This table is available for ADQL queries and through the TAP endpoint.
Resource Description:
The images in this collection were acquired to monitor selected sky fields around eclipsing binary stars at the Kolonica Observatory, Slovakia.
The Kolonica Observatory is located on the Kolonica Saddle and is operated by the Vihorlat Observatory in Humenné. It lies in the northeastern part of Slovakia, within the Poloniny Dark-Sky Park, a location with the darkest night skies in Slovakia and among the darkest in Europe.
Two small telescopes were used to obtain the images in this collection. The first telescope, named ZIGA (PlaneWave CDK20 — Corrected Dall–Kirkham), has a 508 mm aperture and is equipped with a Moravian Instruments G4-16000 CCD camera and UBVRI Bessell photometric filters. The second telescope, named Alica (Explore Scientific MN-152 — Maksutov–Newton), has a 152 mm aperture and is equipped with a Moravian Instruments G2-8300 CCD camera and g′ r′ i′ Sloan photometric filters. Both telescopes are currently in operation, and the archive is expected to be updated with new data.
We publish the photometric time series derived from these images in the upjs_ts collection.
For a list of all services and tables belonging to this table's resource, see Information on resource 'Images From Kolonica Observatory'
Resource Reference URL: Resource info
This table has an associated publication. If you use data from it, it may be appropriate to reference Parimucha, S., in prep. either in addition to or instead of the service reference.
To cite the table as such, we suggest the following BibTeX entry:
@MISC{vo:upjs_img_main,
year=2025,
title={Images From Kolonica Observatory},
author={{UPJŠ}},
url={https://skvo.science.upjs.sk/tableinfo/upjs_img.main},
howpublished={{VO} resource provided by the Pavol Josef Šafárik University Archive}
}
Sorted alphabetically. [Sort by DB column index]
| Name | Table Head | Description | Unit | UCD |
|---|---|---|---|---|
| access_estsize | Size | Estimated size of data product | kbyte | phys.size;meta.file |
| access_format | Media Type | MIME type of the resource at access_url | N/A | meta.code.mime |
| access_url | Access URL | The URL at which to obtain the data set. | N/A | meta.ref.url |
| bandpass_id | Bandpass | Free-form name of the bandpass (filter, detector, whatever else defines the spectral response) this observation was taken in. | N/A | instr.bandpass |
| calib_level | Calibration level | Amount of data processing that has been applied to the data [Note calib] | N/A | meta.code;obs.calib |
| dataproduct_subtype | Subtype | Data product specific type | N/A | meta.code.class |
| dataproduct_type | Product type | High level scientific classification of the data product, taken from an enumeration | N/A | meta.code.class |
| em_max | λ_max | Maximal wavelength represented within the data set | m | em.wl;stat.max |
| em_min | λ_min | Minimal wavelength represented within the data set | m | em.wl;stat.min |
| em_res_power | λ/Δλ | Spectral resolving power lambda/delta lambda | N/A | spect.resolution |
| em_ucd | Spect. UCD | Nature of the product's spectral axis (typically, em.freq, em.wl, or em.energy) | N/A | meta.ucd |
| em_xel | |λ| | Number of elements (typically pixels) along the spectral axis. | N/A | meta.number |
| facility_name | Facility | Name of the facility at which data was taken | N/A | meta.id;instr.tel |
| instrument_name | Instrument | Name of the instrument that produced the data | N/A | meta.id;instr |
| o_ucd | Obs. UCD | UCD for the product's observable | N/A | meta.ucd |
| obs_collection | Collection | Name of a data collection (e.g., project name) this data belongs to | N/A | meta.id |
| obs_creator_did | Creator DID | Dataset identifier assigned by the creator. | N/A | meta.id |
| obs_id | Obs. Id | Unique identifier for an observation | N/A | meta.id |
| obs_publisher_did | Pub. DID | Dataset identifier assigned by the publisher. | N/A | meta.ref.ivoid |
| obs_title | Title | Free-from title of the data set | N/A | meta.title;obs |
| pol_states | Pol. States | List of polarization states in the data set | N/A | meta.code;phys.polarization |
| pol_xel | |Pol| | Number of elements (typically pixels) along the polarization axis. | N/A | meta.number |
| s_dec | Dec | Dec of (center of) observation, ICRS | deg | pos.eq.dec |
| s_fov | FoV | Approximate spatial extent for the region covered by the observation | deg | phys.angSize;instr.fov |
| s_pixel_scale | Pix. Scale | Sampling period in world coordinate units along the spatial axis | arcsec | phys.angSize;instr.pixel |
| s_ra | RA | RA of (center of) observation, ICRS | deg | pos.eq.ra |
| s_region | coverage | Region covered by the observation, as a polygon | N/A | pos.outline;obs.field |
| s_resolution | Space Res. | Best spatial resolution within the data set | arcsec | pos.angResolution |
| s_xel1 | |X| | Number of elements (typically pixels) along the first spatial axis. | N/A | meta.number |
| s_xel2 | |Y| | Number of elements (typically pixels) along the second spatial axis. | N/A | meta.number |
| source_table | Source Table | Name of a TAP-queriable table this data originates from. This source table usually provides more information on the the data than what is given in obscore. See the TAP_SCHEMA of the originating TAP server for details. | N/A | meta.id;meta.table |
| t_exptime | Exp. Time | Total exposure time | s | time.duration;obs.exposure |
| t_max | Max. t | Upper bound of times represented in the data set | d | time.end;obs.exposure |
| t_min | Min. t | Lower bound of times represented in the data set | d | time.start;obs.exposure |
| t_resolution | Res. t | Minimal significant time interval along the time axis | s | time.resolution |
| t_xel | |t| | Number of elements (typically pixels) along the time axis. | N/A | meta.number |
| target_class | Target Class | Class of the target object (star, QSO, ...) | N/A | src.class |
| target_name | Target Name | Object a targeted observation targeted | N/A | meta.id;src |
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.
The calib_level flag takes the following values:
| 0 | Raw Instrumental data requiring instrument-specific tools |
| 1 | Instrumental data processable with standard tools |
| 2 | Calibrated, science-ready data without instrument signature |
| 3 | Enhanced data products (e.g., mosaics) |