[PREVIEW]

Where?DescriptionWhat?
Link

This cube, larger coverage lower resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/V1200/UGC12519.V1200.rscube.fits
Link

This cube, larger coverage lower resolution high-SNR

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/V1200/UGC12519.V1200.rscube.fits
Link (10 kiB)

This cube in Data Release 2 medium resolution (V1200)

#old-version
ivo://org.gavo.dc/~?califa/datadr3/V1200/UGC12519.V1200.rscube.fits
Link (10 kiB)

This cube in Data Release 2 low resolution (V500)

#old-version
ivo://org.gavo.dc/~?califa/datadr3/V1200/UGC12519.V1200.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/V1200/UGC12519.V1200.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/V1200/UGC12519.V1200.rscube.fits
Link (128 MiB)

The full dataset.

#this
ivo://org.gavo.dc/~?califa/datadr3/V1200/UGC12519.V1200.rscube.fits
Link

A preview for the dataset.

#preview
ivo://org.gavo.dc/~?califa/datadr3/V1200/UGC12519.V1200.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 15.943819330871552 and 15.96354156734632

 deg

The latitude coordinate

RA An interval (space-separated pair of numbers), where the limits have to be between 350.000138653268 and 350.02238544700197

 deg

The longitude coordinate

BAND An interval (space-separated pair of numbers), where the limits have to be between 3.65e-07 and 4.839999999999691e-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: 350.0001397619 15.9438193309 350.0001386533 15.9635415525 350.022385447 15.9635415673 350.0223843668 15.9438193457

 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: 350.0114065098 15.9535418456 0.0147431714

 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 78

 

Pixel coordinate along axis 1

PIXEL_2 An interval (space-separated pair of numbers), where the limits have to be between 1 and 72

 

Pixel coordinate along axis 2

PIXEL_3 An interval (space-separated pair of numbers), where the limits have to be between 1 and 1701

 

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.