Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/722/1226 into FORTRAN code for reading data files line by line.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe C============================================================================= C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Mar-29 C============================================================================= * This code was generated from the ReadMe file documenting a catalogue * according to the "Standard for Documentation of Astronomical Catalogues" * currently in use by the Astronomical Data Centers (CDS, ADC, A&A) * (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx) * Please report problems or questions to C============================================================================= implicit none * Unspecified or NULL values, generally corresponding to blank columns, * are assigned one of the following special values: * rNULL__ for unknown or NULL floating-point values * iNULL__ for unknown or NULL integer values real*4 rNULL__ integer*4 iNULL__ parameter (rNULL__=--2147483648.) ! NULL real number parameter (iNULL__=(-2147483647-1)) ! NULL int number integer idig ! testing NULL number C============================================================================= Cat. J/ApJ/722/1226 IR photometry in {lambda} Orionis cluster (Hernandez+, 2010) *================================================================================ *Spitzer observations of the {lambda} Orionis cluster. *II. Disks around solar-type and low-mass stars. * Hernandez J., Morales-Calderon M., Calvet N., Hartmann L., Muzerolle J., * Gutermuth R., Luhman K.L., Stauffer J. * <Astrophys. J., 722, 1226-1239 (2010)> * =2010ApJ...722.1226H C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Compiled membership information of the {lambda} Orionis Cluster integer*4 nr__ parameter (nr__=205) ! Number of records character*98 ar__ ! Full-size record C J2000 position composed of: RAdeg DEdeg integer*4 ID ! [936/7971] Identification number real*8 RAdeg ! (deg) Right Ascension in decimal degrees (J2000) real*8 DEdeg ! (deg) Declination in decimal degrees (J2000) character*12 Name ! Source name (LOriNNN, see ref. 2 or DMNN, see * ref. 1) character*10 SpType ! MK spectral type character*3 r_SpType ! Reference(s) for SpType (1) real*4 RV1 ! (km/s) ? Radial velocity 1 real*4 RV2 ! (km/s) ? Radial velocity 2 real*4 RV3 ! (km/s) ? Radial velocity 3 character*5 r_RV ! Reference(s) for radial velocities (1) character*3 LiI ! Li I present? (Y according to r_LiI) character*3 r_LiI ! Reference(s) for LiI (1) character*11 Memb ! Membership details (G1) character*3 Mm ! Membership flag (2) *Note (1): Reference as follows: * 1 = Dolan & Mathieu (2001, Cat. J/AJ/121/2124; <[DM99] NNN> in Simbad); * 2 = Barrado y Navascues et al. (2007, Cat. J/ApJ/664/481; <lOri-CFHT NNN> in * Simbad); * 3 = Maxted et al. (2008, Cat. J/MNRAS/385/2210; [MJO2008] JHHMMSS.s+DDMMSS> * in Simbad); * 4 = Sacco et al. (2008, Cat. J/A+A/488/167; <[SFR2008] LNN> in Simbad); * 5 = Dolan & Mathieu (2001, Cat. J/AJ/121/2124); * 6 = Barrado y Navascues et al. (2007, Cat. J/ApJ/664/481); * 7 = Sacco et al. (2008, Cat. J/A+A/488/167). *Note (2): Membership flag as follows: * m1 = radial velocity members with LiI in absorption; * m2 = radial velocity members with no LiI information; * m3 = stars with LiI in absorption and radial velocity out of member range; * m4 = both spectral type and photometric data in agreement with cluster * sequence; * m5 = photometric members; * nm1 = non-members based on photometric analysis; * nm2 = non-members based in spectroscopic analysis. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Photometric candidates of the {lambda} Orionis Cluster integer*4 nr__1 parameter (nr__1=436) ! Number of records character*122 ar__1 ! Full-size record C J2000 position composed of: RAdeg DEdeg integer*4 ID_1 ! [30/7968] Identification number character*16 v2MASS ! 2MASS identification number real*8 RAdeg_1 ! (deg) Right Ascension in decimal degrees (J2000) real*8 DEdeg_1 ! (deg) Declination in decimal degrees (J2000) real*4 v_3_6_ ! (mag) Spitzer/IRAC 3.6 micron band magnitude real*4 e__3_6_ ! (mag) Uncertainty in [3.6] real*4 v_4_5_ ! (mag) Spitzer/IRAC 4.5 micron band magnitude real*4 e__4_5_ ! (mag) Uncertainty in [4.5] real*4 v_5_8_ ! (mag) ?=100 Spitzer/IRAC 5.8 micron band magnitude real*4 e__5_8_ ! (mag) ?=99.99 Uncertainty in [5.8] real*4 v_8_0_ ! (mag) ?