Age is Not Just a Number: Perceptions of Pedagogical Content Knowledge, Transformational Teaching, Student-Professor Engagement in Learning, and Deep Learning in the Graduate Classroom

Graduate students in higher education need pedagogical strategies that prepare them with knowledge and critical thinking for their careers. Research conducted in this area concluded that teaching students how to integrate knowledge into the real-world continues to be a challenge for educators across various disciplines in higher education. While scholars have studied effective teaching practices for decades, a broad definition has not been determined. Graduate students’ perceptions of professor pedagogical content knowledge, transformational teaching, student deep learning, and age were compared to determine the behaviors that influence deep learning in business and education programs in the United States and internationally. A survey was administered to 137 students. Findings show that non-traditional learners did not feel as strongly about individualized consideration as traditional learners. The findings suggest that graduate students perceive humor, learning struggles, and relatable content differently

The Role of Second-year College Students\u27 Mindset on Finances and its Impact on Welness

This study examined the differentiation among second-year college students from a small urban religious affiliated college in New York City and their four beliefs about household money on five constructs of wellness. Ninety-two participants completed the “TestWell: Wellness Inventory-College Edition” questionnaire. Discriminant analysis evaluated the differences among groups. It was found that students who believed they have plenty of money revealed higher scores for emotional awareness and physical fitness. Student services on college campuses may use this research to offer student financial planning to support and set short and long term budgeting goals that increase retention rates

Which Matters Most? Perceptions of Family Income or Parental Education on Academic Achievement

The purpose of this study was to examine the impact of college students’ perception of family income, parental education levels, and race on academic achievement. Ninety-four second-year college students from a small, liberal arts, college in New York City responded to the survey during the Fall of 2009. Of the respondents, 52 were female and 42 were male. The survey collected demographic data on student perception of family income, parental education levels, and race. Academic achievement was measured by gathering students’ grade point averages. Findings in the research demonstrated that the education-level of the students’ fathers had the greatest impact on academic achievement

Which Matters Most? Perceptions of Family Income or Parental Education on Academic Achievement

The purpose of this study was to examine the impact of college students’ perception of family income, parental education levels, and race on academic achievement. Ninety-four second-year college students from a small, liberal arts, college in New York City responded to the survey during the Fall of 2009. Of the respondents, 52 were female and 42 were male. The survey collected demographic data on student perception of family income, parental education levels, and race. Academic achievement was measured by gathering students’ grade point averages. Findings in the research demonstrated that the education-level of the students’ fathers had the greatest impact on academic achievement

Which Matters Most? Perceptions of Family Income or Parental Education on Academic Achievement

The purpose of this study was to examine the impact of college students’ perception of family income, parental education levels, and race on academic achievement. Ninety-four second-year college students from a small, liberal arts, college in New York City responded to the survey during the Fall of 2009. Of the respondents, 52 were female and 42 were male. The survey collected demographic data on student perception of family income, parental education levels, and race. Academic achievement was measured by gathering students’ grade point averages. Findings in the research demonstrated that the education-level of the students’ fathers had the greatest impact on academic achievement

Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)

This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Localization and broadband follow-up of the gravitational-wave transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams

Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams. </p