0
Assigned ID: 1103
----- Attempting Submission 1 (Fri Apr 07 23:20:56 GMT 2017) -----
HST Phase I Proposal 1103 (ngc2024.pdf.apt) failed submission.
----- Attempting Submission 2 (Fri Apr 07 23:21:10 GMT 2017) -----
----- Attempting Submission 3 (Fri Apr 07 23:22:51 GMT 2017) -----
HST Phase I Proposal 1103 (ngc2024.pdf.apt) failed submission.
----- Attempting Submission 4 (Fri Apr 07 23:23:04 GMT 2017) -----
HST Phase I Proposal 1103 (ngc2024.pdf.apt) failed submission.
----- Attempting Submission 5 (Fri Apr 07 23:23:32 GMT 2017) -----
HST Phase I Proposal 1103 (ngc2024.pdf.apt) failed submission.
----- Attempting Submission 6 (Fri Apr 07 23:24:09 GMT 2017) -----
HST Phase I Proposal 1103 (ngc2024.pdf.apt) failed submission.
----- Attempting Submission 7 (Fri Apr 07 23:24:33 GMT 2017) -----
HST Phase I Proposal 1103 (ngc2024.pdf.apt) failed submission.
----- Attempting Submission 8 (Fri Apr 07 23:27:28 GMT 2017) -----
This target is not used in this proposal.
change visits 4, 14 to use alternate orient and fgs3.
change visit 17 to alternate orient
add link of -90 to -90 to visit 15
made Massimo contact Co-I
changed orient on visit 15, guide star problem
-1567102484
----- Attempting Submission 1 (Wed Jul 19 00:39:16 GMT 2017) -----
----- Attempting Submission 2 (Fri Sep 08 19:48:26 GMT 2017) -----
HST Phase II Proposal 15334 (15334.apt) successfully submitted.
Receipt: # 15334-2
----- Attempting Submission 3 (Mon Sep 11 10:52:01 GMT 2017) -----
----- Attempting Submission 4 (Mon Sep 11 11:21:19 GMT 2017) -----
----- Attempting Submission 5 (Mon Sep 11 11:35:12 GMT 2017) -----
----- Attempting Submission 8 (Mon Sep 10 17:00:46 GMT 2018) -----
----- Attempting Submission 10 (Mon Sep 10 18:56:07 GMT 2018) -----
HST Phase II Proposal 15334 (15334.apt) successfully submitted.
Receipt: # 15334-10
----- Attempting Submission 11 (Mon Sep 10 19:28:51 GMT 2018) -----
HST Phase II Proposal 15334 (15334.apt) successfully submitted.
Receipt: # 15334-11
----- Attempting Submission 12 (Mon Sep 10 21:25:06 GMT 2018) -----
----- Attempting Submission 13 (Mon Oct 29 13:29:54 GMT 2018) -----
----- Attempting Submission 14 (Wed Oct 31 16:16:19 GMT 2018) -----
HST Phase II Proposal 15334 (15334.apt) successfully submitted.
Receipt: # 15334-14
----- Attempting Submission 15 (Wed Oct 31 16:56:07 GMT 2018) -----
----- Attempting Submission 16 (Thu Nov 08 13:30:39 GMT 2018) -----
----- Attempting Submission 17 (Tue Nov 12 13:17:49 GMT 2019) -----
Towards high accuracy tests on the substellar IMF in young clusters. A survey in NGC 2024.
Measuring the Initial Mass Function in young clusters, and testing its universality, is a fundamental benchmark to constrain the physical processes and theoretical models of star formation. The shape and universality of the stellar IMF are well known. Our observational characterization of the substellar IMF, on the other hand, remains more uncertain, along with its possible environmental variations.
Because of this, the physical processes that play a role in the formation of brown dwarfs are not fully constrained. In Cycle 22 we were awarded HST time to carry out the deepest spectro-photometric census of BDs in a young cluster: the Orion Nebula Cluster. Through deep WFC3/IR narrow band imaging, we are able to obtain Teff and A_V down to ~15Mjup. Preliminary analysis limited to a portion of the total field of view allows us to classify several hundreds BDs, place them in the HRD and obtain, for an extinction limited sample, the complete and consistent IMF down to planetary masses. The substellar slope is consistent with the Galactic IMF but a rapid drop is found at the H-burning limit. We propose to carry out a nearly identical survey with HST in a younger, less massive nearby cluster: NGC2024 in the Flame Nebula. This will allow us to derive the complete census of the young population down to planetary masses, derive the IMF, enabling a consistent comparison with the results in the ONC. We will specifically look for statistically significant IMF variations with environmental properties (cluster mass, density) and investigate primordial mass segregation in the substellar regime. These results will significantly help to constrain the mechanisms involved in BD formation.
This is just a 4x5=20 mosaic with WFC3/IR. Each tile has identical setup (6 exposures in 3 filters) and occupies one orbit.
Two orient ranges, each 10 degrees wide are selected as appropriate for this program, 180 degrees from each other.
Stellar Populations
Stellar Physics
6
false
false
false
false
false
false
false
SUPPORTED
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
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YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
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OPEN CLUSTER
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YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
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YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
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OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
J2000
J2000
STELLAR CLUSTER
OPEN CLUSTER
STAR FORMING REGION
YOUNG ASSOCIATION
This object was generated by the targetselector and retrieved from the SIMBAD database.
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J2000
WFC3/IR
Imaging
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F105W
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F130N
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