Topic: Coefficient of Variance
Student Name: Shakeela
Class: B.Ed. 2.5
Project Name: “Young Teachers' Professional Development (TPD)"
"Project Founder: Prof. Dr. Amjad Ali Arain
Faculty of Education, University of Sindh, Pakistan
Topic: Population And Sample
Student Name: Sidera Saleem
Class: B.Ed. 2.5
Project Name: “Young Teachers' Professional Development (TPD)"
"Project Founder: Prof. Dr. Amjad Ali Arain
Faculty of Education, University of Sindh, Pakistan
In this presentation, we will analyze multicollinearity and inference with interaction terms in regression analysis. We will also analyze partial correlation and interpretation procedures of statistical data.
Topic: Coefficient of Variance
Student Name: Shakeela
Class: B.Ed. 2.5
Project Name: “Young Teachers' Professional Development (TPD)"
"Project Founder: Prof. Dr. Amjad Ali Arain
Faculty of Education, University of Sindh, Pakistan
Topic: Population And Sample
Student Name: Sidera Saleem
Class: B.Ed. 2.5
Project Name: “Young Teachers' Professional Development (TPD)"
"Project Founder: Prof. Dr. Amjad Ali Arain
Faculty of Education, University of Sindh, Pakistan
In this presentation, we will analyze multicollinearity and inference with interaction terms in regression analysis. We will also analyze partial correlation and interpretation procedures of statistical data.
2.0.statistical methods and determination of sample sizesalummkata1
statistical methods and determination of sample size
These guidelines focus on the validation of the bioanalytical methods generating quantitative concentration data used for pharmacokinetic and toxicokinetic parameter determinations.
After covering classical ANOVA procedures for data from manipulative experiments, this lecture emphasizes the use of linear models for data from observational studies.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
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Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Richard's entangled aventures in wonderlandRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
3. Assumptions of ANOVA
A common misconception is that the response variable must be
normally distributed when conducting an ANOVA.
Assumptions of ANOVA Transformations Non-parametrics 3 / 16
4. Assumptions of ANOVA
A common misconception is that the response variable must be
normally distributed when conducting an ANOVA.
This is incorrect because the normality assumptions pertain to the
residuals, not the response variable. The key assumption of
ANOVA is that the residuals are independent and come from a
normal distribution with mean 0 and variance σ2.
Assumptions of ANOVA Transformations Non-parametrics 3 / 16
5. Assumptions of ANOVA
A common misconception is that the response variable must be
normally distributed when conducting an ANOVA.
This is incorrect because the normality assumptions pertain to the
residuals, not the response variable. The key assumption of
ANOVA is that the residuals are independent and come from a
normal distribution with mean 0 and variance σ2.
yij = µ + αi + εij
εij ∼ Normal(0, σ2
)
Assumptions of ANOVA Transformations Non-parametrics 3 / 16
6. Assumptions of ANOVA
A common misconception is that the response variable must be
normally distributed when conducting an ANOVA.
This is incorrect because the normality assumptions pertain to the
residuals, not the response variable. The key assumption of
ANOVA is that the residuals are independent and come from a
normal distribution with mean 0 and variance σ2.
yij = µ + αi + εij
εij ∼ Normal(0, σ2
)
We can assess this assumption by looking at the residuals
themselves or the data within each treatment
Assumptions of ANOVA Transformations Non-parametrics 3 / 16
7. Normality diagnostics
Consider the data:
infectionRates <- read.csv("infectionRates.csv")
str(infectionRates)
## 'data.frame': 90 obs. of 2 variables:
## $ percentInfected: num 0.21 0.25 0.17 0.26 0.21 0.21 0.22 0.27 0.23 0.14 ...
## $ landscape : Factor w/ 3 levels "Park","Suburban",..: 1 1 1 1 1 1 1 1 1 1 ...
summary(infectionRates)
## percentInfected landscape
## Min. :0.010 Park :30
## 1st Qu.:0.040 Suburban:30
## Median :0.090 Urban :30
## Mean :0.121
## 3rd Qu.:0.210
## Max. :0.330
These data are made-up, but imagine they come from a study in which
100 crows are placed in n = 30 enclosures in each of 3 landscapes. The
response variable is the proportion of crows infected with West Nile virus
at the end of the study.
