Assigned ID: 988
----- Attempting Submission 1 (Sat Feb 26 03:12:48 GMT 2011) -----
HST Phase I Proposal 988 (PMC19.apt) successfully submitted.
----- Attempting Submission 2 (Sat Feb 26 03:36:54 GMT 2011) -----
HST Phase I Proposal 988 (PMC19.apt) successfully submitted.
----- Attempting Submission 3 (Sat Feb 26 04:22:52 GMT 2011) -----
HST Phase I Proposal 988 (PMC19.apt) successfully submitted.
----- Attempting Submission 4 (Sat Feb 26 19:59:58 GMT 2011) -----
HST Phase I Proposal 988 (PMC19.apt) successfully submitted.
----- Attempting Submission 5 (Sat Feb 26 20:06:02 GMT 2011) -----
HST Phase I Proposal 988 (PMC19.apt) successfully submitted.
----- Attempting Submission 6 (Sat Feb 26 20:22:48 GMT 2011) -----
----- Attempting Submission 1 (Fri Jul 08 23:21:08 GMT 2011) -----
The Formation and Fundamental Properties of Wide Planetary-Mass Companions
Over the past five years, direct imaging surveys for extrasolar planets have discovered a small but significant number of planetary-mass companions at separations >50 AU from their host stars. These wide companions pose a significant challenge to models of planet formation and of substellar atmospheres and evolution, and there are still many puzzling questions regarding their formation and fundamental properties. To address these open topics, we propose a WFC3 optical imaging survey for 25 orbits to study 12 planetary-mass companions. Our survey has three goals: 1) to use UBV and narrowband Halpha photometry to determine if (and how much) these companions are accreting out of circumplanetary disks, 2) to use broadband optical photometry to measure their temperatures and luminosities by estimating their optical spectral types, and 3) to exploit the stable HST PSF to test whether any of the companions are marginally resolved binary pairs. None of these goals can be pursued from the ground, where high-resolution observing techniques are limited to near-infrared wavelengths and yield less stable PSFs.
The goal of this proposal is to obtain multicolor images for faint (apparently planetary mass) companions to nearby young stars. They have projected separations of 0.7-5.0 arcseconds and contrasts of 5-10 magnitudes in the NIR, so the contrasts in the optical will likely be larger. In almost all cases, the primary star is expected to saturate, but this should not affect the companion. We have chosen to observe at 2 dither positions for most targets, using a CR-Split for any observation of ~700s or longer. However, we also observe most targets in F775W or F850LP (whichever is brightest) using 4 dither positions, to allow superior subsampling and retrieval of as much PSF information as possible.
None
None
STAR FORMATION
12
false
0.0
0.0
false
false
false
false
SUPPORTED
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=16.9, J=20, z~22.3, i~24.1, r~26.7, g~29.2, u~30.6 (predicted photosphere)
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=14.2, J=15.7, z~17.9, i~19.6, r~22.3, g~24.4, u~26.7
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K~16.4, J~18.1, z=20.3, i~22.2, r~24.8, g~27.3, u~28.7
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=15.0, J~16.3, z~18.6, i~20.4, r~23, g~25.5, u~26.9
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=16.2, J=17.9, z~20.2, i~22.0, r~24.6, g~27.1, u~28.5
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=15.5, J=17.9, z~21.6, i~24.5, r~28.5
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=14.9, J=16.6, z~19.7, i~22.1, r~25.8
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=12.3, J~13.4, z~15.4, i~16.8, r~19.4, g~21.1, u~22.9
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=13.3, J~14.6, z~16.7, i~18.4, r~21.3, g~23.3, u~25.3
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=14.1, J=16.2, z~18.4, i~20.3, r~22.9, g~25.4, u~26.8
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=14.8, J=15.9, z~18.1, i~19.9, r~22.6, g~24.7, u~26.3
STAR
LOW MASS COMPANION
PRE-MAIN SEQUENCE STAR
J2000
J2000
Companion: K=13.4, J=14.9, z~17.0, i~18.7, r~21.5, g~23.4, u~25.2
WFC3/UVIS
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POS-TARG
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POS-TARG
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