Chip 1999 November/Chip Kasım 1999.iso/program/astr/cos.exe/OCH.DOC

Text File | 1995-12-14 | 33.6 KB | 736 lines

                               Our Cosmohood
                               version 2.03

                             A 3d View of Our
                            Cosmic Neighborhood

                        (c) 1991-5 by Jeff Bondono

                         [e-mail]


When you look at the night sky, it looks like you are viewing stars,
nebulae, and galaxies which have been glued to a clear sphere which rotates
overhead.  A glance at a star atlas shows the same thing: a two-dimensional
projection of the universe onto a piece of paper.  Of course, the true
universe is a three-dimensional entity. All of the objects you see are so
incredibly distant that your normal three-dimensional perception is
rendered useless.

Our Cosmohood enhances your view of our cosmic neighborhood by letting you
view it in three dimensions.  Our Cosmohood does not deal with objects
within our galaxy, the Milky Way, but rather lets you view the nearest
2,368 galaxies to the Earth.  The source for the program's data is "The
Nearby Galaxies Catalog", by R. Brent Tully.  That book and its companion,
"The Nearby Galaxies Atlas", by R. Brent Tully and J. Richard Fisher, are
highly recommended by this author.

Our Cosmohood runs in two modes.  The first mode, which is completely
general in approach, lets you specify exactly where, in three dimensions,
you wish to place your eye, where you wish to center your field of view,
and how wide you wish the field to be.  It also lets you select subsets of
the dataset to plot, and allows you to select color-coding and object-
labelling.  The second mode, the demonstration, simply lets you view a
"movie" which takes you on a trip through Our Cosmohood.  It is, obviously,
much simpler to operate than the first mode, and is how I recommend you
begin using the program.  To run the demo, just press enter when you see
the main program menu.


TABLE OF CONTENTS
 #1. SYSTEM REQUIREMENTS
 #2. REGISTRATION
 #3. PRELIMINARIES
  #3A. INITIAL INSTALLATION AND CONFIGURATION
  #3B. FILES
  #3C. MAIN MENU OPERATION
  #3D. TECHNIQUES OF INPUT
  #3E. IDENTIFICATION OF OBJECTS
  #3F. BEEPS
 #4. ANIMATION
  #4A. DEFINITIONS OF ANIMATION, FILMS, MOVIES
  #4B. EXAMPLES OF ANIMATION
  #4C. MOVIES
 #5. 3D MODE
 #6. ADVANCED CONFIGURATION
 #7. WARRANTY
 #8. NEW IN THIS VERSION
 #9. OBJECT MEMBERSHIP


Section #1. SYSTEM REQUIREMENTS: Our Cosmohood requires a PC-compatible
with a hard disk and either a VGA or EGA graphics adapter.  A math
coprocessor is optional, and will be used if present.  The program has only
been tested with MS DOS 4.01 and MS DOS 5.0, but I believe it will run with
MS DOS 2.0 or higher.  To run the fast demonstration, your hard disk must
have 2.2 MegaBytes free.  To run the slow demonstration, your hard disk
needs only about 600 KiloBytes free. Our Cosmohood requires about 400K of
free memory.  A mouse is optional.  If you wish to use one, load your mouse
driver before you startup Our Cosmohood.


Section #2. REGISTRATION: Your version Our Cosmohood is complete and is not
crippled in any way.  However, bear in mind that this is NOT FreeWare, but
ShareWare.  You have 14 days to try out the program to see if it is of
interest to you.  If you decide it is not, destroy your copies of the
program and you owe nothing.  If, however, you decide to keep the program,
send a $25 registration fee to me.  Many hours were spent typing and
checking the data, and writing and refining the program and the
demonstration.  If you wish to continue seeing quality, low cost ShareWare
like this program, you must make it worthwhile to spend the time required
to create it.  In return for registration, you will receive instructions
for eliminating the registration reminder screens, and I'll automatically
send you the next upgrade to the program for free.

