; ECANNED2.DAT ; ; This file contains format information for "canned" datasets already on ; the Guide CD-ROM. It is a supplement to ECANNED.DAT. For each ASCII ; dataset, it describes what data appears in the short "click" dialog box, ; and in the "more info" section. The method for this is exactly like ; that used in .TDF files. ; ; Comments can be inserted at any point, on lines starting with a ;. ; This file is called ECANNED2.DAT because it is the English-language version. ; The German-language version is DCANNED2.DAT; the French-language will be ; FCANNED2.DAT, and so forth. If Guide can't find such files, it ; will use ECANNED2.DAT. ; ; 18 Feb 2007: at suggestion of John Greaves, added links for GCVS ; and NSV data from the Sternberg Astronomical Institute. ; ~ngc_ic ~r 1 20 \nComments from the ^NGC-IC Project^:\n ~r 9 0 1 ^Galaxy^\n ~r 9 0 2 Galactic ^nebula^ or ^supernova^ remnant\n ~r 9 0 3 ^Planetary nebula^\n ~r 9 0 4 ^Open cluster^\n ~r 9 0 5 ^Globular cluster^\n ~r 9 0 6 Part of a ^galaxy^ (e.g., HII region)\n ~r 9 0 7 This object is a duplicate of one already in the NGC or IC\n ~r 9 0 8 This object is a duplicate of one already in the NGC\n ~r 9 0 9 Star(s)\n ~r 9 0 0 Not found\n ~r 63 6 Type: %s\n ~r 18 10 ^RA^: %s (^J2000^)\n ~r 29 9 ^declination^: %s\n ~r 41 4 ^Magnitude^: %s\n ~r 46 6 Major axis: %s ^arcminute^s\n ~r 52 6 Minor axis: %s\n ~r 59 3 ^Position angle^: %s\n ~r 13 3 ^Constellation^: %s\n ~r 73 5 ^PGC^ %s\n ~r 80 64 Alternative designations:\n%s\n end ; Starting with Guide 8, a new 'edition' of GCVS is used, and a lot of ; columns were rearranged for no good reason that I can see: ~gcvs4_guide8 ~r 9 9 ^Click here for SIMBAD data//xhttp://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=V* %s^\n ~r 9 6 ^Click here for an AAVSO light curve//xhttp://www.aavso.org/cgi-bin/superstar2.pl?objectname=%s%%20%[15,3]&lastdays=400&visual=on&fainter=on&ccdb=on&ccdv=on&ccdr=on&ccdi=on&ccdu=on&userpepv=on^\n ~r 9 6 ^Click here for AAVSO observation data//xhttp://www.aavso.org/cgi-bin/quickquick.pl?star=%s%%20%[15,3]^\n ~r 9 6 ^Click here for AAVSO charts//xhttp://www.aavso.org/cgi-bin/searchcharts3.pl?name=%s%%20%[15,3]^\n ~r 9 6 ^Click here for current GCVS data//xhttp://www.sai.msu.su/groups/cluster/gcvs/cgi-bin/search.cgi?search=%s+%[15,3]^\n ~r 36 0 : The ^RA^ is accurate to one second of time, and the declination\n ~r 36 0 : is accurate to one tenth of an ^arcminute^.\n ~r 36 0 * The declination is accurate to one ^arcminute^.\n ~r 36 0 ' The ^RA^ is accurate to one minute of time, and the declination\n ~r 36 0 ' is accurate to one ^arcminute^.\n ~r 86 2 ^Photometric band^: %s\n ~r 66 6 ^Maximum magnitude^: %s\n ~r 65 0 > (Above is a faint limit)\n ~r 65 0 < (Above is a bright limit)\n ~r 65 0 ( (Above is actually an amplitude)\n ~r 72 0 : (Maximum magnitude is uncertain)\n ~r 76 6 ^Minimum magnitude^: %s\n ~r 75 0 > (Above is a faint limit)\n ~r 75 0 < (Above is a bright limit)\n ~r 75 0 ( (Above is actually an amplitude)\n ~r 82 0 : (Minimum magnitude is uncertain)\n ~r 89 11 Epoch: ^JD^ 24%s\n ~r 89 11 (Be aware that epoch data from the ^GCVS^ dates back so far\n ~r 89 11 that, for present-day use, it is not all that useful.)