View source for Draft:Original research/MacLaurin series

[[Image:Sintay SVG.svg|thumb|right|250px|This graph show the use of a MacLaurin series to approximate the sine of x, or sin(x), when x = 0, and other values determined by polynomials with degree {{font|color=red|1}}, {{font|color=orange|3}}, {{font|color=yellow|5}}, {{font|color=green|7}}, {{font|color=blue|9}}, {{font|color=indigo|11}} and {{font|color=violet|13}}. Credit: [[commons:User:IkamusumeFan|IkamusumeFan]].]]
A '''MacLaurin series''' is a Taylor series that has a term at (0,0).

A Taylor series is a representation of a function as an infinite sum of terms that are calculated from the values of the function's derivatives at a single point.<ref name="MAT 314">{{ cite web
| publisher=Canisius College
| work=MAT 314
| title=Neither Newton nor Leibniz – The Pre-History of Calculus and Celestial Mechanics in Medieval Kerala
| accessdate=2006-07-09
| url=https://web.archive.org/web/20150223113517/http://www.pas.rochester.edu/~rajeev/papers/canisiustalks.pdf }}</ref><ref name="dani">{{ cite journal
| title=Ancient Indian Mathematics – A Conspectus
| author= S. G. Dani
|journal= Resonance 
|volume=17
|issue=3
|year=2012
|pages=236–246
|doi=10.1007/s12045-012-0022-y }}</ref><ref>Ranjan Roy, The Discovery of the Series Formula for π by Leibniz, Gregory and Nilakantha, Mathematics Magazine Vol. 63, No. 5 (Dec., 1990), pp. 291-306.</ref>
{{clear}}

==Calculuses==
{{main|Calculuses|Calculus}}
[[Image:RandLintegrals.png|thumb|right|250px|This diagram shows an approximation to an area under a curve. Credit: [[commons:User:Dubhe|Dubhe]].]]
'''Notation''': let the symbol <math>\Delta</math> represent '''difference in''' a variable.

'''Notation''': let the symbol <math>d</math> represent an '''infinitesimal difference in''' a variable.

'''Notation''': let the symbol <math>\partial</math> represent an '''infinitesimal difference in''' one input to a function of more than one input.

Let
: <math>y = f(x)</math>
be a function where values of <math>x</math> may be any real number and values resulting in <math>y</math> are also any real number.

: <math>\Delta x</math> is a small finite difference in <math>x</math> which when put into the function <math>f(x)</math> produces a <math>\Delta y</math>.

These small differences can be manipulated with the operations of arithmetic: addition (<math>+</math>), subtraction (<math>-</math>), multiplication (<math>*</math>), and division (<math>/</math>).

: <math>\Delta y = f(x + \Delta x) - f(x)</math>

Dividing <math>\Delta y</math> by <math>\Delta x</math> and taking the limit as <math>\Delta x</math> → 0, produces the slope of a line tangent to f(x) at the point x.

For example,

: <math>f(x) = x^2</math>

: <math>f(x + \Delta x) = (x + \Delta x)^2 = x^2 + 2x\Delta x + (\Delta x)^2</math>

: <math>\Delta y/\Delta x = (x^2 + 2x\Delta x + (\Delta x)^2 - x^2)/\Delta x</math>

: <math>\Delta y/\Delta x = 2x + \Delta x</math>

as <math>\Delta x</math> and<math>\Delta y</math> go towards zero,

: <math>dy/dx = 2x + dx = limit_{\Delta x\to 0}{f(x+\Delta x)-f(x)\over \Delta x} = 2x.</math>

This ratio is called the derivative.

Let

: <math>y = f(x,z)</math>

then

: <math>\partial y = \partial f(x,z) = \partial f(x,z) \partial x + \partial f(x,z) \partial z</math>

: <math>\partial y/ \partial x = \partial f(x,z)</math>

where z is held constant and

: <math>\partial y / \partial z = \partial f(x,z)</math>

where x is held contstant.

