From chemistry-request@server.ccl.net Wed Jul 17 05:34:59 2002
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From: Jamie Platts <Platts@Cardiff.ac.uk>
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To: Stephen  Bowlus <stephen.bowlus@lionbioscience.com>
cc: "'chemistry@ccl.net'" <chemistry@ccl.net>
Subject: Re: CCL:MOLVOL
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  Hi Stephen - we've got the Fortran77 source for MOLVOL, which I'll send
separately. My student has also modified it to read MDL mol files, rather
than the original xyz format - would you prefer that? 

  Cheers,

  Jamie 

----------------------------------------------------------
  Jamie Platts 							 
  Dept. of Chemistry  		Phone: +44 (0) 2920 874950		 
  Cardiff University 	 	Email: platts@cf.ac.uk		 
  P.O. Box 912 			FAX:   +44 (0) 2920 874030		 
  Cardiff CF10 3TB 		www.cf.ac.uk/chemy


On Tue, 16 Jul 2002, Stephen  Bowlus wrote:

> Does anyone know how or from whom one can obtain the program MOLVOL by Dodd
> and Theodorou?  I have been unable to locate a repository for the program,
> or Prof. Dodd, who seems to be (have been?) its curator.
> 
> Thanks in advance for suggestions,
> Steve 
> 
> ***************************************************************
> Stephen B. Bowlus, Ph.D.
> Senior Computational Scientist    
> 
> LION bioscience, Inc.         Stephen.Bowlus@lionbioscience.com
> 9880 Campus Point Dr.                     Phone: (858) 410-6542
> San Diego, CA 92121                         Fax: (858) 410-6665
> ***************************************************************
> 
> 
> 
> 





From chemistry-request@server.ccl.net Wed Jul 17 07:08:08 2002
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To: chemistry@ccl.net
From: Shireen Al Falah <sherin.alfalah@student.uib.no>
Subject: ROMP4 using gaussian
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Hi to ccl users,

I  need to run a ROMP4 using gaussian98. I have tried to do it. But I was 
no lucky.
Do you know a way to do it. The same input file with the keyword ROMP2 worked.
Can you explain the reason for that, please

The input is as follows:

%mem=30000000
%nproc=4
%chk=et_bht_p_ROMP4
#P ROMP4/gen SP  Vshift=300
gfinput IOP(6/7=3) scf=(tight,novaracc,maxcycle=300)
pop=Full units=Ang Guess=Cards

The error message is:

QPERR --- A SYNTAX ERROR WAS DETECTED IN THE INPUT LINE.
#P ROMP4/GEN SP VSHIFT=300 GFINPUT IOP(6/
'
Last state="GCL"
TCursr= 827 LCursr= 3
Error termination via Lnk1e in /usr/local/chemistry/g98/l1.exe.


Best regards,
Sherin Alfalah


From chemistry-request@server.ccl.net Wed Jul 17 07:08:16 2002
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From: Robert Flight <l72k6@unb.ca>
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Subject: Answers to Number of  Atom Types in Autodock
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Thank you to everyone who responded to my question.  I have managed to 
recompile Autodock and Autogrid under Linux using the autocomm.h-extra-maps to 
replace the original autocomm.h in both Autodock and Autogrid.  So now I 
should have up to 15 atom types available for docking calculations.  Note:  I 
tried compiling on my SGI, but the GNU GCC compiler on SGI didn't really like 
the "make" file, therefore I switched to Linux, which compiled with minimal 
problems.  Below is my original question and the responses.

Thanks again to everyone,
Robert


Original Question:

Fellow CCLers,

A question on Autodock and the number of atom types allowed in the ligand used 
for docking. My ligand contains Carbon, Aromatics, Nitrogen, Oxygen, Sulphur, 
Hydrogens, and Fluorine atoms. Apparently Autodock allows only 7 atom types. 
When I try to run the docking with this particular ligand, I get the following 
error message:

autodock3: ERROR: ERROR: 7 atom types declared in "", S_line "CANOSHF"; 
maximum allowed is 6.
Change "ATOM_MAPS" in "autocomm.h"
autodock3: Aborting...

autodock3: Unsuccessful Completion.

