MTA Monitoring Report 12/16/16 - 12/22/16

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: 1.252e-02 CTI/year (3.429e-05 CTI/day)
Detrended slope: 1.527e-02 CTI/year (4.183e-05 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) (847,364) (21,95)   (357,303) (369,376) (669,577) (263,317) (367,511) (161,206)   (335,412)    
Flickering Warm Pixels (692,141) (153,205) (143,700) (910,239) (802,665) (526,66)     (607,281) (282,385) (792,313) (280,313) (258,797) (341,427) (1000,214)   (182,474) (197,241) (139,109)  
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates           510 512 1022   512 1022    
Flickering Warm Column Candidates                    

ACIS Focal Plane Temperature

For this period, 6 peaks are observed.

Weekly focal plane temperature with sun angle, earth angle, and altitude overplotted. Sun angle is the solar array angle, that is the angle between the sun and the optical axis (+X axis). The earth angle is the angle between earth and the ACIS radiator (+Z axis). Altitude varies from 34 kkm to 128 kkm.



SIM Movements

15 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 12/16/16 12/17/16 12/18/16 12/19/16 12/20/16 12/21/16 12/22/16 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
HRMACAV         (284.85)     (293.4)
294.8
(292.8)
295.5
TEMP # HRMA CAVITY AVG
MZOBACONE (221.33)           (221.33) (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
MZOBACONE 303.19           303.12 (260.2)
303.0
(250.2)
308.0
CONE # -Z SIDE OBA
TFTERANGE (0.00) (0.00)   (0.00)   (0.00) (0.00) (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
TFTERANGE 35.31 35.51 34.52 35.46 35.40 35.76 35.49 (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
5EPHINT 340.67 342.97 337.39 343.64 342.31 345.63 342.97 (261.15)
300.15
(258.15)
303.15
K #EPHIN TEMP
HKP5V (5.06) (5.06)   (5.06) (5.06) (5.06) (5.06) (5.08)
5.15
(5.06)
5.17
V #HK 5 Volts Rail - Voltage
HKEBOXTEMP 346.29 349.02 343.76 349.02 347.63 350.47 349.02 (268.15)
336.15
(253.15)
346.15
K #EPHIN HOUSEKEEPING EBOX: TEMPERATURE (5EHSE300)
IMHVLV (99.00) (99.00) (99.00) (99.00) (99.00) (80.00) (80.00) (126.0)
128.0
(125.0)
129.0
(2IMHVLV) #Imaging bot MCP HV monitor
IMHBLV (105.00) (105.00) (105.00) (105.00) (105.00) (87.00) (87.00) (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
SPHBLV             (78.00) (79.0)
128.0
(78.0)
129.0
(2SPHBLV) #Spect bot and top MCP HV monitor
S2HVLV (83.00) (83.00) (83.00) (83.00) (83.00) (64.00) (82.00) (126.0)
128.0
(125.0)
129.0
(2S2HVLV) #Shield PMT 2 HV monitor
SPINATM (-30.96)             (-12.0)
35.0
(-15.0)
40.0
C #Spect det temperature (2SPINATM)
LVPLATM (-51.40)             (-32.0)
50.0
(-35.0)
55.0
C #LVPS plate temperature (2LVPLATM)
SMTRATM 55.20             (-17.0)
45.0
(-20.0)
50.0
C #Selected motor temperature (2SMTRATM)
3TSMXCET 280.77 280.77 280.77 280.77 280.77 280.77 283.26 (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 318.18 318.18 318.18 320.68 318.18 318.18 318.18 (203.15)
283.15
(148.15)
353.15
K #-X TURTLE SHELL NR ACIS SS
ELBV (27.73) (27.58) (27.73) (27.58) (27.73) (27.73) (27.58) (28.0)
32.5
(25.0)
34.6
V #LOAD BUS VOLTAGE
4PRT3AT (258.46) (259.14) (259.14) (258.46) (259.14) (258.46) (258.46) (273.15)
283.15
(53.15)
368.15
K #IP A: PRE-COLLIMATOR PRT 3 TEMPERATURE


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
19393 ACIS-5678 NONE NGC 4654 OK OK
19745 ACIS-7 NONE PG 1302-102 OK OK
17529 ACIS-01236 NONE Cygnus A - E Hotspot OK OK
18939 ACIS-235678 NONE 2MASS J20403364+1529572 OK OK
19510 ACIS-3678 NONE 4C +18.45 OK OK
18278 ACIS-01235 NONE Abell 586 OK OK
18938 ACIS-235678 NONE 2MASS J14211512-0107199 OK OK
19025 ACIS-35678 NONE PS11kj OK OK
19324 ACIS-235678 NONE NGC5557 OK OK
19961 ACIS-01235 NONE Abell 586 OK OK
19962 ACIS-01235 NONE Abell 586 OK OK
19386 ACIS-5678 NONE NGC 4527 OK OK
18942 ACIS-235678 NONE 2MASS J16492028+5101177 OK OK
19323 ACIS-235678 NONE NGC5493 OK OK
19963 ACIS-01235 NONE Abell 586 OK OK
19618 ACIS-7 NONE RXJ1131-1231 OK OK
17519 ACIS-01236 NONE Cygnus A - W Hotspot OK OK
19567 ACIS-23567 NONE 3C 129.1 OK OK
17221 ACIS-01236 NONE Abell 1795 outskirts OK OK
18952 HRC-I NONE IGR J00370+6122 OK OK
19965 ACIS-3567 NONE 3C 129.1 OK OK
18935 ACIS-5678 NONE 2MASS J06170531+8353354 OK OK
19638 ACIS-23678 NONE Q2237+0305 OK OK

Trending

This week's focus is PCAD

Last reported on Sep 29.

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