'''Notation''': let the symbol <math>\nabla</math> be the gradient, i.e., derivatives for multivariable functions.

: <math>\nabla f(x,z) = \partial y = \partial f(x,z) = \partial f(x,z) \partial x + \partial f(x,z) \partial z.</math>

For

: <math>\Delta x * \Delta y = [f(x + \Delta x) - f(x)] * \Delta x</math>

the area under the curve shown in the diagram at right is the light purple rectangle plus the dark purple rectangle in the top figure

: <math>\Delta x * \Delta y + f(x) * \Delta x = f(x + \Delta x) * \Delta x.</math>

Any particular individual rectangle for a sum of rectangular areas is

: <math>f(x_i + \Delta x_i) * \Delta x_i.</math>

The approximate area under the curve is the sum <math>\sum</math> of all the individual (i) areas from i = 0 to as many as the area needed (n):

: <math>\sum_{i=0}^{n} f(x_i + \Delta x_i) * \Delta x_i.</math>

'''Notation''': let the symbol <math>\int </math> represent the '''integral'''.

: <math>limit_{\Delta x\to 0}\sum_{i=0}^{n} f(x_i + \Delta x_i) * \Delta x_i = \int f(x)dx.</math>

This can be within a finite interval [a,b]

: <math>\int_a^b f(x) \; dx</math>

when i = 0 the integral is evaluated at <math>a</math> and i = n the integral is evaluated at <math>b</math>. Or, an indefinite integral (without notation on the integral symbol) as n goes to infinity and i = 0 is the integral evaluated at x = 0.

'''Def.''' a branch of mathematics that deals with the finding and properties ... of infinitesimal differences is called a '''calculus'''.

'''Calculus''' focuses on limits, functions, derivatives, integrals, and infinite series.

"Although ''calculus'' (in the sense of analysis) is usually synonymous with infinitesimal calculus, not all historical formulations have relied on infinitesimals (infinitely small numbers that are nevertheless not zero)."<ref name=InfinitesimalCalculusWikt>{{ cite book
|title=infinitesimal calculus
|publisher=Wikimedia Foundation, Inc
|location=San Francisco, California
|date=September 19, 2012
|url=http://en.wiktionary.org/wiki/infinitesimal_calculus
|accessdate=2013-01-31 }}</ref>

==Series==
{{main|Series}}
Taylor Series:

<math>y= \sum_{n=0}^{\infty }\frac{f^{n}(a)(x-a)^{n}}{n!}=f(a)+{f}'(a)(x-a)+ \frac{{f}''(a)(x-a)^{2})}{2!}+\frac{{f}'''(a)(x-a)^{3}}{3!}+...,</math>

where f<sup>n</sup> refers to the number (n) of derivatives taken.

A MacLaurin series of a function ''ƒ''(''x'') for which a derivative may be taken of the function or any of its derivatives at ''0'' is the power series

:<math>f(0)+\frac {f'(0)}{1!} (x)+ \frac{f''(0)}{2!} (x)^2+\frac{f^{(3)}(0)}{3!}(x)^3+ \cdots. </math>

which can be written in the more compact sigma, or summation, notation as

:<math> \sum_{n=0} ^ {\infty} \frac {f^{(n)}(0)}{n!} \, (x)^{n}</math>

where ''n''! denotes the factorial of ''n'' and ''ƒ''<sup>&nbsp;(''n'')</sup>(''0'') denotes the ''n''th derivative of ''ƒ'' evaluated at the point ''0''. The derivative of order zero ''ƒ'' is defined to be ''ƒ'' itself and {{nowrap|(''x'')<sup>0</sup>}} and 0! are both defined to be&nbsp;1.

