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The journal of observations, given in Table
, summarizes the
spectroscopic and imaging observations carried out with different telescopes
and instrumental setups, and those retrieved from the HST archives.
Table:
Journal of observations
telescope - PA () |
sampling3#3 |
wavelength (Å) |
t
36#36
(s) |
airmass |
|
WHT - 138 |
0.36 |
4757-5141 |
1800 |
1.32 |
|
WHT - 138 |
0.36 |
6493-6881 |
1800 |
1.36 |
|
WHT - 138 |
0.36 |
8506-8882 |
3600 |
1.34 |
|
WHT - 84 |
0.36 |
4757-5141 |
1800 |
1.27 |
|
WHT - 84 |
0.36 |
6493-6881 |
1800 |
1.26 |
|
WHT - 84 |
0.36 |
8506-8882 |
3600 |
1.26 |
|
WHT - 38 |
0.36 |
4757-5141 |
1800 |
1.27 |
|
WHT - 38 |
0.36 |
6493-6881 |
1800 |
1.26 |
|
WHT - 38 |
0.36 |
8506-8882 |
3600 |
1.26 |
|
NOT |
0.18 |
B |
3000 |
1.36 |
|
NOT |
0.18 |
I |
660 |
1.51 |
|
NOT+ARNICA |
0.51 |
J |
1760 (440) |
1.25 |
|
NOT+ARNICA |
0.51 |
Ks |
3520 (880) |
1.5 |
|
3.5m CAHA |
0.32 |
K |
300 |
1.22 |
|
HST - WFPC2 |
0.046 |
V (547M) |
300 |
|
|
HST - NICMOS2 |
0.075 |
J (110W) |
128 |
|
|
HST - NICMOS2 |
0.075 |
H (160W) |
128 |
|
|
3#3 Spatial sampling in arcsec per pixel. The linear dispersion is
0.39 Å pixel-1 for all the spectroscopic observations.
|
Next: Spectroscopy
Up: Circumnuclear structure and kinematics
Previous: Introduction
Enrique Perez
1999-09-29