I found two "autocomm.h" files, and also another called autocomm.h-extra-maps, 
however changing the contents of the autocomm.h files did not correct the 
problem. My questions are:
1- Can autodock support more than 6 different atom types per ligand
2- Am I going to have to recompile Autodock in order to be able to use ligands 
with more than 6 atom types.

I will post the answers to the board.

Thank you in advance.

Robert


REPLIES:
Hi Rob,

did you recompile the code...?

i have autodock with up to 15 atomtypes. if you need help to compile or
modify the code please email me and i will send you a patch file.

you need to modify both autodock and autogrid. its best to hack the
files in the src/autodock/autocomm.h and the same for autogrid
respectively

i did the following

#define MAX_MAPS 16 /* Maximum number of energy
maps */
#define ATOM_MAPS 14 /* Number of atomic affinity
grids */




#define NATOMTYPES 15 /* Number of atom types for atomic
interactions */

#define MAX_TYPES 8 /* Maximum number of atom types used. */


then do a make and a make install


cheers

Kim

************************************************************

I solved this problem by re-compiling autodock. The change required is
in the file autocomm.h:

change line: #define ATOM_MAPS 6
to be: #define ATOM_MAPS 8 (or however many you need)

It sounds like you made this change to autocomm.h already. What is then
required is to re-compile the program by typing the command "make".

Susan Heffron

P.S. In my particular case, on an SGI, I had to make the following
changes to the Makefile to get it to run without error messages:

old line: OLIMIT = $(CSTD) $(OPT) # SGI, Sun, HP, Convex,
>...
new line: OLIMIT = $(CSTD) $(OPT) -OPT:Olimit=2442 # Some SGIs.

old line: DBUG = -DNDEBUG # No debugging and no assert code.
new line: DBUG = # Use assert code. 
==========================================================================
Thanks,
Susan Heffron
****************************************

Hi Rob,
I have had the same problem. Infact, htis problem has been discussed about
two weeks ago in CCL.
To answer your questions:
1.No
2.Yes, but you d have to change a great deal of source code, which was, at
least for me, beyond my capabilities of programming.
I talked to the guys of SCRIPPS and they said it would take some efford to
allow more than six atom types, infact they know about this problem. I
couldn t figure out why they didnt allow lets say ten types right away.
Apart from that, AutoDock works really well.

Hope this helps.

Carsten
~~~~~~~~~~~~~~~~~~~~~~~~~~~
Carsten Detering
University of Washington
Seattle, WA 98195
email detering@u.washington.edu
~~~~~~~~~~~~~~~~~~~~~~~~~~~

I solved this problem by re-compiling autodock. The change required is
in the file autocomm.h:

change line: #define ATOM_MAPS 6
to be: #define ATOM_MAPS 8 (or however many you need)

It sounds like you made this change to autocomm.h already. What is then
required is to re-compile the program by typing the command "make".

Susan Heffron

P.S. In my particular case, on an SGI, I had to make the following
changes to the Makefile to get it to run without error messages:

change: OLIMIT = $(CSTD) $(OPT) # SGI, Sun, HP, Convex, ...
to be: OLIMIT = $(CSTD) $(OPT) -OPT:Olimit=2442 # Some SGIs.

change: DBUG = -DNDEBUG # No debugging and no assert code.
to be: DBUG = # Use assert code.

-- ------------------------------------------------------------------
Susan Heffron
Dept. of Physiology and Biophysics University of California, Irvine
Irvine, CA 92697-4560 U.S.A.
phone: (949) 824-4625
FAX: (949) 824-8540
------------------------------------------------------------------

In general, a program must be recompiled whenever changes are made to
any of the *.h files; these are part of the source code.

=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=
Rick Venable 29/500
FDA/CBER/OVRR Biophysics Lab
1401 Rockville Pike HFM-419
Rockville, MD 20852-1448 U.S.A.
(301) 496-1905 Rick_Venable@nih.gov
ALT email: rvenable@speakeasy.org
=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=+=

********************************
Robert Flight
Masters Student
Department of Chemistry
University of New Brunswick
Fredericton, NB  Canada  E3B 6E2
e-mail: L72K6@unb.ca
********************************


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From: atsutoshi konoo <a-konoo@kubota.co.jp>
Date: Wed, 17 Jul 2002 21:55:48 +0900
To: chemistry@ccl.net
Subject: anyone tell me how to build g98 A11 with ifc 6.0 
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hi CCLers


I am  trouble about compiling Gaussian98 Rev A11 with Intel Fortran
Compiler.
Please tell me how to build it with properly.
It's first compilation g98 with ifc for me.


