INTEGRAL Commissioning & PV planned activities
Revolution 1 (2002/10/17 - 2002/10/20, times in UTC)
-
Lift off at 04:41
-
Separation of 4th Proton stage and spacecraft from third stage at 04:50
-
4th stage main engine burn to enter transfer orbit from 05:43 until 05:50
-
Separation of INTEGRAL spacecraft from 4th Proton stage at 06:13
-
Solar arrays deployed at 06:31
-
The remaining activities for this revolution include:
+ Switch on reaction wheel assembly
+ Switch on star tracker
+ Transition to inertial pointing and slew mode
+ Switch on and activate the Radiation Monitor IREM
+ Slew to outgassing attitude
+ Start of SPI activation, low temp outgassing
+ Start of JEM-X activation
+ Start of IBIS activation
+ Start of OMC activation
+ Slew to Perigee Passage attitude
+ Perigee height = 700 km
Revolution 2 (2002/10/20 - 2002/10/22)
The main activities during this revolution include:
-
IBIS electronic boxes activations
-
JEM-X electronic calibration
-
OMC CCD health check
-
OMC CCD calibration (cover closed)
-
OMC cover release (on 2002/10/21 at 18:15 UTC) and CCD/optics test with
cover open
-
OMC imaging at Perigee Passage attitude
Revolution 3 (2002/10/22 - 2002/10/25)
The main activities during this revolution include:
-
IREM verification
-
Slew to perigee raise burn attitude
-
First perigee raise maneouvre (2002/10/23, 02:25 UT) using INTEGRAL's on-board
propulsion system (new perigee height = 2235 km)
-
JEM-X and OMC instrument configuration after perigee raise burn
-
JEM-X high voltage activation
-
OMC imaging at perigee raise attitude and at outgassing attitude
-
IBIS data processing electronics and periphery s/w dump
-
SPI data processing electronics s/w dump
Revolution 4 (2002/10/25 - 2002/10/28)
The main activities during this revolution include:
-
Tune IREM configuration for nominal operations
-
Slew to perigee raise burn attitude
-
Adjust IREM particle radiation background thresholds on-board for SPI,
IBIS, JEM-X, OMC
-
SPI configuration upload and functional test with hot detectors
-
Instruments safing for perigee raise burn
-
Second perigee raise maneouvre (2002/10/26, 18:44; new perigee height =
4538 km)
-
Third perigee raise maneouvre (2002/10/26, 20:47; new perigee height =
7033 km)
-
Resume instruments configuration
-
JEM-X HV adjustment
-
JEM-X activation completed (JEM-X (1): 27 Oct, JEM-X (2): 28 Oct) and the
instrument is fully operational from this point in time. Any further activity
is dedicated to the optimization of the instrument configuration.
-
OMC imaging at various attitudes (perigee passage, out-gassing, perigee
raise burn)
-
OMC data dump digital processing electronics
Revolution 5 (2002/10/28 - 2002/10/31)
The main activities during this revolution include:
-
Start SPI high temperature outgassing
-
SPI passive cooling (start)
-
SPI event trigger threshold checks
-
SPI anti-coincidence sub-system calibration and tuning of front end electronics
-
JEM-X HV adjustment
-
JEM-X diagnostic data collection
-
Instruments safing for perigee raise burn
-
Fourth perigee raise maneouvre (2002/10/29, 20:16; perigee height = 9040
km)
-
Fifth (and last) perigee raise maneouvre (2002/10/31, 07:34; perigee height
= 9078 km)
-
Resume instruments configuration
-
OMC imaging at various attitudes (perigee passage, out-gassing, perigee
raise burn, apogee adjustment maneouvre)
-
Apogee adjustment maneouvre
Revolution 6 (2002/10/31 - 2002/11/03)
The main activities during this revolution include:
-
Continuation of SPI tuning of anti-coincidence sub-system tuning of front
end electronics
-
SPI anti-coincidence calibration (cont'd)
-
Start of SPI active cooling
-
AOCS thruster calibration
-
SPI pulse-shape discrimination threshold adjustment
-
OMC imaging at star tracker calibrations attitudes
-
End of LEOP (Launch and Early Operations) on 01 Nov, 16:20 UTC
-
Misalignment calibration and disturbance torque calibrations for star trackers
and fine sun sensors
Revolution 7 (2002/11/03 - 2002/11/06)
With revolution 7 the transition phase to nominal PV (performance and
verification) phase will begin. The transition phase will last until the
end of revolution 13. The following activities are planned:
-
Slew to PV target "empty field 1" (RA, Decl) = (09:59:21.79, -00:58:55.2).
