Where? | Description | What? |
---|---|---|
Link (779 kiB) | A map in Halpha derived from this cube. | #derivation ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link (779 kiB) | A map in Hbeta derived from this cube. | #derivation ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link (779 kiB) | A map in [NII]6583 derived from this cube. | #derivation ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link (779 kiB) | A map in [OIII]5007 derived from this cube. | #derivation ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link (779 kiB) | A map in [SII]6716 derived from this cube. | #derivation ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link (779 kiB) | A map in [SII]6730 derived from this cube. | #derivation ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
(Form) | These observations cover five star-forming regions in the Andromeda galaxy (M31) with optical integral field spectroscopy. Each has a field of view of roughly 1 kpc across, at 10pc physical resolution. In addition to the calibrated data cubes, we provide flux maps of the H?, [OIII]5007, H?, [NII]6583, [SII]6716 and [SII]6730 line emission. Line fluxes have not been corrected for dust extinction. All data products have associated error maps. | #proc ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link (381 MiB) | The full dataset. | #this ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |
Link | A preview for the dataset. | #preview ivo://org.gavo.dc/~?ppakm31/data/PPAK_M31_F4_cube.fits |