\n ~r100 0 : (Epoch is uncertain)\n ~r100 0 + (Epoch may be later than that reported)\n ~r100 0 - (Epoch may be earlier than that reported)\n ~r102 4 Year of ^nova^ outburst: %s\n ~r109 16 Period of variation: %s days\n ~r108 0 > (Period is a lower limit)\n ~r108 0 < (Period is an upper limit)\n ~r108 0 ( (Period is the mean cycle time of a ^U Gem^ or ^repeating nova^)\n ~r135 17 ^Spectral type^: %s\n ~r153 11 References: %s\n ~r 38 2 ^J2000^ position: ^RA^ %sh ~r 40 2 %sm ~r 42 4 %ss, ~r 46 3 ^declination^ %s ~r 49 2 %s' ~r 51 2 %s"\n ~r 38 2 (In the current version of the GCVS, better-precision J2000\n ~r 38 2 positions are given for many stars. This may eventually extend\n ~r 38 2 to cover the rest of the catalogue.)\n end ; 6 Nov 2004: in the 'gcvs2004.dat' file, intended for use in ; Guide 9.0, some more columns are rearranged. Aside from the ; changed column numbers, what follows is exactly the same as the ; above 'gcvs4_guide8' data. ~gcvs2004 ~r 9 9 ^Click here for SIMBAD data//xhttp://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=V* %s^\n ~r 9 6 ^Click here for an AAVSO light curve//xhttp://www.aavso.org/cgi-bin/superstar2.pl?objectname=%s%%20%[15,3]&lastdays=400&visual=on&fainter=on&ccdb=on&ccdv=on&ccdr=on&ccdi=on&ccdu=on&userpepv=on^\n ~r 9 6 ^Click here for AAVSO observation data//xhttp://www.aavso.org/cgi-bin/quickquick.pl?star=%s%%20%[15,3]^\n ~r 9 6 ^Click here for AAVSO charts//xhttp://www.aavso.org/cgi-bin/searchcharts3.pl?name=%s%%20%[15,3]^\n ~r 9 6 ^Click here for current GCVS data//xhttp://www.sai.msu.su/groups/cluster/gcvs/cgi-bin/search.cgi?search=%s+%[15,3]^\n ~r 36 0 : The ^RA^ is accurate to one second of time, and the declination\n ~r 36 0 : is accurate to one tenth of an ^arcminute^.\n ~r 36 0 * The declination is accurate to one ^arcminute^.\n ~r 36 0 ' The ^RA^ is accurate to one minute of time, and the declination\n ~r 36 0 ' is accurate to one ^arcminute^.\n ~r 89 2 ^Photometric band^: %s\n ~r 67 6 ^Maximum magnitude^: %s\n ~r 66 0 > (Above is a faint limit)\n ~r 66 0 < (Above is a bright limit)\n ~r 66 0 ( (Above is actually an amplitude)\n ~r 73 0 : (Maximum magnitude is uncertain)\n ~r 78 6 ^Minimum magnitude^: %s\n ~r 76 0 > (Above is a faint limit)\n ~r 76 0 < (Above is a bright limit)\n ~r 76 0 ( (Above is actually an amplitude)\n ~r 84 0 : (Minimum magnitude is uncertain)\n ~r 92 11 Epoch: ^JD^ 24%s\n ~r 92 11 (Be aware that epoch data from the ^GCVS^ dates back so far\n ~r 92 11 that, for present-day use, it is not all that useful.)\n ~r104 0 : (Epoch is uncertain)\n ~r104 0 + (Epoch may be later than that reported)\n ~r104 0 - (Epoch may be earlier than that reported)\n ~r105 4 Year of ^nova^ outburst: %s\n ~r112 16 Period of variation: %s days\n ~r111 0 > (Period is a lower limit)\n ~r111 0 < (Period is an upper limit)\n ~r111 0 ( (Period is the mean cycle time of a ^U Gem^ or ^repeating nova^)\n ~r138 17 ^Spectral type^: %s\n ~r156 11 References: %s\n ~r 38 2 ^J2000^ position: ^RA^ %sh ~r 40 2 %sm ~r 42 4 %ss, ~r 46 3 ^declination^ %s ~r 49 2 %s' ~r 51 2 %s"\n ~r 38 2 (In the current version of the GCVS, better-precision J2000\n ~r 38 2 positions are given for many stars. This may eventually extend\n ~r 38 2 to cover the rest of the catalogue.)