==MacLaurin series for e<sup>x</sup>==
Taylor series is defined as
:{| style="width:100%" border="0" align="left"
|-
|<math> \sum_{n=0} ^ {\infty } \frac {f^{(n)}(t)}{n!} \, (x-t)^{n}</math>
|| <p style="text-align:right;"></p>  
|-
|}
The MacLaurin series occurs when t=0
:{| style="width:100%" border="0" align="left"
|-
|<math> \sum_{n=0} ^ {\infty } \frac {f^{(n)}(0)}{n!} \, (x)^{n}</math>
|| <p style="text-align:right;"></p>  
|-
|}
The derivatives are
:<math>{y}'=e^x</math>
:<math>{y}''=e^x</math>
:<math>{y}'''=e^x</math>
.

.

.

Development of MacLaurin series for <big><math>e^x</math></big>
:{| style="width:100%" border="0" align="left"
|-
|<math>e^x=\frac{1}{0!}+\frac{1}{1!}x+\frac{1}{2!}x^2+\frac{1}{3!}x^3\ldots</math>
|| <p style="text-align:right;"></p>  
|-
|}

:<math>e^x=1+x+\frac{1}{2}x^2+\frac{1}{6}x^3\ldots</math>
<br>
Explicit form can be written as
<br>
:<math> e^x=\sum_{n=0} ^ {\infty } \frac {1}{n!} \, (x)^{n}</math>

==MacLaurin series for the natural logarithm==

The natural logarithm (with base {{mvar|e}}) has Maclaurin series
:<math>\begin{align}
\log(1-x) &= - \sum^{\infty}_{n=1} \frac{x^n}n = -x - \frac{x^2}2 - \frac{x^3}3 - \cdots , \\
\log(1+x) &= \sum^\infty_{n=1} (-1)^{n+1}\frac{x^n}n = x - \frac{x^2}2 + \frac{x^3}3 - \cdots .
\end{align}</math>
They converge for <math>|x| < 1</math>.

==MacLaurin series for sin(x)==

:<math>y=sin(t)</math>
:<math>y'=cos(t)</math>
:<math>y''=-sin(t)</math>
:<math>y'''=-cos(t)</math>
:<math>y^{iv}=sin(t)</math>
:<math>y^{v}=cos(t)</math>
.

.

.

Development of MacLaurin series for <math>sin(x)</math>
:{| style="width:100%" border="0" align="left"
|-
|<math>sin(x)=\frac{0}{0!}+\frac{1}{1!}x-\frac{0}{2!}x^2-\frac{1}{3!}x^3+\frac{0}{4!}x^4+\frac{1}{5!}x^5...</math>
|| <p style="text-align:right;"> </p>  
|-
|}

:<math>sin(x)=1x-\frac{1}{6}x^3+\frac{1}{120}x^5...</math>
<br>
Explicit form can be written as
<br>
:<math> sin(x)=\sum_{n=0} ^ {\infty } \frac {(-1)^n}{(2n+1)!} \, (x)^{(2n+1)}</math>

==MacLaurin series for cos(x)==

Development of MacLaurin series for <math>cos(x)</math>
:<math>y=cos(t)</math>
:<math>y'=-sin(t)</math>
:<math>y''=-cos(t)</math>
:<math>y'''=sin(t)</math>
:<math>y^{iv}=cos(t)</math>
.

.

.

:{| style="width:100%" border="0" align="left"
|-
|<math>cos(x)=\frac{1}{0!}+\frac{0}{1!}x-\frac{1}{2!}x^2+\frac{0}{3!}x^3+\frac{1}{4!}x^4\ldots</math>
|| <p style="text-align:right;"> </p>  
|-
|}

:<math>cos(x)=1-\frac{1}{2}x^2+\frac{1}{24}x^4...</math>
<br>
Explicit form can be written as
<br>
:<math> cos(x)=\sum_{n=0} ^ {\infty} \frac {(-1)^n}{(2n)!} \, (x)^{2n}</math>

