MTA Monitoring Report 05/06/16 - 05/12/16

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: 1.255e-02 CTI/year (3.440e-05 CTI/day)
Detrended slope: 1.522e-02 CTI/year (4.170e-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) (21,95)   (357,303) (369,376) (263,317) (161,206) (1000,214) (335,412) (197,241) (881,53) (139,109)  
Flickering Warm Pixels (692,141) (153,205) (143,700) (427,125) (910,239) (802,665)     (419,163) (885,460) (247,364) (607,281) (669,577) (280,313) (367,511) (258,797) (341,427)     (182,474) (150,374) (636,819)
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, 8 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

8 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 05/06/16 05/07/16 05/08/16 05/09/16 05/10/16 05/11/16 05/12/16 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
1PIN1AT 338.52 343.70 341.11 343.70 344.99 341.11 338.52 (-20.0)
30.0
(-36.5)
36.5
C # PSMC TEMP 1A
HRMACAV (284.85)   (284.85)   (284.85) (284.85) (284.85) (293.4)
294.8
(292.8)
295.5
TEMP # HRMA CAVITY AVG
PZOBACONE           (198.92)   (260.2)
303.0
(250.2)
308.0
CONE # +Z SIDE OBA
TFTERANGE (0.00) (0.00) (0.00) (0.00) (0.00) (0.00)   (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
TFTERANGE 35.43 35.22 34.90 35.26 35.19 35.20   (16.7)
34.5
(11.1)
42.0
K # TFTE VENT/RAD TEMP
5EPHINT 341.76 339.58 338.49 342.97 337.39 340.67   (261.15)
300.15
(258.15)
303.15
K #EPHIN TEMP
HKP5V (5.06) (5.06)   (5.06)   (5.06)   (5.08)
5.15
(5.06)
5.17
V #HK 5 Volts Rail - Voltage
HKP5I       53.28       (35.78)
52.97
(32.78)
55.97
AMP #HK 5 Volts Rail - Current
HKEBOXTEMP 347.63 345.00 343.76 349.02 341.39 346.29   (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) (99.00) (99.00) (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) (105.00) (105.00) (126.0)
128.0
(125.0)
129.0
(2IMHBLV) #Imaging bot and top MCP HV monitor
S2HVLV (83.00) (83.00) (83.00) (83.00) (83.00) (83.00) (83.00) (126.0)
128.0
(125.0)
129.0
(2S2HVLV) #Shield PMT 2 HV monitor
RSRFALV 185.00 185.00 185.00 185.00 185.00 185.00 185.00 (172.0)
174.0
(171.0)
175.0
V #Range switch setting (2RSRFALV)
3TSMXCET 275.78 278.28 275.78 275.78 275.78 275.78 273.29 (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 313.19 315.69 313.19 313.19 313.19 313.19 305.71 (203.15)
283.15
(148.15)
353.15
K #-X TURTLE SHELL NR ACIS SS
4PRT3AT (258.46) (258.46) (258.46) (258.46) (258.46) (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
18828 ACIS-67 NONE UGC 11185 OK OK
18340 ACIS-35678 NONE SN2014C OK OK
17765 ACIS-5678 HETG RY Lup OK //Grat OK
16993 ACIS-23678 NONE NGC4206 OK OK
18146 ACIS-456789 HETG Mkn 876 OK //Grat OK
18592 ACIS-012367 NONE Bootes Cy17-12 OK OK
18844 ACIS-456789 HETG Mkn 876 OK //Grat OK
18843 ACIS-7 NONE 1H 0419-577 OK OK
18842 ACIS-5678 HETG RY Lup OK //Grat OK
17464 ACIS-7 NONE 1H 0419-577 OK OK
17098 ACIS-235678 NONE SDSS J121911.16+042905.8 OK OK
17461 ACIS-0123 NONE NGC 4725 OK OK
18225 ACIS-2357 NONE Abell 2028 OK OK
17146 ACIS-0123 NONE Cygnus A - NW Subcluster OK OK
18310 ACIS-01236 NONE GC-GB interface OK OK
18311 ACIS-01236 NONE GC-GB interface OK OK
18312 ACIS-01236 NONE GC-GB interface OK OK
18313 ACIS-01236 NONE GC-GB interface OK OK
18314 ACIS-01236 NONE GC-GB interface OK OK
18315 ACIS-01236 NONE GC-GB interface OK OK
18316 ACIS-01236 NONE GC-GB interface OK OK
18317 ACIS-01236 NONE GC-GB interface OK OK
18318 ACIS-01236 NONE GC-GB interface OK OK
18319 ACIS-01236 NONE GC-GB interface OK OK
18320 ACIS-01236 NONE GC-GB interface OK OK
18108 ACIS-678 NONE SDSS J1556+1124 OK OK
18846 ACIS-01236 NONE Cygnus A - NW Subcluster OK OK

Trending

This week's focus is HRMA Thermal

Last reported on Feb 18.

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