MTA Monitoring Report 02/20/15 - 02/26/15

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: 1.631e-6 CTI/year (4.468e-9 CTI/day)
Detrended slope: 1.555e-6 CTI/year (4.260e-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)       (335,412)    
Flickering Warm Pixels (692,141) (667,782) (153,205) (143,700) (427,125) (910,239) (802,665) (802,665) (910,239) (703,739)   (669,577) (357,303) (369,376) (607,281) (263,317) (161,206) (341,427) (1000,214)   (182,474) (197,241) (356,902) (881,53) (838,239)  
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, 4 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 10 kkm to 135 kkm.



Telemetry

New violations or new extrema are shown in blue cells.

MSID 02/20/15 02/21/15 02/22/15 02/23/15 02/24/15 02/25/15 02/26/15 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
1DAHBCU 0.58         1.94 0.44 (-998)
0.20
(-999)
999
AMP DA HEATER CURRENT B
1DAHBVO 7.67         28.03 5.27 (-998)
1.0
(-999)
999
V DA HEATER VOLTAGE B
1DAHHBVO 27.92         28.08 28.08 (-998)
1.0
(-999)
999
V DA HOUSING HEATER INPUT VOLTAGE B
OHRTHR27 297.34 297.34 297.34 297.34 297.34 297.34 297.34 (295.48)
297.15
(279.37)
307.15
K RT 20 : PERISCOPE
OHRTHR42 294.64 294.65 294.68 294.66 294.66 294.66 294.66 (292.15)
294.37
(279.37)
307.15
K RT 133: PERISCOPE
OHRTHR43 294.68 294.67 294.77 294.67 294.66 294.66 294.67 (291.59)
293.26
(279.37)
307.15
K RT 134: PERISCOPE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
17602 ACIS-012367 NONE 30 Doradus OK OK
16953 ACIS-01236 NONE RXJ0806 OK OK
16977 ACIS-23678 NONE NGC406 OK OK
17600 ACIS-67 HETG Ser X-1 OK OK
17484 ACIS-23678 NONE Xclass 2305 OK OK
17101 ACIS-235678 NONE SDSS J140447.81+053708.2 OK OK
17630 ACIS-456789 HETG 4U1700-37 OK OK
16031 ACIS-23678 NONE NGC 4387 OK OK
17038 ACIS-23678 NONE J160531.84+174826.1 OK OK
17019 ACIS-23678 NONE CXO J150052.1+015453 OK OK
16709 ACIS-456789 HETG GRS 1915+105 CC OK
16261 ACIS-23678 NONE XMMUJ122939.9 +075333 OK OK
17247 ACIS-235678 NONE 3XMM J172805.7-142109 OK OK
15723 ACIS-012367 NONE IC 5146 OK OK
17379 ACIS-3 NONE E0102-72 I3,-120,-0.5,0.5,0 CAL OK
16030 ACIS-3678 NONE NGC 4339 OK OK
17020 ACIS-235678 NONE M67 - S364 OK OK
16536 ACIS-456789 HETG RCW38/IRS2 OK OK

Trending

This week's focus is Spacecraft Bus and Subsystem Trends.

Last reported on Dec 11.

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