Документ взят из кэша поисковой машины. Адрес оригинального документа : http://star.arm.ac.uk/~csj/idl/FAST/normalise.pro Дата изменения: Thu Sep 18 14:04:41 2014 Дата индексирования: Sun Apr 10 05:46:11 2016 Кодировка: Поисковые слова: http astrokuban.info astrokuban

PRO normalise, creg, cforder ;; convert flux spectra to normalized spectra


; COMMON fileblock
COMMON fitsblock
COMMON procblock
COMMON colorblock

;; Input
;
; creg = [w1l, wlu, w2l, w2u, ....]
; pairs of wavelength defining regions for fitting the continuum

IF ( n_params() LE 1 ) THEN cforder = 3 ;; assumed order for continuum polynomial
print,cforder

;; evaluate the median spectrum

specm=fltarr(nwave)
FOR iw=0,nwave-1 DO BEGIN
specm(iw) = median(spec(iw,0:nspec-1))
ENDFOR


cont = fltarr(nwave,nspec)

;; define continuum regions

ncont = n_elements(creg)
creg_loc = where(wave ge creg(0) and wave le creg(1))

FOR ic = 0,ncont-1,2 DO $
creg_loc =[creg_loc,where(wave ge creg(ic) and wave le creg(ic+1))]


;; create 2d contiuum fit



FOR is = 0,nspec-1 DO BEGIN

;; fit 1d polynomial to continuum

poly = poly_fit(wave(creg_loc)-wave(0), spec(creg_loc,is), cforder)

;; evaluate the continuum polynomial

cont(*,is) = poly(cforder)
FOR ip = cforder-1,0,-1 DO BEGIN
cont(*,is) = cont(*,is)*(wave-wave(0)) + poly(ip)
ENDFOR

ENDFOR


;; divide 2d spectrum by 2d continuum

spec = spec / cont


;; find continuum for median spectrum


cont = fltarr(nwave)

poly = poly_fit(wave(creg_loc)-wave(0), specm(creg_loc), cforder)
cont = poly(cforder)
FOR ip = cforder-1,0,-1 DO BEGIN
cont = cont*(wave-wave(0)) + poly(ip)
ENDFOR


window,30,title="normalise.pro"
p_save = !p.multi
!p.multi=[0,0,2,0,0]
plot,wave,specm
oplot,wave,cont
oplot,wave(creg_loc),specm(creg_loc),color=cols.red

;; normalise median spectrum

specm = specm/cont

plot,wave,specm
!p.multi=p_save


END