MTA Monitoring Report 01/30/15 - 02/05/15

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: 1.776e-6 CTI/year (4.865e-9 CTI/day)
Detrended slope: 1.560e-6 CTI/year (4.274e-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 (153,205) (143,700) (910,239) (802,665)   (811,637) (21,95)            
Flickering Warm Pixels (667,782) (692,141) (427,125) (726,537) (703,739)   (607,281) (357,303) (282,385) (369,376) (669,577) (263,317) (280,313) (367,511) (161,206) (258,797) (341,427) (1000,214) (335,412) (833,325) (182,474) (197,241) (356,902) (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, 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.



Telemetry

New violations or new extrema are shown in blue cells.

MSID 01/30/15 01/31/15 02/01/15 02/02/15 02/03/15 02/04/15 02/05/15 yellow limits
(lower)
upper
red limits
(lower)
upper
Units Description
OHRTHR27 297.34 297.33 297.33 297.34 297.34 297.33   (295.48)
297.15
(279.37)
307.15
K #RT 20 : PERISCOPE
OHRTHR42 294.66 294.58 294.59 294.64 294.64 294.67   (292.15)
294.37
(279.37)
307.15
K #RT 133: PERISCOPE
OHRTHR43 294.73 294.52 294.48 294.68 294.68 294.76   (291.59)
293.26
(279.37)
307.15
K #RT 134: PERISCOPE
3TSMXCET 265.81 273.29 268.30 268.30 273.29     (153.15)
263.15
(148.15)
353.15
K #-X TURTLE SHELL NR HRC CEA
3TSMXSPT 303.22 313.19 303.22 310.70 310.70 303.22   (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 39.19           (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 40.29 40.09           (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
17441 ACIS-56789 HETG tau CMa OK OK
17569 ACIS-35678 NONE SN2014C OK OK
16164 ACIS-7 NONE 1RXS J172231.6-190422 OK OK
17199 ACIS-01236 NONE Abell 1367 OK OK
16163 ACIS-7 NONE 1RXS J170856.9-235936 OK OK
17589 ACIS-01236 NONE Abell 1367 OK OK
15799 ACIS-01237 NONE CXOGBS J173620.2-293338 OK OK
17590 ACIS-01236 NONE Abell 1367 OK OK
17160 ACIS-01236 NONE RM J105417.5+143904.2 OK OK
17577 ACIS-23678 NONE MRC0131-367 OK OK
16528 ACIS-7 NONE 47 Tuc OK OK
15740 ACIS-35678 NONE DK Lac OK OK
16152 ACIS-01236 NONE RXJ1050.5-0236 OK OK
16118 ACIS-23678 NONE SDSS J111729.22+614015.2 OK OK
16076 ACIS-7 NONE SDSSJ1126+1913 OK OK
16117 ACIS-23678 NONE SDSS J105553.64+152027.4 OK OK
15735 ACIS-5678 NONE NGC 1851 OK OK

Trending

This week's focus is SIM.

Last reported on Nov 20 (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