To register, send
     $25
     your name and address
     your current version number (from the title screen)
     the size and capacity of the disk you would like me to send

Send registration to:
     Jeff Bondono
     51054 Kingwood
     Shelby Twp, MI 48316
     810.731.4706 (evenings and weekends)


Section #3. PRELIMINARIES: Before we begin using the program, a few
preliminaries are in order:


Section #3A. INITIAL INSTALLATION AND CONFIGURATION: I will assume that
your floppy drive is drive A:.  If it is something else, then whenever I
refer to A:, use your floppy's drive letter instead.

To install Our Cosmohood onto your hard disk, get to a DOS prompt, put the
installation disk in your floppy drive, type A:INSTALL and press ENTER.
The installation procedure will give you complete instructions for
installing and starting up your version of the Our Cosmohood.

To run Our Cosmohood after you have installed it, switch into the directory
you installed it into and type OCH.


Section #3B. FILES:

These files MUST be available to run Our Cosmohood:
     OCH.EXE   the executable program
     OCH.OBJ   data file of galaxies
     OCH.PNT   data file of galaxies
     OCH.CFG   configuration file
     OCH.HLP   topic-specific help (explains each menu entry)
     OCH.DOC   the file you're reading now (used for general help)
These files are only part of the demonstration, and can be deleted if you
no longer want the demonstration:
     *.DCR     animation descriptor files
     *.ANI     animation detail files
     *.FLM     film files (fast demonstration only)
     *.MVI     movie files
This file is used only the first time Our Cosmohood is run, then is deleted
from your hard disk:
     OCH.TXT   used to build .DCR and .MVI files

To erase the fast demo, if you need the disk space, issue this command at
a DOS prompt:
     ERASE *.FLM


Section #3C. MAIN MENU OPERATION: Simply use your cursor left, right, up,
and down keys to select menu entries, and press ENTER to execute them.
Alternately, you may directly type in the first character of any menu entry
to execute it.  If you wish to use a mouse, you may select menu entries by
moving your mouse, and use the left button to execute them.  Press the ?
key to obtain a complete description of the highlighted menu entry.  The
topic-specific help that you receive by pressing the ? key is NOT included
in this help file.  Centered on the top line of the main menu is the name
of the working file.  If you have made changes to this file since your last
OPEN, SAVE, or MAKEFILM, an asterisk will be shown after the filename.


Section #3D. TECHNIQUES OF INPUT: Whenever you are asked to type in a
number or an alphanumeric string, you may use the CURSOR LEFT, CURSOR
RIGHT, HOME and END keys to move around the input field.  The INSERT key
will switch you between insert and overstrike mode (a box cursor indicates
insert mode and a block cursor indicates overstrike mode).  The DELETE key
will delete the character under the cursor, and the BACKSPACE key will
delete the character to its left.  The CURSOR UP, CURSOR DOWN, PAGE UP, AND
PAGE DOWN keys will all erase the contents of the field and let you start
typing anew.  The ENTER key causes your input to be accepted.  The ESCAPE
key will cancel your input and leave the value unchanged.  In general, the
ESCAPE key will cancel most operations, like playing back movies, films,
and animations.


Section #3E. IDENTIFICATION OF OBJECTS:  The galaxies are identified by one
of the types of names listed below.  If an object can be identified by a
name which appears both higher and lower in the list, the higher one is
used.
     M : Messier
     N : New General Catalog
     I : Index Catalogue
     U : Upsalla General Catalog
     UA: Upsalla General Catalog Appendix
     a name formed from the 1950 right ascension and declination.

Cloud and group affiliations are described in section 9.


Section #3F. BEEPS:  The program will emit a beep occasionally when
calculating a 3d projection.  3d projections are calculated when you build
a movie, or when you display an animation, or when you simply draw a screen
in manual mode.  The beep indicates when a floating point operation
overflow or zero-divide is encountered.  An occasional beep is not a
problem... it merely signifies a galaxy which is right at one of the
boundaries of the volume you are viewing.  If the program goes crazy,
though, and emits many beeps in rapid succession, you have probably
specified some parameter(s) which are out of range.


Section #4. ANIMATION: If you've played around with the program in manual
mode, you've seen that you must really go through a lot of work to get
enough views of the data to really understand the three-dimensional
relationships of the various galaxies.  Animations let you easily define
motion to perform, then draw the frames one after the other, as is done in
the demonstration.


