README web version of /home/usg/OPS/MTS/readme_xml/readme_83027902
Principal Investigator Email Address
Estimated Total Execution Time (hours, including overheads)
General Description
Our observations aim at resolving the nuclear star cluster in the bulgeless
galaxy NGC 3621.
This is the closest late type, bulgeless galaxy known to host both a nuclear star
cluster and a confirmed AGN.
The observations will yield a spatially resolved spectrum of this nuclear star cluster
from which we will determine its stellar populations and kinematics. Modeling of
these data will (1) strongly constrain the formation history for this NC, and (2)
may well provide the first dynamical black hole mass measurement within a bulgeless
galaxy.
The FLAMES data will be complemented by SINFONI and NACO data.
Target: Nuclear star cluster in NGC 3621
Rmag: 15.7 mag
B-R : 2.1 mag
Kmag: 13.3 mag
FWHM: approx. 0.3 arcsec
For LR 02 : GS=11.5; FACB=12.6,12.9,12.4,12.4; HA=+-7h, S/N=25@427.2nm
For LR 08 : GS=11.5; FACB=12.6,12.9,12.4,12.4; HA=+-7h, S/N=25@881.7nm
At the beginning and at the end of each OB we included a short exposure with a simultaneous
Thorium-Argon calibration lamp on top of our target. This is to enable higher radial
velocity accuracy.
Waiver Requests
Critical Observing Condition Constraints
Time-Critical Aspects
Special Execution Requirements
Special Calibration Information
ToO Information
ToO Activators List
Do all your OBs comply with the instrument-specific requirements listed
on the instrument-specific Phase 2 web page ?
Do all your finding charts comply with both the general and instrument-specific
Phase 2 Web Pages ?
If you submitted OBs for standard stars, did you specify the magnitude
and spectral type of all standard stars in the OBs ?
Have you included OBs for any calibrations that you need but which are
not part of the Calibration Plan ?
If you are observing Moving Targets, have you attached suitable ephemeris
files to your OBs?
If you have preferences which OBs should be executed first, did you make
use of the User Priority field in the OBs ?
If this is a run that requires coordinated observations with other facilities,
did you give proper instructions in the Time-Critical Aspects Section ?
Did you specify in your OBs the hour angle range for which your Target
Setup files are valid ?
Did you specify in your OBs the magnitudes of FACBs and Guide Star for
all your fields ?
Are the FACBs and Guide Star in the brightness ranges specified in the
FLAMES manual ?
Did you enter the expected signal to noise in your OBs ?
Last creation of page: Tue Oct 6 15:40:29 2009
If you have comments, please contact usd-help@eso.org