[PREVIEW]

Where?DescriptionWhat?
Link

This cube, larger coverage lower resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/COMB/ARP220.COMB.rscube.fits
Link

This cube, smaller coverage higher resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/COMB/ARP220.COMB.rscube.fits
Link

This cube, larger coverage lower resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/COMB/IC1078.COMB.rscube.fits
Link

This cube, smaller coverage higher resolution

#counterpart
ivo://org.gavo.dc/~?califa/datadr3/COMB/IC1078.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/ARP220.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/ARP220.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/IC1078.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/IC1078.COMB.rscube.fits
Link (141 MiB)

The full dataset.

#this
ivo://org.gavo.dc/~?califa/datadr3/COMB/ARP220.COMB.rscube.fits
Link

A preview for the dataset.

#preview
ivo://org.gavo.dc/~?califa/datadr3/COMB/ARP220.COMB.rscube.fits
Link (132 MiB)

The full dataset.

#this
ivo://org.gavo.dc/~?califa/datadr3/COMB/IC1078.COMB.rscube.fits
Link

A preview for the dataset.

#preview
ivo://org.gavo.dc/~?califa/datadr3/COMB/IC1078.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 23.49416745000268 and 23.513889671631148

 deg

The latitude coordinate

RA An interval (space-separated pair of numbers), where the limits have to be between 233.72682456998362 and 233.74984742014138

 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: 233.7268262931 23.49416745 233.72682457 23.5138896716 233.7498474201 23.5138896716 233.7498456971 23.49416745

 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: 233.7384874497 23.5038900947 0.0146414184

 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 77

 

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 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.

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 9.345661919584932 and 9.365384212189866

 deg

The latitude coordinate

RA An interval (space-separated pair of numbers), where the limits have to be between 224.10967737580071 and 224.12966603314717

 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: 224.1096780143 9.3456619196 224.1096773758 9.3653841412 224.1296660331 9.3653842122 224.1296655383 9.3456619904

 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: 224.119812502 9.3553843173 0.0141421354

 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 72

 

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 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.