\n end ~nsv4_guide8 ~r 1 5 ^Click here for current GCVS data//xhttp://www.sai.msu.su/groups/cluster/gcvs/cgi-bin/search.cgi?search=NSV+%s^\n ~r 31 5 Maximum ^magnitude^: %s\n ~r 36 0 : (Above value is uncertain)\n ~r 40 5 Minimum ^magnitude^: %s\n ~r 39 0 < (Above value is an upper limit)\n ~r 39 0 > (Above value is a lower limit)\n ~r 39 0 ( (Above value is an amplitude)\n ~r 47 0 : (Above value is uncertain)\n ~r 49 1 ^Photometric band^: %s\n ~r 69 2 ^Spectral type^: %s\n end ~nsvs_guide8 ~r 1 5 ^Click here for current GCVS data//xhttp://www.sai.msu.su/groups/cluster/gcvs/cgi-bin/search.cgi?search=NSV+%s^\n ~r 48 7 Max Mag: %s\n ~r 54 0 : (The above maximum magnitude is uncertain.)\n ~r 56 0 ( Amplitude: ~r 56 0 Min magnitude: ~r 60 0 (no value listed) ~r 57 7 %s ~r 56 0 ( \n ~r 56 0 \n ~r 64 1 Photometric system for amplitudes: %s\n ~r 66 0 : Amplitude or minimum magnitude uncertain\n ~r 68 2 Photometric system for magnitudes and amplitudes: %s\n ~r 81 15 ^Spectral Type^: %s\n ~r 8 2 ^RA^ (^B1950^): %sh ~r 10 2 %sm ~r 12 4 %ss\n ~r 16 3 ^declination^: %s ~r 19 2 %s' ~r 21 2 %s"\n ~r 23 0 : The above RA is accurate to one second of time (15" at\n ~r 23 0 : the equator), the declination to .1 arcminute.\n ~r 23 0 * The above RA is accurate to one second of time (15" at\n ~r 23 0 * the equator), the declination to one arcminute.\n ~r 25 2 ^RA^ (^J2000^): %sh ~r 27 2 %sm ~r 29 4 %ss\n ~r 33 3 ^declination^: %s ~r 36 2 %s' ~r 38 2 %s"\n ~r 71 4 Reference for a study of the star (see refs.txt): %s\n ~r 76 4 Chart reference (see refs.txt): %s\n ~r 97 8 Spectral type from ^HD^ (Henry Draper) catalogue: %s\n ~r106 10 Designation in ^GCVS^: %s\n ~r 6 0 * \nNotes from NSVS Remark file:\n\n ~n 1 5 !:\variable\NSVS.not end ~sac_72 ~r 1 1 \nComments from ^SAC^ (Saguaro Astronomy Club) 7.2 database:\n ~r 1 18 %s\n ~r 19 19 %s\n ~r 38 5 Object type: %s\n ~r 44 3 ^Constellation^: %s\n ~r 48 7 ^RA^: %s (^J2000^)\n ~r 56 6 ^declination^: %s\n ~r 80 7 Size: %s ~r 89 7 x %s ~r 80 7 \n ~r 99 3 ^Position angle^: %s\n ~r103 11 Classification: %s\n ~r115 4 %s stars\n ~r121 4 Brightest star is of ^magnitude^ %s\n ~r131 47 %s\n ~r178 71 %s\n ~r 1 1 \n end ~pgc99 ~r 1 8 \nRemarks from the ^PGC^ (^Principal Galaxy Catalog^):\n ~r 1 11 %s\n ~r 13 25 %s\n ~r 38 0 * Coordinates have been determined to be accurate\n ~r 79 10 ^Galactic longitude^: %s\n ~r 89 10 ^Galactic latitude^: %s\n ~r 99 10 Supergalactic longitude: %s\n ~r109 10 Supergalactic latitude: %s\n ~r209 10 ^Position angle^: %s degrees\n ~r125 0 B Barred galaxy\n ~r126 0 R Ringed galaxy\n ~r127 0 M Multiple object galaxy\n ~r128 0 C Compact object\n ~r128 0 D Diffuse object\n ~r219 10 Effective ^surface brightness^: %s ~r229 10 ñ %s ~r229 10 (^magnitude^s per square ^arcsecond^)\n ~r589 10 Effective mean ^surface brightness^ at 25%% level: %s\n ~r589 10 (^magnitude^s per square ^arcsecond^)\n ~r239 10 Total B magnitude: %s ~r249 10 ñ %s ~r239 10 \n ~r279 10 Total U-B color: %s\n ~r289 10 Total B-V color: %s\n ~r299 10 Effective U-B color: %s\n ~r309 10 Effective B-V color: %s\n ~r569 10 Total apparent U-B color: %s\n ~r579 10 Total apparent B-V color: %s\n ~r719 10 Kinematic ^distance modulus^: %s\n ~r719 10 (Above is based on Ho=75 km/sec/mpc)\n ~r729 10 Tentative ^distance modulus^ from astrophysical parameters: %s\n ~r739 10 ^Absolute B magnitude^: %s\n ~r1279 10 Distance: %s mega^parsec^s ~r1289 10 (%s million ^light-year^s)\n ~r1299 10 ^Galactic luminosity^: %s billion suns ~r1309 10 (%s times Milky Way)\n ~r409 10 Far ^infrared^ magnitude: %s\n ~r419 10 Heliocentric ^galaxy RV^ from ^neutral hydrogen^: %s ~r429 10 ñ %s ~r419 20 ^km^/s\n ~r439 10 Heliocentric ^galaxy RV^ from optical observations: %s ~r449 10 ñ %s ~r439 10 ^km^/s\n ~r679 10 ^Galaxy RV^ relative to the ^Local Group^: %s ^km^/second\n ~r689 10 ^Galaxy RV^ relative to the ^GSR^: %s ^km^/second\n ~r699 10 ^Galaxy RV^ corrected for ^Virgo infall^: %s ^km^/second\n ~r709 10 ^Galaxy RV^ relative to the ^3K background^: %s ^km^/sec\n end ~wds2001 ~r 1 10 \nComments from the ^WDS^-2001 catalog:\n # Almost everything from here on down is taken straight from WDS2001.TDF. # Note to translators: you may find it easier to translate WDS2001.TDF, # then paste in the "remarks" parts below. ~r 1 10 WDS %s\n ~b 12 3 ^Discoverer's ID^: %s ~b 15 9 %s ~b102 30 %s ~b 12 12 \n ~r 59 5 ^Magnitude^s %s ~r 65 5 and %s ~r 59 11 \n\n ~r 47 5 ^Separation^: %s ^arcsecond^s ~b 26 4 in %s ~r101 0 6 (Separation is actually in arcminutes)\n ~r 53 5 \nSeparation: %s arcseconds ~b 31 4 in %s ~r101 0 6 (Separation is actually in arcminutes)\n ~r 39 3 \n^Position angle^: %s ^degree^s ~b 26 4 in %s ~r 43 3 \nPosition angle: %s degrees ~b 31 4 in %s ~b 33 4 \n ~r 36 2 %s measurements made\n ~r 81 4 \n^Proper motion^ in RA: %s milliarcseconds/year\n ~r 86 4 ^Proper motion^ in dec: %s milliarcseconds/year\n ~r 71 9 ^Spectral Type^: %s\n ~r 91 3 \n^DM^ %s ~r 94 5 %s\n # # Unfortunately, a 'note' code can occur in any of three columns. # Hence, the repetition in the following text. # ~r100 0 N There are notes for this object.\n ~r101 0 N There are notes for this object.\n ~r102 0 N There are notes for this object.\n ~r100 0 D A difference (delta) in magnitude is given.\n ~r101 0 D A difference (delta) in magnitude is given.\n ~r102 0 D A difference (delta) in magnitude is given.\n ~r100 0 O An orbit has been determined for this object.\n ~r101 0 O An orbit has been determined for this object.\n ~r102 0 O An orbit has been determined for this object.\n ~r100 0 P The proper motion in RA is actually for 100 years.\n ~r101 0 P The proper motion in RA is actually for 100 years.\n ~r102 0 P The proper motion in RA is actually for 100 years.\n ~r100 0 Q The proper motion in dec is actually for 100 years.\n ~r101 0 Q The proper motion in dec is actually for 100 years.\n ~r102 0 Q The proper motion in dec is actually for 100 years.\n ~r100 0 R The proper motion is actually for 100 years.\n ~r101 0 R The proper motion is actually for 100 years.\n ~r102 0 R The proper motion is actually for 100 years.\n ~r100 0 a Data is from an appendix list, not part of the regular numbering.\n ~r101 0 a Data is from an appendix list, not part of the regular numbering.\n ~r102 0 a Data is from an appendix list, not part of the regular numbering.\n ~r100 0 p Position & proper motion are from ACRS, ^PPM^, IRS, and/or ^FK5^.\n ~r101 0 p Position & proper motion are from ACRS, ^PPM^, IRS, and/or ^FK5^.\n ~r102 0 p Position & proper motion are from ACRS, ^PPM^, IRS, and/or ^FK5^.