859 results on '"Pomona College"'
Search Results
2. First annual report of the Laguna Marine Laboratory at Laguna Beach, Orange County, California.
- Author
-
Pomona College (Claremont, Calif.). Laguna Marine Laboratory, Pomono College (Claremont, Calif.). Dept. of Biology, Smithsonian Libraries, Pomona College (Claremont, Calif.). Laguna Marine Laboratory, and Pomono College (Claremont, Calif.). Dept. of Biology
- Subjects
Aquatic biology ,California ,Laguna Marine Laboratory ,Marine biology ,Pomona College (Claremont, Calif.) ,Research - Published
- 1912
3. Pomona College journal of economic botany as applied to subtropical horticulture.
- Author
-
Pomona College (Claremont, Calif.). Department of Biology and Harvard University Botany Libraries
- Published
- 1911
4. Annual report of the Laguna Marine Laboratory
- Author
-
Laguna Marine Laboratory, Pomona College. Dept. of Biology, and Smithsonian Libraries
- Subjects
California ,Marine biology ,Periodicals - Published
- 1912
5. Invertebrata pacifica
- Author
-
Baker, C. F. (Charles Fuller), 1872-1927, Pomona College (Claremont, Calif.). Department of Biology, and Smithsonian Libraries
- Subjects
Insects ,Periodicals - Published
- 1903
6. Pomona journal of entomology.
- Author
-
Pomona College (Claremont, Calif.). Dept. of Biology and Smithsonian Libraries
- Subjects
California ,Entomology ,Periodicals - Published
- 1909
7. Pomona College journal of entomology
- Author
-
Pomona College (Claremont, Calif.). Department of Biology, American Museum of Natural History Library, and Smithsonian Libraries
- Subjects
California ,Entomology ,Periodicals - Published
- 1909
8. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology, American Museum of Natural History Library, and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology - Published
- 1913
9. Annual report of the Laguna Marine Laboratory / Pomona College.
- Author
-
Laguna Marine Laboratory, Pomona College. Dept. of Biology, and MBLWHOI Library
- Subjects
California ,Marine biology ,Periodicals - Published
- 1912
10. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
11. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
12. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
13. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
14. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
15. Annual report of the Laguna Marine Laboratory
- Author
-
Laguna Marine Laboratory, Pomona College (Claremont, Calif.). Department of Biology, and Smithsonian Libraries and Archives
- Subjects
California ,Marine biology ,Periodicals
16. Annual report of the Laguna Marine Laboratory
- Author
-
Laguna Marine Laboratory, Pomona College (Claremont, Calif.). Department of Biology, and Smithsonian Libraries and Archives
- Subjects
California ,Marine biology ,Periodicals
17. Annual report of the Laguna Marine Laboratory
- Author
-
Laguna Marine Laboratory, Pomona College (Claremont, Calif.). Department of Biology, and Smithsonian Libraries and Archives
- Subjects
California ,Marine biology ,Periodicals
18. Annual report of the Laguna Marine Laboratory
- Author
-
Laguna Marine Laboratory, Pomona College (Claremont, Calif.). Department of Biology, and Smithsonian Libraries and Archives
- Subjects
California ,Marine biology ,Periodicals
19. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
20. Invertebrata pacifica
- Author
-
Baker, C. F. (Charles Fuller), 1872-1927, Pomona College (Claremont, Calif.). Department of Biology, and Smithsonian Libraries and Archives
- Subjects
Insects ,Periodicals
21. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
22. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
23. Pomona College journal of entomology
- Author
-
Pomona College (Claremont, Calif.). Department of Biology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Periodicals
24. Pomona College journal of entomology
- Author
-
Pomona College (Claremont, Calif.). Department of Biology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Periodicals
25. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
26. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
27. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
28. Annual report of the Laguna Marine Laboratory
- Author
-
Laguna Marine Laboratory, Pomona College (Claremont, Calif.). Department of Biology, and MBLWHOI Library
- Subjects
California ,Marine biology ,Periodicals
29. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
30. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
31. Pomona College journal of entomology
- Author
-
Pomona College (Claremont, Calif.). Department of Biology and Smithsonian Libraries and Archives
- Subjects
California ,Entomology ,Periodicals
32. Pomona College journal of entomology
- Author
-
Pomona College (Claremont, Calif.). Department of Biology and Smithsonian Libraries
- Subjects
California ,Entomology ,Periodicals
33. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
34. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
35. Journal of entomology and zoology
- Author
-
Pomona College (Claremont, Calif.). Dept. of Zoology and American Museum of Natural History Library
- Subjects
California ,Entomology ,Insects ,Periodicals ,Zoology
36. The 2009 multiwavelength campaign on Mrk 421: Variability and correlation studies
- Author
-
MAGIC Collaboration, J. Aleksić(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), S. Ansoldi(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), L. A. Antonelli(INAF National Institute for Astrophysics, I-00136 Rome, Italy), P. Antoranz(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), A. Babic(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), P. Bangale(Max-Planck-Institut für Physik, D-80805 München, Germany), U. Barres de Almeida(Max-Planck-Institut für Physik, D-80805 München, Germany), J. A. Barrio(Universidad Complutense, E-28040 Madrid, Spain), J. Becerra González(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain), W. Bednarek(University of Lodz, PL-90236 Lodz, Poland), K. Berger(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain), E. Bernardini(Deutsches Elektronen-Synchrotron), A. Biland(ETH Zurich, CH-8093 Zurich, Switzerland), O. Blanch(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), R. K. Bock(Max-Planck-Institut für Physik, D-80805 München, Germany), S. Bonnefoy(Universidad Complutense, E-28040 Madrid, Spain), G. Bonnoli(INAF National Institute for Astrophysics, I-00136 Rome, Italy), F. Borracci(Max-Planck-Institut für Physik, D-80805 München, Germany), T. Bretz(Universität Würzburg, D-97074 Würzburg, Germany), E. Carmona(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, E-28040 Madrid, Spain), A. Carosi(INAF National Institute for Astrophysics, I-00136 Rome, Italy), D. Carreto Fidalgo(Universität Würzburg, D-97074 Würzburg, Germany), P. Colin(Max-Planck-Institut für Physik, D-80805 München, Germany), E. Colombo(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain), J. L. Contreras(Universidad Complutense, E-28040 Madrid, Spain), J. Cortina(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), S. Covino(INAF National Institute for Astrophysics, I-00136 Rome, Italy), P. Da Vela(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), F. Dazzi(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), A. De Angelis(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), G. De Caneva(Deutsches