For the past several months I've been negotiating with Caltech for "ground
rules" governing use of AXA data by professionals with the intent of publishing
results partly based on AXA data. If you're not interested in the history
then you may skip down to the section, Most Likely Final Version of
Ground Rules.
Submissions of data to the AXA after June 7 have been subject to the following
        agreement for professional use of the data. 
                
There is a general consensus among the active observers contributing
        to                                   the AXA that "we want our data
  to   be   used   for    scientific           purposes."           Therefore,
        on  the web  pages    devoted to  each     BTE    there will be 
 links          to data files    that     have been  converted     to   a
standard   format      by the   AXA    webmaster.   Downloading       of
 these    data    files    is unrestricted.      However,      at the time
 that any  of  these      data files is seriously    contemplated       for
  use  in a publication      we    require    that the   observer be notified,
   either     directly    or via  the    AXA webmaster.        There are
two reasons   for   this.   First,    the  observer    is in   the best 
 position    to know   the   strengths   and weaknesses     of    the data,
and it   is to everyone's       benefit that the   data not  be   over-interpreted.
         Second, every     successful  observation    represents     a lot
 of work, all    of   it   unpaid,   and it is only fair that  the observer
     be aware  of  when    his  data   is being used and for what purpose.
   To   the professional    astronomer     interested   in using the data
may  I suggest     that you    will  want to  learn    such things as  whether
  the  amateur's computer     clock is  automatically   adjusted,   whether
  JD  time  tags do indeed  correspond      to  mid-exposure  time, whether
   the filter  set  is photometric  versus  "pretty     picture"  - and many
  other  things   that relate  to the presence  of "systematics"     that
may  exist in  the  amateur  data that are not likely  to exist for professionally
      produced   data. 
                                                                    
      
The biggest  payoff for an observer would be to learn that their data 
        has    contributed            to the discovery  of another    exoplanet 
        using    TTV,    for example,  or   that     it  was used to   discover 
        a  ring system.    So,    for anyone who  is  incorporating      
  AXA    data files  in a study     that   appears to be leading    to a 
scientific         publication     please   notify the   observer either directly
     or  via  the AXA   webmaster.   At  that time we  can establish  communication
           with the observer   to   negotiate    an appropriate  acknowledgement.
          It is   important  that an   observer  be  aware  of any publication
      that   makes use  of his observations    and that   he be given  an
opportunity         to comment on their use before publication.    
                                                                    
              
I recently asked if the following would be acceptable (in anticipation
        of restrictions that will apply to data files transferred to Caltech's
         NStED/AXA): 
                
Downloading         of amateur data files is
unrestricted. However, in recognition of the    fact    that none of this
data has been described in a publication it is   recommended    that when
amateur data is under serious consideration  for  use by a professional 
  astronomer the amateur observer should be contacted   by e-mail. There
are   two reasons for this. First, the observer is in the   best position
to know   the strengths and weaknesses of the data and it is  in everyone's
best interest    that the data not be over-interpreted. Second,   every successful observation represents   a lot of work,
all    of it unpaid, and it is only fair that the observer   be aware of
when that    data is being used as well as the intended purpose   for its
use. Whereas published data includes   a description
of specific    idiosyncrasies that may be present, unpublished   amateur
data should be described   in the same way before it is used. For   example,
a user should want to know   answers to the following: Did seeing vary significantly  during the observing session, 
  were clouds noted at any time, was it windy  enough to shake the telescope, 
  are time tags  for mid-exposure or exposure 
 start, are the  time tags based on an automatic  computer clock setting program
 or is the  computer clock set manually, was  the filter photometric or "pretty
  picture,"  etc. Any potential problems with  observations would be included
  in a publication  of the data so it is prudent  for any user of unpublished
  data to want answers  to the same questions. If  the amateur data are in
 fact included in a publication  it is requested that  the observer be acknowledged
  by name, and if appropriate  that a brief description  of the hardware
be   included.
Most
Likely Final Version of Ground Rules
                Caltech also wants a version that is much shorter to be
included     in  the data file header lines to improve its visibility. The
following   is  under   consideration:
                
"Downloading of amateur data files is unrestricted. However, since these data are unpublished it is recommended the observer be contacted prior to use of data. The observer may be aware of specific aspects of the data that should be taken into consideration when interpreted, such as seeing, clouds, wind, scintillation, clock-setting procedures, optimized photometry apertures, etc. If these data are to be used in a publication, it is requested that the observer be acknowledged by name along with a brief description of the hardware used."
Also, my NStED contact and I are essentially agreed
      upon the following longer version that will appear on its own web page.
    A  link to it will be present on each data page. 
            
"Downloading of amateur data files is unrestricted.
      However, since none of these data are described in a publication it
is   recommended   that the amateur observer should be contacted by e-mail
(see   header of light   curve for contact information) prior to the use
of the  data in publications.   There are two reasons for this: 
            
First, the observer is best familiar with all
      aspects of the observations and can provide guidance in the interpretation
      of the data. Whereas publications (and associated
      data) include a description of specific data idiosyncrasies that may
 be   present,  unpublished amateur data should be described in the same
way  before   they are used. For example, a user should want to know answers
to  such questions    as the following: Did  seeing vary significantly     during the observing
session? Were clouds noted  at any time? Was it windy     enough to shake
the telescope? Are time tags     for mid-exposure
or exposure start? Are   the time tags based on an automatic     computer
clock setting program, or  is the computer clock set manually?  Any   potential
problems with observations   would be included in a publication   of  the
data so it is prudent for any   user of unpublished data to want answers
    to the same questions.
              
____________________________________________________________________
WebMaster: B.
                                                                 Gary. 
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