MTA Monitoring Report 09/10/21 - 09/16/21

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: 5.518e-02 CTI/year (1.512e-04 CTI/day)
Detrended slope: 6.019e-02 CTI/year (1.649e-04 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 (154,9) (143,700) (910,239) (526,66) (665,25) (726,537) (178,149) (811,637) (21,95)   (357,303) (670,387) (335,412)    
Flickering Warm Pixels (692,141) (802,665) (823,191) (919,71) (680,391)   (282,385) (369,376) (161,206) (263,317) (341,427) (884,31) (1000,214)   (881,53) (197,241) (182,474) (139,109) (275,393) (136,65)  
Current Hot Pixels                    
Flickering Hot Pixels                    
Warm column candidates           512 510 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

12 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 09/10/21 09/11/21 09/12/21 09/13/21 09/14/21 09/15/21 09/16/21 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
SPHVLV (67.00) (2.00)           (72.0)
128.0
(71.0)
129.0
(2SPHVLV)Spect Bot MCP HV Monitor
HRMACAV           295.65   (293.4)
294.8
(292.8)
295.5
TEMPHRMA CAVITY AVG TEMP
TCM_PA1 (258.96)         (260.05) (258.16) (269.15)
348.15
(260.15)
413.15
KRF POWER AMP-1 EXT BPL TEMP
OBAAVG           301.51   (282.5)
300.0
(281.4)
301.0
KOBA/TFTE TEMP
TSCTSF3       (268.06) (268.06)     (278.15)
359.15
(269.15)
483.15
KSC-TS FITTING -3 TEMP
TEP_PSU2             (264.06) (283.15)
343.15
(264.15)
393.15
KPSU-2 TEMP
OBADIAGRAD 4.21 4.39 4.33 4.34   3.94   (-1.11)
3.5
(-2.78)
3.9
KOBA DIAM GRAD
IMHVLV (63.00)             (126.0)
128.0
(125.0)
129.0
(2IMHVLV)Imaging Bot MCP HV Monitor
TPCP_RW2             (277.89) (288.15)
363.15
(278.15)
404.15
KRWA -2 TEMP (+Z PCAD COMP)
IMHBLV (16.00)             (126.0)
128.0
(125.0)
129.0
(2IMHBLV)Imaging Bot & Top MCP HV Monitor
OBACONEAVG 303.69     303.03 304.54 305.13   (282.5)
300.0
(281.8)
301.0
KOBA CONE AVG TEMP
SPHBLV (39.00) (25.00)           (79.0)
128.0
(78.0)
129.0
(2SPHBLV)Spect Bot & Top MCP HV Monitor
TCM_PA2 (259.69)           (259.32) (269.15)
348.15
(260.15)
413.15
KRF POWER AMP-2 EXT BPL TEMP
TCM_TX1 (266.97) (268.79) (268.43)     (268.06) (266.61) (283.15)
348.15
(269.15)
404.15
KTRANSPONDER-1 EXT BPL TEMP
PRBSCR   (-8.65)           (1.24)
1.92
(0.9)
2.26
AMPPrimary Bus Current


IRUs

Gyro Bias Drift Gyro Bias Drift Histogram

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
25988 ACIS-7 NONE SNR 0519-69.0 OK OK
23576 ACIS-7 NONE SNR 0519-69.0 OK OK
24349 HRC-S NONE HD 4915 OK OK
24298 ACIS-0123 NONE A1351 OK OK
25986 ACIS-7 NONE PKS2300-18 OK OK
25985 ACIS-7 NONE UGC12237 OK OK
24777 ACIS-01237 NONE 3FGL J1016.5-6034 OK OK
26121 HRC-S NONE HD 4915 OK OK
24392 ACIS-235678 NONE NGC 3998 OK OK
23994 ACIS-0123 NONE GDH23 OK OK
25990 ACIS-235678 NONE NGC 3998 OK OK
23996 ACIS-0123 NONE GDH23 OK OK
23995 ACIS-0123 NONE GDH23 OK OK
23997 ACIS-0123 NONE GDH23 OK OK
23998 ACIS-0123 NONE GDH23 OK OK
23991 ACIS-0123 NONE GDH22 OK OK
23989 ACIS-0123 NONE GDH22 OK OK
23990 ACIS-0123 NONE GDH22 OK OK
24302 ACIS-7 NONE PKS 0023-26 OK OK
23457 ACIS-7 NONE MAXI J1848-015 OK OK
26124 ACIS-7 NONE 2RXS J222749.3-011358 OK OK
26127 ACIS-7 NONE MAXI J1848-015 OK OK
23992 ACIS-0123 NONE GDH22 OK OK
23993 ACIS-0123 NONE GDH22 OK OK

Trending

This week's focus is EPHIN

Last reported on Jul 01.

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


MSIDMeanRMSDelta/YrDelta/Yr/YrUnitDescription
5eiot 0.4740.029(3.38+/-0.18)e20.10 +/- 0.41KEIO TEMP
5ephint 2.3980.012(3.16+/-0.17)e2-0.27 +/- 0.18KEPHIN TEMP
teio 1.6180.024(3.15+/-0.18)e2-0.31 +/- 0.45KEPHIN ELECTRONICS HOUSING TEMP
tephin 2.3990.012(3.16+/-0.17)e2-0.22 +/- 0.18KEPHIN SENSOR HOUSING TEMP


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