==Euler's formula==

Recalling Euler's Formula:
<br>
:<math>e^{i\omega x}=\cos\omega x+i\sin\omega x\!</math>
<br>
<br>
Recall the Taylor Series from above for <math>e^x</math> at :<math>t=0</math> (also called the MacLaurin series)
<br>
:<math>e^{x}=\sum_{n=0}^{\infty}\frac{x^n}{n!}\!</math>
<br>
<br>
By replacing x with <math>i\omega x</math>, the Taylor series for <math>e^{i\omega x}</math> can be found:
<br>
:<math style="padding: 5px; border: 2px solid gray;">e^{i\omega x}=\sum_{n=0}^{\infty}\frac{(i\omega x)^n}{n!}\!</math>
<br>
<br>
even powers of n = 2k:  
<br>
:<math>i^{2k}=(i^2)^k=(-1)^k\!</math>
<br>
odd powers of n = 2k+1:  
<br>
:<math>i^{2k+1}=(i^2)^k i=(-1)^k i\!</math>
<br>
<br>
For <math>i\omega x</math>:
<br>
:<math>e^{i\omega x}=\sum_{n=0}^{\infty}\frac{i^n (\omega x)^n}{n!}=\sum_{k=0}^{\infty}\frac{i^{2k} (\omega x)^{2k}}{(2k)!}+\sum_{k=0}^{\infty}\frac{i^{2k+1} (\omega x)^{2k+1}}{(2k+1)!}\!</math>
<br>
<br>
Using the two previous equations:
<br>
:<math>e^{i \omega x}=\sum_{k=0}^{\infty}\frac{(-1)^{k} (\omega x)^{2k}}{(2k)!}+i\sum_{k=0}^{\infty}\frac{(-1)^{k} (\omega x)^{2k+1}}{(2k+1)!}\!</math>
<br>
<br>
:<math>\Rightarrow e^{i \omega x}=\cos (\omega x)+i \sin (\omega x)\!</math>
<br>
<br>
Therefore, the first part of the equation is equal to the Taylor series for cosine, and the second part is equal to the Taylor series for sine as follows:
<br>
<br>
:<math style="padding: 5px; border: 2px solid gray;">\cos( \omega x)=\sum_{k=0}^{\infty}\frac{(-1)^{k} ( \omega x)^{2k}}{(2k)!}\!</math>
<br>
:<math style="padding: 5px; border: 2px solid gray;">\sin ( \omega x)= \sum_{k=0}^{\infty}\frac{(-1)^{k} ( \omega x)^{2k+1}}{(2k+1)!}\!</math>
<br>

==MacLaurin series for <math>\displaystyle (1-x)^{-a}</math>==

<math>\displaystyle f(x) = \frac {1}{(1-x)^a}</math>

{|  border="1" cellspacing="2" cellpadding="10" align="center"
|colspan="2" | {{center top}}'''Table for Maclaurin Series'''{{center bottom}}
|-
|<math> f(x) = \frac {1}{(1-x)^a}</math>||<math> f(0) = \frac {1}{(1-0)^a}=1</math>
|-
|<math> f '(x) = \frac {a}{(1-x)^{a+1}}</math>||<math> f '(0) = \frac {a}{(1-0)^{a+1}} = a</math>
|-
|<math>f' '(x) = \frac {a(a+1)}{(1-x)^{a+2}}</math>||<math>f' '(0) = \frac {a(a+1)}{(1-0)^{a+2}} = a(a+1)</math>
|-
|<math>f^{(3)}(x) = \frac {a(a+1)(a+2)}{(1-x)^{a+3}}</math>||<math>f^{(3)}(0) = \frac {a(a+1)(a+2)}{(1-0)^{a+3}}= a(a+1)(a+2)</math>
|-
|And so on..||..
|}

Rewriting the Maclaurin series expansion,

:<math>\displaystyle \frac {1}{(1-x)^a} = f(0)+\frac {f'(0)}{1!} (x-0)+ \frac{f''(0)}{2!} (x-0)^2+\frac{f^{(3)}(0)}{3!}(x-0)^3+ \cdots.</math>