During PV phase the empty field will be used for background studies.
-
IBIS switch on and check 3 out of 8 detector sections.
-
SPI camera (Germanium detectors) switch on at 117 K
-
SPI: analyse pulse shape discrimination events
-
SPI: check spectra in 5x5 dithering mode
-
SPI: instrument health status main check
-
SPI: camera performance check during cooling until 90 K det temperature
-
Calibation of the attitude and orbit control system (AOCS), 58 pointings
Revolution 8 (2002/11/06 - 2002/11/09)
The main activities during this revolution include:
-
IBIS switch on and check 5 remaining detector sections
-
Star tracker bright object test
-
IBIS nominal activation: the initial IBIS activation is completed and the
instrument is fully operational from this point in time. Any further activity
is dedicated to the optimization of the instrument configuration.
Revolution 9 (2002/11/09 - 2002/11/12)
The main activities during this revolution include:
-
SPI: camera performance check at operational Germanium detector temperature
of 90K
-
SPI: the initial activation is completed (09 Nov) and the instrument is
fully operational from this point in time. Any further activity is dedicated
to the optimization of the instrument configuration.
-
SPI: check influence of high energy clamping of preamplifier
-
SPI: pulse shape discrimination threshold and analogue front end electronics
energy threshold calibrations
-
IBIS: veto photomultiplier high voltage calibration (empty field 1)
-
IBIS: veto-PICSIT delay anti-coincidence calibration
-
IBIS: veto-ISGRI delay anti-coincidence calibration
-
IBIS: PICSIT-ISGRI synchronisation - Compton mode optimisation
-
IBIS: veto threshold and zoning optimisation
-
JEM-X: diagnostic data collection on Cyg X-1
Revolution 10 (2002/11/12 - 2002/11/15)
The main activities during this revolution include:
-
JEM-X: data taking format verification on complex field (LMC- X1 and LMC
X-3)
-
SPI: Germanium detector high voltage on and threshold update/check for
analogue front end electronics and pulse shape discrimination
-
SPI: timing optimisation; time tag alignment for pulse shape discrimination/analogue
front end electronics
-
SPI: veto pulse and time tag alignment
-
SPI: veto pulse and pulse shape discrimination alignment
-
SPI: Start pulse shape discrimination (PSD) calibration (empty field 1),
step 1
Revolution 11 (2002/11/15 - 2002/11/18)
The main activities during this revolution include:
-
SPI: Determine influence of veto sub-system thresholds on background
-
SPI: Determine influence of saturated events on background
-
SPI: Determine influence of BGO veto and plastic veto parameters on sensitivity:
anti-coincidence (veto) subsystem best configuration (Cygnus X-1 pointing
with hexagonal dither, total exposure = 91.8 ksec)
-
OMC: Flat field exposure sequence
Revolution 12 (2002/11/18 - 2002/11/21)
The main activities during this revolution include:
-
Spacecraft safe pointing for Leonids passage (18 Nov. 16:45 until 19 Nov.
22:45 UTC)
-
SPI: plastic veto effects on sensitivity (empy field 1)
-
PV calibration observation (see table):
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1, on-axis |
19:58:21.68,+35:12:05.8 |
staring |
IBIS. Point spread function, imaging in crowded fields, background
studies, instruments cross-calibration |
15.5 |
Revolution 13 (2002/11/21 - 2002/11/24)
The main activities during this revolution include:
-
SPI: BGO veto and plastic veto final configuration, empty field 1 (see
revolution 7) , 93.9 ksec (PV)
-
SPI: measurement of the background with one BGO veto unit inactive
-
SPI: pulse shape discrimination calibration, step 2a and pulse shape dsicrimination
library uplink (empty field 1, 32.4 ksec PV)
-
SPI: pulse shape discrimination calibration, step 2b and data acquisition
in photon-by-photon mode (24.5 hrs)
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Empty field 1 |
09:59:21.79,-00:58:55.21 |
staring |
IBIS. Background study |
10 |
Revolution 14 (2002/11/24 - 2002/11/27)
With this revolution the Performance and Verification (PV) phase proper
will begin. The main activities during this revolution include:
-
PV calibration observation :
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1 on-axis |
19:58:21.68,+35:12:05.8 |
staring |
IBIS. Point spread function, imaging in crowded fields, background
studies, instruments cross-calibration |
137.4 |
-
Ground segment outage 25 Nov 21:29 until 26 Nov 00:40, no telemetry available
Revolution 15 (2002/11/27 - 2002/11/30)
The main activity during this revolution is:
-