\n end ~hmwxorbi ~r 1 10 \nComments from the ~r 1 0 5 Fifth ~r 1 0 6 Sixth ~r 1 10 Catalog of Orbits of Visual Binary Stars:\n ~r 24 10 ^WDS^ identifier: %s\n ~r 34 11 Discoverer identifier: %s\n ~r 45 6 ADS (Aitken Double Star) number: %s\n ~r 52 6 ^HD^: %s\n ~r 67 5 Magnitude of first component: %s\n ~r 74 5 Magnitude of second component: %s\n ~r 82 11 Orbital period: %s years\n ~r 94 9 Semimajor axis: %s ^arcsecond^s\n ~r133 7 ^Eccentricity^: %s\n ~r 1 10 !Year PA Sep Year PA Sep Year PA Sep(")\n ~r 1 10 ---- -- --- ---- -- --- ---- -- ---\n end ~lightcur ~r 29 8 ^Rotation period^: %s hours\n ~r 50 0 1 (Very tentative result, may be completely wrong.)\n ~r 50 0 2 (Reasonably secure result.)\n ~r 50 0 3 (Secure result, no ambiguity of period.)\n ~r 50 0 4 (Very secure result; a pole position has been reported.)\n ~r 39 9 Magnitude varies by %s\n ~r 52 0 1 One extremum per cycle\n ~r 52 0 3 Three extrema per cycle\n ~r 52 0 A Ambiguous period; the most "likely one" is given.\n ~r 52 0 B Suspected binary.\n ~r 52 0 D Rotation period "determined" from published data, but not given\n ~r 52 0 D by author(s) of original data.\n ~r 52 0 N No lightcurve published.\n ~r 53 0 N No lightcurve published.\n ~r 52 0 P Photographic photometry.\n ~r 52 0 T "Tumbling" minor planet, that is non-principal axis rotation state.\n ~r 52 0 V Visual photometry.\n ~r 53 0 ? (Previous comment is in doubt.)\n end ~satellite # Guide reads in the TLE for a satellite, stuffing the two 69-byte lines # into one 138-byte line, then using the following formatting for display: ~r 1 69 ^Add a trail for this object//!189^\n ~r 1 69 Elements, in ^TLE^ form:\n!%s\n ~r 70 69 %s\n!Breakdown of data from the TLE:\n ~r 3 5 NORAD designation: %s\n ~r 10 2 International designation: ~r 10 > '56' 19 ~r 10 < '57' 20 ~r 10 2 %s-%[12,6]\n ~r 8 = 'U' Elements are unclassified\n ~r 8 <>'U' Elements are classified\n ~r 19 10 ^Epoch of elements^, NORAD-style (year & day of year): ~r 19 > '56' 19 ~r 19 < '57' 20 ~r 19 2 %s %[21,11]\n ~r 34 10 Rate of change of mean motion, revolutions/(day*day): %s\n ~r 55 5 BSTAR drag term: %[54,1].%sE%[60,2]\n ~r 65 4 Bulletin number: %s\n ~r 78 8 ^Inclination of orbit^: %s\n ~r 87 8 Right ascension of ascending node: %s\n ~r 96 7 ^Eccentricity^: 0.%s\n ~r104 8 Argument of perigee: %s\n ~r113 8 ^Mean anomaly^: %s\n ~r122 11 Mean motion: %s revolutions/day\n ~r133 5 Revolution number: %s\n ~r 3 < '9' \n The following two Web sites have useful comments on the names,\n ~r 3 < '9' missions, and orbital parameters of most satellites:\n ~r 3 < '9' ^Comments from Heavens-Above//xhttp://heavens-above.com/orbitdisplay.asp?satid=%[3,5]^\n ~r 3 < '9' ^Comments from n2yo.com//xhttp://www.n2yo.com/satellite.php?s=%[3,5]^\n ~r 10 2 \n The NSSDC (National Space Science Data Centre) offers comments\n ~r 10 2 on most payload satellites. Be warned that for rocket stages and\n ~r 10 2 debris, you usually get a "No record exists" message.\n ~r 10 2 ^Comments from the NSSDC Master Catalogue//xhttp://nssdc.gsfc.nasa.gov/database/MasterCatalog?sc= ~r 10 > '56' 19 ~r 10 < '57' 20 ~r 10 2 %s-%[12,6]^\n\n end ~launch_data ~r 13 15 Launched: %s:%[28,5] ^UT^\n ~r122 23 Launch vehicle: %s\n end ~launch_data_2 ~r 56 31 Payload name: %s\n ~r 56 31 Original payload name: %s\n end