This table is available for ADQL queries and through the TAP endpoint.
For a list of all services and tables belonging to this table's resource, see Information on resource 'CCD700 Ondrejov Spectra'
To cite the table as such, we suggest the following BibTeX entry:
@MISC{vo:ccd700_data, year=2014, title={{CCD700} Ondrejov Spectra}, author={Stellar Department, Czech Acad. of Sciences}, url={http://vos2.asu.cas.cz/tableinfo/ccd700.data}, howpublished={{VO} resource provided by the {AIASCR} VO Services} }
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Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
accref | Product key | Access key for the data | N/A | meta.ref.url;meta.dataset |
accsize | File size | Size of the data in bytes | byte | VOX:Image_FileSize |
dej2000 | Dej2000 | Main value of declination | N/A | pos.eq.dec;meta.main |
detector | Detector | Detector used to capture spectrum | N/A | N/A |
embargo | Embargo ends | Date the data will become/became public | a | N/A |
expval | ExpVal | Photon counts (Mcount) | N/A | N/A |
grat_angle | Tilt | Grating tilt | deg | N/A |
instrument | Instrument | Instrument used to capture spectrum | N/A | N/A |
mhjd | MHJD | Heliocentric Julian Date | N/A | N/A |
mime | Type | MIME type of the file served | N/A | N/A |
obj_name | Object standard name | Unique identifier of 1 object. | N/A | N/A |
observer | Observer | N/A | N/A | N/A |
owner | Owner | Owner of the data | N/A | N/A |
raj2000 | Raj2000 | Observed RA of the object | N/A | pos.eq.ra;meta.main |
spg_setup | Spectrograph Setup | Spectrograph setup (Dichroic mirror/Spectral filter) | N/A | N/A |
ssa_aperture | Aperture | Angular diameter of aperture | deg | instr.fov |
ssa_bandpass | Bandpass | Bandpass (i.e., rough spectral location) of this dataset; use something generic like 'Optical' here. | N/A | instr.bandpass |
ssa_cdate | Proc. Date | Processing/Creation date | N/A | time;meta.dataset |
ssa_creatorDID | C. DID | Dataset identifier assigned by the creator | N/A | meta.id |
ssa_cversion | C. Version | Creator assigned version for this dataset (will be incremented when this particular item is changed). | N/A | meta.version;meta.dataset |
ssa_dateObs | Date Obs. | Midpoint of exposure | d | time.epoch |
ssa_dstitle | Title | Title or the dataset (usually, spectrum) | N/A | meta.title;meta.dataset |
ssa_length | Length | Number of points in the spectrum | N/A | N/A |
ssa_location | Location | ICRS location of aperture center | deg | pos.eq |
ssa_pdate | Pub. Date | Date last published. | N/A | N/A |
ssa_pubDID | P. DID | Dataset identifier assigned by the publisher | N/A | N/A |
ssa_redshift | z | Redshift of target object | N/A | src.redshift |
ssa_snr | SNR | Signal-to-noise ratio estimated for this dataset | N/A | stat.snr |
ssa_specend | Band end | Upper value of spectral coordinate | m | em.wl;stat.max |
ssa_specext | Bandwidth | Width of the spectrum | m | em.wl;instr.bandwidth |
ssa_specmid | Mid. Band | Midpoint of region covered in this dataset | m | em.wl;instr.bandpass |
ssa_specstart | Band start | Lower value of spectral coordinate | m | em.wl;stat.min |
ssa_targclass | Ob. cls | Object class (star, QSO,...; use Simbad object classification http://simbad.u-strasbg.fr/simbad/sim-display?data=otypes if at all possible) | N/A | src.class |
ssa_targetpos | Obj. pos | Equatorial (ICRS) position of the target object. | N/A | pos.eq;src |
ssa_targname | Object | Common name of object observed. | N/A | meta.id;src |
ssa_timeExt | Exp. Time | Exposure duration | s | time.duration |
telescope | Telescope | Telescope used to capture spectrum | N/A | N/A |
vhelio | Vhc | Heliocentric correction applied on spectrum | N/A | N/A |
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 CCD700 archive contains spectra exposed with 700mm camera of coude spectrograph at Ondrejov observatory 2m Perek telescope, Czech Republic. The spectrograph works in first and second order and typical spectral resolving power is 13000 in first order around Halpha region and twice in Hbeta. The propriatory period is set to one year after the exposure with possible exceptions. All spectra were taken by the team of Stellar department of the Astronomical Institute of the Czech Academy of Sciences, Astronomical Institute of the Faculty of Math anf Physics of Charles University, Prague, and Department of Theoretical Physics and Astrophysics of the Faculty of Science, Masaryk University, Brno. All spectra were reduced in IRAF by M. Slechta. VO technical help by Jiri Nadvornik.
Copyright and such: