382 research outputs found
Positive and Negative Emotions Predict Weight Loss Intentions and Behaviors beyond Theory of Planned Behavior Constructs
Get PDFAcknowledgements: This study was funded by the ScienceCampus Tuebingen (TP7.1) awarded to Devin G. Ray and Kai Sassenberg.Peer reviewe
Scott, Kirby, December 10, 2020 [Interview]
No full textKirby Scott was interviewed on December 10, 2020, by Devin McKinney about his childhood, his education at Gettysburg College, and his personal and professional paths in the years since graduation.Reider, Ray; Streeter, Barry; Shoemaker, Howard G.; Hummel, R. Eugene; Sabol, Jim; Haas, Eugene; Ward, James; Biser, Gareth V.; Bugbee, Bruce W.; Gray, Stan; Sims, James; Ayers, Michael; Collier, Glendon; Betterly, TimCarl Arnold Hanson Years
Hely, Lois Davis & Jim
No full textLois Davis Hely and Jim Hely were interviewed on June 30, 2017, by Michael Birkner and Devin McKinney about their childhoods and early education, their meeting at Gettysburg College, and aspects of their college experience relating go the America of the late 1960s.Roosevelt, Franklin D.; Kennedy, John F.; Kenney, Grace C.; Marter, Helen; Henry, Patricia; Books, Woodrow; Heilig, Bonnie; Haas, Eugene M.; Shoemaker, Howard G.; Hummel, R. Eugene; Reider, Ray; Hanson, C. Arnold; Hely, Daniel; Hammann, Louis J.; Biser, Gareth V.; Graham, Bonnie Chadwick; Schreckengaust, Ray; Hartman, David W.; Eddy, Stetson; Dunkelberger, Harold A.; Freed, Edwin D.; Moore, Carey A.; Powers, Janet; Carmody, Robert; Cesere, Paul; Waldman, Robert; Donahue, Sue Niblette; Hook, Wade F.; Collier, GlendonC. Arnold Hanson Years
Henderson, Jim, March 13 and 30, 2014 [Interview]
No full textJim Henderson was interviewed on March 13 and 30, 2014, by Devin McKinney about his life before, during, and after his years at Gettysburg College, with specific focus on his participation in the spring 1971 Christ Chapel production of "Jesus Christ Superstar."Hanson, C. Arnold; Vannorsdall, John W.; Loose, John H.; Pickering, James D.; Buckley, William F.; DeSantis, Tullio F.; Brandenburg, Zane; Henderson, Nancy; Hammann, Louis J.; Richardson, Norman E.; Kirk, Rahsaan Roland; Harrison, George; Winwood, Steve; Stewart, Mary Margaret; Lindeman, Ralph D.; Myers, Joseph; Cavaliere, A. Ralph; Recla, Lawrence R.; Rinehart, Larry; Lowenthal, Lawrence D.; McLaughlin, Harold; Reider, Ray; Cotton, Gene; Gilbert, Ted; Simpson, Charles; Eisenhower, Dwight D.; Nixon, Richard M.; Burdack, Karen; Alsedek, Kelly; Wyatt, Doug; Myers, Whitney; Bauer, DaveCarl Arnold Hanson Years
The investigation of phase synchronization in the cortex during a fatiguing muscle contraction using EEG
No full textIncludes bibliographical references (leaves 140-157)
CTA – the World’s largest ground-based gamma-ray observatory
Get PDFVery-High Energy (VHE) gamma-ray astroparticle physics is a relatively young field, and observations
over the past decade have surprisingly revealed almost two hundred VHE emitters which
appear to act as cosmic particle accelerators. These sources are an important component of the
Universe, influencing the evolution of stars and galaxies. At the same time, they also act as a
probe of physics in the most extreme environments known - such as in supernova explosions, and
around or after the merging of black holes and neutron stars. However, the existing experiments
have provided exciting glimpses, but often falling short of supplying the full answer. A deeper
understanding of the TeV sky requires a significant improvement in sensitivity at TeV energies,
a wider energy coverage from tens of GeV to hundreds of TeV and a much better angular and
energy resolution with respect to the currently running facilities. The next generation gamma-ray
observatory, the Cherenkov Telescope Array Observatory (CTAO), is the answer to this need.
In this talk I will present this upcoming observatory from its design to the construction, and its
potential science exploitation. CTAO will allow the entire astronomical community to explore a
new discovery space that will likely lead to paradigm-changing breakthroughs. In particular, CTA
has an unprecedented sensitivity to short (sub-minute) timescale phenomena, placing it as a key
instrument in the future of multi-messenger and multi-wavelength time domain astronomy. I will
conclude the talk presenting the first scientific results obtained by the LST-1, the prototype of one
CTA telescope type - the Large Sized Telescope, that is currently under commission
Cross-group recognition bias generalizes to diverse non-face representations of digital identity
No full text- …