Section #4A. DEFINITIONS OF ANIMATION, FILMS, MOVIES: Three levels of
animations are used by the program.  The first, an animation, allows you
to specify a single motion to be performed.  Animations alleviate you from
having to type in the several parameters required for each viewpoint, but
they are not especially fast or movie-like.  Therefore, the second level
of animation, a film, is provided.  A film actually calculates the pixel
position of each of the selected galaxies in each step of an animation, and
writes those to a file.  When a film is played-back, the calculations
needed are minimal, and a much higher speed of refreshing the display is
obtained.  The third level of animation, a movie, is used to combine
animations and films, along with many other miscellaneous drawing and
labelling functions.  The demonstration which comes with Our Cosmohood is
a set of movies.  Movies are simple text files which are created outside
of the Our Cosmohood program with your favorite text editor, then played-
back using the WATCHMOVIE command.  The instructions for building a movie
text file are explained in section 4C.


Section #4B. EXAMPLES OF ANIMATION: These three examples let you
familiarize yourself with the process of creating animations.  One word of
caution is in order before we begin, though.  The examples let you take a
walk around the Virgo Cluster.  No one really knows the exact placement of
the galaxies in the Virgo Cluster, though, or any other cluster for that
matter.  The positional data in the Nearby Galaxies Catalog is simply based
on redshift.  If one galaxy has a higher redshift than another, it is
assumed to be further.  This, of course, completely neglects the portion
of the redshift of each galaxy which is due to its own peculiar motion
within the cluster.  However, the redshift is the only data available to
work from, so Tully used it to assign distances to galaxies.  One
correction was made, however.  Assuming that the Virgo Cluster is somewhat
round, Tully corrected the distances to the member galaxies so that the
cluster would appear round in three dimensions.  This process was used for
several clusters of galaxies in the Nearby Galaxies Catalog.  The
conclusion of this discussion is that although the examples will make it
appear that you are walking around an accurate model of the Virgo Cluster,
the data on such a small scale is not yet accurate.  The overall larger-
scale structures shown in the data, such as in the demonstration movie, are
accurate, but the detailed position of each galaxy within those structures
is a subject still being researched.


Example 1: Walking around the Virgo Cluster.  Select FILE, then NEW, then
DEFINE. type in:
     EYE: 0, 0, 0
     VIEW: -3.8, 16.7, -0.7
     ZOOM: 2.2 to 2.2
     LENGTH OF AXES: 1.7
     SELECT: 11-01
     TYPE OF MOTION: EYE AROUND Z
     NUMBER OF STEPS: 72
     FILE
     SAVE: VIRGO (feel free to pick your own filename)
     PLOT
You should now see the Virgo Cluster rotating around on your screen.  When
you've had enough, press ESCAPE.


Example 2: To make that animation more smooth, type in:
     DEFINE
     NUMBER OF STEPS: 360
     FILE
     SAVE: VIRGO (replace it)
     PLOT
You should now see a much smoother animation.  The steps are only 1 degree
per frame.  However, the animation takes a long time to run because of all
the calculations which are being done.


Example 3: To make the animation run quicker, type in:
     FILE
     MAKEFILM
     (go get a cup of coffee -- this will take a while)
     PLOT
     (now sit back and enjoy)


Section #4C. MOVIES: Each line of a movie script file must contain a valid
movie command.  In order to make movies run as quickly as possible, the
commands must conform to some very strict format conventions.  The command
letter must appear in the first position of the line, and must be in
lowercase.  Some commands have parameters which are required to be in
definite formats.  These commands and parameters are now documented:

     ;(comment): Anything following the command character is ignored when
     the movie is played back.

     d(descriptor): This command reads in an animation description (.DCR)
     file and determines which objects meet the selection criteria.
     Everything following the command character is assumed to be the
     filename of the descriptor file, with no extension.

     a(animate): This command plays back an animation.  The descriptor must
     already have been read in.  Everything following the command character
     is assumed to be the filename of the animation (.ANI) file, with no
     extension.

     f(film): This command plays back a film (.FLM file).  The rules are
     the same as for the "a" command.  If the film is not found when the
     movie is played back, this command is converted to an "a" and the
     program tries again.

