WEBDA Interrogation
Contents
- Query design
- Cluster selection
- Cluster page
- Bibliography
- Data sources
- Cross-identifications
Query design
The database access provided by the channel Information has its
limitations, when one needs to form a sample of open clusters fulfilling
different criteria. Therefore, an access to the database is proposed through
different forms. This will produce lists of open clusters, with their
parameters. The cluster names are linked to the cluster pages from where
most information can be reached.
However, no facilities is yet proposed to search all clusters in the database
for some characteristics, or, for example, to list all stars in open clusters
that are brighter than a given magnitude.
Cluster selections
Three forms are proposed to perform selections on the general database
contents according to:
- the quantity of available data.
- This is mostly useful to identify the clusters with the largest
number of observations for a given project or to locate the clusters
requiring modern observations and prepare an observing program.
- the cluster parameters.
- Cluster parameters include coordinates, distances, ages and diameters.
- easons to do selections on the cluster parameters are the same as
those described in the previous item.
- the cluster names
- This permits to display the properties of all the clusters in the list
of any author, like, for example, Trumpler or Stock.
Another facility, based on forms,
is offered to graphically select clusters from plots of their positions in the sky,
either in equatorial or in galactic coordinates, or from their distance to the Sun or
from the galactic plane. The plotted maps are active and information on the selected
clusters can be obtained simply by clicking on the cluster representation.
How to perform selections
- A) On the quantity of available data
- 1) Select the kind of selection you want to perform among the three
possibilities:
- more than N stars observed
- less than N stars observed
- between N1 and N2 stars observed
- 2) Enter the limiting value(s) in the corresponding text area.
- 3) Indicate on which type of data the selection should
be made in the last area.
- 4) Press Submit Query to activate the selection.
- B) On the quantity of available data
and cluster parameters
- 1) Enter the lower and upper limits, when relevant,
corresponding to your criteria,
- Any number of parameters can be used simultaneously, but do not fill
both the distance in [pc] and the distance modulus in [mag].
- The right ascension is given in hours and minute with a space, like 11 30
- The declination is entered in a similar fashion: -30 15
- The other parameters require decimal (floating) numbers.
- 2) Select the kind of selection you want to perform among the three
possibilities:
- more than N stars observed
- less than N stars observed
- between N1 and N2 stars observed
- 3) Enter the limiting value(s) in the corresponding text area.
- 4) Indicate on which type of data the selection should
be made in the last area.
- 5) Press Submit Query to activate the selection.
- C) On cluster parameters
- 1) Enter the lower and upper limits, when relevant,
corresponding to your criteria,
- Any number of parameters can be used simultaneously, but do not fill
both the distance in [pc] and the distance modulus in [mag].
- The right ascension is given in hours and minute with a space, like 11 30
- The declination is entered in a similar fashion: -30 15
- The other parameters require decimal (floating) numbers.
- 2) Press Submit Query to activate the selection.
- D) On cluster names
- 1) Enter a name in the text area,
- 2) Press Submit Query to activate the selection.
- E) On colour maps
- 1) Select the plot in the right-hand frame,
- 2) Fill the form:
- Indicate the limits of the plot in the system of coordinates. Both normal
(hour, minute and degree, minute) or decimal (hh.mm, dd.mm) modes can be used.
- If no criteria are gievn for the declination or latitude, a selection is made
with l = 15°.
- Cluster names may be written on the map if the chosen scale is appropriate.
Use the radio buttons to select the desired mode.
Selection of one cluster
If you already know which cluster you are interested in and want to go directly to its page, use the entry labelled
Display the page of the cluster.
Enter its name in the text area and press Return
.
You can use any NGC or IC numbers, anon. designations, Messier names or
IAU official identifications, in upper or lower cases and
with or without space between the name and cluster number. You can also
use the name of nearby clusters, like Hyades and so on.
Examples
- NGC 2516 or NGC 2516 or ngc2516
- IC 2602 or IC2602 or ic2602
- Trumpler 16 or Tr16 or tr 16
- Messier 6 or M6 or m6
- C0424+151
- Hyades or hyades
- Pleiades, Praesepe, Coma, Alpha Persei, Orion, ...
The cluster page displays first the cluster parameters and the adopted numbering system
for the cluster. It then offers various possibilities to query the database.
Query
A) Search by star numbers
The form allows to search the database for the available data (concerning fundamental,
photometric, spectroscopic and miscellaneous data) for several stars at the same time.
To use the query form
- Select one or more data types (multiple selection),
- Enter a list of star numbers,
- Submit query.
The star numbers should be in the adopted numbering system. But it is also possible to
enter star numbers from another numbering system, if it is present in the cross-reference
table. To do that, follow the link cross-reference table author's list located
above the form, and note the column associated with the reference of your list.
Then enter the star number in the form column number:star number.
For example, if your reference corresponds to column 3 and you want to get data for the
star #5, simply write 3:5. Numbering system may be mixed: 3:5 6:4 125 ...
The output will group the data of one kind for all stars. The field labelled Ref
has a link which allows to get the reference of the source for the data.
To perform selection on star numbers use the selection form described below.
B) Selection on data
The form allows to perform selections on the available, for example to list the red
giant stars or select the stars brighter than a given magnitude.
To get more information on this facitility, look at the usage
explanation.
Bibliography query
The bibliography on open clusters covering the period
from 1969 to present days can be accessed either by keywords or by authors'
names.
- A) Query by keywords
- 1) Enter the initial and final years,
- 2) Enter up to three keywords,
- 3) Press Submit Query to activate the query.
- B) Query by authors'names
- 1) Enter up to three astronomer names, separated by
a space,
- 2) Press Submit Query to activate the query.
The "SIMBAD / NED" bibcodes displayed when defined provide a link to
the article abstract from the ADS Abstract Service.
Data sources
A wide access is provided to the data sources to
perform searches on reference numbers,
authors' names or words in the titles. The ouput is a list of references. Links
are provided on each reference to query the ADS Abstract Service.
How to perform a search
- Select ONE type of data in the upper windows. The data types are separated in
three main groups: fundamental data, photometric data and spectroscopic data.
Information on the data types can be obtained by following the link
Datatypes in the bottom of the form.
- Choose on which criterion the search will be done: reference number, author's name
or word in the titles.
- Enter the appropriate information in the text field,
- Press submit query
Cross-identifications
In many clusters, the brighter stars have entries in major astronomical
catalogues. The facility described here the possibility to check if a given star,
say a bright star or a star from the HD catalogue, is located in the field of an
open cluster. The catalogues that can be queried in this way are the BS,
HD, DM, LSS, SAO, GCVS.
If the answer is psitive, the output will give the cluster name and the number
of the star in the adopted numbering system. The link under the cluster name leads
to the cluster page, and that under the star number displays a new form to query the
database for that star. The star number is already entered in the form.
The form page provides a few examples of the accepted syntaxes.
Last modification: 25 October 2005