Elektronen-Synchrotron), B. De Lotto(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), C. Delgado Mendez(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, E-28040 Madrid, Spain), M. Doert(Technische Universität Dortmund, D-44221 Dortmund, Germany), A. Domínguez(Inst. de Astrofísica de Andalucía), D. Dominis Prester(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), D. Dorner(Universität Würzburg, D-97074 Würzburg, Germany), M. Doro(Università di Padova and INFN, I-35131 Padova, Italy), S. Einecke(Technische Universität Dortmund, D-44221 Dortmund, Germany), D. Eisenacher(Universität Würzburg, D-97074 Würzburg, Germany), D. Elsaesser(Universität Würzburg, D-97074 Würzburg, Germany), E. Farina(Università dell'Insubria, Como, I-22100 Como, Italy), D. Ferenc(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), M. V. Fonseca(Universidad Complutense, E-28040 Madrid, Spain), L. Font(Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain), K. Frantzen(Technische Universität Dortmund, D-44221 Dortmund, Germany), C. Fruck(Max-Planck-Institut für Physik, D-80805 München, Germany), R. J. García López(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain), M. Garczarczyk(Deutsches Elektronen-Synchrotron), D. Garrido Terrats(Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain), M. Gaug(Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain), G. Giavitto(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), N. Godinović(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), A. González Mu\ noz(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), S. R. Gozzini(Deutsches Elektronen-Synchrotron), A. Hadamek(Technische Universität Dortmund, D-44221 Dortmund, Germany), D. Hadasch(Institut de Ciències de l'Espai), A. Herrero(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain), D. Hildebrand(ETH Zurich, CH-8093 Zurich, Switzerland), J. Hose(Max-Planck-Institut für Physik, D-80805 München, Germany), D. Hrupec(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), W. Idec(University of Lodz, PL-90236 Lodz, Poland), V. Kadenius(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland), H. Kellermann(Max-Planck-Institut für Physik, D-80805 München, Germany), M. L. Knoetig(ETH Zurich, CH-8093 Zurich, Switzerland), J. Krause(Max-Planck-Institut für Physik, D-80805 München, Germany), J. Kushida(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan), A. La Barbera(INAF National Institute for Astrophysics, I-00136 Rome, Italy), D. Lelas(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), N. Lewandowska(Universität Würzburg, D-97074 Würzburg, Germany), E. Lindfors(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland), F. Longo(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), S. Lombardi(INAF National Institute for Astrophysics, I-00136 Rome, Italy), M. López(Universidad Complutense, E-28040 Madrid, Spain), R. López-Coto(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), A. López-Oramas(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), E. Lorenz(Max-Planck-Institut für Physik, D-80805 München, Germany), I. Lozano(Universidad Complutense, E-28040 Madrid, Spain), M. Makariev(Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria), K. Mallot(Deutsches Elektronen-Synchrotron), G. Maneva(Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria), N. Mankuzhiyil(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), K. Mannheim(Universität Würzburg, D-97074 Würzburg, Germany), L. Maraschi(INAF National Institute for Astrophysics, I-00136 Rome, Italy), B. Marcote(Universitat de Barcelona), M. Mariotti(Università di Padova and INFN, I-35131 Padova, Italy), M. Martínez(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), D. Mazin(Max-Planck-Institut für Physik, D-80805 München, Germany), U. Menzel(Max-Planck-Institut für Physik, D-80805 München, Germany), M. Meucci(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), J. M. Miranda(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), R. Mirzoyan(Max-Planck-Institut für Physik, D-80805 München, Germany), A. Moralejo(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), P. Munar-Adrover(Universitat de Barcelona), D. Nakajima(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan), A. Niedzwiecki(University of Lodz, PL-90236 Lodz, Poland), K. Nilsson(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland), N. Nowak(6,32,*), R. Orito(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan), A. Overkemping(Technische Universität Dortmund, D-44221 Dortmund, Germany), S. Paiano(Università di Padova and INFN, I-35131 Padova, Italy), M. Palatiello(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), D. Paneque(6,*), R. Paoletti(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), J. M. Paredes(Universitat de Barcelona), X. Paredes-Fortuny(Universitat de Barcelona), S. Partini(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), M. Persic(Università di Udine, and INFN Trieste, I-33100 Udine, Italy), F. Prada(Inst. de Astrofísica de Andalucía), P. G. Prada Moroni(Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy), E. Prandini(Università di Padova and INFN, I-35131 Padova, Italy), S. Preziuso(Università di Siena, and INFN Pisa, I-53100 Siena, Italy), I. Puljak(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), R. Reinthal(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland), W. Rhode(Technische Universität Dortmund, D-44221 Dortmund, Germany), M. Ribó(Universitat de Barcelona), J. Rico(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), J. Rodriguez Garcia(Max-Planck-Institut für Physik, D-80805 München, Germany), S. Rügamer(Universität Würzburg, D-97074 Würzburg, Germany), A. Saggion(Università di Padova and INFN, I-35131 Padova, Italy), K. Saito(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan), M. Salvati(INAF National Institute for Astrophysics, I-00136 Rome, Italy), K. Satalecka(Universidad Complutense, E-28040 Madrid, Spain), V. Scalzotto(Università di Padova and INFN, I-35131 Padova, Italy), V. Scapin(Universidad Complutense, E-28040 Madrid, Spain), C. Schultz(Università di Padova and INFN, I-35131 Padova, Italy), T. Schweizer(Max-Planck-Institut für Physik, D-80805 München, Germany), S. N. Shore(Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy), A. Sillanpää(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland), J. Sitarek(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), I. Snidaric(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), D. Sobczynska(University of Lodz, PL-90236 Lodz, Poland), F. Spanier(Universität Würzburg, D-97074 Würzburg, Germany), V. Stamatescu(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain), A. Stamerra(INAF National Institute for Astrophysics, I-00136 Rome, Italy), T. Steinbring(Universität Würzburg, D-97074 Würzburg, Germany), J. Storz(Universität Würzburg, D-97074 Würzburg, Germany), S. Sun(Max-Planck-Institut für Physik, D-80805 München, Germany), T. Surić(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), L. Takalo(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland), F. Tavecchio(INAF National Institute for Astrophysics, I-00136 Rome, Italy), P. Temnikov(Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria), T. Terzić(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia), D. Tescaro(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain), M. Teshima(Max-Planck-Institut