Aa3d HH $ @d HHHHff@  dA Footnote TableFootnote**.\t.\t/ - :;,.!?%`'`TOCHeading1Heading2   EquationVariables 3} 3. 34 3< 3O 3bmm<$lastpagenum>n<$monthname> <$daynum>, <$year>o"<$monthnum>/<$daynum>/<$shortyear>p;<$monthname> <$daynum>, <$year> <$hour>:<$minute00> <$ampm>Vq"<$monthnum>/<$daynum>/<$shortyear>r<$monthname> <$daynum>, <$year>as"<$monthnum>/<$daynum>/<$shortyear>t <$fullfilename>u <$filename>v <$paratext[Title]>w <$paratext[Heading1]>x <$curpagenum>y <$marker1>z <$marker2>{ (Continued)|+ (Sheet <$tblsheetnum> of <$tblsheetcount>)}Heading & Page <$paratext> on page<$pagenum>~Pagepage<$pagenum> See Heading & Page%See <$paratext> on page<$pagenum>.TO Table All7Table<$paranumonly>, <$paratext>, on page<$pagenum>Table Number & Page'Table<$paranumonly> on page<$pagenum> A}A<     A$ a ! 3/ aoe> 3 b > 3 ci> 3 d" 3 e/um 3 fa 3 g$d 3" he 3# io>/ 3$ j$ea 3% kfi 3& l 3' m 3( nele 3) ote 3* p] 30 qg 35 ra 36 sa 3H tod) 3S u+t 3T vu<$ 3U wn 3V xnge 3W yx p 3X zu 3Y {een 3Z |He 3[ }e< 3\ ~ e 3]  3^ e 3_ ly2t>dqy&agn gedqzdq{|H3R `@q|}{ H3R `@H RH RFootnoteHq3@ `@q}|~{ Hq3@ `@HzHz Single Line"H'q~}{ Footnote  3~     H3D `@q~{ e3*H3D `@HH Double LineH q{)3Su Double Linew 3 x 3 <3\ 3]H q{> Single Lineag 3HZq{q TableFootnoteEGVR `@q{ }EGVR `@EPwEPw TableFootnoteod5pj)+ & 32 )/ & j)+ & $'equal[indexes[0,1,char[lambda],times[char[M],char[A],char[X]]],over[times[prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[]],times[prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[]]]]NGH 33xHH 3y HH d b  HH 3z HH d c  HUV 3z HUV EGVqUU` d H$ 3z oH$ UU` e32 HUV 3y )+HUV bda],timr[UUd fom ]H$ 3y [prH$ []],promptomUUd gmp ,HH 3! HH UT UT` h.79205 AstronomyNAME:________________________ UR UT` l Work sheet +UP UT` iStudio Exercise Week #1 UT` r eU< UT s )Y3. Make a plot of two blackbody spectra for two different temperatures. Indicate vU: UT H sNwhich temperature goes with which plot, and approximately label the axes: W)mQ & 3,W)mQ & W)mQ & $3!'equal[char[sigma],over[times[prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[]],times[prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[],prompt[]]]]NH 3- jStL  3;JUT n 3@npoe w s 3Apss manco s  3B as  dmI;sT5 3C mI;sT5mI;mI;Wavelength l$s@  3D wdi$s@ $$ Radiance Rd 3Itanax:HH 3J HHW'eq], UT UT$ t[]W4. Indicate the limits you chose for your regions of red and blue. Dont forget to proUR UT"L tmpinclude the units. mptsUP UTd u[]TList the values you determined for your color index as a function of temperature: UN UTd v UL UTd w T(K)CI UJ UTd x nUH UTd y @UF UTd zn oUD UTd { w sUB UTd | U@ UTd }  U> UTd ~ U< UTd  .U: UTd  ?U8 UT$ TFinally, make a plot of temperature versus color index. Indicate where color index PU6 UT"L sPis a good way to measure temperature of a star, and where it is a poor way. T/2 3M T/2 T/2 $'atop[leq[prompt[],indexes[0,1,char[lambda],times[char[R],char[E],char[D]]],prompt[]],leq[prompt[],indexes[0,1,char[lambda],times[char[B],char[L],char[U],char[E]]],prompt[]]]TNfH 3NuhodndH3 3atmp ptUPHH 3uymedHHl UT 3gT)d x  3hT  UT v:iT  3i U<v:iT v:%Fv:%FColor Index CIiR  3j ruriR FF Temperature THH 3vzu tHHlHUV 3wzHUV l ndeH$ 3xzcr[H$ l ar[HUV 3yyHUV l H$ 3zyH$ l  3uHH 3{HHl  3gHH 3|xHHl %dyLeftidzRightd{: ReferenceoddiFf ABody. f Ar[ Bulleted\t. f ACellBody. f A CellHeading. f A% Footnote. ftfTA Heading1Body. fT A Heading2Body. fT A  HeadingRunInBody. f Al yIndented. f Ag Numbered.\t. fE At Numbered1.\tNumbered. f Af TableFootnote. fT A  TableTitleT:Table : .  fPA TitleBody. f T A  TableTitleT:Table : . f  A CellHeading. f  ACellBody. f  A CellFooting. f  ABody. @ lHeader. @ blaFooter. fABody. fAll.Body. fABody. fAdyl..Body.  ) ڝ A ) A A EmphasisA EquationVariables [A  ڝڝAtu AwAڝA)A  AAAAAA AZ AZAThinAMediumADoubleAdyThick@A Very Thin 5E5 6AAAHHHHHFormat A 7AAAHHHHHFormat BCCommentAQId ABlackT!BWhiteddACRedddDGreendd EABluedFCyandGMagentad HYellow Times-Roman Times-Bold Times-ItalicHelvetica-BoldSymbolSymbolTimes HelveticaASymbol RegularRegulary BoldRegularItalicG{q:4