=100 Spitzer/IRAC 8.0 micron band magnitude real*4 e__8_0_ ! (mag) ?=100 Uncertainty in [8.0] real*4 F24 ! (mJy) ? Spitzer/MIPS 24 micron flux density real*4 e_F24 ! (mJy) ? Uncertainty in F24 character*8 DType ! Disk type (1) character*3 f_DType ! Flag(s) on DType (2) character*9 Memb_1 ! Membership details (G1) *Note (1): Disk type as follows: * Thk = star with an optically thick disk; * TD = transitional disk candidate; * PTD = pre transitional disk candidate; * EV = star with an evolved (flat) disk; * diskless = star with no infrared excesses. *Note (2): Flag as follows: * 1 = stars with uncertain 24 micron excess. * 2 = stars with uncertain 8 micron excess. * 3 = stars without 24 micron counterpart. * 4 = Faint stars with not reliable excesses at 5.8 micron and 8.0 micron. * 5 = Star with moderate IR excess at 8.0 micron but the 24 micron flux is * consistent with the photospheric fluxes. * 6 = Classified as evolved disk star from the IRAC SED slope. * 7 = The star {lambda} Orionis may mask the detection at 24 micron. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Additional sources with infrared excesses integer*4 nr__2 parameter (nr__2=41) ! Number of records character*115 ar__2 ! Full-size record C J2000 position composed of: RAdeg DEdeg integer*4 ID_2 ! [241/7615] Identification number character*16 v2MASS_1 ! 2MASS identification (HHMMSSss+DDMMSSs) real*8 RAdeg_2 ! (deg) Right ascension in decimal degrees (J2000) real*8 DEdeg_2 ! (deg) Declination in decimal degrees (J2000) real*4 v_3_6__1 ! (mag) Spitzer/IRAC 3.6um band magnitude real*4 e__3_6__1 ! (mag) Uncertainty in [3.6] real*4 v_4_5__1 ! (mag) Spitzer/IRAC 4.5um band magnitude real*4 e__4_5__1 ! (mag) Uncertainty in [4.5] real*4 v_5_8__1 ! (mag) Spitzer/IRAC 5.8um band magnitude real*4 e__5_8__1 ! (mag) Uncertainty in [5.8] real*4 v_8_0__1 ! (mag) Spitzer/IRAC 8.0um band magnitude real*4 e__8_0__1 ! (mag) Uncertainty in [8.0] real*8 F24_1 ! (mJy) Spitzer/MIPS 24um flux density real*4 e_F24_1 ! (mJy) F24 uncertainty character*8 Comm ! Comment (Galaxy or Stellar?) C============================================================================= C Loading file 'table1.dat' ! Compiled membership information of the * {lambda} Orionis Cluster C Format for file interpretation 1 format( + I4,1X,F8.5,1X,F8.5,1X,A12,1X,A10,1X,A3,1X,F5.2,1X,F5.2,1X, + F5.2,1X,A5,1X,A3,1X,A3,1X,A11,1X,A3) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,205 read(1,'(A98)')ar__ read(ar__,1) + ID,RAdeg,DEdeg,Name,SpType,r_SpType,RV1,RV2,RV3,r_RV,LiI, + r_LiI,Memb,Mm if(ar__(52:56) .EQ. '') RV1 = rNULL__ if(ar__(58:62) .EQ. '') RV2 = rNULL__ if(ar__(64:68) .EQ. '') RV3 = rNULL__ c ..............Just test output........... write(6,1) + ID,RAdeg,DEdeg,Name,SpType,r_SpType,RV1,RV2,RV3,r_RV,LiI, + r_LiI,Memb,Mm c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table2.dat' ! Photometric candidates of the {lambda} Orionis * Cluster C Format for file interpretation 2 format( + I4,1X,A16,1X,F8.5,1X,F8.5,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X, + F6.2,1X,F5.2,1X,F6.2,1X,F6.2,1X,F5.2,1X,F4.2,1X,A8,1X,A3,1X,A9) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,436 read(1,'(A122)')ar__1 read(ar__1,2) + ID_1,v2MASS,RAdeg_1,DEdeg_1,v_3_6_,e__3_6_,v_4_5_,e__4_5_, + v_5_8_,e__5_8_,v_8_0_,e__8_0_,F24,e_F24,DType,f_DType,Memb_1 if(ar__1(90:94) .EQ. '') F24 = rNULL__ if(ar__1(96:99) .EQ. '') e_F24 = rNULL__ c ..............Just test output........... write(6,2) + ID_1,v2MASS,RAdeg_1,DEdeg_1,v_3_6_,e__3_6_,v_4_5_,e__4_5_, + v_5_8_,e__5_8_,v_8_0_,e__8_0_,F24,e_F24,DType,f_DType,Memb_1 c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table3.dat' ! Additional sources with infrared excesses C Format for file interpretation 3 format( + I4,1X,A16,1X,F8.5,1X,F8.5,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X, + F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F7.2,1X,F6.2,1X,A8) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,41 read(1,'(A115)')ar__2 read(ar__2,3) + ID_2,v2MASS_1,RAdeg_2,DEdeg_2,v_3_6__1,e__3_6__1,v_4_5__1, + e__4_5__1,v_5_8__1,e__5_8__1,v_8_0__1,e__8_0__1,F24_1,e_F24_1, + Comm c ..............Just test output........... write(6,3) + ID_2,v2MASS_1,RAdeg_2,DEdeg_2,v_3_6__1,e__3_6__1,v_4_5__1, + e__4_5__1,v_5_8__1,e__5_8__1,v_8_0__1,e__8_0__1,F24_1,e_F24_1, + Comm c .......End.of.Just test output........... end do close(1) C============================================================================= stop end