für Physik, D-80805 München, Germany), J. Thaele(Technische Universität Dortmund, D-44221 Dortmund, Germany), O. Tibolla(Universität Würzburg, D-97074 Würzburg, Germany), D. F. Torres(Institut de Ciències de l'Espai), T. Toyama(Max-Planck-Institut für Physik, D-80805 München, Germany), A. Treves(Università dell'Insubria, Como, I-22100 Como, Italy), M. Uellenbeck(Technische Universität Dortmund, D-44221 Dortmund, Germany), P. Vogler(ETH Zurich, CH-8093 Zurich, Switzerland), R. M. Wagner(Max-Planck-Institut für Physik, D-80805 München, Germany), F. Zandanel(Inst. de Astrofísica de Andalucía), R. Zanin(Universitat de Barcelona), VERITAS collaboration(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), (Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), S. Archambault(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), B. Behera(Deutsches Elektronen-Synchrotron), M. Beilicke(Department of Physics, Washington University, St. Louis, MO 63130, USA), W. Benbow(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA), R. Bird(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland), J. H. Buckley(Department of Physics, Washington University, St. Louis, MO 63130, USA), V. Bugaev(Department of Physics, Washington University, St. Louis, MO 63130, USA), M. Cerruti(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA), X. Chen(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany), L. Ciupik(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA), E. Collins-Hughes(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland), W. Cui(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), J. Dumm(School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA), J. D. Eisch(Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA), A. Falcone(Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802, USA), S. Federici(DESY, Platanenallee 6, 15738 Zeuthen, Germany), Q. Feng(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), J. P. Finley(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), H. Fleischhack(Deutsches Elektronen-Synchrotron), P. Fortin(Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA), L. Fortson(School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA), A. Furniss(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA), S. Griffin(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), S. T. Griffiths(Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA), J. Grube(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA), G. Gyuk(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA), D. Hanna(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), J. Holder(Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA), G. Hughes(Deutsches Elektronen-Synchrotron), T. B. Humensky(Physics Department, Columbia University, New York, NY 10027, USA), C. A. Johnson(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA), P. Kaaret(Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA), M. Kertzman(Department of Physics and Astronomy, DePauw University, Greencastle, IN 46135-0037, USA), Y. Khassen(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland), D. Kieda(Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA), H. Krawczynski(Department of Physics, Washington University, St. Louis, MO 63130, USA), F. Krennrich(Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA), S. Kumar(Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA), M. J. Lang(School of Physics, National University of Ireland Galway, University Road, Galway, Ireland), G. Maier(Deutsches Elektronen-Synchrotron), S. McArthur(Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA), K. Meagher(School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, 837 State Street NW, Atlanta, GA 30332-0430), P. Moriarty(Department of Life and Physical Sciences, Galway-Mayo Institute of Technology, Dublin Road, Galway, Ireland), R. Mukherjee(Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027, USA), R. A. Ong(Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA), A. N. Otte(School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, 837 State Street NW, Atlanta, GA 30332-0430), N. Park(Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA), A. Pichel(Instituto de Astronomia y Fisica del Espacio, Casilla de Correo 67 - Sucursal 28), M. Pohl(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany), A. Popkow(Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA), H. Prokoph(Deutsches Elektronen-Synchrotron), J. Quinn(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland), K. Ragan(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), J. Rajotte(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), P. T. Reynolds(Department of Applied Physics and Instrumentation, Cork Institute of Technology, Bishopstown, Cork, Ireland), G. T. Richards(School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, 837 State Street NW, Atlanta, GA 30332-0430), E. Roache(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA), A. C. Rovero(Instituto de Astronomia y Fisica del Espacio, Casilla de Correo 67 - Sucursal 28), G. H. Sembroski(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), K. Shahinyan(School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA), D. Staszak(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), I. Telezhinsky(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany), M. Theiling(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), J. V. Tucci(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), J. Tyler(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada), A. Varlotta(Department of Physics and Astronomy, Purdue University, West Lafayette, IN 47907, USA), S. P. Wakely(Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA), T. C. Weekes(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA), A. Weinstein(Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA), R. Welsing(Deutsches Elektronen-Synchrotron), A. Wilhelm(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany), D. A. Williams(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA), B. Zitzer(Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439, USA), External collaborators(INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese), (INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese), M. Villata(INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese), C. Raiteri(INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese), H. D. Aller(Department of Astronomy, University of Michigan, Ann Arbor, MI 48109-1042, USA), M. F. Aller(Department of Astronomy, University of Michigan, Ann Arbor, MI 48109-1042, USA), W. P. Chen(Graduate Institute of Astronomy, National Central University, Jhongli 32054, Taiwan), B. Jordan(School of Cosmic Physics, Dublin Institute for Advanced Studies, Dublin, 2, Ireland), E. Koptelova(Graduate Institute of Astronomy, National Central University, Jhongli 32054, Taiwan), O. M. Kurtanidze(Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia), A. Lähteenmäki(Aalto University Metsähovi Radio Observatory Metsähovintie 114 FIN-02540 Kylmälä Finland), B. McBreen(University College Dublin, Belfield, Dublin 4, Ireland), V. M. Larionov(Isaac Newton Institute of Chile, St. Petersburg Branch, St. Petersburg, Russia), C. S. Lin(Graduate Institute of Astronomy, National Central University, Jhongli 