Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/496/153 into FORTRAN code for loading all data files into arrays.
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-28 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/A+A/496/153 Molecular hydrogen flows along Ori A cloud (Davis+, 2009) *================================================================================ *A census of molecular hydrogen outflows and their sources along the Orion A *molecular ridge. Characteristics and overall distribution. * Davis C.J., Froebrich D., Stanke T., Megeath S.T., Kumar M.S.N., * Adamson A., Eisloeffel J., Gredel R., Khanzadyan T., Lucas P., Smith M.D., * Varricatt W.P. * <Astron. Astrophys., 496, 153-176 (2009)> * =2009A&A...496..153D C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! H2 jets and outflows in Orion A, from the catalogue of Stanke et al., 2002, Cat. J/A+A/392/239 integer*4 nr__ parameter (nr__=73) ! Number of records character*134 ar__ ! Full-size record C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg (nr__) ! (deg) Right Ascension J2000 real*8 DEdeg (nr__) ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) integer*4 SMZ (nr__) ! Sequential number integer*4 SMZ2 (nr__) ! ? Second SMZ number when association integer*4 RAh (nr__) ! (h) Right ascension (J2000) (1) integer*4 RAm (nr__) ! (min) Right ascension (J2000) (1) real*4 RAs (nr__) ! (s) Right ascension (J2000) (1) character*1 DE_ (nr__) ! Declination sign (J2000) (1) integer*4 DEd (nr__) ! (deg) Declination (J2000) (1) integer*4 DEm (nr__) ! (arcmin) Declination (J2000) (1) integer*4 DEs (nr__) ! (arcsec) Declination (J2000) (1) character*1 n_DEs (nr__) ! [)] ) if position of the brightest knot in * the flow (1) character*11 Outflow (nr__) ! Outflow source name (2) real*4 alpha (nr__) ! ? Spectral index of Outflow (2) character*15 N850 (nr__) ! 850um dust core coincident with the * H_2_ outflow source (3) integer*4 a850 (nr__) ! (arcsec) ? Major axis of the core size at 850um (3) integer*4 b850 (nr__) ! (arcsec) ? Minor axis of the core size at 850um (3) real*4 I850 (nr__) ! (Jy) ? Integrated flux at 850um (3) real*4 F850 (nr__) ! (Jy) ? Flux at 850um (in Jy/beam) (3) character*11 N1200 (nr__) ! 1200um dust core coincident with the * H_2_ outflow source (4) integer*4 a1200 (nr__) ! (arcsec) ? Major axis of the core size at 1200um (4) integer*4 b1200 (nr__) ! (arcsec) ? Minor axis of the core size at 1200um (4) integer*4 O1200 (nr__) ! (deg) ? Orientation of the core major axis real*4 I1200 (nr__) ! (Jy) ? Integrated flux at 1200um (4) real*4 F1200 (nr__) ! (Jy) ? Flux at 1200um (in Jy/beam) (4) character*1 l_L (nr__) ! [~>] Limit flag on L real*4 L (nr__) ! (arcmin) ? Entire length (5) integer*4 theta (nr__) ! (deg) ? Opening angle measured from a cone centred * on the outflow source that includes all * H_2_ features in the flow character*1 l_PA (nr__) ! [~] Limit flag on PA integer*4 PA (nr__) ! (deg) ? Position angle measured east of north character*8 HH (nr__) ! Associated HH objects, if any are known *Note (1): Position of the H_2_ outflow source if one is listed in "Outflow" * column. Otherwise, the position of the brightest knot in the flow is * given (bracket). Note that the well-known sources of the HH 1/2, HH 83 * and V380-Ori-NE flows were not identified in our tables of Spitzer * protostars or disc-excess sources. *Note (2): Most likely H_2_ outflow source from the Spitzer photometry * together with the spectral index, {alpha}. Just a question mark means * there is no obvious H_2_ flow source candidate. *Note (3): 850um dust core coincident with the H_2_ outflow source (from * Nutter & Ward-Thompson, 2007, Cat. J/MNRAS/374/1413). The source must * lie within a 14" radius (the JCMT beam at 850um) of the core position * given by Nutter & Ward-Thompson in their Table A.1. "Emission" or * "undetected" means that no core appears in their table. However, * "emission" means that the source identified in Col. "Outflow" is * associated with diffuse 850um emission (surface brightness * >100mJy/beam, which is roughly equivalent to 5{sigma}); a question * mark means there are cores (or emission) in the vicinity which could * be associated with the outflow or its source; "no obs" means that the * outflow is outside the bounds of the SCUBA