I am using ifc(intel fortran compiler)6.0 evaluate version,and 
it works good.

for building  with ifc,I modified some part of bsd/i386.make like as following.


RUNF77 = ifc
F2CLIB =
LIBS = -lPEPCF90
UNROLL = -unroll
VECTOR = -vec
TWOH =
PC64 =  -pc64
 
and I got build.logs  like as below

-------bldg98.log-------------------------
     .
     .
     .
     .
rm ./as8zmYLF.as

rm ./argt9fLkg.arg

rm -f ml0.f ml0.c
make[1]: Leaving directory `/home/g98'
ifc   -O2 -tp p6  -unroll -vec -D_FILE_OFFSET_BITS=64 -D_LARGEFILE_SOURCE -W0 -v
 -o g98 ml0.o   util.so -lPEPCF90
ifc: warning: -vec is default; use -x and -ax to configure vectorization
ld  \
    /usr/lib/crt1.o \
    /usr/lib/crti.o \
    /opt/intel/compiler60/ia32/lib/crtxi.o \
    -dynamic-linker \
    /lib/ld-linux.so.2 \
    -o \
    g98 \
    ml0.o \
    util.so \
    -lPEPCF90 \
    -Qy \
    /opt/intel/compiler60/ia32/lib/icrt.link \
    -u \
    ___pseudo_link \
    -L/opt/intel/compiler60/ia32/lib \
    -L/usr/lib \
    -Bstatic \
    -lintrins \
    -lIEPCF90 \
    -lF90 \
    -lintrins \
    -limf \
    -Bdynamic \
    -lm \
    -Bstatic \
    -lirc \
    -Bdynamic \
    -lcxa \
    -Bstatic \
    -lcprts \
    -lunwind \
    -Bdynamic \
    -lcxa \
    -Bdynamic \
    -lc \
    /opt/intel/compiler60/ia32/lib/crtxn.o \
    /usr/lib/crtn.o

util.so: undefined reference to `wait_'
util.so: undefined reference to `fork_'
make: *** [g98] Error 1
------------------------------------------

comparing to pgf77 building logs,I found wait_ and fork_ 
is linked pgf77 libs.

if when one use ifc,which libraries must be required?

or,Does anyone know website which has informations about g98 built with ifc?
  
finally,I am sorry for  my silly question.


regards. 


#################################
KGT Inc      systerm service dept
cluster tech group
Atsutoshi Konoo
+81-03-3225-0747                 
a-konoo@kubota.co.jp             
################################# 

--
atsutoshi konoo  a-konoo@kubota.co.jp

From chemistry-request@server.ccl.net Wed Jul 17 01:57:55 2002
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Reply-To: <mark@planaria-software.com>
From: "Mark Thompson" <mark@planaria-software.com>
To: <info@planaria-software.com>
Subject: ArgusLab 3.1 release available !
Date: Tue, 16 Jul 2002 22:59:18 -0700
Message-ID: <000101c22d57$16a59430$0300a8c0@attbi.com>
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*************************************************************
         ArgusLab version 3.1 now available

     Download a full-featured trial version at:
            http://www.arguslab.com
*************************************************************

New features added:

1.  Improved interface in the molecule  builder
2.  Improved for automatically adding bonds
3.  Export images to bitmap, JPEG, and TIFF file formats
4.  Export POV-Ray image files.  (spectacular ray-traced images)
5.  Improved Help System with more Tutorials and FAQs
6.  Improved "clean geometry" will un-flatten rings
7.  Full control over Atom colors
8.  Enter explicit coordinates for atoms from right-click menu
9.  Modify bond lengths from right-click menu
10. Reads older PDB file formats.
11. Lots of bug fixes.


ArgusLab features:
    Extensive support for rendering surfaces.
    Powerful 3D interactive molecule builder.
    Build and optimize structures for the entire periodic table.
    Support for spectroscopy, geometry optimizations, 
                energies, and many properties.
 

=================================
Mark Thompson, Ph.D.
Planaria Software
Seattle, WA. 
http://www.arguslab.com
=================================



From chemistry-request@server.ccl.net Wed Jul 17 10:05:46 2002
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Date: Wed, 17 Jul 2002 16:05:38 +0200
To: atsutoshi konoo <a-konoo@kubota.co.jp>
From: Christoph van =?iso-8859-1?Q?W=FCllen?=  <Christoph.vanWullen@tu-berlin.de>
Subject: Re: CCL:anyone tell me how to build g98 A11 with ifc 6.0
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>hi CCLers
>
>
>I am  trouble about compiling Gaussian98 Rev A11 with Intel Fortran
>Compiler.
>Please tell me how to build it with properly.
>It's first compilation g98 with ifc for me.
>
if wait_ and fork_ are not included in the ifc libs (Try -Vaxlib), then it
is trivial to write a "wrapper" in C (its a one-liner). Wait and Fork are
simply FORTRAN-callable versions of the well-known wait() and fork() 
system calls (look at rs6kdum.F and mdutil.F for hints).

Probably you can use dummies for the first try. I guess that fork() and wait()
are only used in parallel calculations.

+---------------------------------+----------------------------------+
| Prof. Christoph van Wüllen      | Tele-Phone (+49) (0)30 314 27870 |
| Technische Universität Sekr. C3 | Tele-Fax   (+49) (0)30 314 23727 |
| Straße des 17. Juni 135         | eMail                            |
| D-10623 Berlin, Germany         | Christoph.vanWullen@TU-Berlin.De |
+---------------------------------+----------------------------------+


From chemistry-request@server.ccl.net Wed Jul 17 10:36:32 2002
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Date: Wed, 17 Jul 2002 09:36:30 -0500
From: Robert Brunner <rbrunner@uiuc.edu>
To: chemistry@ccl.net
Subject: JMV Molecular Viewer Support within BioCoRE
Message-ID: <20020717093630.A5976@ks.uiuc.edu>
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JMV Molecular Viewer Support within BioCoRE

July 3, 2002:

Urbana, Illinois - The Theoretical Biophysics Group at the University of
Illinois is proud to announce an exciting new feature of BioCoRE, a
Biological Collaborative Research Environment. BioCoRE is freely
accessible at the Theoretical Biophysics Group website and development
is supported by the NIH National Center for Research Resources.

JMV <http://www.ks.uiuc.edu/Development/jmv/> version 1.0 can now be
accessed from within BioCoRE. JMV, a molecular viewer written using Java
and Java 3D, can be used to view molecular files stored within the
BioFS, BioCoRE's shared filesystem. JMV provides several molecular
representations, multiple coloring styles, lighting controls, and
stereoscopic rendering capabilities. Version 1.0 of JMV is currently
only available within BioCoRE, and a standalone release is upcoming.

In addition, several other BioCoRE components have seen key improvements
recently:

* The BioCoRE Control Panel can now be run as a standalone Java
application using Java Web Start. This frees users from the constraints
of running the Control Panel as a Java applet, which allows increased
flexibility and improved robustness since browser crashes no longer kill
the Control Panel.

* Improved overall "look and feel". The BioCoRE web pages no longer rely
on Javascript menus. This makes pages load faster and provides
compatibility with more browsers.

* Users can save JPEG files of states from VMD into BioCoRE
automatically. This allows researchers to browse states visually and
load desired configurations directly into VMD.

* You can now create Interactive accounts within Job Management.
Interactive accounts allow BioCoRE to submit jobs to any computer that
you can log into via SSH. This can be used to run jobs on machines that
BioCoRE doesn't officially support yet. (BioCoRE has built in support
for machines at PSC, NCSA and Globus sites using the Alliance
certificates)

* BioCoRE job management can now upload files to the remote
supercomputer center of your choice before submitting a job. This allows
researchers to keep their input files in the BioCoRE shared filesystem
and let BioCoRE automatically stage the files.


For details, please visit the BioCoRE website at
<http://www.ks.uiuc.edu/Research/biocore/>.

The Theoretical Biophysics group encourages BioCoRE users to be closely
involved in the development process through reporting bugs, contributing
fixes, periodical surveys and via other means. Questions or comments may
be directed to biocore@ks.uiuc.edu.

We are eager to hear from you, and thank you for using our software!




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Subject: G98 B3LYP frequency 
Date: Wed, 17 Jul 2002 09:54:27 -0500
Message-ID: <A29143A40AEAE3459FF829D1DD433161285C65@KC-MAIL2.kc.umkc.edu>
From: "Yang, Shizhong" <sy2b2@umkc.edu>
To: <chemsitry@ccl.net>


Dear CCLers:
  
  I had got two optimized Gaussian98 output files about B3LYP nitrogen and
  silver cluster molecules. But when I try to find the frequency, I got 8
  imaginary frequencies. Did I get the saddle points of the nitrogen and the
  cluster? What should I try next? By the way I donot know why the
  supercomputer's cpu usuage is 97% while memory is only 1.4% at
  most.
   
  Thank you in advance.
  
  Shizhong  Yang
  sy2b2@umkc.edu
  Physics Department
  University of Missouri-Kansas City


From chemistry-request@server.ccl.net Wed Jul 17 12:46:44 2002
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From: miroslavac@health.nb.ca (Miroslava Cuperlovic-Culf)
Subject: isoelectric point
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Dear All,
I am looking for (ideally free) software that can calculate local 
isoelectric point (pI) for amino acids in a relatively large protein 
(~40kDa). Also I would appreciate information about references dealing with 
calculation of reactivity of cysteine residues in proteins.
Thanks a lot for on-going help,
Sincerely
Mira


Miroslava Cuperlovic-Culf
Research Scientist
Beausejour Medical Research Institute
37 Providence Street
Moncton, NB E1C 8X3
Canada
fax: 506-862-4222
tel: 506-862-4848
e-mail: miroslavac@health.nb.ca


From chemistry-request@server.ccl.net Wed Jul 17 13:43:20 2002
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Date: Wed, 17 Jul 2002 13:43:16 -0400 (EDT)
From: Jianquan Chen <jianquan@eden.rutgers.edu>
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To: Carsten Detering <detering@u.washington.edu>
Cc: chemistry@ccl.net
Subject: Re: CCL:Gasteiger charges and Babel
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add -charge switch to babel command line.
Good luck.

jianquan chen
Rutgers Univ.
On Thu, 11 Jul 2002, Carsten Detering wrote:

> Dear CCLers,
> 
> I wonder how it is possible to assign Gasteiger charges to structures with
> Babel. I looked on the web site and in the manual, but couldn't find a hint.
> Would someone be so kind and point out to me how that works??
> Thanks a lot in advance,
> 
> Carsten
> 
> 
> 
> -= This is automatically added to each message by mailing script =-
> CHEMISTRY@ccl.net -- To Everybody  | CHEMISTRY-REQUEST@ccl.net -- To Admins
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> 
> 
> 
> 


From chemistry-request@server.ccl.net Wed Jul 17 15:47:20 2002
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Date: Wed, 17 Jul 2002 15:47:16 -0400 (EDT)
From: "Chun Chung (Jerry) Chan" <chanjcc@speck.niddk.nih.gov>
To: CHEMISTRY@ccl.net
Subject: Sgi workstation for Quanta
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Dear all,

we are considering to buy a new SGI workstation for running Quanta 97. 
Owing to the budget limit, we can only afford the starting configuration
of the Fuel visual workstation (SGI VPro V10 graphics, 32MB of graphics
memory, a 500MHz MIPS R14000A CPU with 2MB L2 cache, and 512MB memory). 
An alternative is to get an O2+ (32 bit) with the best possible
configuration (MIPS@R12000A CPU with 2 MB L2 cache, 1 GB memory). My
question is, does it really worth going for the Fuel visual station (e.g. I 
think a 50% gain in performance does not justify the Fuel)? I would be 
grateful to have your suggestions. 

Regards,
Jerry

*******************************************************************
* Jerry C. C. Chan			      phone: 301-402-4687 *
* Laboratory of Chemical Physics              fax:   301-496-0825 *
* Room 406, Building 5, NIDDK	   http://samson3.uni-muenster.de *
* National Institutes of Health                                   *
* Bethesda, MD20892, USA				          *
******************************************************************* 


From chemistry-request@server.ccl.net Wed Jul 17 13:12:05 2002
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From: eric hu <erichu_linux@yahoo.com>
Subject: cartesian to pdb
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Hi, I wonder if there is an easy way to change the
cartesian coordinates to pdb format. Thanks!

