New Haven, CT, United States

Southern Connecticut State University
New Haven, CT, United States

Southern Connecticut State University is one of four state universities in Connecticut, and is located in the West Rock neighborhood of New Haven, Connecticut. Founded in 1893, it is the third-oldest campus in the Connecticut State University System.SCSU is part of the Connecticut State University System. Its sister schools are Central Connecticut State University, Eastern Connecticut State University, and Western Connecticut State University. The state universities are governed by the Connecticut Board of Regents for Higher Education. Wikipedia.

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News Article | April 17, 2017
Site:, a leading resource provider for higher education and career information, has released its list of Connecticut’s best colleges and universities for 2017. Of the 19 four-year schools that made the list, Yale University, Fairfield University, Quinnipiac University, University of Hartford and University of Connecticut scored highest. Of the 12 two-year schools that were also included, Capital Community College, Manchester Community College, Naugatuck Valley Community College, Three Rivers Community College and Gateway Community College were the top five schools. A full list of the 31 schools is included below. “As Connecticut’s job market fluctuates, many people consider earning a certificate or degree to help change or bolster their career,” said Wes Ricketts, senior vice president of “These Connecticut schools have proven themselves with solid educational programs, but have also taken extra steps to provide resources that translate into career success for students.” To be included on Connecticut’s “Best Colleges” list, schools must be regionally accredited, not-for-profit institutions. Each college is also scored on additional metrics such as employment resources, academic counseling, financial aid availability, annual alumni earnings 10 years after entering college, student/teacher ratios and graduation rates. Complete details on each college, their individual scores and the data and methodology used to determine the “Best Colleges in Connecticut” list, visit: The Best Four-Year Colleges in Connecticut for 2017 include: Albertus Magnus College Central Connecticut State University Connecticut College Eastern Connecticut State University Fairfield University Goodwin College Mitchell College Quinnipiac University Sacred Heart University Southern Connecticut State University Trinity College University of Bridgeport University of Connecticut University of Hartford University of New Haven University of Saint Joseph Wesleyan University Western Connecticut State University Yale University The Best Two-Year Colleges in Connecticut for 2017 include: Asnuntuck Community College Capital Community College Gateway Community College Housatonic Community College Manchester Community College Middlesex Community College Naugatuck Valley Community College Northwestern Connecticut Community College Norwalk Community College Quinebaug Valley Community College Three Rivers Community College Tunxis Community College ### About Us: was founded in 2013 to provide data and expert driven information about employment opportunities and the education needed to land the perfect career. Our materials cover a wide range of professions, industries and degree programs, and are designed for people who want to choose, change or advance their careers. We also provide helpful resources and guides that address social issues, financial aid and other special interest in higher education. Information from has proudly been featured by more than 700 educational institutions.

— Des Hague, along with The Stamford Youth Foundation (SYF), is celebrating a huge success at this year’s annual Odyssey of the Mind tournament, which took place at Southern Connecticut State University. Competing against more than 160 teams from throughout the state, SYF saw three of their ten teams advance to the World Finals, which will be held at Michigan State University in May. Odyssey of the Mind is a rigorous academic competition for students from kindergarten through college, held in every US state, with finalists competing nationally. Stamford Youth Foundation board member Des Hague, a prominent retail executive and motivational speaker, has congratulated the teams on their victory. Recently elevated to the board of the Stamford Youth Foundation (SYF), Hague has been running the Corporate Donations Fundraising since, applying his decades of experience in raising money for non-profits on a global scale to the local organization, which allowed them to send their teams to the prestigious tournament. “I couldn’t be more proud of SYF’s success in the Connecticut State Odyssey of the Mind competition,” said Des Hague. “It is a tribute to the hard work of both our students and our teacher coaches who share in the victory. I’m happy to be associated with a great organization like the Stamford Youth Foundation and look forward to the upcoming world finals.” Developed in 1978 to promote team problem solving skills, the Odyssey of the Mind competition includes students in all 50 states and a number of foreign countries, amongst them the United Kingdom, Japan, China, and Russia. Students are presented with five long-term problems to solve, each incorporating the use of critical thinking skills. Areas covered by the tournament include mechanics, literature, architecture, and much more, challenging the creativity of its young participants. Teams of five to seven members select from five given problems, work together for several months on a solution, and then deliver it as an eight-minute presentation at the state tournament. With the support of Mr. Hague’s corporate fundraising efforts, this year’s Stamford Youth Foundation saw two of their teams place first in their assigned problem and division. Both teams also received the special Jill Riggles Award for Excellence in having placed first in the spontaneous portion of the competition. Des Hague is an internationally renowned corporate executive and inspirational speaker who can tap into vast experience in the public and private sectors. Over the course of his career he repeatedly demonstrated an impressive level of excellence in leading companies onto a path of growth and success. Hague invests much of is time and energy in supporting worthy causes, as a private individual as well as throughout his professional life. In his position at CEO of Centerplate, the largest event hospitality company in North America, where he managed 43,000 from 2009 to 2014, he established a corporate fundraising program that collected more than $100 million in charitable donations that benefitted a large number of non-profit organizations, including the Stamford Youth Foundation. For more information, please visit

ARMONK, N.Y., July 20, 2017 /PRNewswire/ -- IBM (NYSE: IBM) announced today that Southern Connecticut State University (SCSU) has integrated IBM Watson Analytics to help create new services and programs based on data-driven insights to improve students' academic achievement and...

