Conversion of standardized ReadMe file for
file /./ftp/cats/III/227 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.
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 2017-Nov-17 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. III/227 General Catalog of galactic Carbon stars, 3d Ed. (Alksnis+ 2001) *================================================================================ *A general catalogue of galactic carbon stars by C.B. Stephenson. Third edition. * Alksnis A., Balklavs A., Dzervitis U., Eglitis I., Paupers O., Pundure I. * <Baltic Astronomy, 10, 1 (2001)> * =2001BaltA..10....1A C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'catalog.dat' ! General catalogue of galactic carbon stars integer*4 nr__ parameter (nr__=6891) ! Number of records character*137 ar__ ! Full-size record C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0 real*8 DEdeg (nr__) ! (deg) Declination J2000.0 C ---------------------------------- ! (position vector(s) in degrees) character*9 Jname (nr__) ! Star designation (based on J2000 position) integer*4 CGCS (nr__) ! CGCS number (1) integer*4 RAh (nr__) ! (h) Right ascension (J2000.0) (2) integer*4 RAm (nr__) ! (min) Right ascension J2000.0) real*4 RAs (nr__) ! (s) Right ascension J2000.0) character*1 DE_ (nr__) ! [-+] Declination sign integer*4 DEd (nr__) ! (deg) Declination J2000.0) integer*4 DEm (nr__) ! (arcmin) Declination J2000.0) integer*4 DEs (nr__) ! (arcsec) Declination J2000.0) character*1 l_Bmag (nr__) ! [<] limit flag on B real*4 Bmag (nr__) ! (mag) ? B magnitude (3) character*1 u_Bmag (nr__) ! [:] uncertainty flag on B real*4 Vmag (nr__) ! (mag) ? V magnitude (4) character*1 u_Vmag (nr__) ! [:] uncertainty flag on V real*4 irmag (nr__) ! (mag) ? red or near-IR magnitude (5) character*1 n_irmag (nr__) ! [rRJHKL ] IR band character*1 u_irmag (nr__) ! [:] uncertainty flag on ir real*4 GLON (nr__) ! (deg) Galactic longitude real*4 GLAT (nr__) ! (deg) Galactic latitude character*18 Sp (nr__) ! ? Spectral type (6) character*34 Names (nr__) ! Designations (7) character*8 Notes (nr__) ! ? Notes (8) integer*4 Pr (nr__) ! ? Precision class of the coordinates (9) *Note (1): This is the number from the first column of the catalog from the * 2nd edition (CGCCS, Cat. <III/156>). We have not introduced a new * running number to avoid overcrowding of identifiers for an object. For * new entries the running numbers begin with No. 6001 and are given in * the sequence of R.A. (J2000). *Note (2): * In case of multiple finding lists, the coordinates are averages from * multiple sources, heavily weighted in favour of the most accurate, if * any. When Ste (for Stephenson) is included among the designations, * the star has almost invariably been measured for position at the * Warner and Swasey Obs. on one or even more objective-prism plates, * with a resulting precision of 1-2". The astrometric reduction * procedure used by Stephenson is explained in Publs. Warner and Swasey * Obs. Vol. 2, No. 4, Sec. II. More than 2000 stars of the catalog have * post CCCS position determinations done at the Warner and Swasey * Observatory. * * The coordinates are given to 0.1 sec in RA and 1 arcsec in DEC, * notwithstanding the precision class of the position of the object. * The estimated precision of the coordinates is indicated in the last * column. For many stars of CGCCS the equatorial coordinates have been * improved on the basis of new determinations, e.g., by Aaronson et al. * (1989ApJS...70..637A, 1990ApJS...73..841A), MacConnell (2000, Priv. * Comm.), Maehara & Soyano (1988AnTok..22...59M, 1990PNAOJ...1..207M), * Soyano & Maehara (1991PNAOJ...2..203M, 1993PNAOJ...3..259S, * 1999PNAOJ...5..149S). * * For more than 300 carbon stars equatorial coordinates were taken from * the Hipparcos Catalogue (<I/239>) after approximation to the format of * this catalog. These stars can be recognized as bright stars with the * highest precision class 0 in the last column of the catalog. *Note (3): * B magnitudes essentially all come from photographic plates; thousands * of them are based only upon an average plate calibration used for an * entire survey. Thus the magnitudes are almost never accurate to 0.1 * mag, to which they are commonly given, and errors of over a whole * magnitude should be common, even discounting