32054, Taiwan), M. G. Nikolashvili(Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia), E. Angelakis(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany), M. Capalbi(ASI-Science Data Center, Via del Politecnico, I-00133 Rome, Italy), A. Carrami\ nana(Instituto Nacional de Astrofísica, Óptica y Electrónica, Tonantzintla, Puebla 72840, Mexico), L. Carrasco(Instituto Nacional de Astrofísica, Óptica y Electrónica, Tonantzintla, Puebla 72840, Mexico), P. Cassaro(INAF Istituto di Radioastronomia, Sezione di Noto, Contrada Renna Bassa, 96017 Noto), A. Cesarini(Department of Physics, University of Trento, I38050, Povo, Trento, Italy), L. Fuhrmann(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany), M. Giroletti(INAF Istituto di Radioastronomia, 40129 Bologna, Italy), T. Hovatta(Cahill Center for Astronomy and Astrophysics, California Institute of Technology, 1200 E California Blvd, Pasadena, CA 91125), T. P. Krichbaum(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany), H. A. Krimm(Astro Space Center of the Lebedev Physical Institute, 117997 Moscow, Russia), W. Max-Moerbeck(Cahill Center for Astronomy and Astrophysics, California Institute of Technology, 1200 E California Blvd, Pasadena, CA 91125), J. W. Moody(Department of Physics and Astronomy, Brigham Young University, Provo, Utah 84602, USA), G. Maccaferri(INAF Istituto di Radioastronomia, Stazione Radioastronomica di Medicina, I-40059 Medicina), Y. Mori(Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152-8551, Japan), I. Nestoras(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany), A. Orlati(INAF Istituto di Radioastronomia, Stazione Radioastronomica di Medicina, I-40059 Medicina), C. Pace(Indiana University, Department of Astronomy, Swain Hall West 319, Bloomington, IN 47405-7105, USA), R. Pearson(Department of Physics and Astronomy, Brigham Young University, Provo, Utah 84602, USA), M. Perri(INAF National Institute for Astrophysics, I-00136 Rome, Italy), A. C. S. Readhead(Cahill Center for Astronomy and Astrophysics, California Institute of Technology, 1200 E California Blvd, Pasadena, CA 91125), J. L. Richards(Department of Physics, Purdue University, 525 Northwestern Ave, West Lafayette, IN 47907), A. C. Sadun(Department of Physics, University of Colorado, Denver, CO 80220, USA), T. Sakamoto(Department of Physics and Mathematics, College of Science and 952 Engineering, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuoku, Sagamihara-shi Kanagawa 252-5258, Japan), J. Tammi(Aalto University Metsähovi Radio Observatory Metsähovintie 114 FIN-02540 Kylmälä Finland), M. Tornikoski(Aalto University Metsähovi Radio Observatory Metsähovintie 114 FIN-02540 Kylmälä Finland), Y. Yatsu(Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152-8551, Japan), A. Zook(Department of Physics and Astronomy, Pomona College, Claremont CA 91711-6312, USA), Aleksić, J, Ansoldi, Stefano, Antonelli, L. A., Antoranz, P., Babic, A., Bangale, P., Barres De Almeida, U., Barrio, J. A., Becerra González, J., Bednarek, W., Berger, K., Bernardini, E., Biland, A., Blanch, O., Bock, R. K., Bonnefoy, S., Bonnoli, G., Borracci, F., Bretz, T., Carmona, E., Carosi, A., Carreto Fidalgo, D., Colin, P., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., Da Vela, P., Dazzi, F., De Angelis, A., De Caneva, G., De Lotto, B., Delgado Mendez, C., Doert, M., Domínguez, A., Dominis Prester, D., Dorner, D., Doro, M., Einecke, S., Eisenacher, D., Elsaesser, D., Farina, E., Ferenc, D., Fonseca, M. V., Font, L., Frantzen, K., Fruck, C., García López, R. J., Garczarczyk, M., Garrido Terrats, D., Gaug, M., Giavitto, G., Godinović, N., González Muñoz, A., Gozzini, S. R., Hadamek, A., Hadasch, D., Herrero, A., Hildebrand, D., Hose, J., Hrupec, D., Idec, W., Kadenius, V., Kellermann, H., Knoetig, M. L., Krause, J., Kushida, J., La Barbera, A., Lelas, D., Lewandowska, N., Lindfors, E., Longo, Francesco, Lombardi, S., López, M., López Coto, R., López Oramas, A., Lorenz, E., Lozano, I., Makariev, M., Mallot, K., Maneva, G., Mankuzhiyil, N., Mannheim, K., Maraschi, L., Marcote, B., Mariotti, M., Martínez, M., Mazin, D., Menzel, U., Meucci, M., Miranda, J. M., Mirzoyan, R., Moralejo, A., Munar Adrover, P., Nakajima, D., Niedzwiecki, A., Nilsson, K., Nowak, N., Orito, R., Overkemping, A., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Paredes Fortuny, X., Partini, S., Persic, M., Prada, F., Prada Moroni, P. G., Prandini, E., Preziuso, S., Puljak, I., Reinthal, R., Rhode, W., Ribó, M., Rico, J., Rodriguezgarcia, J., Rügamer, S., Saggion, A., Saito, K., Salvati, M., Satalecka, K., Scalzotto, V., Scapin, V., Schultz, C., Schweizer, T., Shore, S. N., Sillanpää, A., Sitarek, J., Snidaric, I., Sobczynska, D., Spanier, F., Stamatescu, V., Stamerra, A., Steinbring, T., Storz, J., Sun, S., Surić, T., Takalo, L., Tavecchio, F., Temnikov, P., Terzić, T., Tescaro, D., Teshima, M., Thaele, J., Tibolla, O., Torres, D. F., Toyama, T., Treves, A., Uellenbeck, M., Vogler, P., Wagner, R. M., Zandanel, F., Zanin, R., Archambault, S., Behera, B., Beilicke, M., Benbow, W., Bird, R., Buckley, J. H., Bugaev, V., Cerruti, M., Chen, X., Ciupik, L., Collins Hughes, E., Cui, W., Dumm, J., Eisch, J. D., Falcone, A., Federici, S., Feng, Q., Finley, J. P., Fleischhack, H., Fortin, P., Fortson, L., Furniss, A., Griffin, S., Griffiths, S. T., Grube, J., Gyuk, G., Hanna, D., Holder, J., Hughes, G., Humensky, T. B., Johnson, C. A., Kaaret, P., Kertzman, M., Khassen, Y., Kieda, D., Krawczynski, H., Krennrich, F., Kumar, S., Lang, M. J., Maier, G., Mcarthur, S., Meagher, K., Moriarty, P., Mukherjee, R., Ong, R. A., Otte, A. N., Park, N., Pichel, A., Pohl, M., Popkow, A., Prokoph, H., Quinn, J., Ragan, K., Rajotte, J., Reynolds, P. T., Richards, G. T., Roache, E., Rovero, A. C., Sembroski, G. H., Shahinyan, K., Staszak, D., Telezhinsky, I., Theiling, M., Tucci, J. V., Tyler, J., Varlotta, A., Wakely, S. P., Weekes, T. C., Weinstein, A., Welsing, R., Wilhelm, A., Williams, D. A., Zitzer, B., Villata, M., Raiteri, C., Aller, H. D., Aller, M. F., Chen, W. P., Jordan, B., Koptelova, E., Kurtanidze, O. M., Lähteenmäki, A., Mcbreen, B., Larionov, V. M., Lin, C. S., Nikolashvili, M. G., Angelakis, E., Capalbi, M., Carramiñana, A., Carrasco, L., Cassaro, P., Cesarini, A., Fuhrmann, L., Giroletti, M., Hovatta, T., Krichbaum, T. P., Krimm, H. A., Max Moerbeck, W., Moody, J. W., Maccaferri, G., Mori, Y., Nestoras, I., Orlati, A., Pace, C., Pearson, R., Perri, M., Readhead, A. C. S., Richards, J. L., Sadun, A. C., Sakamoto, T., Tammi, J., Tornikoski, M., Yatsu, Y., Zook, A., Department of Radio Science and Engineering, Aalto-yliopisto, Aalto University, and Universitat de Barcelona
- Subjects
Astrofísica ,Brightness ,Ciencias Físicas ,blazars ,Astrophysics ,telescope ,x-ray variability ,01 natural sciences ,Spectral line ,BL Lacertae objects ,individual ,Mrk 421 ,purl.org/becyt/ford/1 [https] ,Raigs gamma ,emission ,MAGIC (telescope) ,010303 astronomy & astrophysics ,Physics ,astro-ph.HE ,High Energy Astrophysical Phenomena (astro-ph.HE) ,individual: Mrk 421 [BL Lacertae objects] ,Galaxies: BL Lacertae objects: individual: Markarian 421 ,Spectral energy distribution ,Electrónica ,Electricidad ,Astrophysics - High Energy Astrophysical Phenomena ,CIENCIAS NATURALES Y EXACTAS ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Context (language use) ,Astrophysics::Cosmology and Extragalactic Astrophysics ,power spectra ,BL Lacertae object ,tev photons ,0103 physical sciences ,Nucli galàctic actiu ,bl lacertae objects: individual: mrk 421 ,Blazar ,Astronomy and Astrophysics ,Space and Planetary Science ,Active galactic nuclei ,010308 nuclear & particles physics ,light curves ,Gamma rays ,Institut für Physik und Astronomie ,purl.org/becyt/ford/1.3 [https] ,Light curve ,Galaxies ,Galàxies ,Astronomía ,Crab Nebula ,optical variability ,active galactic nuclei ,Galàxies actives ,Active galaxies ,markarian-421 ,ddc:520 - Abstract
