TARGET: 3748 Tatum SESSION NUMBER: 375 DATE/TIME: 2009 Apr 04 @ 08:21 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 135.38 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 13:12 APPROX. DEC: - 4 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00728d UNITY CORR: -5 * log(SunDist * EarthDist): -2.2758 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.456
BASE CORRECTION: +0.000
PHASE/DIST CORR: +0.000
P/D ADJUST (-/DAY):-0.029
P/D ADJUST (+/DAY):+0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 376 DATE/TIME: 2009 Apr 05 @ 08:21 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 135.38 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 13:11 APPROX. DEC: - 4 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00729d UNITY CORR: -5 * log(SunDist * EarthDist): -2.2795 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.360
BASE CORRECTION: -0.096
PHASE/DIST CORR: -0.027
P/D ADJUST (-/DAY):-0.025
P/D ADJUST (+/DAY):+0.025
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 377 DATE/TIME: 2009 Apr 06 @ 08:27 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 135.38 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 13:10 APPROX. DEC: - 4 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00729d UNITY CORR: -5 * log(SunDist * EarthDist): -2.2804 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.751
BASE CORRECTION: +0.295
PHASE/DIST CORR: -0.050
P/D ADJUST (-/DAY):-0.016
P/D ADJUST (+/DAY):+0.016
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 378 DATE/TIME: 2009 Apr 07 @ 08:09 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 135.38 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 13:09 APPROX. DEC: - 4 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00730d UNITY CORR: -5 * log(SunDist * EarthDist): -2.2831 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.539
BASE CORRECTION: +0.083
PHASE/DIST CORR: -0.059
P/D ADJUST (-/DAY):-0.009
P/D ADJUST (+/DAY):-0.009
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 380 DATE/TIME: 2009 Apr 18 @ 07:20 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.87 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 270 APPROX. RA: 12:59 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00745d UNITY CORR: -5 * log(SunDist * EarthDist): -2.3434 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.139
BASE CORRECTION: -0.317
PHASE/DIST CORR: +0.280
P/D ADJUST (-/DAY):+0.032
P/D ADJUST (+/DAY):-0.032
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 381 DATE/TIME: 2009 Apr 19 @ 07:12 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.33 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 270 APPROX. RA: 12:58 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00747d UNITY CORR: -5 * log(SunDist * EarthDist): -2.3520 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.597
BASE CORRECTION: +0.141
PHASE/DIST CORR: +0.312
P/D ADJUST (-/DAY):+0.032
P/D ADJUST (+/DAY):-0.032
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 382 DATE/TIME: 2009 Apr 20 @ 05:08 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.38 CAMERA: Alta U6 1 x binning TEMP (C): -27 EXPOSURE (s): 240 APPROX. RA: 12:57 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00749d UNITY CORR: -5 * log(SunDist * EarthDist): -2.3580 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.639
BASE CORRECTION: +0.183
PHASE/DIST CORR: +0.341
P/D ADJUST (-/DAY):+0.032
P/D ADJUST (+/DAY):-0.032
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 383 DATE/TIME: 2009 Apr 22 @ 07:37 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.50 CAMERA: Alta U6 1 x binning TEMP (C): -27 EXPOSURE (s): 240 APPROX. RA: 12:55 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00755d UNITY CORR: -5 * log(SunDist * EarthDist): -2.3775 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +12.717
BASE CORRECTION: -0.739
PHASE/DIST CORR: +0.406
P/D ADJUST (-/DAY):+0.031
P/D ADJUST (+/DAY):-0.031
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 384 DATE/TIME: 2009 Apr 26 @ 09:49 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.63 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 12:52 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00768d UNITY CORR: -5 * log(SunDist * EarthDist): -2.4194 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.961
BASE CORRECTION: +0.505
PHASE/DIST CORR: +0.529
P/D ADJUST (-/DAY):+0.029
