Anderson University

Anderson, IN, United States

Anderson University

Anderson, IN, United States
SEARCH FILTERS
Time filter
Source Type

News Article | April 17, 2017
Site: www.prweb.com

LearnHowToBecome.org, a leading resource provider for higher education and career information, has released its list of Indiana’s best colleges for 2017. Of the 46 schools honored, 44 four-year schools made the list with University of Notre Dame, Purdue University, DePauw University, Valparaiso University and Butler University taking the top five spots. Ivy Tech Community College and Ancilla College were also included as the best two-year schools in the state. A list of all schools is included below. “Education can make a huge difference when it comes to the job market,” said Wes Ricketts, senior vice president of LearnHowToBecome.Org. “These schools in Indiana have not only shown a commitment to providing quality degree programs, but also the employment services that contribute to student success as they pursue careers.” To be included on the “Best Colleges in Indiana” list, schools must be regionally accredited, not-for-profit institutions. Each college is also scored on additional data that includes annual alumni earnings 10 years after entering college, employment and academic services offered, student/teacher ratio, graduation rate and the availability of financial aid. Complete details on each college, their individual scores and the data and methodology used to determine the LearnHowToBecome.org “Best Colleges in Indiana” list, visit: Indiana’s Best Colleges for 2017 include: Ancilla College Anderson University Ball State University Bethel College-Indiana Butler University Calumet College of Saint Joseph DePauw University Earlham College Franklin College Goshen College Grace College and Theological Seminary Hanover College Huntington University Indiana Institute of Technology Indiana State University Indiana University-Bloomington Indiana University-East Indiana University-Kokomo Indiana University-Northwest Indiana University-Purdue University-Fort Wayne Indiana University-Purdue University-Indianapolis Indiana University-South Bend Indiana University-Southeast Indiana Wesleyan University Ivy Tech Community College Manchester University Marian University Martin University Oakland City University Purdue University-Calumet Campus Purdue University-Main Campus Purdue University-North Central Campus Rose-Hulman Institute of Technology Saint Joseph’s College Saint Mary-of-the-Woods College Saint Mary's College Taylor University Trine University Trine University-Regional/Non-Traditional Campuses University of Evansville University of Indianapolis University of Notre Dame University of Saint Francis-Fort Wayne University of Southern Indiana Valparaiso University Wabash College About Us: LearnHowtoBecome.org 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 LearnHowtoBecome.org has proudly been featured by more than 700 educational institutions.


-- Shermco Industries, one of North America's largest independent electrical testing, maintenance and engineering services companies, has announced that Don Gibson has been engaged as the director of sales for Shermco's services and products for the renewable energy market. Gibson comes from a major wind energy utility where he was the business development manager after serving as a regional site operations manager overseeing five windfarms. He brings that depth of experience to help grow Shermco's specialty services into the wind energy market. Gibson also previously served as the operations planning manager for a major wind turbine manufacturer.Gibson has a bachelor of arts in communication from Grace College, Winona Lake, Indiana and a MBA from Anderson University. He will be based out of Indianapolis and will help focus Shermco's sales efforts in the Midwest as well as their more established service locations in the Southwest."We have known Don for many years as a wind industry leader and we are very pleased to have him join Shermco and lead our expanded sales efforts into the industry," said Paul Idziak, vice- president of Shermco's Machine Services Division."I am looking forward to supporting Don as we expand our wind energy field services and generator remanufacturing capabilities into new geographic areas," said Steve Camber, senior vice-president of sales.###ABOUT SHERMCOShermco Industries is the leading independent provider of safe and reliable acceptance testing, commissioning, maintenance, repair and remanufacturing of electrical equipment and power distribution systems. With service centers located throughout North America, certified technicians and engineers focus on servicing both scheduled and unexpected projects for large commercial, industrial and utility customers. Shermco, a leader in electrical safety and technical training, focuses on industrial electrical contracting, utility, wind turbine maintenance and disaster recovery services. Shermco Industries is a member in good standing with the Electrical Apparatus Service Association, American Wind Energy Association, Professional Electrical Apparatus Recyclers League, and the InterNational Electrical Testing Association. For more information about Shermco Industries, visit http://www.shermco.com


