Data overview for HE0212-0059


Basic parameters
HES name: | HE0212-0059 |
Alternative name: | Mrk590 |
redshift: | 0.026394 |
type of nucleus: | changing-look AGN |
Morphology | unbarred disc-dominated galaxy |
MB | -21.17 mag |
f0.1-2.4keV | 25.5±0.8×10-12 erg/s/cm2 |
f1.4GHz | 9.90±0.14 mJy |
ICO(1-0) | 3.51±0.11 K km/s |
log(MH2/[M☉]) | 8.55±0.64 |
log(MHI/[M☉]) | 9.79±0.04 |

Telescope: | VLT |
IFU Instrument: | MUSE |
IFU setup: | WFM-NOAO-N |
IFU grating: | |
IFU field-of-view: | 60.0" × 60.0" |
IFU sampling: | 0.2" × 0.2" |
Wavelength coverage: | 4750.0 Å - 9350.0 Å |
Spectral resolution: | 2.4 Å |
Program ID: | 099.B-0249(A) |
Total exposure time: | 7700.0 sec |
Seeing of the observation: | 0.6" |
Absolute photometric scale factor: | 0.97 |
Comments for the observation: | None |
Path to the reduced data cube: | dr1/cubes/HE0212-0059.MUSE.WFM-NOAO.observed.fits.gz |
Path to the AGN data cube: | dr1/cubes/HE0212-0059.MUSE.WFM-NOAO.AGN.fits.gz |
Path to the host galaxy data cube: | dr1/cubes/HE0212-0059.MUSE.WFM-NOAO.Host.fits.gz |
Path to the continuum model data cube: | dr1/cubes/HE0212-0059.MUSE.WFM-NOAO.Host_continuum.fits.gz |
Path to the binned Host data cube: | dr1/cubes/HE0212-0059.MUSE.WFM-NOAO.Host_binned.fits.gz |
Path to the full 2D maps: | dr1/maps/HE0212-0059.MUSE.WFM-NOAO.maps-full.fits |
Path to the binned 2D maps: | dr1/maps/HE0212-0059.MUSE.WFM-NOAO.maps-binned.fits |
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Ionized gas area | 2141.16 arcsec2 | |
SF area fraction | 0.45 | |
inter area fraction | 0.39 | |
LINER area fraction | 0.02 | |
AGN area fraction | 0.03 | |
SFR fraction | ||
SFRHα(HII)/[M☉/yr] | 3.5 ± 0.4 | |
SFRHα(BPT)/[M☉/yr] | 3.4 ± 0.3 | |
RENLR,max | 15.6 ± 0.3 kpc | |
RENLR,16 | 0.5 ± 0.3 kpc | |
RENLR,15 | 0.5 ± 0.3 kpc | |
12+log(O/H) (O3N2 scale) | 8.70 ± 0.00 | |
α/[reff] (O3N2 scale) | -0.019 ± 0.005 | |
12+log(O/H) (T04 scale) | 8.99 ± 0.00 | |
α/[reff] (T04 scale) | -0.050 ± 0.015 |
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![]() Inferred parameters
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Available photometry
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morphology | bar presence | environment | host size | ||||||||||||||||||||||||||||||||||||
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