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XavierHaubois - 02 Jun 2014
Table of L0 metadata (observation logs)to display. Example for the CHARA case:
Those we get from the local observatories servers:
field |
unit |
datatype |
sample |
description |
Notes |
target_name |
|
text |
HD31964 |
Object name |
|
star_type |
|
text |
OBJ |
Calib ou science object ? |
|
obs_id |
|
text |
M6 |
A unique identifier |
obs_creator_name |
|
text |
Theo ten Brummelaar |
instrumentPI (or dataPI when available) |
|
t_min |
[d] |
real |
55141.1 |
Lower bound of times represented in the data set, as MJD |
|
t_max |
[d] |
real |
55141.5 |
Upper bound of times represented in the data set, as MJD |
|
instrument_name |
|
text |
CLIMB |
Name of the instrument (detector) that produced the data |
|
telescope_configuration |
|
text |
S2E1E2W2 |
Telescope configuration |
|
instrument_mode |
|
text |
J |
For CLIMB/CLASSIC: choose among J, H, K-Prime, K-Cont,B-gamma |
|
obs_conditions |
|
text |
|
Summary of the atmospheric turbulence measurements of the night |
Copy-paste from CHARA logs ? With theta_0 in arcsec. |
comments |
|
text |
|
Observing notes |
Notes from CHARA REPORT |
Those we can deduce from the above: