liberg, Olof -- Majic, Aleksandra -- Mannil, Peep -- Manz, Ralph -- Marboutin, Eric -- Marucco, Francesca -- Melovski, Dime -- Mersini, Kujtim -- Mertzanis, Yorgos -- Myslajek, Robert W -- Nowak, Sabina -- Odden, John -- Ozolins, Janis -- Palomero, Guillermo -- Paunovic, Milan -- Persson, Jens -- Potocnik, Hubert -- Quenette, Pierre-Yves -- Rauer, Georg -- Reinhardt, Ilka -- Rigg, Robin -- Ryser, Andreas -- Salvatori, Valeria -- Skrbinsek, Tomaz -- Stojanov, Aleksandar -- Swenson, Jon E -- Szemethy, Laszlo -- Trajce, Aleksander -- Tsingarska-Sedefcheva, Elena -- Vana, Martin -- Veeroja, Rauno -- Wabakken, Petter -- Wolfl, Manfred -- Wolfl, Sybille -- Zimmermann, Fridolin -- Zlatanova, Diana -- Boitani, Luigi -- New York, N.Y. -- Science. 2014 Dec 19;346(6216):1517-9. doi: 10.1126/science.1257553.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Grimso Wildlife Research Station, Department of Ecology, Swedish University of Agricultural Sciences, 73091 Riddarhyttan, Sweden. gchapron@carnivoreconservation.org guillaume.chapron@slu.se. ; Research Institute of Wildlife Ecology, University of Veterinary Medicine, Vienna, Savoyenstrasse 1, 1160 Vienna, Austria. ; Norwegian Institute for Nature Research, Post Office Box 5685 Sluppen, 7485 Trondheim, Norway. ; KORA, Thunstrasse 31, 3074 Muri bei Bern, Switzerland. ; Biology Department of the Faculty of Veterinary Medicine, University of Zagreb, Heinzelova 55, 10000 Zagreb, Croatia. ; Grimso Wildlife Research Station, Department of Ecology, Swedish University of Agricultural Sciences, 73091 Riddarhyttan, Sweden. ; Grimso Wildlife Research Station, Department of Ecology, Swedish University of Agricultural Sciences, 73091 Riddarhyttan, Sweden. Research Unit of Biodiversity (UO/CSIC/PA), Oviedo University, 33600 Mieres, Spain. ; State Nature Conservancy of Slovak Republic, Tajovskeho 28B, 974 01 Banska Bystrica, Slovakia. ; CIBIO/InBio, Centro de Investigacao em Biodiversidade e Recursos Geneticos, Universidade do Porto, 4485-661 Vairao, Portugal. ; Harz Nationalpark, Lindenallee 35, 38855 Wernigerode, Germany. ; Nature Research Centre, Akademijos 2, 08412 Vilnius, Lithuania. ; Association for Nature Conservation "Baltijos vilkas," Visoriu 6A-54, 08300 Vilnius, Lithuania. ; Slovak Wildlife Society, Post Office Box 72, 03301 Liptovsky Hradok, Slovakia. ; Biology Department of the Faculty of Natural Sciences, University of Tirana, Boulevard Zog I, Tirana, Albania. ; Wolf Project, Consultores en Biologia de la Conservacion, Calle Manuela Malasana 24, 28004 Madrid, Spain. ; KORA, Thunstrasse 31, 3074 Muri bei Bern, Switzerland. Centre for Fish and Wildlife Health, Vetsuisse Faculty, University of Bern, Langgassstrasse 122, 3012 Bern, Switzerland. ; Department of Game Management and Wildlife Biology, Czech University of Life Sciences in Prague, Kamycka 129, 165 21 Prague, Czech Republic. ; Ministry of Environment of the Republic of Lithuania, Jaksto 4/9, 01105 Vilnius, Lithuania. ; Department of Biology and Biotechnologies, University of Rome "La Sapienza," Viale dell'Universita 32, 00185 Roma, Italy. ; Balkani Wildlife Society, Boulevard Dragan Tzankov 8, 1164 Sofia, Bulgaria. ; Lynx Project Austria Northwest, Linzerstrasse 14, 4170 Haslach/Muhl, Austria. ; Nationalpark Kalkalpen, Nationalpark Zentrum Molln, Nationalpark Allee 1, 4591 Molln, Austria. ; Provincia Autonoma di Trento - Servizio Foreste e Fauna, Via Trener no. 3, 38100 Trento, Italy. ; Finnish Game and Fisheries Research Institute, Viikinkaari 4, 00790 Helsinki, Finland. ; Protection and Preservation of Natural Environment in Albania, Rruga Vangjush Furxhi 16/1/10, Tirana, Albania. ; Callisto Wildlife and Nature Conservation Society, Mitropoleos 123, 54621 Thessaloniki, Greece. ; Faculty of Silviculture and Forest Engineering, Department of Silviculture, Transilvania University, 1 Beethoven Lane, 500123 Brasov, Romania. Forest Research Institute (ICAS) Bulevardul Eroilor Number 128, Voluntari, Ilfov, 077190 Romania. ; State Institute for Nature Protection, Trg Mazuranica 5, 10000 Zagreb, Croatia. ; University of Ljubljana, Biotechnical Faculty, Jamnikarjeva 101, 1000 Ljubljana, Slovenia. ; LUPUS - German Institute for Wolf Mnitoring and Research, Dorfstrasse 20, 02979 Spreewitz, Germany. ; Finnish Game and Fisheries Research Institute, Oulu Game and Fisheries Research, Tutkijantie 2E, 90570 Oulu, Finland. ; Department of Forest Protection and Game Management, Faculty of Forestry, Technical University of Zvolen, T.G. Masaryka 20, 960 53 Zvolen, Slovakia. ; Faculty of Forestry, University of Sarajevo, Zagrebacka 20, 71000 Sarajevo, Bosnia and Herzegovina. ; Department of Forest Protection and Wildlife Management, Faculty of Forestry and Wood Technology, Mendel University in Brno, Zemedelska 3, 61300 Brno, Czech Republic. Friends of the Earth Czech Republic, Olomouc Branch, Dolni Namesti 38, 77900 Olomouc, Czech Republic. ; Estonian Environment Agency, Roomu tee 2, 51013 Tartu, Estonia. ; Office National de la Chasse et de la Faune Sauvage, ZI Mayencin, 5 Allee de Bethleem, 38610 Gieres, France. ; Centro Gestione e Conservazione Grandi Carnivori, Piazza Regina Elena 30, Valdieri 12010, Italy. ; Macedonian Ecological Society, Arhimedova 5, Skopje 1000, FYR Macedonia. Department of Wildlife Sciences, Georg-August University, Busgenweg 3, 37077 Gottingen, Germany. ; National Veterinary Epidemiology Unit, Food Safety and Veterinary Institute, Rruga Aleksander Moisiu 10 Tirana, Albania. ; Institute of Genetics and Biotechnology, Faculty of Biology, University of Warsaw, Pawinskiego 5a, 02-106 Warszawa, Poland. ; Association for Nature "Wolf," Twardorzeczka 229, 34-324 Lipowa, Poland. ; Latvian State Forest Research Institute "Silava," Rigas Iela 111, Salaspils, 2169 Latvia. ; Fundacion Oso Pardo, Calle San Luis 17, 4 degrees A, 39010 Santander, Spain. ; Natural History Museum, Njegoseva 51, 11000 Belgrade, Serbia. ; ONCFS-CNERA PAD, Equipe Ours, Chef de Projet, Impasse de la Chapelle, 31800 Villeneuve de Riviere, France. ; Istituto di Ecologia Applicata, Via B. Eustachio 10, 00161 Rome, Italy. ; Macedonian Ecological Society, Arhimedova 5, Skopje 1000, FYR Macedonia. ; Norwegian Institute for Nature Research, Post Office Box 5685 Sluppen, 7485 Trondheim, Norway. Department of Ecology and Natural Resource Management, Norwegian University of Life Sciences, Postbox 5003, 1432 As, Norway. ; St. Istvan Unversity Institute for Wildlife Conservation, Pater Karoly 1, 2103 Godollo, Hungary. ; Friends of the Earth Czech Republic, Olomouc Branch, Dolni Namesti 38, 77900 Olomouc, Czech Republic. ; Hedmark University College, Evenstad, 2480 Koppang, Norway. ; Bavarian Agency of Environment, Hans-Hogn-Strasse 12, 95030 Hof/Saale, Germany. ; Lynx Project Bavaria, Trailling 1a, 93462 Lam, Germany. ; Department of Zoology and Anthropology, Faculty of Biology/Sofia University "St. Kliment Ohridski," Boulevard Dragan Tzankov 8, 1164 Sofia, Bulgaria.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25525247" target="_blank"〉PubMed〈/a〉