variability. *Note (4): * V magnitudes essentially all come from photographic plates; For some * stars V magnitudes from Paupers et al. (1993BaltA...2..268P) are used. *Note (5): * The infrared magnitudes are normally the sort defined by a Kodak * N-type photographic plate exposed through a filter similar to the * Schott RG8 or 695 filter. Such infrared magnitudes are close to the * system of Kron & Smith (1951ApJ...113..324K), and have now been * published for several thousand carbon stars. *Note (6): * This column displays the earliest more reliable determinations of * spectral type in the R/N notation. Here also are classifications in * the scheme of Morgan & Keenan (1941ApJ....94..501K); this scheme is * still a good compact description of the spectrum. Sources of quoted * classifications are coded here in parentheses. * * Below we list abbreviations for papers consisting mainly of * reobservation of stars selected from finding lists: * * Bidun Bidelman, unpublished. * De Dean (1976AJ.....81..364D). * HD, HDE Henry Draper Catalogue and the extensions (Cat. <III/135>). * The second extension, HA 112, is cited as CannMay49.. * Her52 Herbig (1952, Trans. I.A.U., Vol. 8, 807). * IRAS C Little-Marenin et al. (1987AJ.....93..663L) * K-M Keenan & Morgan (1941ApJ....94..501K) * Lund21 Lundmark (1921PASP...33..314). * San41 Sanford (1941PASP...53..291S). * San Sanford (1944ApJ....99..145S). * Sh Shane (1928, Bull. Lick Obs., 13, 123). * War Warner (1963MNRAS.126...61W). * WPB Bidelman (1954ApJS....1..175B). * Yam Yamashita (1972AnTok..13..169Y, 1975AnTok..15...47Y). * * Carbon star candidates in this column are marked by lower case c * (Guglielmo et al., 1998A&A...334..609G and references therein). *Note (7): * This column gives the star's occurence in various finding lists, * including unpublished ones. Some CCCS stars repeated here are still * called unpublished, which means only that I had no reference to a * separate publication when the CCCS went to press. For some of those * stars, the CCCS is the only place they have been published; for * others, they have since appeared in separate lists by their * discoverers. In the latter case I have sometimes changed the * discoverer designation to reflect separate subsequent publication, and * sometimes not; in the great majority of cases, CCCS stars there called * unpublished have since been confirmed in other surveys. * * There are finding lists with no special concentration on carbon stars. * These are the Bright Star Catalog number, cited, as in all editions of * the Bright Star Catalog, as an HR number (and usually put at the head * of the list); HD or HDE numbers (listed as a number without other * characters); BD or CD numbers in a notation close to the usual one; * and the GCVS designation. The intent was to give CD numbers only if * the CD magnitude is 9.5 or brighter. Any CPD (Cape Photographic * Durchmusterung) nos. in the catalog are inadvertent unless spelled out * as such, a fact due to the circumstance that carbon stars are red * stars and the CD is red-biased, not only relative to the CPD but even, * though this does not appear to be widely known, relative to the BD. * * Other finding lists: an explanation for the coding of these are in the * "lists.dat" file. The largest unpublished lists are by Stephenson * (Ste), a combination of stars now published in the CCCS and infrared * survey products appearing in the present catalog; Sanduleak (Sndlk), * whose entries are almost exclusively confined to CCCS stars; Victor * Blanco (VB); and MacConnell (MacCon). Although there are several * published MacConnell lists cited here, some of the MacCons may have * since become separately published; but see also the special nope unfeb * MacCon in the lists.dat file. * * Coding: Whenever a number appears separated from the initial part of * the designation by a blank space, the number is a published one * assigned by the corresponding discoverer, hyphens if any separating * table numbers from numbers within tables. Numbers following alphabetic * abbreviations without a blank space represent the year of publication * where this was for some reason helpful to me (generally, where the * same author has produced more than one paper). So "Kurt88 4" means * star No. 4 in a table of carbon stars in Westerlund (1988, * Astrofizika, 