MIRC/VEGA: Difference between revisions
From Monnier Group Research Wiki
Jump to navigationJump to search
Monnierast (talk | contribs) No edit summary |
Monnierast (talk | contribs) No edit summary |
||
| Line 1: | Line 1: | ||
'''Cophasing of VEGA and MIRC on UT 2010-10-12:''' | '''Cophasing of VEGA and MIRC on UT 2010-10-12: (SK)''' | ||
MIRC ealing mount position after cophasing: | MIRC ealing mount position after cophasing: | ||
| Line 8: | Line 8: | ||
'''Cophasing of VEGA and MIRC on UT 2010-10-13/14:''' | '''Cophasing of VEGA and MIRC on UT 2010-10-13/14: (SK)''' | ||
For the E1-E2-W2-W1 configuration, the MIRC ealing mount positions were still suitable. | For the E1-E2-W2-W1 configuration, the MIRC ealing mount positions were still suitable. | ||
However, when we changed to the S1-S2-W2-W1 configuration and tracked with MIRC, the fringes were somewhat off-centered at VEGA, possibly due to differences in the LDCs of the individual telescopes. | However, when we changed to the S1-S2-W2-W1 configuration and tracked with MIRC, the fringes were somewhat off-centered at VEGA, possibly due to differences in the LDCs of the individual telescopes. | ||
Revision as of 07:14, 15 October 2010
Cophasing of VEGA and MIRC on UT 2010-10-12: (SK)
MIRC ealing mount position after cophasing:
IR1=58350, IR2=65449, IR3=66000, IR4=71600
(Configuration: E1-E2-W2-W1; B1-B2-B3-B4)
Cophasing of VEGA and MIRC on UT 2010-10-13/14: (SK)
For the E1-E2-W2-W1 configuration, the MIRC ealing mount positions were still suitable.
However, when we changed to the S1-S2-W2-W1 configuration and tracked with MIRC, the fringes were somewhat off-centered at VEGA, possibly due to differences in the LDCs of the individual telescopes.
