PPAKM31 – Optical Integral Field Spectroscopy of Star-Forming Regions in M31

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 Hβ, [OIII]5007, Hα, [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.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/ppakm31/q/pub
Related Identifier http://dc.zah.uni-heidelberg.de/browse/ppakm31/q
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/ppakm31/q/pub
Provenance
Creator Kreckel, K.; Tomičić, N.; Sandstrom, K.; Groves, B.
Instrument Potsdam Multi-aperture Spectrophotometer (PMAS) with the PPaK fiber-bundle
Publisher The GAVO DC team
Publication Year 2020
OpenAccess true
Contact GAVO Data Centre Team <gavo(at)ari.uni-heidelberg.de>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Physics
Temporal Coverage 2011-09-15T12:00:00Z 2011-09-15T12:00:00Z