MTA Monitoring Report 01/23/15 - 01/29/15

Archive of all weekly reports
Archive of monthly reports


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).

Average of ACIS-I CCDs (MnKa) slope: 1.680e-6 CTI/year (4.603e-9 CTI/day)
Detrended slope: 1.524e-6 CTI/year (4.175e-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 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 (153,205) (910,239) (726,537) (811,637) (21,95)       (335,412)    
Flickering Warm Pixels (143,700) (692,141) (427,125) (802,665)       (607,281) (357,303) (369,376) (669,577) (263,317) (161,206) (341,427)     (182,474) (197,241) (881,53)  
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, 5 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 01/23/15 01/24/15 01/25/15 01/26/15 01/27/15 01/28/15 01/29/15 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
OHRTHR27 297.33 297.33 297.33 297.33 297.33 297.33 297.34 (295.48)
297.15
(279.37)
307.15
K RT 20 : PERISCOPE
OHRTHR42 294.57 294.57 294.59 294.59 294.53 294.60 294.66 (292.15)
294.37
(279.37)
307.15
K RT 133: PERISCOPE
OHRTHR43 294.44 294.47 294.51 294.55 294.38 294.59 294.73 (291.59)
293.26
(279.37)
307.15
K RT 134: PERISCOPE
3FLCABPT   293.45   293.45       (253.15)
293.15
(235.65)
310.65
K FLCA BASEPLATE (+X)
3TSMXCET 268.30 273.29 273.29 268.30 273.29   273.29 (153.15)
263.15
(148.15)
353.15
K -X TURTLE SHELL NR HRC CEA
3TSMXSPT 308.21 308.21 308.21 310.70 310.70 300.72 313.19 (203.15)
294.15
(148.15)
354.15
K -X TURTLE SHELL NR ACIS SS
ESAMYI   (0.06)     (0.06)     (7.0)
27.0
(6.0)
33.0
AMP S/A -Y CURRENT
ESAMYI   39.39     39.59     (7.0)
27.0
(6.0)
33.0
AMP S/A -Y CURRENT
ESAPYI   (0.14)     (0.14)     (7.0)
27.0
(6.0)
33.0
AMP S/A +Y CURRENT
ESAPYI   40.49     40.49     (7.0)
27.0
(6.0)
33.0
AMP S/A +Y CURRENT
EPOVSPR   1.00     1.00     (-1.0)
0.85
(-2.0)
0.90
PRI O/V SENSOR


IRUs

Recent Observations

OBSID DETECTOR GRATING TARGET ANALYSIS ACA
16771 ACIS-01237 NONE CXOU J164043.5-463135 OK OK
17583 ACIS-012367 NONE Abell 3411 OK OK
17579 ACIS-01237 NONE CXOU J164043.5-463135 OK OK
17496 ACIS-012367 NONE Abell 3411 OK OK
17580 ACIS-01237 NONE CXOU J164043.5-463135 OK OK
17581 ACIS-01237 NONE CXOU J164043.5-463135 OK OK
17584 ACIS-01236 NONE Abell 3411 OK OK
17082 ACIS-7 NONE SDSS J111119.10+133603.8 OK OK
17576 ACIS-456789 HETG 3C 120 OK OK
17441 ACIS-56789 HETG tau CMa OK OK

Trending

This week's focus is Ground Computations.

Last reported on Oct 30 (2014).

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