Aliu E.,Barnard College | Aliu E.,University of Barcelona | Archambault S.,McGill University | Archer A.,Washington University in St. Louis | And 84 more authors.
Astrophysical Journal | Year: 2015

We present the results of 71.6 hr of observations of the Geminga pulsar (PSR J0633+1746) with the VERITAS very-high-energy gamma-ray telescope array. Data taken with VERITAS between 2007 November and 2013 February were phase-folded using a Geminga pulsar timing solution derived from data recorded by the XMM-Newton and Fermi-LAT space telescopes. No significant pulsed emission above 100 GeV is observed, and we report upper limits at the 95% confidence level on the integral flux above 135 GeV (spectral analysis threshold) of 4.0 × 10-13 s-1 cm-2 and 1.7 × 10-13 s-1 cm-2 for the two principal peaks in the emission profile. These upper limits, placed in context with phase-resolved spectral energy distributions determined from 5 yr of data from the Fermi-Large Area Telescope (LAT), constrain possible hardening of the Geminga pulsar emission spectra above ∼50 GeV. © 2015. The American Astronomical Society. All rights reserved.


Aliu E.,Barnard College | Archer A.,Washington University in St. Louis | Aune T.,University of California at Los Angeles | Barnacka A.,Harvard - Smithsonian Center for Astrophysics | And 90 more authors.
Astrophysical Journal | Year: 2015

We present results from VERITAS observations of the BL Lac object PG 1553+113 spanning the years 2010, 2011, and 2012. The time-averaged spectrum, measured between 160 and 560 GeV, is well described by a power law with a spectral index of 4.33 ± 0.09. The time-averaged integral flux above 200 GeV measured for this period was (1.69 ± 0.06) × 10-11 photons cm-2 s-1, corresponding to 6.9% of the Crab Nebula flux. We also present the combined γ-ray spectrum from the Fermi Large Area Telescope and VERITAS covering an energy range from 100 MeV to 560 GeV. The data are well fit by a power law with an exponential cutoff at 101.9 ± 3.2 GeV. The origin of the cutoff could be intrinsic to PG 1553+113 or be due to the γ-ray opacity of our universe through pair production off the extragalactic background light (EBL). Given lower limits to the redshift of z > 0.395 based on optical/UV observations of PG 1553+113, the cutoff would be dominated by EBL absorption. Conversely, the small statistical uncertainties of the VERITAS energy spectrum have allowed us to provide a robust upper limit on the redshift of PG 1553+113 of z ≤ 0.62. A strongly elevated mean flux of (2.50 ± 0.14) × 10-11 photons cm-2 s-1 (10.3% of the Crab Nebula flux) was observed during 2012, with the daily flux reaching as high as (18.3% of the Crab Nebula flux) on MJD 56048. The light curve measured during the 2012 observing season is marginally inconsistent with a steady flux, giving a χ2 probability for a steady flux of 0.03%. © 2015. The American Astronomical Society. All rights reserved.


Aliu E.,Barnard College | Aune T.,University of California at Los Angeles | Barnacka A.,Harvard - Smithsonian Center for Astrophysics | Beilicke M.,Washington University in St. Louis | And 95 more authors.
Astrophysical Journal Letters | Year: 2014

Prompt emission from the very fluent and nearby (z = 0.34) gamma-ray burst GRB130427A was detected by several orbiting telescopes and by ground-based, wide-field-of-view optical transient monitors. Apart from the intensity and proximity of this GRB, it is exceptional due to the extremely long-lived high-energy (100 MeV to 100 GeV) gamma-ray emission, which was detected by the Large Area Telescope on the Fermi Gamma-Ray Space Telescope for ∼70 ks after the initial burst. The persistent, hard-spectrum, high-energy emission suggests that the highest-energy gamma rays may have been produced via synchrotron self-Compton processes though there is also evidence that the high-energy emission may instead be an extension of the synchrotron spectrum. VERITAS, a ground-based imaging atmospheric Cherenkov telescope array, began follow-up observations of GRB130427A ∼71 ks (∼20 hr) after the onset of the burst. The GRB was not detected with VERITAS; however, the high elevation of the observations, coupled with the lowredshift of theGRB, make VERITAS a very sensitive probe of the emission from GRB130427A for E > 100 GeV. The non-detection and consequent upper limit derived place constraints on the synchrotron self-Compton model of high-energy gamma-ray emission from this burst. © 2014. The American Astronomical Society. All rights reserved.