Eric

__________________________________________________
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Yahoo! Autos - Get free new car price quotes
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From chemistry-request@server.ccl.net Wed Jul 17 16:41:15 2002
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Date: Wed, 17 Jul 2002 15:44:33 -0400
From: "Dr. Richard L. Wood" <rlw28@cornell.edu>
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Hi all

I have what I think is a very strange problem.

I'm curently using a "big" version of CHARMm, one that will handle
60,000+ atoms.
I have built a system that consists of a glycosylated peptide having 27
amino acids and
21 mannoses.  The system is solvated with 14,375 TIP3P waters, giving a
total of 43,915
atoms.  When I try and calculate the energy of the system with all the
waters present, the
energy goes through the roof; that is to say, I get stars instead of
numbers for the energy.
However, if I change the number of waters in the lines

READ SEQUENCE TIP3 8844
GENERATE WAT NOANGLE NODIHE

READ SEQUENCE TIP3 5531
GENERATE WAT2 NOANGLE NODIHE

to this:

READ SEQUENCE TIP3 5700
GENERATE WAT NOANGLE NODIHE

CHARMm is able to read the structure in and calculate its energy.

The other way, with 14,375 waters defined in the input file, it will
read the structure in,
but claculates the energy as *********.  I don't want to go with only
5700 waters as my peptide
won't be completely solvated.  With the 14,375 waters, I have a shell
around the peptide about 18 A
thick.

Obviously, I'm under the 60,000 atom limit, but I'm over some other
limit that I'm not aware of.
Has anyone encountered this problem before and how is it handled?

Thank you in advance.

Richard

--
Richard L. Wood, Ph. D.
Physical/Computational Chemist
Post-doctoral Associate
Department of Food Science
120 Stocking Hall
Cornell University, Ithaca, NY 14853





From chemistry-request@server.ccl.net Wed Jul 17 13:59:44 2002
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From: "=?iso-8859-1?Q?Andr=E9_M._de_Oliveira?=" <amolive@dedalus.lcc.ufmg.br>
To: <chemistry@ccl.net>
Subject: CSSR containg charge information
Date: Thu, 1 Jan 1998 01:31:50 -0200
Organization: UFOP
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Dear CCLers,

    Is anyone aware of any free PC-based conversion file able to =
generate CSD CSSR files containing charge information (just like the =
CSSR file from Tsar)?
    BABEL makes this conversion, but only with coordinates. I intend to =
use this format in Somfa calculations.

    Regards.

Andr=E9 Mauricio de Oliveira
------------------------------------------------------------------
N=FAcleo de Estudos em Qu=EDmica Medicinal
Departamento de Qu=EDmica
Universidade Federal de Minas Gerais
VOICE: 55-31-499-5765
FAX: 55-31-499-5700
amolive@dedalus.lcc.ufmg.br
www.qui.ufmg.br/~nequim

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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
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<META content=3D"text/html; charset=3Diso-8859-1" =
http-equiv=3DContent-Type>
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3D"Book Antiqua">Dear CCLers,</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Book Antiqua">&nbsp;&nbsp;&nbsp; Is anyone aware of =
any free=20
PC-based conversion file able to generate CSD CSSR files containing =
charge=20
information (just like the CSSR file from Tsar)?</FONT></DIV>
<DIV><FONT face=3D"Book Antiqua">&nbsp;&nbsp;&nbsp; BABEL makes this =
conversion,=20
but only with coordinates. I intend to use this format in Somfa=20
calculations.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Book Antiqua">&nbsp;&nbsp;&nbsp; =
Regards.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=3D"Book Antiqua">Andr=E9 Mauricio de=20
Oliveira<BR>-------------------------------------------------------------=
-----<BR>N=FAcleo=20
de Estudos em Qu=EDmica Medicinal<BR>Departamento de =
Qu=EDmica<BR>Universidade=20
Federal de Minas Gerais<BR>VOICE: 55-31-499-5765<BR>FAX: =
55-31-499-5700<BR><A=20
href=3D"mailto:amolive@dedalus.lcc.ufmg.br">amolive@dedalus.lcc.ufmg.br</=
A><BR><A=20
href=3D"http://www.qui.ufmg.br/~nequim">www.qui.ufmg.br/~nequim</A></FONT=
></DIV></BODY></HTML>

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From chemistry-request@server.ccl.net Sat Jul 13 12:15:39 2002
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From: Swang Ole <Ole.Swang@sintef.no>
To: "'chemistry@ccl.net'" <chemistry@ccl.net>
Subject: Sorption isotherm simulation
Date: Sat, 13 Jul 2002 18:15:35 +0200


Dear all,
 
I need to perform simulations of isotherms for adsorption in crystalline
microporous materials. Sorption energies are small; in the van der Waals
range. So far, I have used an MC approach, as implemented in the SORPTION
package sold by Accelrys. However, the software only is licensed for an old,
slow workstation used by a number of people, severely limiting my
possibilities. In the literature, most groups appear to use homebrew
software for this kind of work. Some questions:
 
What kind of software is available for this kind of calculations?
Preferrably capable of grand canonical ensemble simulations. Two-body
potentials will be sufficient.
 
MC appears to be the favoured method for sorption calculations. Is simulated
annealing a feasible alternative (I'd probably have to revert to non-grand
canonical ensemble)?
 
Any advice will be highly appreciated. I'll summarize if asked to do so.
 
Thanks in advance,
 
Ole Swang
 
 

From chemistry-request@server.ccl.net Wed Jul 17 20:36:25 2002
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Date: Thu, 18 Jul 2002 10:36:17 +1000 (EST)
From: Paul Darwen <darwen@protagonist.com.au>
To: chemistry@ccl.net
Subject: Problem with Kabsch measure for RMSD on planar molecules
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I have a problem with the Kabsch method of measuring root-mean-square
distance (RMSD) between molecules, as described in Kabsch 1978, Acta 
Cryst A34:827-828.

As far as I can make out, the Kabsch method works so long as three 
or more planes are needed to intersect all the atoms.  This means 
that if a molecule happens to (say) be in a single flat plane, then 
the Kabsch method chokes. 

For example, consider a molecule that's two carbon rings joined by 
a bridge.  This makes it flat.  

Below are two Sybyl2 copies of this molecule, but rotated and translated.
Their root-mean-square distance (RMSD) after alignment should be zero. 

But running Tinker's "superpose" program will align them lengthwise, 
but they're still rotated about the lengthwise axis and not aligned.  
The same thing happens in VMD if you try to align them with the script 
   /usr/local/lib/vmd/scripts/vmd/rmsd.tcl
Both of these incorrectly return an RMSD that's way more than zero. 

Has anyone written an RMSD measure that copes with planar molecules
like this?  If you can run the following two molecules through your 
align-and-measure-RMSD routine and get zero for an answer, I'd be 
grateful for a copy.  

__________________________________________________________________

Paul Darwen                          www.protagonist.com.au/darwen
Protagonist Pty Ltd                      darwen@protagonist.com.au
Brisbane 4064 Australia                     Phone: +61-7-3377-0304


--------------- This is the first of two molecules ---------------

@<TRIPOS>MOLECULE
Bridge bond between two carbon rings
      22      23       1
SMALL
NO_CHARGES

@<TRIPOS>ATOM
       1   C1           1.304260    1.349055   -0.389125   C.2 
       2   C2           1.980455    0.216229   -0.145061   C.2 
       3   C3           1.892984   -0.380446    1.046579   C.2 
       4   C4           1.123138    0.166682    1.990862   C.2 
       5   C5           0.447667    1.299539    1.744975   C.2 
       6   C6           0.512887    1.932896    0.546310   C.2 
       7   H7          -0.161845    1.681260    2.577240   H   
       8   H8           1.043615   -0.318373    2.979753   H   
       9   H9           2.448954   -1.312367    1.248134   H   
      10   H10          2.614125   -0.227590   -0.933089   H   
      11   H11          1.432842    1.773440   -1.395729   H   
      12   C12         -0.113409    3.725645   -0.903027   C.2 
      13   C13         -0.788738    4.858585   -1.148921   C.2 
      14   C14         -1.558584    5.405739   -0.204656   C.2 
      15   C15         -1.646220    4.808998    0.986939   C.2 
      16   C16         -0.970147    3.676100    1.230993   C.2 
      17   C17         -0.178748    3.092243    0.295605   C.2 
      18   H18         -1.098820    3.251664    2.237563   H   
      19   H19         -2.279900    5.252856    1.774946   H   
      20   H20         -2.114383    6.337763   -0.406164   H   
      21   H21         -0.709092    5.343685   -2.137780   H   
      22   H22          0.496097    3.343872   -1.735268   H   

