README file for the NACO SV Seyfert Program

Contact person names: Yann Clénet and Valentin Ivanov
Contact person email addresses: yann.clenet@obspm.fr, vivanov@eso.org
Contact person telephone numbers: 33 1 45 07 75 48 and 56 2 463 3062

Estimated total execution time (excluding overheads): 
	6.7h (3.2 in spectro, 3.4 in imaging)


Program description
===================

Imaging and spectroscopy of Seyfert galaxies in J, H and K bands


OB information
==============

List of OB with associated finding charts
-----------------------------------------

Total number of submitted science OBs: 27
Total number of submitted finding charts: 3

There are three different targets in imaging: NGC 1097 (priority 1)
and NGC 1386 (priority 2) and a calibration star, HD19904, which is
common to the two galaxies For each target, three different bands: K
(priority 1), H (priority 2) and J (priority 3) The associated finding
charts are NGC1097_2MASS_Ks_2p5x2p5_FC.ps,
NGC1386_1mESO_R_2p5x2p5_FC.ps and HD19904_FC.ps The reference source
is the target itself (galaxy nucleus or calibration star) For the 3
targets, a 4-position dithering pattern (twisted diamond) is followed
on the source and on the sky.  For the galaxies, source and sky
exposures are made alternatively while sky exposures are made after
source ones for the calibration stars.  Sky positions is 3' north from
the source positions.  For the positions of the NGC1097 OB: DIT=100 in
J and H (C13 camera), 20 in K (C27 camera), NDIT=3 in J and H, 4 in K
For the positions of the NGC1386 OB: DIT=120 in J and H (C13 camera),
30 in K (C27 camera), NDIT=3 in J and H, 4 in K For the positions of
the HD19904 OB: DIT=0.3 in J and H (C13 camera), 0.2 in K (C27
camera), NDIT=8 in J H and K + a ND

There are three different targets in spectroscopy: 
NGC 7582 (priority 1), NGC 1097 (priority 2) and NGC 1386 (priority 3).

For each target, three different wavelength domains: K (priority 1), H
(priority 2) and J (priority 3) The associated finding charts are
NGC7582_1mESO_R_2p5x2p5_FC.ps, NGC1097_2MASS_Ks_2p5x2p5_FC.ps,
NGC1386_1mESO_R_2p5x2p5_FC.ps The reference source is the nucleus
itself.

There are two slit positions per galaxies to observe structures at:
 PA=244° and 64° for NGC 7582
 PA=54° and -36° for NGC 1097
 PA=1° and -89° for NGC 1386

Two exposures are made with the nucleus along the slit (separated by
1") alternatively with two sky exposures, at 3' north and south from
the nucleus DIT=120 in J (S54_4_SJ mode) and H (S54_3_H mode), 240 in
K (S27_3_SK mode), NDIT=4 for all bands