Science case
------------
We have discovered an extremely compact, luminous starburst nucleus inside a larger,
low-surface brightness galaxy at relatively low redshift (z=0.22). It is believed
that this object resembles typical star-forming galaxies in the early-Universe.
Its low redshift allows us to study in detail many starburst-related processes such
as outflows, low-luminosity AGN, supernovae, burst mass, SFR and age, and extinction.
The broad wavelength coverage of X-Shooter is ideal for targeting the relevant spectroscopic
features that occur throughout the UV, VIS and NIR.
Technical details
-----------------
Granted time: 1h
Slit: 1"
Orientation: 10 degrees from North to East
Nodding on slit (4 arcsec nod-throw)
- 2 cycles (ABBA sequence)
- 1 arcsec jitter box
- 1 UVB, 2 VIS and 3 NIR exposures per position
- integration times 690s in UVB in 1x2 slow, 320s in VIS in 1x2 slow,
and DIT=240s (NDIT=1) in the NIR.
Total Execution Time: 59m24s
Target Acquisition:
-------------------
The target is relatively bright (V~18 mag), and should show up in the acquisition
image since it can also be seen in the DSS finder chart image. Nonetheless, we have
counted on using an offset star for the acquisition:
Target coordinates: 02:13:48.542, +12:59:51.72
Reference star: 02:13:50.10, +13:00:46.69
Offsets RA,DEC: -22.772, -54.965 (arcsec,arcsec)
Two finder charts are given: FC_OBJ.jpg (target) and FC_REF.jpg (reference star).
Centering:
----------
Since the object contains a bright (unresolved) core in the middle of a lower surface
brightness disk, it would be much appreciated if the slit could be centered on the
bright nucleus of highest surface brightness.
Visibility:
-----------
The target is a morning target during August-September.