@<TRIPOS>BOND
       1       1       2       1
       2       1       6       1
       3       1      11       1
       4       2       3       1
       5       2      10       1
       6       3       4       1
       7       3       9       1
       8       4       5       1
       9       4       8       1
      10       5       6       1
      11       5       7       1
      12       6      17       1
      13      12      13       1
      14      12      17       1
      15      12      22       1
      16      13      14       1
      17      13      21       1
      18      14      15       1
      19      14      20       1
      20      15      16       1
      21      15      19       1
      22      16      17       1
      23      16      18       1

@<TRIPOS>SUBSTRUCTURE
       1            ****       1


--------------- This is the second of two molecules ---------------

@<TRIPOS>MOLECULE
Bridge bond between two carbon rings
      22      23       1
SMALL
NO_CHARGES

@<TRIPOS>ATOM
       1   C1           0.054840    0.525138   -1.730657   C.2 
       2   C2           1.112013   -0.267815   -1.962393   C.2 
       3   C3           2.327386    0.082664   -1.533765   C.2 
       4   C4           2.474774    1.233137   -0.871667   C.2 
       5   C5           1.416448    2.024847   -0.640943   C.2 
       6   C6           0.167392    1.700650   -1.061558   C.2 
       7   H7           1.626775    2.952893   -0.089236   H   
       8   H8           3.475262    1.532683   -0.512794   H   
       9   H9           3.197548   -0.569107   -1.724045   H   
      10   H10          0.978844   -1.216950   -2.510944   H   
      11   H11         -0.908118    0.160964   -2.117910   H   
      12   C12         -0.802543    3.687019   -0.155836   C.2 
      13   C13         -1.859722    4.479966    0.075891   C.2 
      14   C14         -3.075096    4.129477   -0.352705   C.2 
      15   C15         -3.222482    2.979014   -1.014814   C.2 
      16   C16         -2.164151    2.187340   -1.245587   C.2 
      17   C17         -0.915090    2.511520   -0.824932   C.2 
      18   H18         -2.374444    1.259272   -1.797273   H   
      19   H19         -4.223035    2.679500   -1.373569   H   
      20   H20         -3.945250    4.781258   -0.162414   H   
      21   H21         -1.726500    5.429133    0.624380   H   
      22   H22          0.160424    4.051217    0.231410   H   

@<TRIPOS>BOND
       1       1       2       1
       2       1       6       1
       3       1      11       1
       4       2       3       1
       5       2      10       1
       6       3       4       1
       7       3       9       1
       8       4       5       1
       9       4       8       1
      10       5       6       1
      11       5       7       1
      12       6      17       1
      13      12      13       1
      14      12      17       1
      15      12      22       1
      16      13      14       1
      17      13      21       1
      18      14      15       1
      19      14      20       1
      20      15      16       1
      21      15      19       1
      22      16      17       1
      23      16      18       1

@<TRIPOS>SUBSTRUCTURE
       1            ****       1

--------------- End of the second of two molecules ---------------



From chemistry-request@server.ccl.net Wed Jul 17 19:19:16 2002
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Date: Wed, 17 Jul 2002 19:18:42 -0400
From: "Peter Gannett" <pgannett@hsc.wvu.edu>
To: <chemistry@ccl.net>, <erichu_linux@yahoo.com>
Cc: <pdb-l@rcsb.org>
Subject: Re: CCL:cartesian to pdb
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Eric:

While I'm not exactly sure what your cartesian coordinate file looks
like, you might try babel

http://smog.com/chem/babel/ 

Pete

>>> eric hu <erichu_linux@yahoo.com> 07/17/02 01:12PM >>>
Hi, I wonder if there is an easy way to change the
cartesian coordinates to pdb format. Thanks!

Eric

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