     g(stolen film): This command plays back a film (.FLM file), also,
     except it uses a different film file that would normally be used.
     This command was included only to save you disk space on the demo
     (several of the animations all use data from one common film file),
     and I recommend that you do NOT use it.

     p(pause): This command writes out the "SPACE=CONTINUE....." message
     and waits for the user to press a key or a timer to expire.  Anything
     following the command character is ignored.

     t(text): This command writes text to the screen.  Positions 2 through
     4 are a 3-digit horizontal position on the screen where the text will
     be written.  On your 640x350 screen, the leftmost edge of the screen
     is position 000, and the rightmost is 639.  Position 5 is ignored.
     Positions 6 through 8 are the 3-digit vertical position of the text,
     ranging from 000 on the top to 349 at the bottom.  Position 9 is
     ignored.  Positions 10 through 12 are the color of the text, which in
     16-color mode are: 000=black, 001=blue, 002=green, 003=cyan, 004=red,
     005=magenta, 006=brown, 007=lightgray, 008=darkgray, 009=lightblue,
     010=lightgreen, 011=lightcyan, 012=lightred, 013=lightmagenta,
     014=yellow, and 015=white.  Position 13 is ignored.  The rest of the
     record is the text to write.

     s(select): This command redefines the selection criteria for the
     records to be plotted.  It follows the same conventions as the other
     selection criteria in the program.  Everything after the command
     character must be the selection criteria.

     m(markers): This command redefines the markers which are used.  It
     follows the same conventions as the main menu markers line.
     Everything after the command character must be the markers value.

     h(heading): This command defines a text heading which is written on
     the top line of the screen whenever objects are plotted on the screen.
     Everything after the command character is the text heading.

     r(redraw): This command forces the objects on the screen to be redrawn
     using the last defined projection criteria.  Everything after the
     command character is ignored.

     x(text at xyz): This command writes text at the location projected for
     an x,y,z coordinate.  Following the command character is an x
     coordinate and a comma, then a y coordinate and a comma, then a z
     coordinate and a comma, then a 3-character color code and a comma,
     then the text to write.

     y(line): This draws a line in 3d space. Following the command
     character is an x coordinate and a comma, a y coordinate and a comma,
     and a z coordinate and a comma.  This x,y,z coordinate is at one end
     of the line.  Next is the other end of the line, specified in an
     identical way.  Next is a 3-character color code and a comma.  The
     rest of the line is ignored.

     c(call): This command calls another movie file.  Movie files can be
     nested 3 movies deep.  Everything after the command character is the
     filename of the movie file (.MVI), without any extension.

While playing back a movie, you may press the PAUSE key on your keyboard
at any time to pause the program.  Press any other key to take the computer
out of the pause.  Also, you may press the F key to advance the movie
forward (ie, cancel the currently-running animation or film).


Section #5. 3D MODE:  3D mode lets you view the displays of Our Cosmohood
in true three dimensional mode.  All that is required is a pair of standard
3d-viewing glasses.  These glasses have a red transparancy in the left lens
and a green one in the right lens.  If you don't have any 3d viewing
glasses, any transparencies will do.  For example, I seem to get the best
views using the colored filters I use to observe planets through a
telescope.  They seem to be more efficient at letting only one color
through.

To turn on 3d mode, use the 3D command in the DEFINE menu entry.  You will
then be prompted for 3 values; just respond with the defaults.  Those
values are explained in the topic-specific help entry for the 3D command,
and you can play around with them later if you wish.  Next, run any PLOT.
S30 is an especially good example.  To run it, press F, O, S30, ENTER, and
P.  You should see some galaxies floating in front of and behind other
galaxies.  If you do not, the rest of this section suggests what you can
try.

First, try moving your face further or closer to the screen.  You should
probably get the best 3d view when your eyes are about as far from the
screen as the screen is wide.  You can also try adjusting the brightness
and contrast on your monitor.  I find the best 3d views on my system are
with both turned all the way up.

