COS SMOV Morning Update 18 August 2009

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COS SMOV Morning Update
18 August 2009
This presentation contains material that is embargoed until after the SM4
ERO press conference. Images/spectra of external (astronomical) objects
may not be altered, distributed, reproduced, published, displayed, or used in
any other way without the consent of the STScI Director or the HST Project.
1
Agenda
•
•
•
•
Recent Activity
SMOV Program Status
Recent Results and Analysis
Upcoming COS SMOV Timeline
2
Recent Activity
• Friday 14 August (Day 226)
– 11486 visit 09 (FUV Target Acquisitions)
– 11472 visit 05 (NUV Dispersed Light Acquisitions)
• Saturday 15 August (Day 227)
– 11471 visit 03 (NUV Imaging Acquisitions)
– 11486 visit 03 (FUV Target Acquisitions)
• Sunday 16 August (Day 228)
– 11476 visit 02 (NUV External Spectroscopic Perf. I)
• Monday 17 August (Day 229)
– 11492 visit 12 (FUV Spectroscopic Sensitivity)
– 11486 visit 10 (FUV Target Acquisitions)
3
COS SMOV Status
Activity
COS02
COS03
COS04
COS05
COS06
P ropID
11353
11354
11355
11466
11467
Title
Memory Check
Science Data Buffer Check
NU V Initial On-Orbit Turn-On
NU V Darks
NU V Functional Test
PI
Welty
Welty
Welty
Sahnow
Sahnow
COS07
11355, v5
NU V Fold Test
Welty
COS08
COS09
COS10
COS10/COS27
11468
11469
11470
11496
COS to FGS Alignment
NU V Optics Alignment and Focus
NU V Internal Wavelength
Lamp2/GET
Hartig
Hartig
Keyes
Keyes
COS11
COS12
11471
11472
NU V Imaging Target Acquisition
NU V Dispersed Light TA
COS13
COS14
COS15
COS16
11473
11474
11475
11476
NU V
NU V
NU V
NU V
COS17
COS18
11477
11478
COS19
COS20
COS21
COS23
Visits Done
1
14
9
17
1
Total Visits
1
14
9
20
1
Status
Done
Done
Done
Analysis
Done
N/A
Done
6
14
4
3
6
14
4
3
Done
Done
Done
Done
Soderblom
Soderblom
3
2
8
4
Analysis
Analysis
Goodfrooij
Keyes
Keyes
Ghavamian
1
6
4
2
4
7
4
3
Analysis
Analysis
Analysis
Analysis
NU V Spectroscopic Performance II
NU V Flats
Ghavamian
Ake
0
36
3
36
Analysis
11479
11480
11481
11356
NU V Sensitivity
NU V Struc. & Thermal Stability
NU V High S/N Verification
FU V Initial On-Orbit Turn-On
Massa
Smith
Sahnow
Welty
3
0
0
13
5
3
2
13
Analysis
COS24
COS25
COS26
COS27
COS28
COS29
11482
11483
11484
11485
11486
11487
FU V
FU V
FU V
FU V
FU V
FU V
Darks
Functional Test
Optics Alignment and Focus
Internal Wavelength Scale
Dispersed Light TA
Int/Ext Wavelength Scales
Sahnow
Sahnow
Hartig
Keyes
Soderblom
Keyes
18
1
6
1
4
3
20
1
9
1
5
6
Analysis
Done
Waiting for more data
Analysis
Analysis
Analysis
COS30
COS31
COS32
COS33
COS34
11488
11489
11490
11491
11492
FU V
FU V
FU V
FU V
FU V
Internal Wavelength Verf.
Spectroscopic Performance I
Spectroscopic Performance II
Ext Flats
Sensitivity
Keyes
Friedman
Ghavamian
Sahnow
Keyes
4
0
0
0
3
4
3
2
2
7
COS35
COS36
11493
11494
FU V Struc. & Thermal Stability
FU V High S/N Verification
0
0
179
2
2
228
Imaging Performance
Int/Ext Wavelength Scales
Internal Wavelength Verf.
Spectroscopic Performance I
Smith
Sahnow
Done
`
Analysis
Analysis
Analysis
79%
4
FUV Focus Status
• Modeling is underway to simulate the upcoming
focus run using STIS spectrum and raytraced
PSFs.
• Two new targets (Sk-155, WD2218+706) with
STIS spectra chosen to check resolution in
program 11489 (FUV External Spectroscopic
Performance I)
– Updated visits will be submitted soon.
– Plan is to schedule them after the focus adjustment,
early in SMS 243.
5
NUV Sensitivity (11479)
Preliminary Results
• Data for the first three visits, using
GRW+70D5824 and GD71 have allowed us to
derive (preliminary) independent sensitivity
curves for each grating and stripe.
– Similar to prelaunch predictions
• G230L second order contribution still being
quantified (but was expected)
6
Embargoed figure - Do not distribute
NUV Sensitivity (11479)
Preliminary Results
7
FUV Lower HVNom
• New HVNom values loaded last week.
• HV will be cycled early in SMS 236
(HVLow→OPERATE→HVLow) so that the
HVMax values are loaded to the DCE.
• DCE Memory Dump will be done at the same
time to look for evidence of HV Transients.
8
Target Acquisitions
• Initial looks show that dispersed light and imaging
target acquisitions for both channels have been
performing well.
• Two exposures of 1147205 (NUV Dispersed Light
Acquisitions) were lost last weekend due to
missing lock.
– Preliminary analysis indicates we will not have to
repeat them.
9
Upcoming COS SMOV Timeline
• NUV Spectroscopic Sensitivity
– 11479 04 233:15:41 – 233:22:43
• FUV Spectroscopic Sensitivity
– 11492 11 234:04:29 – 234:13:19
• FUV Target Acquisition Algorithm Verification
– 11486 04 234:14:18 – 234:17:31
10
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