To the extent possible under law, the publisher has waived all copyright and related or neighboring rights to the HDAP scans. For details, see the Creative Commons CC0 1.0 Public Domain dedication. Of course, you should still give proper credit when using this data as required by good scientific practice.
![[CC0]](/static/img/cc0.png)
Table Description:
This table is available for ADQL queries and through the TAP endpoint.
Resource Description:
For a list of all services and tables belonging to this table's resource, see Information on resource 'HDAP -- Heidelberg Digitized Astronomical Plates'
This table has an associated publication. If you use data from it, it may be appropriate to reference http://www.lsw.uni-heidelberg.de/projects/scanproject either in addition to or instead of the service reference.
To cite the table as such, we suggest the following BibTeX entry:
![[Operator logo]](/static/img/logo_medium.png){kind=logo}
@MISC{vo:lsw_wolfpalisa,
year=2007,
title={{HDAP} -- Heidelberg Digitized Astronomical Plates},
author={Mandel, H. and Birkle, K. and Demleitner, M. and Landessternwarte Heidelberg},
url={http://dc.zah.uni-heidelberg.de/tableinfo/lsw.wolfpalisa},
howpublished={{VO} resource provided by the {GAVO} Data Center},
doi = {10.21938/haTEMZmoaCTEK6XZvGU.fQ}
}
To the extent possible under law, the publisher has waived all copyright and related or neighboring rights to the HDAP scans. For details, see the Creative Commons CC0 1.0 Public Domain dedication. Of course, you should still give proper credit when using this data as required by good scientific practice.
The scanning of the plate archive at Landessternwarte Heidelberg was initiated by Holger Mandel and Kurt Birkle in 2006 and was funded by the Klaus-Tschira-Foundation. Almost all usable direct plates in the archives are now scanned, and the funded phase of the project is over. Only minor additions are expected any more.
The plate archive consists of plates from many different sources. The following table gives an overview of the instruments at which the plates were taken:
| plate letter | name | eff. focal length [mm] | aperture ratio | scale [as/mm] | plate size | latitude | longitude | height |
|---|---|---|---|---|---|---|---|---|
| A | Calar Alto Schmidt telescope | 2400 | f/3 | 86 | 24x24cm | 37.22417 N | +2.5375 W | 2168 m |
| B | Königstuhl Bruce telescope | 2000 | f/5 | 103 | 24x30cm or 30x30cm | 49.39861 N | -8.72083 E | 560 m |
| C | 1.23m in Casseg. focus with corrector | 9857 | f/8 | 20.9 | 24x24cm | 37.22361 N | +2.5461 W | 2138 m |
| D | 72cm Walz- Reflektor | 2815 | f/3.9 | 73.3 | 13x18cm or 9x12cm | 49.39861 N | -8.72083 E | 560 m |
| E | 2.2m in Cassegrain focus with corrector | 17037 | f/7.744 | 12.1 | 20x25cm (8x10in) or 24x24 cm | 37.22361 N | +2.5461 W | 2138 m |
| F | 3.5m in primary focus with 3-lens corrector | 13761 | f/3.93 | 15 | 20x25cm (8x10in) | 37.22361 N | +2.5461 W | 2138 m |
| F | 3.5m in primary focus with 2-lens corrector | 12195 | f/3.48 | 16.9 | 12.5x20 (5x8in) | 37.22361 N | +2.5461 W | 2138 m |
| H | 2.2m MPG ESO/La Silla | 17679 | f/8 | 12 | 20x25cm | -29.257225 S | +70.734595 W | 2335 m |
| G | Wolf's Doppel- astrograph (15cm) on Königstuhl (7/1897-1909) | 900mm | f/6 | 230 | 13x18cm or 9x12cm | +49.39861 N | -8.72083 E | 560m |
| G | Wolf's Doppel- astrograph (15cm) in Märzgasse (1887-7/1897) | 900mm | f/6 | 230 | 13x18cm or 9x12cm | +49.60988 N | -8.69387 E | 110m |
Unfortunately, instrument data on the 2.2m MPG telescope on La Silla are lost. If anyone can help out, please contact gavo@ari.uni-heidelberg.de.
The Observation logs of the more ancient observations are available from UB Heidelberg.
The project was discussed on a poster shown at the 2007 meeting of the Astronomische Gesellschaft in Würzburg.
A slightly more technical article appeared in the proceedings of the 2014 Astroplate conference.
This is what the photographic plates these scans were prepared from look like --
The archive of plates from Wolf's eight-inch telescope --
The Bruce archive -- the rack's bend indicates the plates are kept beneath an observatory dome --
The scanner used by this project (Heidelberg Nexscan F4100; the resolution is 100 pixels per millimeter at 200 pixels per millimeter optical scanner resolution) --
Sorted alphabetically. [Sort by DB column index]
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| plateID | Plate | Plate name as specified in observation catalogue | N/A | N/A |
| w_p_id | Wolf-Palisa | Plate number in the Wolf-Palisa survey | N/A | meta.id |
Columns that are parts of indices are marked like this.
The following services may use the data contained in this table:
VO nerds may sometimes need VOResource XML for this table.