29, 405). * * The meaning of the abbreviations are in the "lists.dat" file. * Here some comments on some abbreviations: * * D : The Dearborn Observatory objective-prism surveys for red stars. * The carbon stars thus found were abstracted as lists of * exclusively carbon stars, in the papers just cited, and were * duplicated in longer lists containing all red stars found; the * D numbers given in the catalog refer to the short lists, with one * or two exceptions spelled out in the notes to the table. * * The notes also refer in other contexts to the "longer" Dearborn * lists, with the meaning just explained. The "short" list numbers * for carbon stars are continuous from paper to paper. * * Hen : Rybski (1972, unpublished). Most of the carbon stars discussed by * Rybski were found on objective-prism plates by Henize, and by * him assigned the numbers which Rybski refers to as Hen numbers * and Stephenson quote in the catalog. There is no connection between * these Hen numbers and others occurring in the literature -- even * in the case of the occasional Hen numbers for carbon stars cited * by Wray (1966, unpublished), who however, also assigns his own * numbers and which are quoted in the catalog as Wray. * * Krum : L.E. Krumenaker, unpublished. At Warner and Swasey we had by 1972 * taken duplicate objective-prism plates of the northern Milky Way * for about half of the fields surveyed by Hamburg in the * Hamburg-Cleveland survey for luminous stars in the Northern * Milky Way. Although carbon stars were identified and measured * for position by the Hamburg workers, and eventually published * (Hardorp et al., 1973A&A....22..129H), the Hamburg limiting * magnitude for carbon stars was not very faint (cf. Hardorp et * al., 1973A&A....22..129H ). Hence Krumenaker searched for carbon * stars on the new Case material already mentioned. On the other * hand, the mag. limit for R/N classification is already fairly * uniform between Hamburg and Cleveland (Stephenson, * 1989PW&SO...3...53S). * * Kub : W.R. Kubinec, unpublished. These carbon stars are discussed by * Kbinec, without position data, in 1989PW&SO...3...53S. He * measured the approximate positions specially for the catalog. * * NassCol : The numerical C types quoted from this paper are defined in the * paper; they essentially describe the CN strength, and the * redness, of the spectrum in the infrared. *Note (8): * Four symbols were introduced in the CCCS and are retained here: * * (1) An asterisk indicates that the catalog equates two or more data in * literal contradiction to one or more papers cited; for example, a much * later paper may be reporting a new carbon star already so identified * in a much earlier paper, which implies that perhaps there are two * carbon stars in the area. This was a natural flag to use in the CCCS, * where carbon stars were mainly reported in a few large and well-known * surveys. It is no longer natural now, where the main pre-publication * comparison has been with the CCCS, and there have meanwhile been many * relatively short lists. Thus, I have added few if any new asterisks. * Finally, a single asterisk meant that my fusing of two or more reports * was based on coordinates alone, without any plate re-examination. In * fact, many or most of these cases have now been routinely re-examined * through later, systematic, surveys; but I have retained the asterisk * to show the historical order. * * (2) A double asterisk means the same as a single one, except that I have * specially re-examined plates with the identification problem in mind. * As in (1), many of these have been further checked routinely by later, * systematic surveys, where the finding of only one star allows the * strong presumption that only one carbon star is involved. There are * few or no new double asterisks in the present edition. * * (3) A plus sign signals a GCVS identification made by me by comparing an * objective prism plate with a published identification chart. These, * too, are mostly holdovers from the CCCS, because the host of more * accurate coordinates for carbon stars in the present edition usually * restricts any challenge to identifying a carbon star with a GCVS * cool-giant variability type to the question (at least on deep plates): * is there any other banded spectrum near the