We performed a 4.5-month multi-instrument campaign (from radio to VHE gamma rays) on Mrk421 between January 2009 and June 2009, which included VLBA, F-GAMMA, GASP-WEBT, Swift, RXTE, Fermi-LAT, MAGIC, and Whipple, among other instruments and collaborations. Mrk421 was found in its typical (non-flaring) activity state, with a VHE flux of about half that of the Crab Nebula, yet the light curves show significant variability at all wavelengths, the highest variability being in the X-rays. We determined the power spectral densities (PSD) at most wavelengths and found that all PSDs can be described by power-laws without a break, and with indices consistent with pink/red-noise behavior. We observed a harder-when-brighter behavior in the X-ray spectra and measured a positive correlation between VHE and X-ray fluxes with zero time lag. Such characteristics have been reported many times during flaring activity, but here they are reported for the first time in the non-flaring state. We also observed an overall anti-correlation between optical/UV and X-rays extending over the duration of the campaign. The harder-when-brighter behavior in the X-ray spectra and the measured positive X-ray/VHE correlation during the 2009 multi-wavelength campaign suggests that the physical processes dominating the emission during non-flaring states have similarities with those occurring during flaring activity. In particular, this observation supports leptonic scenarios as being responsible for the emission of Mrk421 during non-flaring activity. Such a temporally extended X-ray/VHE correlation is not driven by any single flaring event, and hence is difficult to explain within the standard hadronic scenarios. The highest variability is observed in the X-ray band, which, within the one-zone synchrotron self-Compton scenario, indicates that the electron energy distribution is most variable at the highest energies., Comment: Accepted for publication in A&A, 18 pages, 14 figures (v2 has a small modification in the acknowledgments, and also corrects a typo in the field "author" in the metadata)
- Published
- 2015
- Full Text
- View/download PDF
37. Building the green office, Claremont Colleges sustainability initiative proposal.
- Author
-
Hazlett, Rick (Director, Environmental Analysis Program, Pomona College); Jackson, Hunter (student, Claremont McKenna College); Blouin, Michael (student, Pomona College); Zucker, Daniel (student, Pomona College); Hansen, Jim (Director of Campus Planning and Maintenance, Pomona College) and Hazlett, Rick (Director, Environmental Analysis Program, Pomona College); Jackson, Hunter (student, Claremont McKenna College); Blouin, Michael (student, Pomona College); Zucker, Daniel (student, Pomona College); Hansen, Jim (Director of Campus Planning and Maintenance, Pomona College)
- Subjects
- Sustainable development., Energy conservation., Environmental auditing California., College campuses California Claremont., Conservation of Energy Resources, Développement durable., Économies d'énergie., Vérification environnementale Californie., Campus Californie Claremont., sustainable development., energy conservation., College campuses., Energy conservation., Environmental auditing., Sustainable development., California., California Claremont.
- Abstract
CONTENTS: Team leader Team members Issue to be addressed Background information Proposed project Anticipated follow-up implementation Proposed itemized budget.
- Published
- 2008
38. Card from Pomona College
- Author
-
Pomona College and Pomona College
- Published
- 2012
39. Pomona College Bulletin
- Author
-
Pomona College
- Subjects
gymnasium ,football ,baseball ,Pomona College ,track ,faculty ,tennis ,athletics ,physical examination ,committes ,physical training department ,interscholastic ,Walter Hempel - Abstract
Booklet describing physical training department at Pomona College.
- Published
- 1904
40. Karl Benjamin: The Pomona Years 1979-1994
- Author
-
Pomona College, Bassett/Shearer Productions, Bassett, Bob, Chamberlain, Richard, Pomona College, Bassett/Shearer Productions, Bassett, Bob, and Chamberlain, Richard
- Abstract
This video contains Benjamin’s artistic philosophy on abstract painting and his autobiography of his artistic career. Benjamin discusses the beginning of his art career while teaching elementary school. Chamberlain discusses Benjamin’s enrollment in Claremont Graduate School and his seminal work in the exhibition “For Abstract Classicists”. Benjamin discusses the exhibition’s influence on the 1950s art world, and how critics canonized his art as “Hard Edge” painting. Benjamin discusses theory of color and painting methodology as “impulses”. He cites Dewey’s “Art as Experience” as a major influence. He also discusses critical perception of his work, particularly his relationship with Clement Greenberg and the competitive art world. Chamberlain then discusses Benjamin’s role as Professor of Art at Pomona College and Professor of Art at Claremont Graduate School. Benjamin discusses his teaching methodology and philosophy on the artistic process. The documentary ends with an announcement of an exhibition of Karl’s work at Pomona College’s Montgomery Gallery., California Audiovisual Preservation Project (CAVPP)
41. Reference star differential imaging of close-in companions and circumstellar disks with the NIRC2 vortex coronagraph at W.M. Keck Observatory
- Author
-
Maddalena Reggiani, Carlos A. Gomez Gonzalez, Elsa Huby, Garreth Ruane, Nicole Wallack, Dimitri Mawet, Olivier Absil, Keith Matthews, Henry Ngo, Elodie Choquet, W. Jerry Xuan, Eugene Serabyn, Tiffany Meshkat, Therese Cook, Caltech Department of Astronomy [Pasadena], California Institute of Technology (CALTECH), NRC Herzberg Institute of Astrophysics, National Research Council of Canada (NRC), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), University of California [Los Angeles] (UCLA), University of California (UC), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Infrared Processing and Analysis Center (IPAC), Department of Mathematics - Pomona College, Pomona College, California Institute of Technology (CALTECH)-NASA, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), University of California, Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
