On the Accuracy of SonarQube Technical Debt Remediation Time - presentation slides

This document discusses supplier management in construction projects to prevent delays and non-compliance with contractual requirements. It notes that 45% of delays are due to management problems and costs of poor quality can reach 30% of sales price. The objectives are to analyze management of metalworking, electrical, and civil suppliers to prevent cost overruns from delays or non-compliance. Supplier management services seeks to minimize delays, failures to meet requirements or changes, and additional costs from claims. It provides supplier evaluation, quality assurance, and shop expediting to help meet delivery times and anticipate non-compliance consequences.

Supplier Management Service

Canberra Institute of technology

According to Juran, for the average American manufacturer, the costs of not quality in some cases come to represent 30% of the sales price. For the builder or client company, a non compliance of contract causes delays in the delivery date, affecting site operations, these delays can generate additional costs not covered: costs of Labor, equipment and penalties if it affect start up of the project. In Peru, in national projects, 75% of projects had delays of up to 60 days. In this situation, Supplier Management should be an alternative that allows early identification of a delay in delivery date, decline in the quality requirements, the possibility to capture information relevant to decision-making, in order to prevent and mitigate its effects on the project progress.

Practical assessment-Construct, assemble and install timber external stairs

This document provides instructions and assessment materials for students to construct a set of timber external stairs, including a balustrade and handrail. Students are required to calculate rise and goings of stairs, balustrade spacing, list required tools and materials, and construct the stairs to code and working drawings within 7 hours. The assessment will take place at the CIT Bruce workshop under teacher supervision and students may have up to two attempts. Upon completion, students must deconstruct the stairs and dispose of materials properly.

Blockchain: Background and Data61 Research Overview

Ingo Weber

Inforln.com ERP LN 10.3 & 10.4 Project Peg Audit History Differences

Dan Aldridge, ERP Software Evangelist, LION

Inforum 2014 Infor ERP differences training for Infor Ming.le, Infor Cloudsuites and Infor ERP LN. These presentations explain how to use new functionality enhancements in Infor LN 10.4 and other applications within the vertical industry Cloudsuites. There are Cloudsuites for Financials, Aerospace and Defense (A&D), Automotive, Industrial Machining and Equipment and other discrete manufacturing industries. If you still have Baan 4, FourthShift, Microsoft Dynamics GP, SAP R/3 or any other legacy ERP, then you might want to consider Infor LN. We specialize in Baan 4 to LN migrations but can handle upgrades from virtually any manufacturing ERP system to the new Infor CloudSuites. For more information and how-to content, visit http://inforln.com or contact Dan Aldridge, CEO of Performa Apps, at 703.251.4504.

Project to Product: Unlocking Product Agility

Cprime

Adherence to time, budget, and scope has been the gold standard measure of project success since the beginning of time. Many occasions, we are delighted if we can meet even two of those targets. Now, as the digital world shifts from thinking in fixed-time period projects to ongoing product efforts (with associated teams, markets, and horizons), adherence to time, budget, and scope has little to do with the actual success of an initiative. In this webinar, Anne Steiner, CEO at Cprime, will cover the challenges and advantages companies and teams unlock when they apply product thinking over project thinking. We’ll explore topics including: - Team formation - Budgeting and planning - Reducing cycle times in order to fuel continuous product learning. You’ll be challenged to think beyond traditional project management ways of work and to elevate the delivery of value as the gold standard for success.

3 Ways That Data Helps Reduce Review Cycles - Webinar, May 2016

Aconex

Metrics To Support An Agile Transformation

Hugo Messer

Real Estate Property Valuation Online Certificate Course | REMI

Real Estate Management Institute - REMI

Construction of 6 CPCL Oil storage tankers - A critical Project Management pe...

Shanmukha S. Potti

IRJET- Critical Chain Project Management in Construction Projects

IRJET Journal

This document discusses Critical Chain Project Management (CCPM) and its application to construction projects. CCPM differs from traditional project scheduling methods like Critical Path Method in that it aggregates uncertainty into buffers at the end of activity paths. This allows for more predictable project durations. The document reviews the literature on CCPM in construction, finding that projects using CCPM typically complete with 10-50% less time and cost compared to traditional methods. It then provides details on a sample villa construction project, outlining 15 activities, and discusses procedures for implementing CCPM, such as using average task durations and protecting critical resources and chains with buffers.

Mouyadin moumin abdillahi.pptx

Zakaria156221

This document summarizes the construction of a G+2 residential building project in Djibouti. It discusses the company undertaking the project, the traditional delivery method and fixed-price contract being used. It then outlines the project scheduling and management, including why scheduling is important, determining activity durations, and using activity references and crashing to optimize the schedule. Finally, it discusses safety and quality control measures, including reinforcement, formwork, elevation, and concrete controls.