PV calibration observation :
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1 on-axis |
19:58:21.68,+35:12:05.8 |
staring |
IBIS. Point spread function, imaging in crowded fields, background
studies, instruments cross-calibration |
215.5 |
Revolution 16 (2002/11/30 - 2002/12/03)
The main activity during this revolution is:
-
PV calibration observation :
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1 on-axis |
19:58:21.68,+35:12:05.8 |
staring |
IBIS. Point spread function, imaging in crowded fields, background
studies, instruments cross-calibration |
203 |
-
Ground segment outage, NASA Goldstone ground station not available 02 Dec,
19:19 - 22:40, no telemetry available
Revolution 17 (2002/12/03 - 2002/12/06)
The main activity during this revolution is:
-
PV calibration observation :
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1 on-axis |
19:58:21.68,+35:12:05.8 |
staring |
IBIS. Point spread function, imaging in crowded fields, background
studies, instruments cross-calibration |
218 |
-
JEM-X detector off-axis calibrations along +y at Cyg X-1 off-axis positions
RA/Decl = 301.225/+33.724, 302.022/+33.977,
302.811/+33.231. 303.585/+31.476, 304.373/30.738 with a duration of
(1ksec,2ksec,4,ksec,10ksec,50ksec) respectively
Revolution 18 (2002/12/06 - 2002/12/09)
The main activities during this revolution are:
-
PV calibration observations :
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1 on-axis |
19:58:21.68,+35:12:05.8 |
staring |
IBIS. Point spread function, imaging in crowded fields, background
studies, instruments cross-calibration |
219.6 |
Revolution 19 (2002/12/09 - 2002/12/12)
The main activities during this revolution are:
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1, 2.67 deg off-axis |
20:05:37.06,+37:25:36.0 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
187.2 |
-
Ground segment outage 11 Dec, 18:42 - 23:40, no telemetry available
Revolution 20 (2002/12/12 - 2002/12/15)
The main activities during this revolution are:
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1 on-axis |
19:58:21.68,+35:12:05.8 |
hexagonal |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration. |
82.2 |
Cyg X-1, 2.67 deg off-axis |
19:34:17.37,+40:55:05.4 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
95.4 |
Revolution 21 (2002/12/15 - 2002/12/18)
The main activities during this revolution are:
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1, 7.4 deg off-axis |
19:34:17.37,+40:55:05.4 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
57.2 |
Cyg X-1, on-axis |
19:58:21.68,+35:12:05.8 |
hexagonal |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration. |
129.8 |
-
Station outage from 16/12 20:06 to 17:12 00:40
-
Start of nominal end of Commissioning Phase 17/12 06:30
Revolution 22 (2002/12/18 - 2002/12/21)
The main activities during this revolution are:
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1, 7.4 deg off-axis |
19:34:17.37,+40:55:05.4 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
207.6 |
Revolution 23 (2002/12/21 - 2002/12/24)
The main activities during this revolution are:
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Cyg X-1, 7.4 deg off-axis |
19:34:17.37,+40:55:05.4 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
19.8 |
Cyg X-1, 9.65 deg off-axis |
20:26:01.19,+43:14:23.5 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
184.8 |
Revolution 24 (2002/12/24 - 2002/12/27)
The main activities during this revolution are:
-
OMC flat field sequence (36 ksec)
-
IBIS in photon-by-photon mode for 90 ksec
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Empty field 2 |
22:15:13.10,-02:03:59.4 |
staring |
IBIS. Background study |
217 |
Revolution 25 (2002/12/27 - 2002/12/30)
The main activities during this revolution are:
-
OMC flat field #8, 13 h elapsed time
-
PV calibration observations:
Cal target |
RA, Decl. |
Dither mode |
Prime instrument and purpose of calibration |
Exposure (ksec) |
Empty field 2 |
22:15:13.10,-02:03:59.4 |
staring |
IBIS. Background study |
43 |
Cyg X-1, 9.65 deg off-axis |
20:26:01.19,+43:14:23.5 |
5x5 |
SPI. Point spread function, extended and diffuse emission, line emission,
crowded fields, background studies, instruments cross-calibration, IBIS
imaging in dither mode. |
88 |
-
Galactic plane scan (24.2 ksec) from (RA, Decl.) = (19:45:44.81,+37:22:21.0)
on 28 Dec, 05:08 (UT) until (RA, Decl.) = (01:41:35.07, +64:29:41.0) on
28 Dec, 09:19 (UT)
-
End of nominal PV cal observations
-
Start of AO-1 observing programme. The short term schedule
for AO-1 can be found here.