planets and satellites: detection ,W. M. Keck Observatory ,010504 meteorology & atmospheric sciences ,TELESCOPE ,detection [planets and satellites] ,IMAGES ,FOS: Physical sciences ,Astrophysics ,Star (graph theory) ,Astronomy & Astrophysics ,01 natural sciences ,law.invention ,LIMITS ,stars: individual: 2MASS J16042165-2130284 ,law ,0103 physical sciences ,Sensitivity (control systems) ,Differential (infinitesimal) ,010303 astronomy & astrophysics ,Coronagraph ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,0105 earth and related environmental sciences ,Physics ,Earth and Planetary Astrophysics (astro-ph.EP) ,Science & Technology ,protoplanetary disks ,high angular resolution [techniques] ,techniques: high angular resolution ,Astronomy and Astrophysics ,Circumstellar disk ,imaging [stars] ,stars: imaging ,Vortex ,[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM] ,Space and Planetary Science ,Physical Sciences ,stars: individual: MWC 758 ,1ST LIGHT ,Astrophysics - Instrumentation and Methods for Astrophysics ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,individual (MWC 758, 2MASS J16042165-2130284) [stars] ,Reference frame ,Optics (physics.optics) ,Astrophysics - Earth and Planetary Astrophysics ,Physics - Optics - Abstract
Reference star differential imaging (RDI) is a powerful strategy for high contrast imaging. Using example observations taken with the vortex coronagraph mode of Keck/NIRC2 in $L^\prime$ band, we demonstrate that RDI provides improved sensitivity to point sources at small angular separations compared to angular differential imaging (ADI). Applying RDI to images of the low-mass stellar companions HIP 79124 C (192 mas separation, $\Delta L^\prime$=4.01) and HIP 78233 B (141 mas separation, $\Delta L^\prime$=4.78), the latter a first imaging detection, increases the significance of their detections by up to a factor of 5 with respect to ADI. We compare methods for reference frames selection and find that pre-selection of frames improves detection significance of point sources by up to a factor of 3. In addition, we use observations of the circumstellar disks around MWC 758 and 2MASS J16042165-2130284 to show that RDI allows for accurate mapping of scattered light distributions without self-subtraction artifacts., Comment: Accepted for publication in The Astronomical Journal
- Published
- 2019
- Full Text
- View/download PDF
42. The Structure and Stability of Persistence Modules
- Author
-
Frédéric Chazal, Vin de Silva, Marc Glisse, Steve Oudot, Understanding the Shape of Data (DATASHAPE), Inria Sophia Antipolis - Méditerranée (CRISAM), Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Inria Saclay - Ile de France, Institut National de Recherche en Informatique et en Automatique (Inria), Geometric computing (GEOMETRICA), Department of Mathematics - Pomona College, Pomona College, ANR-13-BS01-0008,TopData,Analyse Topologique des Données : Méthodes Statistiques et Estimation(2013), and European Project: 339025,EC:FP7:ERC,ERC-2013-ADG,GUDHI(2014)
- Subjects
[MATH.MATH-AT]Mathematics [math]/Algebraic Topology [math.AT] ,010102 general mathematics ,computational topology ,010103 numerical & computational mathematics ,Persistent homology ,0101 mathematics ,stability ,[INFO.INFO-CG]Computer Science [cs]/Computational Geometry [cs.CG] ,01 natural sciences ,persistence modules - Abstract
International audience; This book is a comprehensive treatment of the theory of persistence modules over the real line. It presents a set of mathematical tools to analyse the structure and to establish the stability of such modules, providing a sound mathematical framework for the study of persistence diagrams. Completely self-contained, this brief introduces the notion of persistence measure and makes extensive use of a new calculus of quiver representations to facilitate explicit computations.Appealing to both beginners and experts in the subject, The Structure and Stability of Persistence Modules provides a purely algebraic presentation of persistence, and thus complements the existing literature, which focuses mainly on topological and algorithmic aspects.
- Published
- 2016
43. Persistence Stability for Geometric complexes
- Author
-
Vin de Silva, Frédéric Chazal, Steve Oudot, Geometric computing (GEOMETRICA), Inria Sophia Antipolis - Méditerranée (CRISAM), Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Inria Saclay - Ile de France, Institut National de Recherche en Informatique et en Automatique (Inria), Department of Mathematics - Pomona College, and Pomona College
- Subjects
Computational Geometry (cs.CG) ,FOS: Computer and information sciences ,Pure mathematics ,Cellular homology ,Mathematics::General Topology ,Totally bounded space ,010103 numerical & computational mathematics ,Algebraic geometry ,Homology (mathematics) ,Cech complex ,[INFO.INFO-CG]Computer Science [cs]/Computational Geometry [cs.CG] ,01 natural sciences ,Mathematics::Algebraic Topology ,Mathematics::K-Theory and Homology ,51F99 55N99 ,FOS: Mathematics ,Vietoris–Rips complex ,Algebraic Topology (math.AT) ,Mathematics - Algebraic Topology ,Persistent homology ,0101 mathematics ,Mathematics::Symplectic Geometry ,Vietoris-Rips complex ,Mathematics ,Discrete mathematics ,Gromov-Hausdorff distance ,010102 general mathematics ,Metric space ,[MATH.MATH-AT]Mathematics [math]/Algebraic Topology [math.AT] ,Computer Science - Computational Geometry ,Geometry and Topology ,Relative homology - Abstract
In this paper we study the properties of the homology of different geometric filtered complexes (such as Vietoris-Rips, Cech and witness complexes) built on top of precompact spaces. Using recent developments in the theory of topological persistence we provide simple and natural proofs of the stability of the persistent homology of such complexes with respect to the Gromov--Hausdorff distance. We also exhibit a few noteworthy properties of the homology of the Rips and Cech complexes built on top of compact spaces., Comment: We include a discussion of ambient Cech complexes and a new class of examples called Dowker complexes
- Published
- 2014
- Full Text
- View/download PDF
44. The observable structure of persistence modules
- Author
-
Frédéric Chazal, Vin de Silva, William Crawley-Boevey, Geometric computing (GEOMETRICA), Inria Sophia Antipolis - Méditerranée (CRISAM), Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Inria Saclay - Ile de France, Institut National de Recherche en Informatique et en Automatique (Inria), Department of Pure Mathematics, University of Leeds, Department of Mathematics - Pomona College, Pomona College, and ANR-13-BS01-0008,TopData,Analyse Topologique des Données : Méthodes Statistiques et Estimation(2013)
- Subjects
Large class ,Pure mathematics ,Persistent homology ,persistence module ,[MATH.MATH-RT]Mathematics [math]/Representation Theory [math.RT] ,010102 general mathematics ,Natural number ,Observable ,010103 numerical & computational mathematics ,Persistence diagram ,01 natural sciences ,persistent homology ,Mathematics (miscellaneous) ,FOS: Mathematics ,0101 mathematics ,Invariant (mathematics) ,Representation Theory (math.RT) ,Real line ,Finite set ,Mathematics - Representation Theory ,Mathematics - Abstract
In persistent topology, q-tame modules appear as a natural and large class of persistence modules indexed over the real line for which a persistence diagram is de- finable. However, unlike persistence modules indexed over a totally ordered finite set or the natural numbers, such diagrams do not provide a complete invariant of q-tame modules. The purpose of this paper is to show that the category of persistence modules can be adjusted to overcome this issue. We introduce the observable category of persistence modules: a localization of the usual category, in which the classical properties of q-tame modules still hold but where the persistence diagram is a complete isomorphism invariant and all q-tame modules admit an interval decomposition.
