SMAKCED H-band images of Early-Type Virgo Dwarf Galaxies

The Stellar content, MAss and Kinematics of Cluster Early-type Dwarf galaxies (SMAKCED) project is a survey of 121 Virgo cluster early type galaxies. This service publishes deep near-infrared (H band) images obtained by SMAKCED together with resulting decompositions and other properties of the galaxies in the sample.

A spatial constraint using SIAPv2 CIRCLE, RANGE, or POLYGON shapes and respective values in decimal degrees.
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Wavelength interval that should intersect with the dataset coverage
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Time interval that should intersect with the dataset coverage
Polarisation states as per Obscore (i.e., from the set I Q U V RR LL RL LR XX YY XY YX POLI POLA
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Lower and upper bound for the field of view of the observation
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Lower and upper bound for the spatial resolution of the image(s)
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Lower and upper bound for the spectral resolving power λ/Δλ in spectrally resolved observations
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Lower and upper bound for the integration times of the observation
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Lower and upper bound for the (absolute) resolution on the time axis
A dataset identifier to match. Note that contrary to the SIAP v2 REC, we do not compare the IVOIDs case-insensitively. This should not be an issue if you got the IVOID from this service. For IVOIDs obtained in other ways, you may need to use ILIKE or a similar facility through ObsTAP.
A name of a data collection within the service (use ObsTAP to find out the possible values).
A name of a facility (usually a telescope) used to make the observation.
A name of an instrument used to acquire the data.
Select either image or cube.
Calibration level of the data (0=raw data .. 3=processed science-ready data)
A name of an observation target.
Media type (like application/fits) or similar of the data product searched
No selection matches all, multiple values legal.
VCC identifier (like 'VCC0009')
Sort by
Limit to items.
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