If this doesn't do it, you'd better go back to some basics.  Exit the plot
and select HELP, then COLORS.  You should see a table of the 16 colors your
display can generate.  Close your right (green) eye and look at the table
through your left (red) eye.  You should see the red color easily, and the
green color should be completely invisible.  If you switch to your green
eye, the green should show through well, and the red should be invisible.
If this is not the case, try adjusting your monitor, or choosing a
different set of filters.  You may also select different colors (rather
than red or green), for the 3d views, then change the OCH.CFG configuration
file (see section 6) to have Our Cosmohood use those colors for the 3d
displays.  Remember that your true goal is to get some combination of
colors, monitor adjustments, and colored filters which will allow each eye
to see only one of the colors.


Section #6. ADVANCED CONFIGURATION: You may modify your OCH.CFG
configuration file to suit your needs.  Use your favorite text editor to
make the changes, and be sure to save the file as an ASCII text file.  It
is advisable to make a copy of the original file before you make changes
to it in case you really mess it up.  Each of the following parameters
takes up one line in your configuration file.  To test out color changes,
use the COLOR function of the HELP menu.  Lines that are identified as
foreground colors can be any color, from 0 to 15.  Background colors should
only be 0 to 7.

-Insert Mode.  If this line contains Y or y, Our Cosmohood will come up in
     Insert mode, otherwise it will come up in Overstrike mode.
-Foreground color of the left lens on your 3d glasses.
-Foreground color for objects which should show through both the left and
     right lenses of your 3d glasses, at the same intensity as your left
     and right colors.
-Foreground color of the right lens on your 3d glasses.
-Foreground color of non-highlighted entries in the main menus.
-Background color of non-highlighted entries in the main menus.
-Foreground color used for the first character of non-highlighted entries
     in the main menus.
-Foreground color of highlighted entries in the main menus.
-Background color of highlighted entries in the main menus.
-Foreground color of highlighted choice in a multiple-choice prompt.
-Background color of highlighted choice in a multiple-choice prompt.
-Foreground color of non-highlighted choice in a multiple-choice prompt.
-Background color of non-highlighted choice in a multiple-choice prompt.
-Foreground color of input prompts.
-Background color of input prompts.
-Foreground color of input fields.
-Background color of input fields.
-Foreground color of heading in the file picker.
-Foreground color of instructions in the file picker.
-Background color of instructions/heading in the file picker.
-Foreground color of non-selected filenames in the file picker.
-Background color of non-selected filenames in the file picker.
-Foreground color of the selected filename in the file picker.
-Background color of the selected filename in the file picker.
-Foreground color of error messages in the file picker.
-Background color of error messages in the file picker.
-Foreground color of topic-specific help.
-Background color of topic-specific help.
-Foreground color of topic-specific help prompt.
-Foreground color to restore when program halts.
-Foreground color of bright general purposes (prompts, messages, help)
-Foreground color of normal general purposes (prompts, messages, help)
-Speed of mouse through menus horizontally (1=fastest, 300=slowest)
-Speed of mouse through menus vertically   (1=fastest, 120=slowest)
-Warn if fast demo is not found:  If this line contains a Y or y, when
     RUNDEMO is chosen and 020.flm does not exist, a warning will be given
     with an option to build the fast demo.  If you wish for this warning
     to be suppressed (if you have a math coprocessor or are low on disk
     space, for example), change the line so it contains no Y or y.
-Delay. Adjust this number to get comfortable demo speeds. The range
     is 0 to 2147483647.  I suggest 0 for an 386sx16, about 100000 for
     a for 486dx66, and 2000000000 for your new Octium.  The value specified
     here is the default value given when you run the demo.


Section #7. WARRANTY:  This program is provided "as is" without warranty
of any kind.  All warranties are disclaimed, including damage to hardware
and/or software from use of this product, and implied warranties of
merchantability and fitness.  In no event will I be liable to you for any
damages, including lost profits, lost savings or other incidental or
consequential damages arising out of your use or inability to use the
program, or any other claim by any other party.  In no case shall my
liability exceed the registration fees paid for the right to use the
software.


Section #8. NEW IN THIS VERSION:
NEW IN VERSION 2.01:
     New and improved user-interface.
     3D mode.
     Improved help interface.
     Topic-specific help.
     Configuration file for custom colors.
     Dropped support for CGA and HERCULES graphics adapters.
     Added support for non-enhanced keyboards.
     A math coprocessor is now automatically supported.
     A NOTE TO VERSION 1 USERS:  Version 1 .FLM files are not compatable
          with version 2, so the INSTALL process deleted all of them.  Use
          OPEN and MAKEFILM to remake any which you wish.  Sorry for the
          inconvenience.
NEW IN VERSION 2.02:
     Configuration file documentation corrected.
     Entry of an object not on the screen during identify mode would
          sometimes did not display the error message correctly on the
          screen, and the display would therefore not show the true state
          of the program.


Section #9. OBJECT MEMBERSHIP:  The first 2 digits of a galaxy's membership
is a cloud name.  After the cloud name is either one or two sets of a sign
and a 2-digit number.  If the sign is negative, it indicates a group.  If
it is positive it indicates an association.  The table below shows the
cloud names as headings, with the groups and association within those
clouds underneath.  Only groups and associations which I was able to
identify with a standard group name are shown.

11:Virgo Cluster / Southern Extension
     01:Virgo Cluster                20:N5054
     03:N4532                        21:N5084
     04:N4536                        22:N5101
     05:N4339                        23:N4965
     08:N4666                        24:N4235=Virgo West Cluster
     10:N4699                        25:N4385
     11:N4697                        27:N4658
     12:N4958                        28:N5254
     13:UA312                        29:N4593
     14:N4594=M104                   30:N4902
     15:N4856                        31:N5044
     17:N4995                        32:N5161
     18:N5170                        33:UA327
     19:N5042                        34:N4433
                                     35:I4351
12:Ursa Major Cloud
     01:N3992=Ursa Major Cluster     11:N2146
     02:N3631                        12:N3613
     03:N3998                        13:N3445
     04:U6534                        14:N3065
     05:N4036                        16:N3780
     06:N4151                        17:N2551
     07:N2985                        18:N3656
     08:N3403                        19:U2855
     09:N3259                        20:U2729
     10:N2655                        21:U4576

13:Ursa Major Southern Spur
     01:N3079                        06:N2768
     02:N3353                        07:N3813
     03:U6029                        08:N3665
     04:N2685                        09:N3900
     05:N2805                        10:N3694
                                     11:N4158
14:Coma-Sculptor Cloud
     01:N4565=Coma I Cluster         11:I342/Maffei
     02:N4725                        12:N224=Local
     04:N4258=Canes Venatici II      13:N55=Sculptor
     05:N5194                        14:N1313
     06:N4631                        15:N5128=Centaurus
     07:N4736=Canes Venatici I       16:1424-46
     09:N5457=M101                   17:UA320
     10:N3031=M81                    18:N4517

15:Leo Spur
     01:N3368=M96 Cluster            05:N3115
     02:N3627=M66                    06:N2683
     03:N3423                        09:N3675
     04:N3486                        10:N2681
                                     11:N2541
16:Centaurus Spur
     01:N5643                        03:1418-46
     02:N5483                        04:N5121
                                     05:N5398
17:Triangulum Spur
     01:N1023                        04:N628=M74
     02:N278                         05:N672
     03:N1012                        07:0102-06

18:Perseus Cloud
     01:N1169                        02:U2531

19:Pavo-Ara Cloud
     01:N6744                        05:I5201
     02:N6300                        06:N7424
     03:N6221                        07:N7713
     04:N7090                        08:N45

21:Leo Cloud
     01:N3607                        10:N3166
     02:N3501                        11:N3640
     03:N3507                        12:N3003
     04:N3810                        13:N3032
     05:N3338                        14:U5349
     06:N3190                        15:N2859
     07:N3504                        16:N2798
     08:N3245                        17:N2852
     09:N3430                        18:N2770

22:Crater Cloud
     01:N4038                        06:N3585
     02:N3892                        07:N3672
     03:1213-11                      08:N3818
     04:N3923                        09:N3952
     05:N4105                        10:N4030
                                     11:N4123
23:Centaurus Cloud
     01:N4696                        05:I3253
     02:N5064                        06:N4588
     03:N5266                        07:N4835
     04:N5333                        08:I3896
                                     09:N4976
24:Lynx Cloud
     01:N2273                        02:U3574
                                     03:N2460
31:Antlia-Hydra Cloud
     01:N3312                        13:N2907
     02:N3258=Antlia Cluster         14:N2781
     03:N3347                        15:N2992
     04:N3095                        16:N2855
     05:N3089                        18:N2974
     06:N3256                        19:N3023
     07:N3250                        20:U5249
     08:1010-47                      21:N2559
     10:N3557                        22:N2613
     11:N3706                        23:N2775
     12:N2935                        24:U3912

32:Cancer-Leo Cloud
     01:N2750                        04:N3367

33:Carina Cloud
     01:N2842                        03:0916-62
     02:0913-601                     04:N2417

34:Lepus Cloud
     01:N2217                        04:N1888
     02:N1964                        06:N2227
     03:N1832                        08:N2207

41:Virgo-Libra Cloud
     01:N5846 Cluster                07:N5364
     02:N5775                        08:N5248
     03:N5566                        10:N5878
     04:N5496                        11:N4903
     05:N5665                        12:N5427
     06:N5861                        13:N5468
                                     14:N5595
42:Canes Venatici-Camelopardalis Cloud
     01:N5371 Cluster                08:N5322
     02:N5198                        12:U7168
     03:N5676                        13:N4589
     04:N5448                        14:N3735
     05:N5783                        16:N2276
     06:N5473                        17:N2336
     07:N5678                        18:N1530
                                     19:U2824
43:Canes Venatici Spur
     01:N5005                        02:N5145
                                     03:U9562
44:Draco Cloud
     01:N5866=M102                   05:N6340
     02:N6015                        06:N6236
     03:U10736                       07:N6412
     04:N6207                        08:N6643

45:Coma Cloud
     01:N5012

51:Fornax Cluster / Eridanus Cloud
     01:N1316=Fornax Cluster         08:N1407
     03:N1097                        09:UA87
     04:N1332=Eridanus Cluster       10:UA95
     05:N1302                        11:N1421
     06:N1187                        13:0312-04
     07:N1232                        14:N1209

52:Cetus-Aries Cloud
     01:N1084                        08:N701
     02:N1068=M77                    09:N720
     03:N936                         10:N864
     04:N1087                        11:N676
     05:N779                         12:N488
     06:N908                         13:U1102
     07:N584                         14:N772
                                     15:N691
53:Dorado Cloud
     01:N1566 Cluster                12:N1800
     02:N1559                        13:N1532
     03:N1672                        14:N2188
     04:N1947                        15:0737-50
     05:N1511                        16:N2427
     06:N2101                        17:N2442
     07:N1448                        18:N3059
     08:I1954                        19:0756-76
     09:N1291                        20:N1637
     10:N1808                        21:N3136
     11:0515-37                      22:N2788

54:Antlia Cloud
     01:N2997                        03:N2835
     02:N3175                        05:N3511

55:Apus Cloud
     01:N5833                        03:N6438
     02:N5612                        04:1409-87
                                     05:0000-80
61:Telescopium-Grus Cloud
     01:N6868 Cluster                13:N7205
     02:N6902                        14:N7307
     03:2041-46                      15:I5269
     04:N6707 Cluster                16:N7552=Grus
     05:N6810                        17:N7418
     06:N7079                        18:N134
     07:N7196                        19:N289
     09:N7166                        20:N150
     10:N7049                        21:N255
     11:N7213                        22:N210
     12:N7144                        23:N337
                                     24:0049-00
62:Pavo-Indus Spur
     01:N7083                        02:N7192
                                     03:N7125

63:Pisces Austrinus Spur
     01:N7172                        03:UA427
     02:N7135                        04:N7171
                                     06:N7727
64:Pegasus Cloud
     01:N7448                        07:U12843
     02:N7479                        08:N7817
     03:N7280                        09:N7541
     04:N7497                        10:N7714
     06:N7743                        12:N7177

65:Pegasus Spur
     01:N7331                        04:N7640
     02:N7332                        06:N7814
     03:N7741                        07:U12423

66:Sagittarius Cloud
     01:N6835

71:Serpens Cloud
     01:N5962                        04:N6070
     02:N5970                        05:U9977
     03:U10086                       06:N5961

72:Bootes Cloud
     01:N5930

73:Ophiuchus Cloud
     01:N6574                        02:N6509
                                     03:N6384