Substituting the values from the table, we get

:<math>\displaystyle \frac {1}{(1-x)^a} = 1 +\frac {a}{1!} (x)+ \frac{a(a+1)}{2!} (x)^2+\frac{a(a+1)(a+2)}{3!}(x)^3+ \cdots. </math>

:<math>\displaystyle \frac {1}{(1-x)^a} = \sum_{n=0} ^ {\infin } (a)_k \frac {x^k}{n!} </math>

Using

:<math>(a)_0 := 1</math>

:<math>(a)_k := a(a+1)(a+2)\cdots(a+k-1)</math>

We can represent 

:<math> \sum_{n=0} ^ {\infin } \frac{(a)_k \, (b)_k}{(c)_k}\, \frac {x^k}{n!} = F(a,b;c;x) </math>

:<math>\sum_{n=0} ^ {\infin } \frac{(a)_k (b)_k}{(b)_k}\frac {x^k}{n!} = F(a,b;b;x)</math>

== Binomial series ==

The binomial series is the power series

:<math>(1+x)^\alpha = \sum_{n=0}^\infty \binom{\alpha}{n} x^n</math>

whose coefficients are the generalized binomial coefficients

: <math>\binom{\alpha}{n} = \prod_{k=1}^n \frac{\alpha-k+1}k = \frac{\alpha(\alpha-1)\cdots(\alpha-n+1)}{n!}.</math>

(If {{math| ''n'' {{=}} 0}}, this product is an empty product and has value 1.)  It converges for <math>|x| < 1</math> for any real or complex number {{mvar|α}}.

When {{math|''α'' {{=}} −1}}, this is essentially the infinite geometric series mentioned in the previous section.  The special cases {{math|''α'' {{=}} {{sfrac|1|2}}}} and {{math|''α'' {{=}} −{{sfrac|1|2}}}} give the square root function and its inverse:

:<math>\begin{align} 
(1+x)^\frac12 &= 1 + \tfrac{1}{2}x - \tfrac{1}{8}x^2 + \tfrac{1}{16}x^3 - \tfrac{5}{128}x^4 + \tfrac{7}{256}x^5 - \ldots, \\
(1+x)^{-\frac12} &= 1 -\tfrac{1}{2}x + \tfrac{3}{8}x^2 - \tfrac{5}{16}x^3 + \tfrac{35}{128}x^4 - \tfrac{63}{256}x^5 + \ldots.
\end{align}</math>

When only the linear term is retained, this simplifies to the binomial approximation.

==MacLaurin series for <math>\displaystyle arctan(1+x)</math>==

We have the function 

<math>\displaystyle arctan(1+x)</math>

Expand <math>\displaystyle arctan(1+x)</math>

{|  border="1" cellspacing="2" cellpadding="10" align="center"
|colspan="2" | {{center top}}'''Table for Maclaurin Series'''{{center bottom}}
|-
|<math> f(x) = arctan(1+x) </math>||<math> f(0) = arctan(1+0) = \frac{\pi}{4}</math>
|-
|<math> f '(x) = \frac {1}{1+(1+x)^{2}}</math>||<math> f '(0) = \frac {1}{1+(1+0)^{2}} = \frac {1}{2}</math>
|-
|<math>f' '(x) = \frac {-2(x+1)}{\left[1+(1+x)^2\right]^2}</math>||<math>f' '(0) = \frac {-2(0+1)}{\left[1+(1+0)^2\right]^2}= \frac{-1}{2}</math>
|-
|<math>f^{(3)}(x) = \frac {2(3x^2+6x+2)}{\left[1+(1+x)^2\right]^3}</math>||<math>f^{(3)}(0) = \frac {2(3(0)^2+6(0)+2)}{\left[1+(1+0)^2\right]^3} = \frac{1}{2}</math>
|-
|And so on..||..
|}

