FUTURE INTERESTS - STATUTE ABOLISHING THE RULE IN SHELLEY\u27S CASE APPLIED TO THE WORTHIER TITLE DOCTRINE

Plaintiff set up an irrevocable trust of $75,000 to pay the income to himself for life, and upon his death to distribute the remainder of the trust to his heirs at law according to the laws of succession of the State of California in existence at his death. He later brought suit to terminate the trust on the theory that the worthier title doctrine prevented the creation of a remainder in his heirs at law, and that as sole beneficiary of the trust, he was entitled to termination. Held, the worthier title doctrine was inapplicable because of a statute which changed the word heirs from a word of limitation to a word of purchase, thereby creating a remainder in the settlor\u27s heirs, and preventing termination of the trust. Bixby v. California Trust Co., (Cal. App. 1948) 190 P. (2d) 321

Oil and Gas Interests in a Decedent\u27s Estate

Oil and Gas Interests in a Decedent\u27s Estat

Oil and Gas Interests in a Decedent\u27s Estate

Oil and Gas Interests in a Decedent\u27s Estat

Note and Comment

Attendance at the Law School; An Extreme Case in the Application of the Safety Appliance Act; Advisory Opinions; Refusal of Specific Performance Where Subsequent Unexpected Events Render it Inequitable; Is Vasectomy a Cruel Punishmen

The Ursinus Weekly, January 16, 1956

Thirteen seniors to appear in \u2756 Who\u27s who • February 20 set as deadline for May Day pageants • High school hears U.C. choral group • Dr. Miller\u27s class visits Bryn Mawr • Bloodmobile visits Ursinus Feb. 15 • Cupid hits U.C. over vacation • Editorial: How strong the foundation? • Sorority row • Fraternity row • Dillio gives some advice to the T-G. delinquents • The boy friend reveals realities of the roaring \u2720s • Schedule for final exams • Bears seek victory tonight after dropping four straight • Fords, Leopards drop grapplers; Garnet stopped by Bruins, 19-11 • Belles confident of another good year • Dave Burger receives All-American honors • Shreiner set to repeat as champshttps://digitalcommons.ursinus.edu/weekly/1441/thumbnail.jp

The masking-level difference in low-noise noise

In experiment 1 NoSo and NoS pi thresholds for a 500-Hz pure tone were obtained in a low-fluctuation masking noise and a high-fluctuation masking noise for six normal-hearing listeners. The noise bandwidth was 10 Hz. In agreement with previous investigations, the NoSo thresholds were lower in low-fluctuation noise than in high-fluctuation noise. For three listeners, NoS pi thresholds were similar for the two types of noise, while for the other three listeners, Nos pi thresholds were higher for low-fluctuation noise than for high-fluctuation noise. In experiment 2, the masker was created by amplitude modulating a 500-Hz pure tone by a 0-10-Hz low-pass noise. The degree of masker fluctuation was controlled by adjusting the average modulation depth (100%, 63%, 40%, and 25%). The signal was a 10-Hz-wide noise centered on 500 Hz. Results were similar to those of experiment 1: for the NoSo conditions, signal detection improved with decreasing degree of fluctuation, and for NoS pi conditions, the results were subject dependent. For three listeners, NoS pi thresholds were again similar in the two types of noise, while for the other three listeners, NoS pi thresholds were again higher in low-fluctuation noise than in high-fluctuation noise. The results showed that a high degree of masker fluctuation sometimes facilitates NoS pi detection. It is possible that the binaural detection mechanism utilizes the relatively good signal-to-noise ratios that occur in the low power or "dip" regions of fluctuating masker waveforms

Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction

With the unprecedented photometric precision of the Kepler Spacecraft, significant systematic and stochastic errors on transit signal levels are observable in the Kepler photometric data. These errors, which include discontinuities, outliers, systematic trends and other instrumental signatures, obscure astrophysical signals. The Presearch Data Conditioning (PDC) module of the Kepler data analysis pipeline tries to remove these errors while preserving planet transits and other astrophysically interesting signals. The completely new noise and stellar variability regime observed in Kepler data poses a significant problem to standard cotrending methods such as SYSREM and TFA. Variable stars are often of particular astrophysical interest so the preservation of their signals is of significant importance to the astrophysical community. We present a Bayesian Maximum A Posteriori (MAP) approach where a subset of highly correlated and quiet stars is used to generate a cotrending basis vector set which is in turn used to establish a range of "reasonable" robust fit parameters. These robust fit parameters are then used to generate a Bayesian Prior and a Bayesian Posterior Probability Distribution Function (PDF) which when maximized finds the best fit that simultaneously removes systematic effects while reducing the signal distortion and noise injection which commonly afflicts simple least-squares (LS) fitting. A numerical and empirical approach is taken where the Bayesian Prior PDFs are generated from fits to the light curve distributions themselves.Comment: 43 pages, 21 figures, Submitted for publication in PASP. Also see companion paper "Kepler Presearch Data Conditioning I - Architecture and Algorithms for Error Correction in Kepler Light Curves" by Martin C. Stumpe, et a

Geochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous Environments

Ongoing research on martian meteorites and a new set of observations of carbonate minerals provided by an unprecedented series of robotic missions to Mars in the past 15 years help define new constraints on the history of martian climate with important crosscutting themes including: the CO_2 budget of Mars, the role of Mg-, Fe-rich fluids on Mars, and the interplay between carbonate formation and acidity. Carbonate minerals have now been identified in a wide range of localities on Mars as well as in several martian meteorites. The martian meteorites contain carbonates in low abundances (<1 vol.%) and with a wide range of chemistries. Carbonates have also been identified by remote sensing instruments on orbiting spacecraft in several surface locations as well as in low concentrations (2–5 wt.%) in the martian dust. The Spirit rover also identified an outcrop with 16 to 34 wt.% carbonate material in the Columbia Hills of Gusev Crater that strongly resembled the composition of carbonate found in martian meteorite ALH 84001. Finally, the Phoenix lander identified concentrations of 3–6 wt.% carbonate in the soils of the northern plains. The carbonates discovered to date do not clearly indicate the past presence of a dense Noachian atmosphere, but instead suggest localized hydrothermal aqueous environments with limited water availability that existed primarily in the early to mid-Noachian followed by low levels of carbonate formation from thin films of transient water from the late Noachian to the present. The prevalence of carbonate along with evidence for active carbonate precipitation suggests that a global acidic chemistry is unlikely and a more complex relationship between acidity and carbonate formation is present