Crawford S.,Southern Connecticut State University
Therapeutic Advances in Medical Oncology | Year: 2014

The chronic, progressive clinical characteristics of many adult solid tumor malignancies suggest that a more effective therapeutic approach to cancer management may require long-term intervention using nontoxic systemic agents that block critical components of abnormal tumor physiology. Two highly promising systemic targets common to the development, progression and recurrence of many common cancers are dysregulated inflammatory and oxidation/reduction (redox) pathways. Compelling clinical data support the use of anti-inflammatory and antioxidant agents as a therapeutic modality for long-term use in patients diagnosed with several common cancers, including colon cancer and breast cancer. The therapeutic paradigm presented in this paper is the product of a synthesis of what is currently understood about the biological effects of inflammation and oxidative stress that contribute to tumorigenesis, disease progression and recurrence as well as results obtained from research on the use of prophylactics with anti-inflammatory or antioxidant properties in cancer prevention and treatment. © The Author(s), 2014.

Crawford S.,Southern Connecticut State University
Frontiers in Pharmacology | Year: 2013

U.S. SEER (Surveillance Epidemiology and End Results) data for age-adjusted mortality rates for all cancers combined for all races show only a modest overall 13% decline over the past 35 years. Moreover, the greatest contributor to cancer mortality is treatment-resistant metastatic disease. The accepted therapeutic paradigm for the past half-century for the treatment of advanced cancers has involved the use of systemic chemotherapy drugs cytotoxic for cycling cells (both normal and malignant) during DNA synthesis and/or mitosis. The failure of this therapeutic modality to achieve high-level, consistent rates of disease-free survival for some of the most common cancers, including tumors of the lung, colon breast, brain, melanoma, and others is the focus of this paper. A retrospective assessment of critical milestones in cancer chemotherapy indicates that most successful therapeutic regimens use cytotoxic cell cycle inhibitors in combined, maximum tolerated, dose-dense acute treatment regimens originally developed to treat acute lymphoblastic leukemia and some lymphomas. Early clinical successes in this area led to their wholesale application to the treatment of solid tumor malignancies that, unfortunately, has not produced consistent, long-term high cure rates for many common cancers. Important differences in therapeutic sensitivity of leukemias/lymphomas versus solid tumors can be explained by key biological differences that define the treatment-resistant solid tumor phenotype. A review of these clinical outcome data in the context of recent developments in our understanding of drug resistance mechanisms characteristic of solid tumors suggests the need for a new paradigm for the treatment of chemotherapy-resistant cancers. In contrast to reductionist approaches, the systemic approach targets both microenvironmental and systemic factors that drive and sustain tumor progression. These systemic factors include dysregulated inflammatory and oxidation pathways shown to be directly implicated in the development and maintenance of the cancer phenotype. The paradigm stresses the importance of a combined preventive/therapeutic approach involving adjuvant chemotherapies that incorporate anti-inflammatory and anti-oxidant therapeutics. © 2013 Crawford.

Disclosed are extracts prepared from primitive plants and fungi that have anti-cancer properties. The extracts are prepared by pulverizing the biological matter in a diluent. The extract can be administered to an individual or animal to kill cancer cells, prevent growth of cancer cells and teat cancer. The extracts may be used in combination with other therapeutic protocols.

Agency: NSF | Branch: Standard Grant | Program: | Phase: | Award Amount: 49.97K | Year: 2012

Loline alkaloids are made by the endophytic fungus Neotyphodium sp. as part of a symbiotic relationship to keep insect herbivores from consuming their tall fescue host. Previous research has indicated that some epiphytic bacterial colonizers of tall fescue can use these alkaloids as a sole carbon source. Such bacteria grow to higher population sizes on loline containing grasses than other bacterial strains. It is thought that a multi-trophic symbiosis is occurring on the grass phyllosphere between the loline catabolizing bacteria, the host, and the endophytic fungus. This project will test the potential positive impact of loline catabolizing bacterial epiphytes on growth of the host. The bacteria will be screened for production of the plant growth regulators, auxin and cytokinin, through growth assays, microscopy, and biochemistry. Additionally, the protective impacts of loline catabolizing bacteria on the host grasses will be investigated by screening them for the antimicrobial production. The ability of the bacteria to protect their hosts via niche exclusion will also be examined. A combination of culturing and biochemistry techniques will be conducted for these tests. Finally, the potential to take advantage of the affinity of loline catabolizing strains to Neotyphodium sp. harboring grasses for the bioremediation of the major pollutant Atrazine will be tested.

The data collected from this work will have broad implications on the current scientific knowledge concerning microbe:microbe interactions. Potentially, this work may result in an efficient way to remove atrazine from the environment, which would generate safer ground water for future generations.