Aliu E.,Barnard College | Archambault S.,McGill University | Arlen T.,University of California at Los Angeles | Aune T.,University of California at Los Angeles | And 99 more authors.
Astrophysical Journal | Year: 2014

We summarize broadband observations of the TeV-emitting blazar 1ES 1959+650, including optical R-band observations by the robotic telescopes Super-LOTIS and iTelescope, UV observations by Swift Ultraviolet and Optical Telescope, X-ray observations by the Swift X-ray Telescope, high-energy gamma-ray observations with the Fermi Large Area Telescope, and very-high-energy (VHE) gamma-ray observations by VERITAS above 315 GeV, all taken between 2012 April 17 and 2012 June 1 (MJD 56034 and 56079). The contemporaneous variability of the broadband spectral energy distribution is explored in the context of a simple synchrotron self Compton (SSC) model. In the SSC emission scenario, we find that the parameters required to represent the high state are significantly different than those in the low state. Motivated by possible evidence of gas in the vicinity of the blazar, we also investigate a reflected emission model to describe the observed variability pattern. This model assumes that the non-thermal emission from the jet is reflected by a nearby cloud of gas, allowing the reflected emission to re-enter the blob and produce an elevated gamma-ray state with no simultaneous elevated synchrotron flux. The model applied here, although not required to explain the observed variability pattern, represents one possible scenario which can describe the observations. As applied to an elevated VHE state of 66% of the Crab Nebula flux, observed on a single night during the observation period, the reflected emission scenario does not support a purely leptonic non-thermal emission mechanism. The reflected emission model does, however, predict a reflected photon field with sufficient energy to enable elevated gamma-ray emission via pion production with protons of energies between 10 and 100 TeV. © 2014. The American Astronomical Society. All rights reserved.


Archer A.,Washington University in St. Louis | Benbow W.,Harvard - Smithsonian Center for Astrophysics | Bird R.,University College Dublin | Buchovecky M.,University of California at Los Angeles | And 76 more authors.
Astrophysical Journal | Year: 2016

The Galactic Center ridge has been observed extensively in the past by both GeV and TeV gamma-ray instruments revealing a wealth of structure, including a diffuse component and the point sources G0.9+0.1 (a composite supernova remnant) and Sgr A∗ (believed to be associated with the supermassive black hole located at the center of our Galaxy). Previous very high energy (VHE) gamma-ray observations with the H.E.S.S. experiment have also detected an extended TeV gamma-ray component along the Galactic plane in the >300 GeV gamma-ray regime. Here we report on observations of the Galactic Center ridge from 2010 to 2014 by the VERITAS telescope array in the >2 TeV energy range. From these observations we (1) provide improved measurements of the differential energy spectrum for Sgr A∗ in the >2 TeV gamma-ray regime, (2) provide a detection in the >2 TeV gamma-ray emission from the composite SNR G0.9+0.1 and an improved determination of its multi-TeV gamma-ray energy spectrum, and (3) report on the detection of VER J1746-289, a localized enhancement of >2 TeV gamma-ray emission along the Galactic plane. © 2016. The American Astronomical Society. All rights reserved..


Aliu E.,Barnard College | Archambault S.,McGill University | Arlen T.,University of California at Los Angeles | Aune T.,University of California at Los Angeles | And 100 more authors.
Astrophysical Journal | Year: 2014