- Published
- 2014
- Full Text
- View/download PDF
45. Sharing wintering grounds does not synchronize annual survival in a high Arctic seabird, the little auk
- Author
-
Katarzyna Wojczulanis-Jakubas, Maria Gavrilo, Børge Moe, Yuri Krasnov, Dariusz Jakubas, David Grémillet, Benjamin Merkel, Hallvard Strøm, Jorg Welcker, Nina J. Karnovsky, Jérôme Fort, Kurt Jerstad, Sébastien Descamps, Rémi Choquet, Harald Steen, Norwegian Polar Institute, Centre d’Ecologie Fonctionnelle et Evolutive (CEFE), Université Paul-Valéry - Montpellier 3 (UPVM)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro)-École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), LIttoral ENvironnement et Sociétés - UMRi 7266 (LIENSs), Université de La Rochelle (ULR)-Centre National de la Recherche Scientifique (CNRS), Association Maritime Heritage, Faculty of Biology [Gdansk, Poland], University of Gdańsk (UG), Jerstad Viltforvaltning, Pomona College, Norwegian Institute for Nature Research (NINA), BIOCONSULT BREMEN DEU, Partenaires IRSTEA, Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA), Université Paul-Valéry - Montpellier 3 (UPVM)-École Pratique des Hautes Études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut Agro - Montpellier SupAgro, Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro), LIttoral ENvironnement et Sociétés (LIENSs), and La Rochelle Université (ULR)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
0106 biological sciences ,[SDV]Life Sciences [q-bio] ,Aquatic Science ,migration ,010603 evolutionary biology ,01 natural sciences ,non-breeding distribution ,Survival data ,biology.animal ,capture-markrecapture ,14. Life underwater ,Ecology, Evolution, Behavior and Systematics ,Extinction ,Ecology ,biology ,010604 marine biology & hydrobiology ,synchrony ,Capture mark recapture ,Alle alle ,15. Life on land ,Geography ,Arctic ,[SDE]Environmental Sciences ,geolocator ,Seabird ,Vital rates - Abstract
Sharing the same wintering grounds by avian populations breeding in various areas may synchronize fluctuations in vital rates, which could increase the risk of extinction. Here, by combining multi-colony tracking with long-term capture-recapture data, we studied the winter distribution and annual survival of the most numerous Arctic seabird, the little aukAlle alle. We assessed whether little auks from different breeding populations in Svalbard and Franz Josef Land use the same wintering grounds and if this leads to synchronized survival. Our results indicate that birds from the Svalbard colonies shared similar wintering grounds, although differences existed in the proportion of birds from each colony using the different areas. Little auks from Franz Josef Land generally spent the winter in a separate area, but some individuals wintered in the Iceland Sea with Svalbard populations. Survival data from 3 Svalbard colonies collected in 2005-2018 indicated that sharing wintering grounds did not synchronize little auk annual survival rates. However, it is clear that the Iceland Sea is an important wintering area for little auks, and environmental changes in this area could have widespread impacts on many populations.
- Published
- 2021
- Full Text
- View/download PDF
46. The structure and stability of persistence modules
- Author
-
Chazal, Frederic, de Silva, Vin, Glisse, Marc, Oudot, Steve, Geometric computing (GEOMETRICA), Inria Sophia Antipolis - Méditerranée (CRISAM), Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Inria Saclay - Ile de France, Institut National de Recherche en Informatique et en Automatique (Inria), Department of Mathematics - Pomona College, Pomona College, ANR-09-BLAN-0331,GIGA(2009), and European Project: 255827,EC:FP7:ICT,FP7-ICT-2009-C,CG LEARNING(2010)
- Subjects
Computational Geometry (cs.CG) ,FOS: Computer and information sciences ,[MATH.MATH-AT]Mathematics [math]/Algebraic Topology [math.AT] ,FOS: Mathematics ,Computer Science - Computational Geometry ,Algebraic Topology (math.AT) ,Mathematics - Category Theory ,Category Theory (math.CT) ,Mathematics - Algebraic Topology ,[INFO.INFO-CG]Computer Science [cs]/Computational Geometry [cs.CG] - Abstract
We give a self-contained treatment of the theory of persistence modules indexed over the real line. We give new proofs of the standard results. Persistence diagrams are constructed using measure theory. Linear algebra lemmas are simplified using a new notation for calculations on quiver representations. We show that the stringent finiteness conditions required by traditional methods are not necessary to prove the existence and stability of the persistence diagram. We introduce weaker hypotheses for taming persistence modules, which are met in practice and are strong enough for the theory still to work. The constructions and proofs enabled by our framework are, we claim, cleaner and simpler., Comment: New version. We discuss in greater depth the interpolation lemma for persistence modules
- Published
- 2012
47. Choice Architecture to Improve Financial Decision Making
- Author
-
Julian C. Jamison, Jeffrey P. Carpenter, Andrea Robbett, Dustin Beckett, Peter Hans Matthews, Emiliano Huet-Vaughn, Middlebury College, Pomona College, Department of Economics, Consumer Financial Protection Bureau, University of Exeter, Aalto-yliopisto, and Aalto University
- Subjects
Economics and Econometrics ,choice architecture ,Exploit ,Computer science ,media_common.quotation_subject ,Psychological intervention ,prepaid card ,convex time budget ,Presentation ,attribute overload ,0502 economics and business ,050207 economics ,Marketing ,media_common ,consumer finance ,time preference ,experiment ,05 social sciences ,Structural estimation ,risk preference ,Consumer finance ,Choice architecture ,welfare ,050211 marketing ,Time preference ,Welfare ,structural estimation ,Social Sciences (miscellaneous) - Abstract
We exploit the principles of choice architecture to evaluate interventions in the market for reloadable prepaid cards. Participants are randomized into three card menu presentation treatments—the market status quo, a regulation-inspired reform, or an enhanced reform designed to minimize attribute overload—and offered choices based on prior structural estimation of individual preferences. Consumers routinely choose incorrectly under the status quo, with tentative evidence that the regulation-inspired presentation may increase best card choice and clear evidence that the enhanced reform reduces worst card choice. Welfare analysis suggests the regulation-inspired presentation offers modest gains, while the enhanced policy generates substantial benefits.