Agency: NSF | Branch: Standard Grant | Program: | Phase: STELLAR ASTRONOMY & ASTROPHYSC | Award Amount: 160.59K | Year: 2016

This collaborative project will use imaging and spectrophotometry to study 2,000 of the nearest stars. The high spatial resolution images will be capable of revealing bound planets. The spectrophotometry will provide information about the systems? temperatures and orbital characteristics. The work will focus on a type of star called M-dwarfs, which are cooler and less massive than the Sun. These stars are also considered more likely to have rocky planets habitable to life than stars like the Sun. Observations will be made with two telescopes in Arizona and one in California. Scientific results will be incorporated into an outreach program with the Discovery Channel. Students from Northern Arizona University and Southern Connecticut State University will participate in the research.

The team will use the Differential Speckle Survey Instrument (DSSI) on Lowell Observatory 4.5m telescope and the R=600 visible-light multi-object spectrophotometer on Lowell?s 31-inch telescope. Through the comparison of speckle patterns simultaneously observed at two wavelengths, DSSI can measure separations of companions below the diffraction limit. Follow-up spectrophotometry will provide data for stellar characterization and spectral energy distribution fitting. The team will also use the Palomar 200-inch telescope to assess bound companions using data from an infrared camera or optical integral field spectrometer and isochrone modeling.

Agency: NSF | Branch: Standard Grant | Program: | Phase: MAJOR RESEARCH INSTRUMENTATION | Award Amount: 300.00K | Year: 2014

In the continual effort to obtain better images of objects in the universe, the emphasis has generally been centered on orbiting observatories or ever-larger ground-based facilities with laser correction of atmospheric turbulence. Both are expensive endeavors with physical limitations. A quite different approach, intensity interferometry, has a significant history in radio astronomy, but was last seriously used for the optical regime in the 1970s using the simple detectors available at the time. Dr. E. Horch of Southern Connecticut State University (SCSU) has recognized that todays very sensitive, extremely fast solid-state detectors motivates that the technique be re-examined, as it would offer the possibility of obtaining separations of orbiting binary stars, stellar diameters, and even complete stellar images using a small array of inexpensive, modest-sized telescopes and commercially available instrumentation. Indeed, the SCSU project is being promoted as an activity well-suited to student involvement at a small undergraduate university.

Intensity interferometry for astronomy utilizes the Bose-Einstein correlation of bosons (and therefore photons) to provide information on the angular size of the radiating source. For telescopes with somewhat less than 1-m aperture distributed over the SCSU campus, Dr. Horch predicts that an angular resolution of 0.1 milliarcseconds can be achieved down to a visual magnitude of ~3.5, allowing detailed inspection of about 200 stars. For comparison, the Sun moved to a distance that yields this apparent magnitude would have an angular diameter of 2 milliarcseconds. Moreover, the effect can be monitored in several wavebands simultaneously through the use of Single Photon Avalanche Diode (SPAD) arrays that have quantum efficiencies near 0.5 and time response of ~0.1 nanoseconds, and the data recorded using GPS technology.

Funding for the development of a modern two-telescope prototype of an intensity interferometer array for the optical is being provided by NSFs Division of Astronomical Sciences through its participation in the Major Research Instrumentation program.

Agency: NSF | Branch: Continuing grant | Program: | Phase: STELLAR ASTRONOMY & ASTROPHYSC | Award Amount: 220.35K | Year: 2015

This project will explore the environments of more than 2000 of the nearest star systems to the Sun. The objectives are to (a) discover how unusual our Sun is in its stellar solitude, (b) understand how many stars of different types are multiples, (c) provide fundamental statistics that will drive our knowledge of how stars form, and (d) provide a list of stars where analogues of our Solar System might be found. The project allows us to place our own Sun in context in our Galaxy, answering the broad question, How does our Sun compare to other stars? It will also provide important information about the likelihood of habitable worlds. The project provides opportunities for graduate and undergraduate student training at both institutions, each of which includes significant fractions of minority students. Both institutions will develop supplemental observing programs for students and general public using local facilities, and they will integrate these with their educational programs.

Two high-resolution imaging surveys will be completed using the Differential Speckle Survey Instrument (DSSI), a unique speckle imaging system that provides diffraction-limited imaging in two colors simultaneously. Observations will primarily be taken at Lowell Observatorys 4.3-meter Discovery Channel Telescope and at the Gemini North 8.1-meter Telescope. The first survey will target more than 1500 stars within 25 parsecs with V magnitudes brighter than 16. Observing nearby stars with DSSI will enable mapping of their stellar environments down to separations smaller than the distance of Mercury to the Sun, even at the horizon of the sample. The results will provide crucial insight into the star formation process, and the statistics of stellar multiplicity will be the benchmark for other types of multiplicity studies, with an emphasis on the Solar System scales crucial for planet formation. The second survey will target more than a thousand K-dwarfs within 50 parsecs in an equatorial sample that can be observed from both the northern and southern hemispheres. Incorporating other techniques together with DSSI images, these stars will be surveyed for companions down to Jovian masses to provide a unique data set of companions spanning a mass range of 1000 for this specific spectral type, providing a legacy data set that can be referenced for decades to come.

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