MTA Monitoring Report 08/07/15 - 08/13/15

Archive of all weekly reports
Archive of monthly reports


Radiation

Quiet

Detrended CTI

Although we prefer to quote CTI values of the cleanest data (FT <= -119.7 C, int time > 7000sec), the data that fulfills these conditions are getting rare. We now quote CTI based on temperature corrected data for Focal plane temperature <= -118.5 C).

The unit is now CTI/year not CTI/day.

Average of ACIS-I CCDs (MnKa) slope: 1.628e-6 CTI/year (4.460e-9 CTI/day)
Detrended slope: 1.561e-6 CTI/year (4.277e-9 CTI/day)

ACIS Warm Pixels

We display all bad pixels that have showed up in past, and, if any, previously unknown bad pixels appeared in the last 14 days. We also list hot pixels (defined as 1000 above the average of bias background). Warm columns 509-514 are probably due to boundaries.

New definitions of warm pixels and flickering pixels (May 15, 2014). If a pixel displays the level beyond a threshold for more than 70% of the time in the past two weeks, the pixel is categorized as a "warm" pixel. If a pixel is above the threshold more than 30% of time but less than 70% of the time in the past two weeks, the pixel is categorized as a "flickering" pixel.

 CCD0CCD1CCD2CCD3CCD4CCD5CCD6CCD7CCD8CCD9
Previously Unknown Bad Pixels                    
Current Warm Pixels     (726,537) (21,95)   (357,303) (369,376) (607,281) (161,206)   (335,412)    
Flickering Warm Pixels (692,141) (667,782) (153,205) (143,700) (427,125) (910,239) (802,665)   (811,637)   (669,577) (263,317) (367,511) (280,313) (258,797) (341,427) (1000,214)   (182,474) (197,241) (356,902) (881,53)  
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates         884 510 512 1022   512 1022    
Flickering Warm Column Candidates                    

ACIS Focal Plane Temperature

For this period, 2 peaks are observed.

Weekly focal plane temperature with sun angle and altitude overplotted. Sun angle is the solar array angle, that is the angle between the sun and the optical axis (+X axis). Altitude varies from 13 kkm to 135 kkm.



SIM Movements

7 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 08/07/15 08/08/15 08/09/15 08/10/15 08/11/15 08/12/15 08/13/15 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
1DAHBCU         0.98 0.36 0.42 (-998)
0.20
(-999)
999
AMP DA HEATER CURRENT B
1DAHBVO         12.82 3.83 4.91 (-998)
1.0
(-999)
999
V DA HEATER VOLTAGE B
1DAHHBVO         28.55 28.55 28.55 (-998)
1.0
(-999)
999
V DA HOUSING HEATER INPUT VOLTAGE B
RSRFALV 190.00 190.00 190.00 190.00 190.00 190.00 190.00 (172.0)
174.0
(171.0)
175.0
V Range switch setting (2RSRFALV)
OHRTHR27 297.34 297.32 297.32 297.31 297.34 297.34 297.32 (295.48)
297.15
(279.37)
307.15
K RT 20 : PERISCOPE
OHRTHR42 294.65 294.65 294.69 294.68 294.68 294.66 294.69 (292.15)
294.37
(279.37)
307.15
K RT 133: PERISCOPE
OHRTHR43 294.71 294.70 294.78 294.78 294.76 294.73 294.81 (291.59)
293.26
(279.37)
307.15
K RT 134: PERISCOPE
TCYLAFT6 310.16         310.16 310.16 (259.93)
309.93
(226.59)
348.82
K CNT CYL TEMP:16-IN FWD OF SC-TS FIT-6


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
16734 ACIS-235678 NONE KS 1731-260 OK OK
17318 ACIS-7 NONE GJ667C OK OK
17710 ACIS-01236 NONE Cygnus A - E Hotspot OK OK
17317 ACIS-7 NONE GJ667C OK OK
16749 ACIS-235678 NONE M28 OK OK
17706 ACIS-235678 NONE KS 1731-260 OK OK
17707 ACIS-235678 NONE KS 1731-260 OK OK
17216 ACIS-01236 NONE CGRaBS J2334+0736 OK OK
17208 ACIS-01236 NONE SPT-CLJ2341-5724 OK OK
17857 ACIS-456789 HETG AX J1745.6-2901 OK OK

Trending

This week's focus is SIM

Last reported on May 14.

Only the most interesting or representative msids are shown below. For a full listing choose the bulletted link.

Min/max envelopes in dark blue appear on the trending plots. The envelopes are 4th degree fits to the monthly minimum and maximum values for each MSID. The final polynomial form and binning are still being experimented with. We will soon add to the trending pages a report of the fits and predictions they give on future limit violations. The light blue curve is our original smoothing of all the data over 30 day moving boxcars. The green/yellow line is a linear fit to all the data; the break occurs at a limit change.




If you have any questions, please contact: swolk@head.cfa.harvard.edu