- Published
- 2021
- Full Text
- View/download PDF
48. Transient Probability Functions: A Sample Path Approach
- Author
-
Alan C. Krinik, Gerardo Rubino, Randall J. Swift, Michael L. Green, Carrie Mortensen, Department of Mathematics - Pomona College, Pomona College, Architectures and network models (ARMOR), Institut de Recherche en Informatique et Systèmes Aléatoires (IRISA), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-INRIA Rennes, Institut National de Recherche en Informatique et en Automatique (Inria)-Ecole Nationale Supérieure des Télécommunications de Bretagne, Cyril Banderier and Christian Krattenthaler, Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-Université de Rennes 1 (UR1), and Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-Institut National de Recherche en Informatique et en Automatique (Inria)-Centre National de la Recherche Scientifique (CNRS)-INRIA Rennes
- Subjects
General Computer Science ,sample paths ,[INFO.INFO-DS]Computer Science [cs]/Data Structures and Algorithms [cs.DS] ,Markov process ,[INFO.INFO-DS] Computer Science [cs]/Data Structures and Algorithms [cs.DS] ,transient probability functions ,[INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM] ,[INFO.INFO-CG]Computer Science [cs]/Computational Geometry [cs.CG] ,dual processes ,Theoretical Computer Science ,Dual (category theory) ,[MATH.MATH-CO] Mathematics [math]/Combinatorics [math.CO] ,symbols.namesake ,[INFO.INFO-DM] Computer Science [cs]/Discrete Mathematics [cs.DM] ,[INFO.INFO-CG] Computer Science [cs]/Computational Geometry [cs.CG] ,[MATH.MATH-CO]Mathematics [math]/Combinatorics [math.CO] ,symbols ,Discrete Mathematics and Combinatorics ,Transient (computer programming) ,Sample path ,randomization ,Algorithm ,Mathematics - Abstract
A new approach is used to determine the transient probability functions of Markov processes. This new solution method is a sample path counting approach and uses dual processes and randomization. The approach is illustrated by determining transient probability functions for a three-state Markov process. This approach also provides a way to calculate transient probability functions for Markov processes which have specific sample path characteristics.
- Published
- 2003
- Full Text
- View/download PDF
49. Ethics, New Colonialism, and Lidar Data: A Decade of Lidar in Maya Archaeology
- Author
-
Adrian S. Z. Chase, Arlen F. Chase, Diane Z. Chase, Arizona State University [Tempe] (ASU), Claremont Graduate University [Claremont, CA ], and Pomona College
- Subjects
010506 paleontology ,Archeology ,History ,[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistory ,mesoamerican archaeology ,Looting ,Colonialism ,01 natural sciences ,lcsh:QA75.5-76.95 ,Sovereignty ,Maya ,0601 history and archaeology ,lcsh:CC1-960 ,ComputingMilieux_MISCELLANEOUS ,lidar ,0105 earth and related environmental sciences ,Structure (mathematical logic) ,060102 archaeology ,new colonialism ,sovereignty ,06 humanities and the arts ,ethics ,Archaeology ,Field (geography) ,Computer Science Applications ,Lidar ,Paradigm shift ,lcsh:Archaeology ,lcsh:Electronic computers. Computer science ,looting - Abstract
Maya archaeology has witnessed a paradigm shift in interpretations of the past with regards to the structure and organization of ancient societies as a result of the introduction of lidar to the field a decade ago. Lidar provided control of spatial parameters in a way that had not been previously possible. But, the introduction of this technology has also involved researchers in a series of broader ethical debates. While archaeology has always provided huge data sets for processing, the digital lidar files are even larger and also need appropriate long-term storage and management considerations. It is here that there are differences of opinion worldwide on how to treat lidar data as scientific and open yet national and protected datasets. Some countries do not want fully public access to these files because of the potential danger posed to the looting of their heritage and security or military concerns. Yet, to a large extent, technology is overtaking some of the debate over accessibility, especially as newer satellite technology will surely alter the perceived physical boundaries and challenge the sovereignty of modern nation-states. However, how lidar is used and accessed in the future has become a cross-national issue that is worthy of being addressed in greater detail.
- Published
- 2020
- Full Text
- View/download PDF
50. Post-foraging in-colony behaviour of a central-place foraging seabird
- Author
-
Katarzyna Wojczulanis-Jakubas, Antoine Grissot, Marion Devogel, Lauraleen Altmeyer, Tessa Fujisaki, Dariusz Jakubas, Dorota Kidawa, Nina Karnovsky, University of Gdańsk (UG), UMS 3343 (OSU), Observatoire des Sciences de l'Univers de Rennes (OSUR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Pomona College, and National Science Centre (NCN) [2017/25/B/NZ8/01417, 2017/26/D/NZ8/00005]
- Subjects
Birds ,Male ,Charadriiformes ,Multidisciplinary ,Ecology ,Predatory Behavior ,[SDE]Environmental Sciences ,Animals ,Female ,Feeding Behavior - Abstract
Studies on time allocation of various activities are crucial to understand which behavioural strategy is the most profitable in a given context, and so why animals behave in a particular way. Such investigations usually focus on a time window when the studied activity is performed, often neglecting how the time devoted to focal activity affects time allocation to following-up behaviours, while that may have its own fitness consequences. In this study, we examined time allocation into three post-foraging activities (entering the nest with food, nest attendance, and colony attendance) in a small seabird species, the little auk (Alle alle). Since little auks alternate foraging trips of different duration (short and long) and purpose (offspring feeding and primarily self-feeding, respectively) we expected that duration of the following up in-colony activities would also vary, being longer after a long absence in the colony (because of greater need of reassessment of the current predation pressure and social interactions in the colony, and re-establishing the bond with the offspring and/or partner and/or neighbours after longer absence). We found that it was not always the case, as time allocation of the post-foraging in-colony activities was primarily year- and sex-specific. It highlights the need to consider year and sex effects in studies of behavioural ecology, as not doing so may lead to spurious conclusions. Interestingly, and despite a great inter-individual variation in time allocation in the post-foraging in-colony activities, little auk individuals were quite repeatable in their behavioural performance, which suggests these activities may reflect birds behavioural profile. Overall, post-foraging in-colony activity of the little auk, although not much dependent on duration/type of the preceding foraging flights, varies with respect to year and sex, and as such may be a proxy of behavioural plasticity of the population.
- Published
- 2022
- Full Text
- View/download PDF
Catalog
Discovery Service for Jio Institute Digital Library
For full access to our library's resources, please sign in.