This submission requests that visits 06 and 07 schedule between 27-SEP-2008
and 02-OCT-2008, so that they execute before SM4. Previously, visits 06 and 07 were
scheduled to execute *during* SM4. -EN
back to restricted, use FGS 3 scenario
----- Attempting Submission 1 (Wed Apr 25 17:18:01 GMT 2007) -----
----- Attempting Submission 2 (Wed Apr 25 18:29:18 GMT 2007) -----
----- Attempting Submission 3 (Wed May 02 00:25:44 GMT 2007) -----
----- Attempting Submission 4 (Wed May 02 13:56:57 GMT 2007) -----
----- Attempting Submission 5 (Thu May 03 14:04:00 GMT 2007) -----
----- Attempting Submission 6 (Fri Aug 10 18:28:22 GMT 2007) -----
----- Attempting Submission 7 (Fri Oct 05 13:57:45 GMT 2007) -----
Phase II Proposal 11228 (11228.apt) successfully submitted.
----- Attempting Submission 8 (Fri Oct 05 15:39:31 GMT 2007) -----
----- Attempting Submission 9 (Mon Oct 08 18:25:37 GMT 2007) -----
Phase II Proposal 11228 (11228.apt) successfully submitted.
----- Attempting Submission 10 (Mon Oct 08 19:34:18 GMT 2007) -----
----- Attempting Submission 11 (Mon Aug 11 18:08:30 GMT 2008) -----
----- Attempting Submission 12 (Mon Aug 11 19:07:57 GMT 2008) -----
Phase II Proposal 11228 (11228.apt) successfully submitted.
----- Attempting Submission 13 (Mon Aug 11 20:18:11 GMT 2008) -----
The "available" has been changed from "RESTRICTED" to "SUPPORTED" since the NICMOS
visits (which needed the RESTRICTED) have already executed. Not sure if I should have
done this. -EN
FIN Submission
Assigned ID: 1318
----- Attempting Submission 1 (Fri Feb 09 14:14:30 EST 2007) -----
Phase I Proposal 1318 (xo2_cycle16_Nic) successfully submitted.
----- Attempting Submission 2 (Fri Feb 09 19:26:29 EST 2007) -----
Phase I Proposal 1318 (xo2_cycle16_Nic) successfully submitted.
----- Attempting Submission 3 (Fri Feb 09 19:54:24 EST 2007) -----
Extrasolar Planet XO-2b
We propose observations of the newly discovered extrasolar planet XO-2b
and its twin star XO-2. When combined with the transit light curve, the
FGS-derived parallax will constrain the stellar mass of the host star
XO-2. From the high signal-to-noise near-IR time series resulting from
NICMOS grism spectroscopy, we will refine the system parameters, in
particular radii of the star and planet. From the same data, we will
search for evidence of water vapor in the atmosphere via transmission
spectroscopy. Differential observations with NICMOS in the spectroscopic
mode will be used to search for the small spectral changes that occur
during planetary transits resulting from absorption of stellar light as
it passes through the planetary atmosphere. Water is an important
constituent, the detection of which would provide information on Oxygen,
and it has a convenient strong band well-positioned for NICMOS.
XO-2 will be observed for 3 visits each of 5 HST orbits with the NICMOS G141 grism.
The visits will be phased to provide full phase coverage of the XO-2b transit.
XO-2 is 2.97 mags fainter in H than HD 209458, therefore the 1.99s exposures used
in GO-9832 become 32s which can be done with STEP8, NSAMP=9. Taking into account
the 10s overhead we will maintain 76% duty cycle. Each integration will provide
3e7 electrons summed over wavelength, with roughly one third in blue-continuum,
H2O band and red-continuum.
Loose orient constraints of -23 to 77 and 157 to 257 keep both component spectra for this
visual binary with 30.8 arcsec separation within the NIC3 field of view (with a couple
arcsec margin).
Defocus is adopted using the same values from GO-9832 and the approach used in
GO-11335.
IMPLEMENTION NOTES: the new parameter CAMERA-FOCUS=DEFOCUS and aperture
NIC3-FIXD is used on all exposures to place the NIC3 focus mechanism at -0.5mm and
adjust the target placement in the aperture for the defocus respectively.
STAR FORMATION
12
false
0.0
0.0
false
false
false
false
false
RESTRICTED
STAR
K V-IV
Coordinates supplied are the mean of components A and B that are separated
by 31 arcsecs. We will use orient constraints (55% of full range) to keep the first
order grism spectra from both stars within the detector field of view.
J2000
07 48 6.5000
+50 13 32.90
J2000
STAR
F0-F2
N2302133722
J2000
00 00 0.0000
+00 00 0.00
J2000
STAR
F0-F2
N2302133726
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
N2302133731
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=14.77 R = 13.15
N23021133727
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=14.14, R=13.09
N2302133718
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=13.41, R=12.45
N2302133716
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=12.94, R=11.89
N2302133714
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=14.6, R=13.38
N2302133736
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=15.7, R=14.4
N2302133738
J2000
00 00 0.0000
+00 00 0.00
J2000
CALIBRATION
ASTROMETRIC
B=15.14, R=14.12
N2302133720
J2000
00 00 0.0000
+00 00 0.00
J2000
NIC3
Spectroscopic
No
No
G141
FGS
POS
No
F583W
/Users/alisonvick/Desktop/OP-cache/11228-v01.xml
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