map. The flux is measured * towards each IRS source (not necessarily the peak flux of the * associated core). *Note (4): Same as for the 850um cores, but for cores identified from our * analysis of the 1200 observations of Stanke et al. (in prep.). In this * case the source must lie within 11" of the core centroid; "emission" * corresponds to a surface brightness >75mJy/beam^-1^ (~5{sigma}). *Note (5): Entire length of all H_2_ knots (in both lobes), or the distance * from the source to the most distant H_2_ knot if only one flow lobe is * identified c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! New H2 jets in Orion A (additions to the catalogue of Stanke et al., 2002, Cat. J/A+A/392/239) integer*4 nr__1 parameter (nr__1=43) ! Number of records character*134 ar__1 ! Full-size record C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000 real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) integer*4 SMZ_1 (nr__1) ! Sequential number integer*4 SMZ2_1 (nr__1) ! ? Second SMZ number when association integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000) (1) integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000) (1) real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000) (1) character*1 DE__1 (nr__1) ! Declination sign (J2000) (1) integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000) (1) integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000) (1) integer*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000) (1) character*1 n_DEs_1 (nr__1) ! [)] ) if position of the brightest knot in * the flow (1) character*11 Outflow_1 (nr__1) ! Outflow source name (2) real*4 alpha_1 (nr__1) ! ? Spectral index of Outflow (2) character*15 N850_1 (nr__1) ! 850um dust core coincident with the * H_2_ outflow source (3) integer*4 a850_1 (nr__1) ! (arcsec) ? Major axis of the core size at 850um (3) integer*4 b850_1 (nr__1) ! (arcsec) ? Minor axis of the core size at 850um (3) real*4 I850_1 (nr__1) ! (Jy) ? Integrated flux at 850um (3) real*4 F850_1 (nr__1) ! (Jy) ? Flux at 850um (in Jy/beam) (3) character*11 N1200_1 (nr__1) ! 1200um dust core coincident with the * H_2_ outflow source (4) integer*4 a1200_1 (nr__1) ! (arcsec) ? Major axis of the core size at 1200um (4) integer*4 b1200_1 (nr__1) ! (arcsec) ? Minor axis of the core size at 1200um (4) integer*4 O1200_1 (nr__1) ! (deg) ? Orientation of the core major axis real*4 I1200_1 (nr__1) ! (Jy) ? Integrated flux at 1200um (4) real*4 F1200_1 (nr__1) ! (Jy) ? Flux at 1200um (in Jy/beam) (4) character*1 l_L_1 (nr__1) ! [~>] Limit flag on L real*4 L_1 (nr__1) ! (arcmin) ? Entire length (5) integer*4 theta_1 (nr__1) ! (deg) ? Opening angle measured from a cone centred * on the outflow source that includes all * H_2_ features in the flow character*1 l_PA_1 (nr__1) ! [~] Limit flag on PA integer*4 PA_1 (nr__1) ! (deg) ? Position angle measured east of north character*8 HH_1 (nr__1) ! Associated HH objects, if any are known *Note (1): Position of the H_2_ outflow source if one is listed in "Outflow" * column. Otherwise, the position of the brightest knot in the flow is * given (bracket). Note that the well-known sources of the HH 1/2, HH 83 * and V380-Ori-NE flows were not identified in our tables of Spitzer * protostars or disc-excess sources. *Note (2): Most likely H_2_ outflow source from the Spitzer photometry * together with the spectral index, {alpha}. Just a question mark means * there is no obvious H_2_ flow source candidate. *Note (3): 850um dust core coincident with the H_2_ outflow source (from * Nutter & Ward-Thompson, 2007, Cat. J/MNRAS/374/1413). The source must * lie within a 14" radius (the JCMT beam at 850um) of the core position * given by Nutter & Ward-Thompson in their Table A.1. "Emission" or * "undetected" means that no core appears in their table. However, * "emission" means that the source identified in Col. "Outflow" is * associated with diffuse 850um emission (surface brightness * >100mJy/beam, which is roughly equivalent to 5{sigma}); a question * mark means there are cores (or emission) in the vicinity which could * be associated with the outflow or its source; "no obs" means that the * outflow is outside the bounds of the SCUBA map. The flux is measured * towards each IRS source (not necessarily the peak flux of the * associated core). *Note (4): Same as for the 850um cores, but for cores identified from our * analysis of the 1200 observations of Stanke et al. (in prep.). In this * case the source must lie within 11" of the core centroid; "emission" * corresponds to a surface brightness >75mJy/beam^-1^ (~5{sigma}). *Note (5): Entire length of all H_2_ knots (in both lobes), or the distance * from the source to the most distant H_2_ knot if only one flow lobe is * identified c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tableb1.dat' ! Proper motions of H2 features integer*4 nr__2 parameter (nr__2=147) ! Number of records character*76 ar__2 ! Full-size record C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000 real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) integer*4 SMZ_2 (nr__2) ! Sequential number integer*4 SMZ2_2 (nr__2) ! ? Second SMZ number when association character*1 n_SMZ2 (nr__2) ! [*] Note (1) character*7 Knot (nr__2) ! Knot designation integer*4 RAh_2 (nr__2) ! (h) Right ascension (J2000) integer*4 RAm_2 (nr__2) ! (min) Right ascension (J2000) real*4 RAs_2 (nr__2) ! (s) Right ascension (J2000) character*1 DE__2 (nr__2) ! Declination sign (J2000) integer*4 DEd_2 (nr__2) ! (deg) Declination (J2000) integer*4 DEm_2 (nr__2) ! (arcmin) Declination (J2000) integer*4 DEs_2 (nr__2) ! (arcsec) Declination (J2000) real*4 shift_x (nr__2) ! (pix) Shift along x axis real*4 shift_y (nr__2) ! (pix) Shift along y axis real*4 shiftpix (nr__2) ! (pix) Total shift in pixel real*4 shift (nr__2) ! (arcsec) Total shift in arcsec real*4 Vel (nr__2) ! (km/s) Tangential velocity (2) real*4 Position (nr__2) ! (deg) Angle of the PM vector, measured E of N integer*4 Flag (nr__2) ! Status Flag. Those with value 2 are uncertain *Note (1): In these objects clusters of knots are labelled A, B, etc., with * the individual knots themselves labelled A1, A2, etc. and B1, B2, etc. * The PM of 5-23 G, for example, is for all knots G1-G5 measured together. *Note (2): A nominal error of 21km/s has been adopted (see text for details). C============================================================================= C Loading file 'table2.dat' ! H2 jets and outflows in Orion A, from the catalogue * of Stanke et al., 2002, Cat. J/A+A/392/239 C Format for file interpretation 1 format( + I3,1X,I3,1X,I1,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,I2,A1,1X,A11, + 1X,F5.2,1X,A15,2X,I2,1X,I2,1X,F4.1,1X,F4.2,1X,A11,I3,1X,I2,1X, + I3,1X,F4.2,1X,F4.2,1X,A1,F5.2,1X,I2,1X,A1,I3,1X,A8) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,73 read(1,'(A134)')ar__ read(ar__,1) + SMZ(i__),SMZ2(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),n_DEs(i__),Outflow(i__),alpha(i__), + N850(i__),a850(i__),b850(i__),I850(i__),F850(i__),N1200(i__), + a1200(i__),b1200(i__),O1200(i__),I1200(i__),F1200(i__), + l_L(i__),L(i__),theta(i__),l_PA(i__),PA(i__),HH(i__) if(ar__(5:7) .EQ. '') SMZ2(i__) = iNULL__ if(ar__(41:45) .EQ. '') alpha(i__) = rNULL__ if(ar__(64:65) .EQ. '') a850(i__) = iNULL__ if(ar__(67:68) .EQ. '') b850(i__) = iNULL__ if(ar__(70:73) .EQ. '') I850(i__) = rNULL__ if(ar__(75:78) .EQ. '') F850(i__) = rNULL__ if(ar__(91:93) .EQ. '') a1200(i__) = iNULL__ if(ar__(95:96) .EQ. '') b1200(i__) = iNULL__ if(ar__(98:100) .EQ. '') O1200(i__) = iNULL__ if(ar__(102:105) .EQ. '') I1200(i__) = rNULL__ if(ar__(107:110) .EQ. '') F1200(i__) = rNULL__ if(ar__(113:117) .EQ. '') L(i__) = rNULL__ if(ar__(119:120) .EQ. '') theta(i__) = iNULL__ if(ar__(123:125) .EQ. '') PA(i__) = iNULL__ RAdeg(i__) = rNULL__ DEdeg(i__) = rNULL__ c Derive coordinates RAdeg and DEdeg from input data c (RAdeg and DEdeg are set to rNULL__ when unknown) if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15. if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4. if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240. if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__) if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60. if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600. if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__) c ..............Just test output........... write(6,1) + SMZ(i__),SMZ2(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),n_DEs(i__),Outflow(i__),alpha(i__), + N850(i__),a850(i__),b850(i__),I850(i__),F850(i__),N1200(i__), + a1200(i__),b1200(i__),O1200(i__),I1200(i__),F1200(i__), + l_L(i__),L(i__),theta(i__),l_PA(i__),PA(i__),HH(i__) write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table3.dat' ! New