[PREVIEW]

Where?DescriptionWhat?
Link

This cube, larger coverage lower resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
Link

This cube, smaller coverage higher resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
Link (10 kiB)

This cube in Data Release 2 medium resolution (V1200)

#old-version
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
Link (10 kiB)

This cube in Data Release 2 low resolution (V500)

#old-version
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
(Form)

The Calar Alto Legacy Integral Field Area (CALIFA) survey provides spatially resolved spectroscopic information for 667 galaxies, mainly within the local universe (0.005 < z < 0.03). CALIFA data was obtained using the PPAK integral field unit (IFU), with a hexagonal field-of-view of 1.3 square arcmin, with a 100% covering factor by adopting a three-pointing dithering scheme. has been taken in two setups: V500 (6 ? bin size, 646 galaxies) and V1200 (2.3 ? bin size, 484 galaxies). A final product ("COMBO") combining both data sets, covering 3700-7500 ? at 6 ? bin size, is made availble for 484 galaxies. CALIFA is a legacy survey, intended for the community. This is the (final) Data Release 3.

#proc
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
(Form)

The Calar Alto Legacy Integral Field Area (CALIFA) survey provides spatially resolved spectroscopic information for 667 galaxies, mainly within the local universe (0.005 < z < 0.03). CALIFA data was obtained using the PPAK integral field unit (IFU), with a hexagonal field-of-view of 1.3 square arcmin, with a 100% covering factor by adopting a three-pointing dithering scheme. has been taken in two setups: V500 (6 ? bin size, 646 galaxies) and V1200 (2.3 ? bin size, 484 galaxies). A final product ("COMBO") combining both data sets, covering 3700-7500 ? at 6 ? bin size, is made availble for 484 galaxies. CALIFA is a legacy survey, intended for the community. This is the (final) Data Release 3.

#proc
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
Link (137 MiB)

The full dataset.

#this
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits
Link

A preview for the dataset.

#preview
ivo://org.gavo.dc/~?califa/datadr3/COMB/UGC12519.COMB.rscube.fits

CALIFA Cube Datalink Service

The Calar Alto Legacy Integral Field Area (CALIFA) survey provides spatially resolved spectroscopic information for 667 galaxies, mainly within the local universe (0.005 < z < 0.03). CALIFA data was obtained using the PPAK integral field unit (IFU), with a hexagonal field-of-view of 1.3 square arcmin, with a 100% covering factor by adopting a three-pointing dithering scheme. has been taken in two setups: V500 (6 Å bin size, 646 galaxies) and V1200 (2.3 Å bin size, 484 galaxies). A final product ("COMBO") combining both data sets, covering 3700-7500 Å at 6 Å bin size, is made availble for 484 galaxies. CALIFA is a legacy survey, intended for the community. This is the (final) Data Release 3.

DEC An interval (space-separated pair of numbers), where the limits have to be between 15.944056961219744 and 15.963501448436203

 deg

The latitude coordinate

RA An interval (space-separated pair of numbers), where the limits have to be between 350.00039483228625 and 350.0220637828915

 deg

The longitude coordinate

BAND An interval (space-separated pair of numbers), where the limits have to be between 3.701e-07 and 7.501e-07

 m

Vacuum wavelength limits

POS

 

Region to (approximately) cut out, as Circle, Region, or Polygon

POLYGON A shape on the sky (space-separated numbers in degrees). Maximum extent: 350.0003959253 15.9440569612 350.0003948323 15.9635014051 350.0220637829 15.9635014484 350.0220627739 15.9440570045

 deg

A polygon (as a flattened array of ra, dec pairs) that should be covered by the cutout.

CIRCLE A shape on the sky (space-separated numbers in degrees). Maximum extent: 350.0113737815 15.9536405869 0.0144451119

 deg

A circle (as a flattened array of ra, dec, radius) that should be covered by the cutout.

PIXEL_1 An interval (space-separated pair of numbers), where the limits have to be between 1 and 76

 

Pixel coordinate along axis 1

PIXEL_2 An interval (space-separated pair of numbers), where the limits have to be between 1 and 71

 

Pixel coordinate along axis 2

PIXEL_3 An interval (space-separated pair of numbers), where the limits have to be between 1 and 1901

 

Pixel coordinate along axis 3

KIND Select zero, one, or possibly more options

 

Set to HEADER to retrieve just the primary header, leave empty for data.