Rewriting the Maclaurin series expansion,

:<math>\displaystyle arctan(1+x) = f(0)+\frac {f'(0)}{1!} (x-0)+ \frac{f''(0)}{2!} (x-0)^2+\frac{f^{(3)}(0)}{3!}(x-0)^3+ \cdots.</math>

Substituting the values from the table, we get

:<math>\displaystyle arctan(1+x) = \frac{\pi}{4} + \frac {1}{2*1!} (x)- \frac{1}{2*2!} (x)^2+\frac{1}{2*3!}(x)^3+ \cdots.</math>

==MacLaurin series for <math>arctan(x)</math>==

<math>arctan(x)</math>

Expanding <math>arctan(x)</math> using Maclaurin's series

{|  border="1" cellspacing="2" cellpadding="10" align="center"
|colspan="2" | {{center top}}'''Table for Maclaurin Series'''{{center bottom}}
|-
|<math> f(x) = arctan(x) </math>||<math> f(0) = arctan(0) = 0</math>
|-
|<math> f '(x) = \frac {1}{1+x^{2}}</math>||<math> f '(0) = \frac {1}{1+(0)^{2}} = 1</math>
|-
|<math>f' '(x) = \frac {-2x}{\left[1+x^2\right]^2}</math>||<math>f' '(0) = \frac {-2(0)}{\left[1+(0)^2\right]^2}= 0</math>
|-
|<math>f^{(3)}(x) = \frac {6x^2-2}{\left[1+x^2\right]^3}</math>||<math>f^{(3)}(0) = \frac {6(0)^2-2}{\left[1+(0)^2\right]^3} = -2 </math>
|-
|<math>f^{(4)}(x) = \frac {-24x(x^2-1)}{\left[1+x^2\right]^4}</math>||<math>f^{(4)}(0) = \frac {-24(0)((0)^2-1)}{\left[1+(0)^2\right]^4}= 0 </math>
|-
|<math>f^{(5)}(x) = \frac {24(5x^4-10x^2+1)}{\left[1+x^2\right]^5}</math>||<math>f^{(5)}(x) = \frac {24(5(0)^4-10(0)^2+1)}{\left[1+(0)^2\right]^5} = 24</math>
|-
|And so on..||..
|}

Rewriting the Maclaurin series expansion,

:<math>\displaystyle arctan(x) = f(0)+\frac {f'(0)}{1!} (x-0)+ \frac{f''(0)}{2!} (x-0)^2+\frac{f^{(3)}(0)}{3!}(x-0)^3+ \cdots.</math>

Substituting the values from the table, we get

:<math>\displaystyle arctan(x) = 0 +\frac {1}{1!} (x)+ \frac{0}{2!} (x)^2+\frac{-2}{3!}(x)^3+ \frac{0}{4!}(x)^4 + \frac{24}{5!}(x)^5 \cdots.</math>

==MacLaurin series for trigonometric functions==

:<math>\begin{align}
\sin x &= \sum^{\infty}_{n=0} \frac{(-1)^n}{(2n+1)!} x^{2n+1} &&= x - \frac{x^3}{3!} + \frac{x^5}{5!} - \cdots && \text{for all } x\\[6pt]
\cos x &= \sum^{\infty}_{n=0} \frac{(-1)^n}{(2n)!} x^{2n} &&= 1 - \frac{x^2}{2!} + \frac{x^4}{4!} - \cdots && \text{for all } x\\[6pt]
\tan x &= \sum^{\infty}_{n=1} \frac{B_{2n} (-4)^n \left(1-4^n\right)}{(2n)!} x^{2n-1} &&= x + \frac{x^3}{3} + \frac{2 x^5}{15} + \cdots && \text{for }|x| < \frac{\pi}{2}\\[6pt]
\sec x &= \sum^{\infty}_{n=0} \frac{(-1)^n E_{2n}}{(2n)!} x^{2n} &&=1+\frac{x^2}{2}+\frac{5x^4}{24}+\cdots && \text{for }|x| < \frac{\pi}{2}\\[6pt]
\arcsin x &= \sum^{\infty}_{n=0} \frac{(2n)!}{4^n (n!)^2 (2n+1)} x^{2n+1} &&=x+\frac{x^3}{6}+\frac{3x^5}{40}+\cdots && \text{for }|x| \le 1\\[6pt]
\arccos x &=\frac{\pi}{2}-\arcsin x\\&=\frac{\pi}{2}- \sum^{\infty}_{n=0} \frac{(2n)!}{4^n (n!)^2 (2n+1)} x^{2n+1}&&=\frac{\pi}{2}-x-\frac{x^3}{6}-\frac{3x^5}{40}-\cdots&& \text{for }|x| \le 1\\[6pt]
\arctan x &= \sum^{\infty}_{n=0} \frac{(-1)^n}{2n+1} x^{2n+1} &&=x-\frac{x^3}{3} + \frac{x^5}{5}-\cdots && \text{for }|x| \le 1,\ x\neq\pm i
\end{align}</math>

All angles are expressed in radians. The numbers {{math|''B<sub>k</sub>''}} appearing in the expansions of {{math|tan ''x''}} are the Bernoulli numbers. The {{math|''E''<sub>''k''</sub>}} in the expansion of {{math|sec ''x''}} are Euler numbers.

==Engineering==
{{main|Literature/Engineering|Engineering}}
The "performance of a Markov system under different operating strategies [can be estimated] by observing the behavior of the system under the [strategy of having] a Maclaurin series for the performance measures of [the] Markov chains."<ref name=Cao>{{ cite journal
|author=Xi-Ren Cao
|title=The Maclaurin Series for Performance Functions of Markov Chains
|journal=Advances in Applied Probability
|month=
|year=1998
|volume=30
|issue=
|pages=676-92
|url=http://www.ece.ust.hk/~eecao/paper/60.pdf
|arxiv=
|bibcode=
|doi=
|pmid=
|accessdate=2014-07-23 }}</ref>

==Hypotheses==
{{main|Hypotheses}}
# Any non-convergent function can be represented by a MacLaurin series.

==See also==
{{div col|colwidth=20em}}
* [[Draft:MacLaurin series|MacLaurin series]] (18 kB) (3 February 2020)
* [[Draft:Mathematics|Mathematics]] (41 kB) (17 September 2019)
* [[:File:3.PNG|Solution for sin(t)]]
* [[:File:2.7 Wiki2.pdf|Solutions to problem set 2.7]]
{{Div col end}}

==References==
{{reflist|2}}

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* [http://www.questia.com/ Questia - The Online Library of Books and Journals]
* [http://online.sagepub.com/ SAGE journals online]
* [http://www.adsabs.harvard.edu/ The SAO/NASA Astrophysics Data System]
* [http://www.scirus.com/srsapp/advanced/index.jsp?q1= Scirus for scientific information only advanced search]
* [http://cas.sdss.org/astrodr6/en/tools/quicklook/quickobj.asp SDSS Quick Look tool: SkyServer]
* [http://simbad.u-strasbg.fr/simbad/ SIMBAD Astronomical Database]
* [http://simbad.harvard.edu/simbad/ SIMBAD Web interface, Harvard alternate]
* [http://nssdc.gsfc.nasa.gov/nmc/SpacecraftQuery.jsp Spacecraft Query at NASA]
* [http://www.springerlink.com/ SpringerLink]
* [http://www.tandfonline.com/ Taylor & Francis Online]
* [http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/convcoord/convcoord.pl Universal coordinate converter]
* [http://onlinelibrary.wiley.com/advanced/search Wiley Online Library Advanced Search]
* [http://search.yahoo.com/web/advanced Yahoo Advanced Web Search]

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