This slideshare is about expressions. It is divided into expressions 1 and expressions 2. Expression 1 focuses on evaluating expressions which deals with substituting the known values in an equation to solve for the unknown. While, expressions 2 focuses on transposition of formula; change of subject of formula in a given equation.
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2018 Geometri Transformasi Perkalian 5 Isometri Kelompok 8 Rombel 3Yosia Adi Setiawan
Tugas Akhir Mata Kuliah Geometri Transformasi FMIPA Unnes Rombel 03 Kelompok 8
Ria Risqiana Agustina (4101415015)
Siti Nurzulifa (4101415030)
Dea Amara P. (4101415053)
Muchamad Idris (4101415091)
Luluk Syarifatun N. (4101415132)
Info: fauzi1997@students.unnes.ac.id
2018 Geometri Transformasi Perkalian 5 Isometri Kelompok 8 Rombel 3Yosia Adi Setiawan
Tugas Akhir Mata Kuliah Geometri Transformasi FMIPA Unnes Rombel 03 Kelompok 8
Ria Risqiana Agustina (4101415015)
Siti Nurzulifa (4101415030)
Dea Amara P. (4101415053)
Muchamad Idris (4101415091)
Luluk Syarifatun N. (4101415132)
Info: fauzi1997@students.unnes.ac.id
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
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 presentation explores a brief idea about the structural and functional attributes of nucleotides, the structure and function of genetic materials along with the impact of UV rays and pH upon them.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
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.
10. TRANSPOSITION OF FORMULA
Transpose the formula v= u + at to make ‘a’ the subject of
formula
v= u + at we want ‘a’ to stand alone
Move ‘u’ to the other side of the equation
v − u= at
This can be written as v − u= a × t
We still want ‘a’ to stand on its own, what can we do?
Divide both sides by t
(v − u) / t= a
Thus, a= (v − u) / t
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11. Transposition of Formula
Transpose d= 2 √h(2r − h) to make r the subject
d= 2 √h(2r − h) we want ‘r’ to stand alone.
This can be written as d= 2 × √h(2r − h)
We can divide both sides by 2
d/2 = √h(2r − h)
Square both sides
(d/2)2 = [√h(2r − h)]2
d2 /4 = h(2r − h)
Expand the bracket at the LHS
d2 /4 = 2rh − h2
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12. Transposition of Formula
Move h2 to the other side
d2 /4 + h2 = 2rh
Evaluate the LHS
(d2 + 4h2 ) / 4 = 2rh
Divide both sides by 2h
(d2 + 4h2 ) / 4 ÷ 2h = 2rh / 2h
(d2 + 4h2 ) / (4 × 2h) = r
(d2 + 4h2 ) / 8h = r
r = (d2 + 4h2 ) / 8h
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13. Transposition of Formula
Transpose v= [πh (3R2 + h2)] / 6 make R the subject of the
formula
v= [πh (3R2 + h2)] / 6
Cross multiply
6v = πh (3R2 + h2)
This can also be written as 6v = πh × (3R2 + h2)
Divide both sides by πh
6v / πh = 3R2 + h2
move h2 to the LHS
(6v / πh) − h2 = 3R2
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14. Transposition of Formula
Evaluate the LHS
(6v − πh3) / πh = 3R2
Divide both sides by 3
(6v − πh3) / πh ÷ 3 = R2
(6v − πh3) / 3πh = R2
Take the square root of both sides
√[(6v − πh3) / 3πh ] = R
R = √ [(6v − πh3) / 3πh ]
R = √ [(6v / 3πh ) − (πh3 / 3πh) ]
R = √ [(2v /πh ) − (h2 / 3) ]
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15. Transposition of Formula
Transpose the formula F = S(M − m) ⁄ M + m Make m the subject of
formula
F = S(M − m) ⁄ M + m
Cross multiply
F(M + m) = S(M − m)
Expand the brackets
FM + Fm = SM − Sm
Collect like terms
Fm + Sm = SM − FM
Factorise
m(F + S) = M(S − F)
Divide both sides by F + S
m= M(S − F) / (F + S)
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Expressions
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