MTA Monitoring Report 07/03/15 - 07/09/15

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: 1.627e-6 CTI/year (4.458e-9 CTI/day)
Detrended slope: 1.559e-6 CTI/year (4.271e-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       (21,95)   (357,303) (369,376) (161,206)     (197,241) (881,53)  
Flickering Warm Pixels (692,141) (153,205) (143,700) (910,239) (802,665) (726,537) (811,637) (419,163) (247,364) (607,281) (669,577) (263,317) (280,313) (341,427) (1000,214) (335,412) (182,474) (150,374)
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, 3 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

11 TSC moves this period

Telemetry

New violations or new extrema are shown in blue cells.

MSID 07/03/15 07/04/15 07/05/15 07/06/15 07/07/15 07/08/15 07/09/15 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
OHRTHR27 297.35 297.34 297.34 297.35 297.35 297.34 297.35 (295.48)
297.15
(279.37)
307.15
K #RT 20 : PERISCOPE
OHRTHR42 294.60 294.60 294.60 294.61 294.66 294.61 294.65 (292.15)
294.37
(279.37)
307.15
K #RT 133: PERISCOPE
OHRTHR43 294.59 294.59 294.56 294.55 294.67 294.54 294.63 (291.59)
293.26
(279.37)
307.15
K #RT 134: PERISCOPE
3TSMXCET 273.29 270.79 275.78 273.29 273.29 273.29 273.29 (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 310.70 310.70 310.70 313.19 310.70 308.21 310.70 (203.15)
294.15
(148.15)
354.15
K #-X TURTLE SHELL NR ACIS SS


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
17392 ACIS-456789 HETG MKN421 CAL OK
17042 ACIS-678 NONE SDSS J1125+0029 OK OK
16739 ACIS-5678 HETG H1743-322 OK OK
17667 ACIS-0123 NONE NGC2442 OK OK
17691 ACIS-0123 NONE IRAS 16562-3959 OK OK
17242 ACIS-235678 NONE NuSTAR J163600-4748.4 OK OK
16653 ACIS-456789 HETG HD191612 OK OK
17304 ACIS-012367 NONE UDS OK OK
17065 ACIS-5678 NONE UGC 2698 OK OK
17121 ACIS-67 NONE Mrk477 OK OK
16737 ACIS-012367 NONE XMMU J183245-0921539 OK OK
17325 HRC-I NONE Vega CAL OK
17326 HRC-S NONE Vega CAL OK
17327 HRC-S NONE Vega CAL OK
17328 HRC-S NONE Vega CAL OK
17329 HRC-S NONE Vega CAL OK
17305 ACIS-012367 NONE UDS OK OK
17668 ACIS-2367 NONE Kes 73 OK OK
17306 ACIS-012367 NONE UDS OK OK
17692 ACIS-2367 NONE Kes 73 OK OK
17307 ACIS-012367 NONE UDS OK OK

Trending

This week's focus is HRC.

Last reported on Apr 16.

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