Assumptions of ANOVA Transformations Non-parametrics 4 / 16
11. Are group variances equal?
bartlett.test(percentInfected~landscape, data=infectionRates)
##
## Bartlett test of homogeneity of variances
##
## data: percentInfected by landscape
## Bartlett's K-squared = 42.926, df = 2, p-value = 4.773e-10
We reject the null hypothesis that the group variances are equal
Assumptions of ANOVA Transformations Non-parametrics 7 / 16
12. Histogram of residuals
resids <- resid(anova1)
hist(resids, col="turquoise", breaks=10, xlab="Residuals")
Histogram of resids
Residuals
Frequency
−0.10 −0.05 0.00 0.05 0.10
051015202530
Assumptions of ANOVA Transformations Non-parametrics 8 / 16
13. Normality test on residuals
shapiro.test(resids)
##
## Shapiro-Wilk normality test
##
## data: resids
## W = 0.95528, p-value = 0.003596
Assumptions of ANOVA Transformations Non-parametrics 9 / 16
14. Normality test on residuals
shapiro.test(resids)
##
## Shapiro-Wilk normality test
##
## data: resids
## W = 0.95528, p-value = 0.003596
We reject the null hypothesis that the residuals come from a
normal distribution. Time to consider transformations and/or
nonparametric tests.
Assumptions of ANOVA Transformations Non-parametrics 9 / 16
15. Logarithmic Transformation
y = log(u + C)
• The constant C is often 1, or 0 if there are no zeros in the
data (u)
• Useful when group variances are proportional to the means
Assumptions of ANOVA Transformations Non-parametrics 10 / 16
16. Square Root Transformation
y =
√
u + C
• C is often 0.5 or some other small number
• Useful when group variances are proportional to the means
Assumptions of ANOVA Transformations Non-parametrics 11 / 16
17. Arcsine-square root Transformation
y = arcsin(
√
u)
• Used on proportions.
• logit transformation is an alternative: y = log( u
1−u
)
Assumptions of ANOVA Transformations Non-parametrics 12 / 16
18. Reciprocal Transformation
y =
1
u + C
• C is often 1 but could be 0 if there are no zeros in u
• Useful when group SDs are proportional to the squared
group means
Assumptions of ANOVA Transformations Non-parametrics 13 / 16
19. ANOVA on transformed data
Tranformation can be done in the aov formula
anova2 <- aov(log(percentInfected)~landscape,
data=infectionRates)
summary(anova2)
## Df Sum Sq Mean Sq F value Pr(>F)
## landscape 2 60.93 30.46 303.5 <2e-16 ***
## Residuals 87 8.73 0.10
## ---
## Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Assumptions of ANOVA Transformations Non-parametrics 14 / 16
20. ANOVA on transformed data
Tranformation can be done in the aov formula
anova2 <- aov(log(percentInfected)~landscape,
data=infectionRates)
summary(anova2)
## Df Sum Sq Mean Sq F value Pr(>F)
## landscape 2 60.93 30.46 303.5 <2e-16 ***
## Residuals 87 8.73 0.10
## ---
## Signif. codes: 0 '***' 0.001 '**' 0.01 '*' 0.05 '.' 0.1 ' ' 1
Now we fail to reject the normality assumption – good news
shapiro.test(resid(anova2))
##
## Shapiro-Wilk normality test
##
## data: resid(anova2)
## W = 0.97092, p-value = 0.04106
Assumptions of ANOVA Transformations Non-parametrics 14 / 16
21. Non-parametric Tests
Wilcoxan rank sum test
• For 2 group comparisons
• a.k.a. the Mann-Whitney U test
• wilcox.test
Assumptions of ANOVA Transformations Non-parametrics 15 / 16
22. Non-parametric Tests
Wilcoxan rank sum test
• For 2 group comparisons
• a.k.a. the Mann-Whitney U test
• wilcox.test
Kruskal-Wallis One-Way ANOVA
• For testing differences in > 2 groups
• kruskal.test
Assumptions of ANOVA Transformations Non-parametrics 15 / 16
23. Non-parametric Tests
Wilcoxan rank sum test
• For 2 group comparisons
• a.k.a. the Mann-Whitney U test
• wilcox.test
Kruskal-Wallis One-Way ANOVA
• For testing differences in > 2 groups
• kruskal.test
These two functions can be used in almost the exact same way
as t.test and aov , respectively.
Assumptions of ANOVA Transformations Non-parametrics 15 / 16
24. Assignment
(1) Decide which transformation is best for the infectionRates data by
conducting an ANOVA on the untransformed and transformed data. Use
graphical assessments, Bartlett’s test, and Shapiro’s test to evaluate each
of the following tranformations:
log
square-root
acrsine square-root
reciprocal
(2) Does transformation alter the conclusion about the null hypothesis of no
difference in means? If not, were the transformations necessary?
(3) Test the hypothesis that infection rates are equal between suburban and
urban landscapes using a Wilcoxan rank sum test. What is the
conclusion?
(4) Conduct a Kruskal-Wallis test on the data. What is the conclusion?
Use comments in your R script to explain your answers. Upload your results to
ELC at least one day before your next lab.
Assumptions of ANOVA Transformations Non-parametrics 16 / 16