Management Control System- Delhi Metro_10042016

Anil Kumar Gupta

The document provides details about the management control systems used for the Delhi Metro project. It summarizes the key reasons for project overruns and how the Delhi Metro project overcame these issues. Specifically, it discusses the MC1A contract between DMRC and KSHI-JV for the Vishwavidyalaya to Kashmere Gate underground corridor. It highlights the salient strategies used such as technology risk management, knowledge management, advance preparation, mobilization strategies, worker training, traffic management, environmental management, and quality and safety inspections that helped ensure the project was completed on time.

Jha Ajachi_NIT Jamshedpur_CV

Ajachi Jha

This document provides a summary of Jha Ajachi Radhakrishna Binod's professional experience and qualifications. It details his previous roles as a Construction Manager and Assistant Manager, outlining his responsibilities and achievements. These included commissioning projects, developing cost and quality strategies, and ensuring safety standards. It also lists his education qualifications including a B.Tech in Civil Engineering and academic projects involving concrete cracking and trenchless tunneling. His software skills and extracurricular activities developing an advanced robotic arm are highlighted.

Technical evaluation in cpv systems

Victor Martinez Camero

This document discusses technical evaluation in CPV (concentrated photovoltaic) systems. It outlines Mott MacDonald's role as an independent engineer in conducting technical due diligence and assessing the bankability of CPV technologies. The technical due diligence process for CPV systems must go beyond standard PV modules to also evaluate the quality control and integration of the entire CPV system, including optics, tracking systems, and performance over long periods of operation. Achieving a 'bankable' status for CPV remains challenging due to the lack of extensive operational data from different locations, but compliance with quality and performance standards as well as independent review and testing can help boost investor and lender confidence in CPV technologies.

Network Rail & Innovate UK: Scope of "SBRI Innovation in Automated Tunnel Exa...

KTN

Two new SBRIs have been announced to drive efficiency and safety in the rail industry. Network Rail will work with Innovate UK, part of UK Research and Innovation, to invest up to £3m to address two of the objectives identified in Network Rail’s CP6 funding strategy for research and development: - Automated tunnel examination - Security surveillance analytics for stations This briefing event is an opportunity for you to find out more about the two SBRI competitions and how to apply, and there will be ample time for networking. The webcast recording is now available: https://youtu.be/Uqq452lk90c Find out more about the Transport Interest Group at https://ktn-uk.co.uk/interests/transport Join the KTN Transport group on LinkedIn at https://www.linkedin.com/groups/4148691/

Project management - not just for work - 23rd April 2015

Association for Project Management

This document discusses how project management skills can be used outside of work through volunteering on community projects. It details Barnaby Beere's involvement with the Wotton Community Sports Foundation, including developing sports facilities through "hard" construction projects and taking over management of a local sports center through a "soft" organizational change project. It highlights lessons learned around fundraising, stakeholder engagement, procurement, and managing challenges that arise during periods of change.

Clinical periodontology and implant dentistry 2003.pdf

RAYMUNDONAVARROCORON

Describing and Interpreting an Immersive Learning Case with the Immersion Cub...

Current descriptions of immersive learning cases are often difficult or impossible to compare. This is due to a myriad of different options on what details to include, which aspects are relevant, and on the descriptive approaches employed. Also, these aspects often combine very specific details with more general guidelines or indicate intents and rationales without clarifying their implementation. In this paper we provide a method to describe immersive learning cases that is structured to enable comparisons, yet flexible enough to allow researchers and practitioners to decide which aspects to include. This method leverages a taxonomy that classifies educational aspects at three levels (uses, practices, and strategies) and then utilizes two frameworks, the Immersive Learning Brain and the Immersion Cube, to enable a structured description and interpretation of immersive learning cases. The method is then demonstrated on a published immersive learning case on training for wind turbine maintenance using virtual reality. Applying the method results in a structured artifact, the Immersive Learning Case Sheet, that tags the case with its proximal uses, practices, and strategies, and refines the free text case description to ensure that matching details are included. This contribution is thus a case description method in support of future comparative research of immersive learning cases. We then discuss how the resulting description and interpretation can be leveraged to change immersion learning cases, by enriching them (considering low-effort changes or additions) or innovating (exploring more challenging avenues of transformation). The method holds significant promise to support better-grounded research in immersive learning.