carbon star? * * (4) An R signals further remarks at the end of the catalog. * * The object of the remarks is twofold. First, remarks are intended as * an extension to the entries Designations and Spectrum of the catalog * comprising matter for which there was no place in the catalog. Second, * remarks contain information about considerable disagreement in the * position of a star determined by different authors or cases when there * is some doubt if the data refer to the same star. We repeat * Stephenson's remarks, although in a shortened form, in which he * confirms discoveries or points to certain spectral and photometric * peculiarities (outstanding spectral lines and bands, very red color * etc.). Also we indicate the cases when a carbon star lies in the sky * within boundaries of some star clusters and note conclusions about the * membership, if possible. Also the stars with such distinguishing * features as circumstellar silicate envelopes, detached gas and dust * shells, maser emission, binarity and bipolar molecular outflows are * marked. *Note (9): * Estimated precision class of the equatorial coordinates of the star: * 0-1 for +/-0.1 arcsec, * 2 for +/-1 arcsec, * 3 for +/-0.1 arcmin. * Values of the precision class have been estimated by comparing * coordinates of the stars determined by different authors. The highest * precision class 0 was assigned only to the positions determined by * Hipparcos, by MacConnell (2000, Priv. Comm) and for dwarf carbon stars. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'remarks.dat' ! Individual remarks integer*4 nr__1 parameter (nr__1=1867) ! Number of records character*80 ar__1 ! Full-size record character*9 Jname_1 (nr__1) ! Star designation (based on J2000 position) integer*4 CGCS_1 (nr__1) ! CGCS number, as in catalog.dat file character*64 Rem (nr__1) ! Text of the remark c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'lists.dat' ! Abbreviations and References integer*4 nr__2 parameter (nr__2=278) ! Number of records character*192 ar__2 ! Full-size record character*15 Code (nr__2) ! Reference list abbreviation, or blank character*19 BibCode (nr__2) ! BibCode character*25 Aut (nr__2) ! Author names character*130 Com (nr__2) ! Comments C============================================================================= C Loading file 'catalog.dat' ! General catalogue of galactic carbon stars C Format for file interpretation 1 format( + A9,2X,I4,2X,I2,1X,I2,1X,F4.1,2X,A1,I2,1X,I2,1X,I2,2X,A1,F4.1, + A1,2X,F4.1,A1,2X,F4.1,A1,A1,2X,F5.1,1X,F5.1,2X,A18,A34,A8,I1) C Effective file loading open(unit=1,status='old',file= +'catalog.dat') write(6,*) '....Loading file: catalog.dat' do i__=1,6891 read(1,'(A137)')ar__ read(ar__,1) + Jname(i__),CGCS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),l_Bmag(i__),Bmag(i__),u_Bmag(i__), + Vmag(i__),u_Vmag(i__),irmag(i__),n_irmag(i__),u_irmag(i__), + GLON(i__),GLAT(i__),Sp(i__),Names(i__),Notes(i__),Pr(i__) if(ar__(42:45) .EQ. '') Bmag(i__) = rNULL__ if(ar__(49:52) .EQ. '') Vmag(i__) = rNULL__ if(ar__(56:59) .EQ. '') irmag(i__) = rNULL__ if(ar__(137:137) .EQ. '') Pr(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) + Jname(i__),CGCS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),l_Bmag(i__),Bmag(i__),u_Bmag(i__), + Vmag(i__),u_Vmag(i__),irmag(i__),n_irmag(i__),u_irmag(i__), + GLON(i__),GLAT(i__),Sp(i__),Names(i__),Notes(i__),Pr(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 'remarks.dat' ! Individual remarks C Format for file interpretation 2 format(A9,2X,I4,1X,A64) C Effective file loading open(unit=1,status='old',file= +'remarks.dat') write(6,*) '....Loading file: remarks.dat' do i__=1,1867 read(1,'(A80)')ar__1 read(ar__1,2)Jname_1(i__),CGCS_1(i__),Rem(i__) c ..............Just test output........... write(6,2)Jname_1(i__),CGCS_1(i__),Rem(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'lists.dat' ! Abbreviations and References C Format for file interpretation 3 format(A15,1X,A19,1X,A25,1X,A130) C Effective file loading open(unit=1,status='old',file= +'lists.dat') write(6,*) '....Loading file: lists.dat' do i__=1,278 read(1,'(A192)')ar__2 read(ar__2,3)Code(i__),BibCode(i__),Aut(i__),Com(i__) c ..............Just test output........... write(6,3)Code(i__),BibCode(i__),Aut(i__),Com(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end