Project Learn: The Development and Assessment of a Cross-Platform Tutor Finder

creation of an online tutor finder application, called "Project Learn", aimed to address the difficulty in finding a tutor for any subject in today's fast-paced world. To achieve this, the study utilized a developmental research design to create an application that connects students with qualified tutors. Students can view a tutor's background and the subjects they teach before choosing the best fit for their needs. To evaluate the system's technical quality, a survey was conducted with 20 end-users and 10 IT-experts. The survey was based on ISO 25010 software quality standards and included components such as functional suitability, reliability, usability, performance efficiency, security, compatibility, portability, and maintainability. The survey results indicated that both the end-users and IT-experts rated the system above 3.26, which equates to a "very acceptable" grade. This suggests that the system's overall internal and external performance exhibited consistency and met the compliance requirements. However, there is still room for improvement to better serve the needs of its users. The success of the development and assessment of the online tutor finder application demonstrates the potential impact it can have in connecting students with qualified tutors. The study's use of a developmental research design and adherence to ISO 25010 software quality standards ensured the technical quality of the system. With further improvements, the application can continue to make a significant impact in helping students find the right tutor to achieve academic success

HALF OF THE MOST LUMINOUS QUASARS MAY BE OBSCURED: INVESTIGATING THE NATURE OF WISE-SELECTED HOT DUST-OBSCURED GALAXIES

The Wide-field Infrared Survey Explorer mission has unveiled a rare population of high-redshift (z = 1–4.6), dusty, hyper-luminous galaxies, with infrared luminosities L[subscript IR] > 10[superscript 13] L[subscript ⊙], and sometimes exceeding 10[superscript 14] L[subscript ⊙]. Previous work has shown that their dust temperatures and overall far-infrared spectral energy distributions (SEDs) are significantly hotter than expected to be powered by star formation. We present here an analysis of the rest-frame optical through mid-infrared SEDs for a large sample of these so-called "hot, dust-obscured galaxies" (Hot DOGs). We find that the SEDs of Hot DOGs are generally well modeled by the combination of a luminous, yet obscured active galactic nuclei (AGNs) that dominates the rest-frame emission at λ > 1 µm and the bolometric luminosity output, and a less luminous host galaxy that is responsible for the bulk of the rest optical/UV emission. Even though the stellar mass of the host galaxies may be as large as 10[superscript 11]–10[superscript 12] M[subscript ⊙], the AGN emission, with a range of luminosities comparable to those of the most luminous QSOs known, require that either Hot DOGs have black hole masses significantly in excess of the local relations, or that they radiate significantly above the Eddington limit, at a level at least 10 times more efficiently than z ~ 2 QSOs. We show that, while rare, the number density of Hot DOGs is comparable to that of equally luminous but unobscured (i.e., Type 1) QSOs. This may be at odds with the trend suggested at lower luminosities for the fraction of obscured AGNs to decrease with increasing luminosity. That trend may, instead, reverse at higher luminosities. Alternatively, Hot DOGs may not be the torus-obscured counterparts of the known optically selected, largely unobscured, hyper-luminous QSOs, and may represent a new component of the galaxy evolution paradigm. Finally, we discuss the environments of Hot DOGs and statistically show that these objects are in regions as dense as those of known high-redshift proto-clusters