We summarize broadband observations of the TeV-emitting blazar 1ES 1959+650, including optical R-band observations by the robotic telescopes Super-LOTIS and iTelescope, UV observations by Swift Ultraviolet and Optical Telescope, X-ray observations by the Swift X-ray Telescope, high-energy gamma-ray observations with the Fermi Large Area Telescope, and very-high-energy (VHE) gamma-ray observations by VERITAS above 315 GeV, all taken between 2012 April 17 and 2012 June 1 (MJD 56034 and 56079). The contemporaneous variability of the broadband spectral energy distribution is explored in the context of a simple synchrotron self Compton (SSC) model. In the SSC emission scenario, we find that the parameters required to represent the high state are significantly different than those in the low state. Motivated by possible evidence of gas in the vicinity of the blazar, we also investigate a reflected emission model to describe the observed variability pattern. This model assumes that the non-thermal emission from the jet is reflected by a nearby cloud of gas, allowing the reflected emission to re-enter the blob and produce an elevated gamma-ray state with no simultaneous elevated synchrotron flux. The model applied here, although not required to explain the observed variability pattern, represents one possible scenario which can describe the observations. As applied to an elevated VHE state of 66% of the Crab Nebula flux, observed on a single night during the observation period, the reflected emission scenario does not support a purely leptonic non-thermal emission mechanism. The reflected emission model does, however, predict a reflected photon field with sufficient energy to enable elevated gamma-ray emission via pion production with protons of energies between 10 and 100 TeV. © 2014. The American Astronomical Society. All rights reserved.


Archambault S.,McGill University | Archer A.,Washington University in St. Louis | Aune T.,University of California at Los Angeles | Barnacka A.,Harvard - Smithsonian Center for Astrophysics | And 88 more authors.
Astrophysical Journal Letters | Year: 2016

The TeV binary system LS I +61 303 is known for its regular, non-thermal emission pattern that traces the orbital period of the compact object in its 26.5 day orbit around its B0 Ve star companion. The system typically presents elevated TeV emission around apastron passage with flux levels between 5% and 15% of the steady flux from the Crab Nebula (>300 GeV). In this article, VERITAS observations of LS I +61 303 taken in late 2014 are presented, during which bright TeV flares around apastron at flux levels peaking above 30% of the Crab Nebula flux were detected. This is the brightest such activity from this source ever seen in the TeV regime. The strong outbursts have rise and fall times of less than a day. The short timescale of the flares, in conjunction with the observation of 10 TeV photons from LS I +61 303 during the flares, provides constraints on the properties of the accelerator in the source. © 2016. The American Astronomical Society. All rights reserved..


News Article | February 27, 2017
Site: www.prweb.com

The Community for Accredited Online Schools, a leading resource provider for higher education information, has released its list of Indiana’s Best Online Schools for 2017. Of the 31 four-year schools ranked, Purdue University, Indiana University, Ball State University, Valparaiso University and Indiana University Purdue University Indianapolis came in as the top five. Two of Indiana’s two-year universities, Ancilla College and Ivy Tech Community College, were also honored. “As online educational technology improves, students in Indiana are becoming more inclined to earn degrees outside of a traditional classroom,” said Doug Jones, CEO and founder of AccreditedSchoolsOnline.org. “The schools on our list exemplify the best aspects of an online education: high quality curriculum, strong graduation rates and post-college career resources.” To earn a spot on the Best Online Schools list, Iowa colleges and universities must be institutionally accredited, public or private not-for-profit schools. Each college is also ranked on more than a dozen unique data points that include student resources, total online program offerings and financial aid availability. For more details on where each school falls in the rankings and the data and methodology used to determine the lists, visit: The Best Online Four-Year Schools in Indiana for 2017 include the following: Anderson University Ball State University Bethel College-Indiana Calumet College of Saint Joseph Grace College and Theological Seminary Huntington University Indiana Institute of Technology Indiana State University Indiana University Indiana University-East Indiana University-Kokomo Indiana University-Northwest Indiana University-Purdue University-Fort Wayne Indiana University-Purdue University-Indianapolis Indiana University-South Bend Indiana University-Southeast Indiana Wesleyan University Manchester University Marian University Oakland City University Ottawa University-Jeffersonville Purdue University Northwest Purdue University-Main Campus Saint Mary-of-the-Woods College Taylor University Trine University-Regional/Non-Traditional Campuses University of Indianapolis University of Saint Francis-Fort Wayne University of Southern Indiana Valparaiso University Vincennes University ### About Us: AccreditedSchoolsOnline.org was founded in 2011 to provide students and parents with quality data and information about pursuing an affordable, quality education that has been certified by an accrediting agency. Our community resource materials and tools span topics such as college accreditation, financial aid, opportunities available to veterans, people with disabilities, as well as online learning resources. We feature higher education institutions that have developed online learning programs that include highly trained faculty, new technology and resources, and online support services to help students achieve educational success.

Loading Anderson University collaborators
Loading Anderson University collaborators