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Clinical periodontology and implant dentistry 2003.pdf

RAYMUNDONAVARROCORON

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Immersive Learning That Works: Research Grounding and Paths Forward

International Food Policy Research Institute- South Asia Office

We will metaverse into the essence of immersive learning, into its three dimensions and conceptual models. This approach encompasses elements from teaching methodologies to social involvement, through organizational concerns and technologies. Challenging the perception of learning as knowledge transfer, we introduce a 'Uses, Practices & Strategies' model operationalized by the 'Immersive Learning Brain' and ‘Immersion Cube’ frameworks. This approach offers a comprehensive guide through the intricacies of immersive educational experiences and spotlighting research frontiers, along the immersion dimensions of system, narrative, and agency. Our discourse extends to stakeholders beyond the academic sphere, addressing the interests of technologists, instructional designers, and policymakers. We span various contexts, from formal education to organizational transformation to the new horizon of an AI-pervasive society. This keynote aims to unite the iLRN community in a collaborative journey towards a future where immersive learning research and practice coalesce, paving the way for innovative educational research and practice landscapes.

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vadgavevedant86

SDSS1335+0728: The awakening of a ∼ 106M⊙ black hole⋆

Context. The early-type galaxy SDSS J133519.91+072807.4 (hereafter SDSS1335+0728), which had exhibited no prior optical variations during the preceding two decades, began showing significant nuclear variability in the Zwicky Transient Facility (ZTF) alert stream from December 2019 (as ZTF19acnskyy). This variability behaviour, coupled with the host-galaxy properties, suggests that SDSS1335+0728 hosts a ∼ 106M⊙ black hole (BH) that is currently in the process of ‘turning on’. Aims. We present a multi-wavelength photometric analysis and spectroscopic follow-up performed with the aim of better understanding the origin of the nuclear variations detected in SDSS1335+0728. Methods. We used archival photometry (from WISE, 2MASS, SDSS, GALEX, eROSITA) and spectroscopic data (from SDSS and LAMOST) to study the state of SDSS1335+0728 prior to December 2019, and new observations from Swift, SOAR/Goodman, VLT/X-shooter, and Keck/LRIS taken after its turn-on to characterise its current state. We analysed the variability of SDSS1335+0728 in the X-ray/UV/optical/mid-infrared range, modelled its spectral energy distribution prior to and after December 2019, and studied the evolution of its UV/optical spectra. Results. From our multi-wavelength photometric analysis, we find that: (a) since 2021, the UV flux (from Swift/UVOT observations) is four times brighter than the flux reported by GALEX in 2004; (b) since June 2022, the mid-infrared flux has risen more than two times, and the W1−W2 WISE colour has become redder; and (c) since February 2024, the source has begun showing X-ray emission. From our spectroscopic follow-up, we see that (i) the narrow emission line ratios are now consistent with a more energetic ionising continuum; (ii) broad emission lines are not detected; and (iii) the [OIII] line increased its flux ∼ 3.6 years after the first ZTF alert, which implies a relatively compact narrow-line-emitting region. Conclusions. We conclude that the variations observed in SDSS1335+0728 could be either explained by a ∼ 106M⊙ AGN that is just turning on or by an exotic tidal disruption event (TDE). If the former is true, SDSS1335+0728 is one of the strongest cases of an AGNobserved in the process of activating. If the latter were found to be the case, it would correspond to the longest and faintest TDE ever observed (or another class of still unknown nuclear transient). Future observations of SDSS1335+0728 are crucial to further understand its behaviour. Key words. galaxies: active– accretion, accretion discs– galaxies: individual: SDSS J133519.91+072807.4

The binding of cosmological structures by massless topological defects

Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is mitigated, at least in part.

Candidate young stellar objects in the S-cluster: Kinematic analysis of a sub...