H2 jets in Orion A (additions to the catalogue * of Stanke et al., 2002, Cat. J/A+A/392/239) C Format for file interpretation 2 format( + I3,1X,I3,1X,I1,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,I2,A1,1X,A11, + 1X,F5.2,1X,A15,2X,I2,1X,I2,1X,F4.1,1X,F4.2,1X,A11,I3,1X,I2,1X, + I3,1X,F4.2,1X,F4.2,1X,A1,F5.2,1X,I2,1X,A1,I3,1X,A8) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,43 read(1,'(A134)')ar__1 read(ar__1,2) + SMZ_1(i__),SMZ2_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__), + DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),n_DEs_1(i__), + Outflow_1(i__),alpha_1(i__),N850_1(i__),a850_1(i__), + b850_1(i__),I850_1(i__),F850_1(i__),N1200_1(i__),a1200_1(i__), + b1200_1(i__),O1200_1(i__),I1200_1(i__),F1200_1(i__), + l_L_1(i__),L_1(i__),theta_1(i__),l_PA_1(i__),PA_1(i__), + HH_1(i__) if(ar__1(5:7) .EQ. '') SMZ2_1(i__) = iNULL__ if(ar__1(41:45) .EQ. '') alpha_1(i__) = rNULL__ if(ar__1(64:65) .EQ. '') a850_1(i__) = iNULL__ if(ar__1(67:68) .EQ. '') b850_1(i__) = iNULL__ if(ar__1(70:73) .EQ. '') I850_1(i__) = rNULL__ if(ar__1(75:78) .EQ. '') F850_1(i__) = rNULL__ if(ar__1(91:93) .EQ. '') a1200_1(i__) = iNULL__ if(ar__1(95:96) .EQ. '') b1200_1(i__) = iNULL__ if(ar__1(98:100) .EQ. '') O1200_1(i__) = iNULL__ if(ar__1(102:105) .EQ. '') I1200_1(i__) = rNULL__ if(ar__1(107:110) .EQ. '') F1200_1(i__) = rNULL__ if(ar__1(113:117) .EQ. '') L_1(i__) = rNULL__ if(ar__1(119:120) .EQ. '') theta_1(i__) = iNULL__ if(ar__1(123:125) .EQ. '') PA_1(i__) = iNULL__ RAdeg_1(i__) = rNULL__ DEdeg_1(i__) = rNULL__ c Derive coordinates RAdeg_1 and DEdeg_1 from input data c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown) if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15. if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4. if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240. if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__) if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60. if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600. if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__) c ..............Just test output........... write(6,2) + SMZ_1(i__),SMZ2_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__), + DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),n_DEs_1(i__), + Outflow_1(i__),alpha_1(i__),N850_1(i__),a850_1(i__), + b850_1(i__),I850_1(i__),F850_1(i__),N1200_1(i__),a1200_1(i__), + b1200_1(i__),O1200_1(i__),I1200_1(i__),F1200_1(i__), + l_L_1(i__),L_1(i__),theta_1(i__),l_PA_1(i__),PA_1(i__), + HH_1(i__) write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'tableb1.dat' ! Proper motions of H2 features C Format for file interpretation 3 format( + I3,1X,I3,A1,2X,A7,2X,I1,1X,I2,1X,F4.1,1X,A1,I1,1X,I2,1X,I2,1X, + F6.3,1X,F6.3,1X,F4.2,1X,F4.2,1X,F5.1,1X,F6.1,1X,I1) C Effective file loading open(unit=1,status='old',file= +'tableb1.dat') write(6,*) '....Loading file: tableb1.dat' do i__=1,147 read(1,'(A76)')ar__2 read(ar__2,3) + SMZ_2(i__),SMZ2_2(i__),n_SMZ2(i__),Knot(i__),RAh_2(i__), + RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__), + DEs_2(i__),shift_x(i__),shift_y(i__),shiftpix(i__),shift(i__), + Vel(i__),Position(i__),Flag(i__) if(ar__2(5:7) .EQ. '') SMZ2_2(i__) = iNULL__ RAdeg_2(i__) = rNULL__ DEdeg_2(i__) = rNULL__ c Derive coordinates RAdeg_2 and DEdeg_2 from input data c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown) if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15. if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4. if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240. if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__) if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60. if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600. if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__) c ..............Just test output........... write(6,3) + SMZ_2(i__),SMZ2_2(i__),n_SMZ2(i__),Knot(i__),RAh_2(i__), + RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__), + DEs_2(i__),shift_x(i__),shift_y(i__),shiftpix(i__),shift(i__), + Vel(i__),Position(i__),Flag(i__) write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end