| [253] | 1 | subroutine ave_stelspec(STELLAR) |
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| [135] | 2 | |
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| 3 | !================================================================== |
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| 4 | ! |
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| 5 | ! Purpose |
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| 6 | ! ------- |
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| 7 | ! Average the chosen high resolution stellar spectrum over the |
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| 8 | ! visible bands in the model. |
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| 9 | ! |
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| 10 | ! Authors |
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| 11 | ! ------- |
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| 12 | ! Robin Wordsworth (2010). |
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| 13 | ! |
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| 14 | ! Called by |
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| 15 | ! --------- |
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| 16 | ! setspv.F |
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| 17 | ! |
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| 18 | ! Calls |
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| 19 | ! ----- |
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| 20 | ! none |
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| 21 | ! |
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| 22 | !================================================================== |
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| 23 | |
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| 24 | use radinc_h, only: L_NSPECTV |
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| 25 | use radcommon_h, only: BWNV, DWNV, tstellar |
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| 26 | |
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| 27 | implicit none |
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| 28 | |
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| 29 | #include "datafile.h" |
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| [253] | 30 | #include "callkeys.h" |
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| [135] | 31 | |
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| 32 | real*8 STELLAR(L_NSPECTV) |
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| [253] | 33 | ! integer startype |
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| [135] | 34 | |
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| 35 | integer Nfine |
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| 36 | parameter(Nfine=5000) |
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| 37 | integer ifine |
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| 38 | |
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| 39 | real lam(Nfine) |
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| 40 | real stel_f(Nfine) |
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| 41 | real band |
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| 42 | real dl |
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| 43 | |
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| 44 | character(len=50) :: file_id |
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| 45 | character(len=100) :: file_path |
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| 46 | |
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| [253] | 47 | real lam_temp |
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| 48 | double precision stel_temp |
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| 49 | |
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| [135] | 50 | STELLAR(:)=0.0 |
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| 51 | |
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| 52 | ! load high resolution wavenumber data |
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| 53 | file_id='/stellar_spectra/lam.txt' |
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| 54 | file_path=datafile(1:LEN_TRIM(datafile))//file_id(1:LEN_TRIM(file_id)) |
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| 55 | |
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| 56 | open(110,file=file_path,form='formatted') |
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| 57 | do ifine=1,Nfine |
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| 58 | read(110,*) lam(ifine) |
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| 59 | enddo |
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| 60 | close(110) |
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| 61 | |
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| 62 | dl=lam(2)-lam(1) |
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| 63 | |
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| [253] | 64 | |
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| 65 | if(stelbbody)then |
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| 66 | tstellar=stelTbb |
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| 67 | do ifine=1,Nfine |
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| 68 | lam_temp=lam(ifine) |
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| 69 | call blackl(dble(lam_temp*1e-6),dble(tstellar),stel_temp) |
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| 70 | stel_f(ifine)=stel_temp |
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| 71 | enddo |
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| [135] | 72 | else |
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| [253] | 73 | ! load high resolution stellar data |
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| 74 | if(startype.eq.1)then |
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| 75 | file_id='/stellar_spectra/sol.txt' |
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| 76 | tstellar=5800. |
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| 77 | elseif(startype.eq.2)then |
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| 78 | file_id='/stellar_spectra/gl581.txt' |
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| 79 | tstellar=3200. |
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| 80 | elseif(startype.eq.3)then |
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| 81 | file_id='/stellar_spectra/adleo.txt' |
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| 82 | tstellar=3200. |
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| 83 | elseif(startype.eq.4)then |
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| 84 | file_id='/stellar_spectra/gj644.txt' |
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| 85 | print*,'Find out tstellar before using this star!' |
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| 86 | call abort |
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| 87 | elseif(startype.eq.5)then |
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| 88 | file_id='/stellar_spectra/hd128167.txt' |
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| 89 | tstellar=6700. ! Segura et al. (2003) |
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| 90 | else |
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| 91 | print*,'Error: unknown star type chosen' |
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| 92 | call abort |
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| 93 | endif |
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| 94 | file_path=datafile(1:LEN_TRIM(datafile))//file_id(1:LEN_TRIM(file_id)) |
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| 95 | |
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| 96 | open(111,file=file_path,form='formatted') |
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| 97 | do ifine=1,Nfine |
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| 98 | read(111,*) stel_f(ifine) |
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| 99 | enddo |
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| 100 | close(111) |
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| [135] | 101 | endif |
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| 102 | |
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| [253] | 103 | |
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| [135] | 104 | ! sum data by band |
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| 105 | band=1 |
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| 106 | do ifine = 1,Nfine |
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| 107 | |
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| 108 | if(lam(Nfine-ifine+1) .lt. real(10000.0/BWNV(band+1)))then |
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| 109 | band=band+1 |
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| 110 | endif |
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| 111 | if(band .gt. L_NSPECTV)then |
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| 112 | goto 9999 ! ok, ok, I know they're evil |
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| 113 | endif |
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| 114 | STELLAR(band)=STELLAR(band)+stel_f(Nfine-ifine+1)*dl |
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| 115 | |
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| 116 | end do |
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| 117 | |
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| 118 | 9999 continue |
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| 119 | STELLAR=STELLAR/sum(STELLAR) |
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| 120 | |
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| [253] | 121 | |
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| [135] | 122 | end subroutine ave_stelspec |
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