Context. The observation of several L-band emission sources in the S cluster has led to a rich discussion of their nature. However, a definitive answer to the classification of the dusty objects requires an explanation for the detection of compact Doppler-shifted Brγ emission. The ionized hydrogen in combination with the observation of mid-infrared L-band continuum emission suggests that most of these sources are embedded in a dusty envelope. These embedded sources are part of the S-cluster, and their relationship to the S-stars is still under debate. To date, the question of the origin of these two populations has been vague, although all explanations favor migration processes for the individual cluster members. Aims. This work revisits the S-cluster and its dusty members orbiting the supermassive black hole SgrA* on bound Keplerian orbits from a kinematic perspective. The aim is to explore the Keplerian parameters for patterns that might imply a nonrandom distribution of the sample. Additionally, various analytical aspects are considered to address the nature of the dusty sources. Methods. Based on the photometric analysis, we estimated the individual H−K and K−L colors for the source sample and compared the results to known cluster members. The classification revealed a noticeable contrast between the S-stars and the dusty sources. To fit the flux-density distribution, we utilized the radiative transfer code HYPERION and implemented a young stellar object Class I model. We obtained the position angle from the Keplerian fit results; additionally, we analyzed the distribution of the inclinations and the longitudes of the ascending node. Results. The colors of the dusty sources suggest a stellar nature consistent with the spectral energy distribution in the near and midinfrared domains. Furthermore, the evaporation timescales of dusty and gaseous clumps in the vicinity of SgrA* are much shorter ( 2yr) than the epochs covered by the observations (≈15yr). In addition to the strong evidence for the stellar classification of the D-sources, we also find a clear disk-like pattern following the arrangements of S-stars proposed in the literature. Furthermore, we find a global intrinsic inclination for all dusty sources of 60 ± 20◦, implying a common formation process. Conclusions. The pattern of the dusty sources manifested in the distribution of the position angles, inclinations, and longitudes of the ascending node strongly suggests two different scenarios: the main-sequence stars and the dusty stellar S-cluster sources share a common formation history or migrated with a similar formation channel in the vicinity of SgrA*. Alternatively, the gravitational influence of SgrA* in combination with a massive perturber, such as a putative intermediate mass black hole in the IRS 13 cluster, forces the dusty objects and S-stars to follow a particular orbital arrangement. Key words. stars: black holes– stars: formation– Galaxy: center– galaxies: star formation

Compexometric titration/Chelatorphy titration/chelating titration

Vandana Devesh Sharma

Classification Metal ion ion indicators Masking and demasking reagents Estimation of Magnisium sulphate Calcium gluconate Complexometric Titration/ chelatometry titration/chelating titration, introduction, Types- 1.Direct Titration 2.Back Titration 3.Replacement Titration 4.Indirect Titration Masking agent, Demasking agents formation of complex comparition between masking and demasking agents, Indicators/Metal ion indicators/ Metallochromic indicators/pM indicators, Visual Technique,PM indicators (metallochromic), Indicators of pH, Redox Indicators Instrumental Techniques-Photometry Potentiometry Miscellaneous methods. Complex titration with EDTA.

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Travis Hills MN

Authoring a personal GPT for your research and practice: How we created the Q...

Thematic analysis in qualitative research is a time-consuming and systematic task, typically done using teams. Team members must ground their activities on common understandings of the major concepts underlying the thematic analysis, and define criteria for its development. However, conceptual misunderstandings, equivocations, and lack of adherence to criteria are challenges to the quality and speed of this process. Given the distributed and uncertain nature of this process, we wondered if the tasks in thematic analysis could be supported by readily available artificial intelligence chatbots. Our early efforts point to potential benefits: not just saving time in the coding process but better adherence to criteria and grounding, by increasing triangulation between humans and artificial intelligence. This tutorial will provide a description and demonstration of the process we followed, as two academic researchers, to develop a custom ChatGPT to assist with qualitative coding in the thematic data analysis process of immersive learning accounts in a survey of the academic literature: QUAL-E Immersive Learning Thematic Analysis Helper. In the hands-on time, participants will try out QUAL-E and develop their ideas for their own qualitative coding ChatGPT. Participants that have the paid ChatGPT Plus subscription can create a draft of their assistants. The organizers will provide course materials and slide deck that participants will be able to utilize to continue development of their custom GPT. The paid subscription to ChatGPT Plus is not required to participate in this workshop, just for trying out personal GPTs during it.

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sammy700571

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The cost of acquiring information by natural selection

Carl Bergstrom

This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome. It's based on the first part of this research paper: The cost of information acquisition by natural selection Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577

AJAY KUMAR NIET GreNo Guava Project File.pdf

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Methods of grain storage Structures in India.pdf

PirithiRaju

•Post-harvestlossesaccountforabout10%oftotalfoodgrainsduetounscientificstorage,insects,rodents,micro-organismsetc., •Totalfoodgrainproductioninindiais311milliontonnesandstorageis145mt.InIndia,annualstoragelosseshavebeenestimated14mtworthofRs.7,000croreinwhichinsectsaloneaccountfornearlyRs.1,300crores. •InIndiaoutofthetotalproduction,about30%ismarketablesurplus •Remaining70%isretainedandstoredbyfarmersforconsumption,seed,feed.Hence,growerneedstoragefacilitytoholdaportionofproducetosellwhenthemarketingpriceisfavourable •TradersandCo-operativesatmarketcentresneedstoragestructurestoholdgrainswhenthetransportfacilityisinadequate

Anti-Universe And Emergent Gravity and the Dark Universe

Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.

Discovery of An Apparent Red, High-Velocity Type Ia Supernova at 𝐳 = 2.9 wi...