P/D ADJUST (+/DAY):-0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 385 DATE/TIME: 2009 Apr 27 @ 06:47 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.96 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 12:52 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00771d UNITY CORR: -5 * log(SunDist * EarthDist): -2.4285 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +12.987
BASE CORRECTION: -0.469
PHASE/DIST CORR: +0.555
P/D ADJUST (-/DAY):+0.029
P/D ADJUST (+/DAY):-0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 386 DATE/TIME: 2009 Apr 28 @ 06:40 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.81 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 12:51 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00774d UNITY CORR: -5 * log(SunDist * EarthDist): -2.4401 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.212
BASE CORRECTION: -0.244
PHASE/DIST CORR: +0.584
P/D ADJUST (-/DAY):+0.029
P/D ADJUST (+/DAY):-0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 388 DATE/TIME: 2009 Apr 30 @ 04:29 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.25 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 12:50 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00781d UNITY CORR: -5 * log(SunDist * EarthDist): -2.4613 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.958
BASE CORRECTION: +0.502
PHASE/DIST CORR: +0.640
P/D ADJUST (-/DAY):+0.029
P/D ADJUST (+/DAY):-0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 389 DATE/TIME: 2009 May 01 @ 06:21 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 134.38 CAMERA: Alta U6 1 x binning TEMP (C): -30 EXPOSURE (s): 240 APPROX. RA: 12:49 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00785d UNITY CORR: -5 * log(SunDist * EarthDist): -2.4744 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.728
BASE CORRECTION: +0.272
PHASE/DIST CORR: +0.671
P/D ADJUST (-/DAY):+0.029
P/D ADJUST (+/DAY):-0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
********************************************************************************************* TARGET: 3748 Tatum SESSION NUMBER: 392 DATE/TIME: 2009 May 04 @ 15:00 FILTER: C TELESCOPE: 0.35m SCT FOCAL LENGTH: 135.28 CAMERA: SBIG ST-8E TEMP (C): -15 EXPOSURE (s): 180 APPROX. RA: 12:47 APPROX. DEC: - 3 EXPOSURE JD: Mid-exposure JD CORR METHOD: Light-time JD CORRECTION: JD = JD(raw) - 0.00797d UNITY CORR: -5 * log(SunDist * EarthDist): -2.5099 NOTE: The unity correction is NOT included in the reduced magnitudes. MAG. METHOD: Instrumental
NOTE: For multiple sessions, differential magnitudes include
adjustments ADDED to the Obj-CAvg value to compensate
for changing phase angle, distance, and refinements to
the base average value of the comparison stars.
The phase angle calculations include the effects of
the phase parameter, G. This value is taken from the
MPCORB value at the time the calculations were made.
BASE COMP VALUE: +13.412
BASE CORRECTION: -0.044
PHASE/DIST CORR: +0.749
P/D ADJUST (-/DAY):+0.029
P/D ADJUST (+/DAY):-0.029
THE P/D ADJUSTMENTS ARE INCLUDED IN THE VALUES BELOW.
ERROR CALC: The magnitude error is calculated by the following:
Err = sqrt(sqr(ERR[target]) + sqr(Err[Comps]))
where Err[Target] = 1.0857/SNR[target]
Err[Comps] = sqrt(sqr(1.0857/SNR[Comp1])... + sqr(1.0857/SNR[CompN])) / N
The factor of 1.0857 converts flux to magnitudes (Howell)
*********************************************************************************************
------------------------------------------- J.D. Obj-CAvg Err Session ------------------------------------------- 2454925.70550 +1.261 0.013 375 2454925.70870 +1.273 0.012 375 2454925.71164 +1.262 0.012 375 2454925.71458 +1.270 0.012 375 2454925.71752 +1.247 0.012 375 2454925.72046 +1.268 0.012 375 2454925.72340 +1.265 0.011 375 2454925.72634 +1.256 0.011 375 2454925.72927 +1.253 0.011 375 2454925.73222 +1.283 0.011 375 2454925.73516 +1.253 0.010 375 2454925.73809 +1.277 0.010 375 2454925.74103 +1.255 0.010 375 2454925.74397 +1.272 0.010 375 2454925.74691 +1.266 0.010 375 2454925.75147 +1.274 0.009 375 2454925.75441 +1.306 0.009 375 2454925.75734 +1.279 0.009 375 2454925.76028 +1.303 0.009 375 2454925.76321 +1.277 0.009 375 2454925.76616 +1.255 0.009 375 2454925.76908 +1.284 0.009 375 2454925.77203 +1.279 0.009 375 2454925.77497 +1.297 0.009 375 2454925.77792 +1.300 0.009 375 2454925.78086 +1.272 0.008 375 2454925.78379 +1.299 0.009 375 2454925.78673 +1.281 0.008 375 2454925.78967 +1.305 0.008 375 2454925.79260 +1.301 0.008 375 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END OF FIXED DATA SECTION. DO NOT MAKE ANY CHANGES ABOVE THIS LINE.
