Context dependence of the event-related brain potential associated with reward and punishment

The error-related negativity (ERN) is an event-related brain potential elicited by error commission and by presentation of feedback stimuli indicating incorrect performance. In this study, the authors report two experiments in which participants tried to learn to select between response options by trial and error, using feedback stimuli indicating monetary gains and losses. The results demonstrate that the amplitude of the ERN is determined by the value of the eliciting outcome relative to the range of outcomes possible, rather than by the objective value of the outcome. This result is discussed in terms of a recent theory that holds that the ERN reflects a reward prediction error signal associated with a neural system for reinforcement learning

Treaty Signed Between the Allied Powers and His Majest the Emperor Napoleon

“Traité de Fontainebleau (1814)” or the Treaty of Fontainebleau, is the treaty that ended the first reign of Emperor Napoleon Bonaparte over France on April 11, 1814. The treaty was negotiated by representatives of the Allied Powers- Austria, Hungary, Bohemia, Russia and Prussia- and signed by Emperor Napoleon Bonaparte. The treaty in addition to ending Emperor Napoleon’s rule over France, granted him the island of Elba as an autonomous principality over which Napoleon would have sole power. Emperor Napoleon, after discovering the success of the treaty in the French Senate on April 3rd, attempted a final routing of the allied powers, but failed to successfully relinquish his power in favor of his son with the Empress Josephine as regent. The sovereigns of the Allied Powers were not willing to negotiate this change in leadership, and rejected Napoleon’s attempt to maintain power. Napoleon’s conditional relinquishment was not accepted, and he was left with no military options. He succumbed to his fate of exile on the island of Elba with extremely limited powers. The Treaty of Fontainebleau was signed by the Allied powers on April 11th and ratified by the Senate on April 13th

The Thousand Asteroid Light Curve Survey

We present the results of our Thousand Asteroid Light Curve Survey (TALCS) conducted with the Canada-France-Hawaii Telescope in September 2006. Our untargeted survey detected 828 Main Belt asteroids to a limiting magnitude of g'~22.5 corresponding to a diameter range of 0.4 km <= D <= 10 km. Of these, 278 objects had photometry of sufficient quality to perform rotation period fits. We debiased the observations and light curve fitting process to determine the true distribution of rotation periods and light curve amplitudes of Main Belt asteroids. We confirm a previously reported excess in the fraction of fast rotators but find a much larger excess of slow rotating asteroids (~15% of our sample). A few percent of objects in the TALCS size range have large light curve amplitudes of ~1 mag. Fits to the debiased distribution of light curve amplitudes indicate that the distribution of triaxial ellipsoid asteroid shapes is proportional to the square of the axis-ratio, (b/a)^2, and may be bi-modal. Finally, we find six objects with rotation periods that may be less than 2 hours with diameters between 400 m and 1.5 km, well above the break-up limit for a gravitationally-bound aggregate. Our debiased data indicate that this population represents <4% of the Main Belt in the 1-10 km size range.Comment: Accepted to Icarus. Full tables to appear there in electronic format, or contact autho

Face Coverings Differentially Alter Valence Judgments of Emotional Expressions

Face masks that prevent disease transmission obscure facial expressions, impairing nonverbal communication. We assessed the impact of lower (masks) and upper (sunglasses) face coverings on emotional valence judgments of clearly valenced (fearful, happy) and ambiguously valenced (surprised) expressions, the latter of which have both positive and negative meanings. Masks, but not sunglasses, impaired judgments of clearly valenced expressions compared to faces without coverings. Drift diffusion models revealed that lower, but not upper, face coverings slowed evidence accumulation and affected differences in non-judgment processes (i.e., stimulus encoding, response execution time) for all expressions. Our results confirm mask-interference effects in nonverbal communication. The findings have implications for nonverbal and intergroup communication, and we propose guidance for implementing strategies to overcome mask-related interference

Custom Unit Pump Development for the EVA PLSS

This paper describes the effort by the Texas Engineering Experiment Station (TEES) and Honeywell for NASA to design and test a pre-flight prototype pump for use in the Extra-vehicular activity (EVA) portable life support subsystem (PLSS). Major design decisions were driven by the need to reduce the pump s mass, power, and volume compared to the existing PLSS pump. In addition, the pump must accommodate a much wider range of abnormal conditions than the existing pump, including vapor/gas bubbles and increased pressure drop when employed to cool two suits simultaneously. A positive displacement, external gear type pump was selected because it offers the most compact and highest efficiency solution over the required range of flow rates and pressure drops. An additional benefit of selecting a gear pump design is that it is self priming and capable of ingesting non-condensable gas without becoming air locked. The chosen pump design consists of a 28 V DC, brushless, seal-less, permanent magnet motor driven, external gear pump that utilizes a Honeywell development that eliminates the need for magnetic coupling. The pump design was based on existing Honeywell designs, but incorporated features specifically for the PLSS application, including all of the key features of the flight pump. Testing at TEES verified that the pump meets the design requirements for range of flow rates, pressure drop, power consumption, working fluid temperature, operating time, gas ingestion, and restart capability under both ambient and vacuum conditions. The pump operated at 40 to 240 lbm/hr flow rate, 35 to 100 oF pump temperature, and 5 to 10 psid pressure rise. Power consumption of the pump controller at the nominal operating point in both ambient and vacuum conditions was 9.5 W, which was less than the 12 W predicted. Gas ingestion capabilities were tested by injecting 100 cc of air into the fluid line; the pump operated normally throughout this test

Star Clusters in M31: I. A Catalog and a Study of the Young Clusters

We present an updated catalog of 1300 objects in the field of M31, including 670 likely star clusters of various types. Archival images were inspected to confirm cluster classifications where possible, but most of the classifications were based on spectra taken of ~1000 objects with the Hectospec fiber positioner and spectrograph on the 6.5m MMT. The spectra and images of young clusters are analyzed in detail in this paper. Ages, reddenings and masses of 140 young clusters are derived by comparing the observed spectra and photometry with model spectra. We find these to have masses as great as 10^5 with a median of 10^4 M_sun, and a median age of 0.25 Gyr. Thus these clusters are similar in mass to the LMC young massive clusters, and are in between Milky Way open clusters and the globulars of M31 and the Milky Way. Most of the M31 young clusters have the low concentration typical of Milky Way open clusters, and we expect that most of these will be disrupted in the next Gyr, but a few have high concentrations and will likely survive longer. The spatial distribution of the young clusters is well correlated with the star-forming regions as mapped out by mid-IR emission. A kinematic analysis likewise confirms the spatial association of the young clusters with the young disk in M31.Comment: 18 pages of text and figures, 23 of tables, to appear in AJ. http://www.cfa.harvard.edu/oir/eg/m31clusters/M31_Hectospec.html is a new M31 web site containing tables and postage stamp images of the entire catalo