5rd submission. Properly account for overhead in exposure time.-1210865829Assigned ID: 5967
----- Attempting Submission 1 (Wed Nov 06 18:20:41 GMT 2024) -----
HST Phase I Proposal 5967 successfully submitted.
Receipt: # 5967-1
----- Attempting Submission 2 (Thu Nov 07 10:00:24 GMT 2024) -----
HST Phase I Proposal 5967 successfully submitted.
Receipt: # 5967-2
----- Attempting Submission 3 (Thu Nov 07 11:42:13 GMT 2024) -----
HST Phase I Proposal 5967 successfully submitted.
Receipt: # 5967-3
----- Attempting Submission 4 (Thu Nov 07 21:24:36 GMT 2024) -----
HST Phase I Proposal 5967 successfully submitted.
Receipt: # 5967-4
----- Attempting Submission 5 (Thu Nov 07 22:44:49 GMT 2024) -----
HST Phase I Proposal 5967 successfully submitted.
Receipt: # 5967-5POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.Third submission.
We set the dither parttern same as the three-points dither suggested by our support contacts.
We also extend some exposure time to best use the orbits.863759922----- Attempting Submission 1 (Thu Jan 30 00:27:48 GMT 2025) -----
HST Phase II Proposal 17913 successfully submitted.
Receipt: # 17913-1
----- Attempting Submission 2 (Thu Jan 30 18:30:12 GMT 2025) -----
HST Phase II Proposal 17913 successfully submitted.
Receipt: # 17913-2
----- Attempting Submission 3 (Sat Mar 08 06:36:35 GMT 2025) -----All the warnings are from the target position settings for exposures taking with a ramp filters.
We change the dither patterns to values as suggested by our support contancts.The False positive in the Lyman Continuum escape fraction estimationWhen calculating the reionization history, the Lyman Continuum escape fraction (fesc) cannot be measured directly at high redshift and therefore remains severely unconstrained. The fesc can only be referred from the indirect fesc indicators derived from the low-z studies. However, the indirect fesc indicators are only derived from spatially integrated properties, neglect the false positives in the regression, and imply an overproduction of ionizing photons that would lead to a very early reionization history.
This proposal aims at understanding the discrepancy between observed reionization constraints and the local Lyman Continuum emitters. We propose imaging 4 galaxies with resolved maps of escape fraction proxies derived from optical emission lines to identify for the first time their spatial variations in these galaxies. These 4 galaxies are exclusively selected from the false positive sample in the Lyman Continuum escape fraction estimation. Their emission line maps can only be produced by the ACS/WFC ramp filters. This will allow us to understand whether the global (integrated) properties of these galaxies (star formation rate density, [OIII]/[OII] ratio, and dust extinction) are a good indicator of their estimated Lyman Continuum escape fraction. The applicability of these results to faint z>6 galaxies will become increasingly important for studying galaxies in the epoch of reionization.We observe 4 galaxies in 4 pointings, separated into 7 visits (3galaxies with 2 visit, and 1galaxy with 1 visit.)
For each galaxies, we are taking 6 sets of images. For Each set of images, we uses 1 filter, subarray aperture, and split the image into 3-dither exposures. (18 exposures for each galaxies).
We manually setup the three-point dithers pattern to arrange the exposures into the orbits. The dither pattern (-0.125, 0.125), ( 0, 0), ( 0.1125, -0.1125) is setted. The difference in the last point is intentional to give us 2.5 and 2.25 pixel shifts for better sampling.
To easy scheduling, we do not request special observation requirements for the 7 pointings. However, ideally an execution of visits at a similar time
within a few weeks would be appreciated.Dr. Yu-Heng Lin is expert of analysis nebular emission liness and modeling reionization history. He has experience in the analysis of imaging products from HST SBC.
Dr. Andreas Faisst is an expert in the study of galaxy evolution and galaxies in the epoch of reionization. He has extensive expertise in the analysis of imaging products from HST and the measurement of emission lines using photometric filters.
Dr. Harry Teplitz is an expert in multiwavelength studies of galaxy evolution back to reionization, has extensive
analysis experience with large imaging data sets from HST.
Dr. Danial Masters is an expert in galaxy evolution. He has extensive expertise in the analysis of imaging products from HST.
Prof. Claudia Scarlata has substantial experience with observations and interpretation of galaxy spectra and images, both of
local analogs of high redshift galaxies (e.g., Green Pea galaxies, the Lyman alpha Reference Sample, etc) and high redshift galaxies.
Prof. Matthew Hayes is an expert in Lyman Continuum Lyman alpha emitting galaxies, and has extensive
analysis experience with large imaging data sets from HST.
Dr Axel Runnholm is an expert on Lyman alpha emitting galaxies and has significant previous experience with long pass filter imaging of Lyman alpha and emission line mapping.
Dr. Alexandra Le Reste is an expert in local analogs to EoR galaxies, and has extensive experience with data reduction and analysis of HST imaging.
Dr. Annalisa Citro is an expert in the spectroscopy of galaxies, with particular experience in the analysis of the UV spectra of gravitationally lensed sources, and chemical abundances. She has also experience with HST UV imaging, and the connection between LyC leakage and Lya emission.
Dr. Vihang Mehta has expertise in extreme star-forming galaxies. He has extensive experience with deriving stellar population dust extinction with HST images.
Dr. Keunho J. Kim is an expert on sub-galactic structure of LyC emitters. He has extensive experience on analysis of UV continuum slope images.
Dr Noah Rogers is an expert on local star-forming galaxies and HII regions. He has extensive experience with sub-galactic structures of UV emission lines.Galaxies6falsefalsefalsefalsefalsefalseSUPPORTEDGALAXYSTARBURSTJ2000J2000GALAXYSTARBURSTJ2000J2000GALAXYSTARBURSTJ2000J2000GALAXYSTARBURSTJ2000J2000ACS/WFCRampFilterNoNoFR505NACS/WFCRampFilterNoNoFR647MACS/WFCRampFilterNoNoFR656NACS/WFCRampFilterNoNoFR914MACS/WFCRampFilterNoNoFR931NACS/WFCImagingNoNoF550MACS/WFCImagingNoNoF775WACS/WFCRampFilterNoNoFR505NACS/WFCRampFilterNoNoFR656NACS/WFCRampFilterNoNoFR853NACS/WFCRampFilterNoNoFR551NACS/WFCRampFilterNoNoFR647MACS/WFCRampFilterNoNoFR716NACS/WFCRampFilterNoNoFR914MACS/WFCRampFilterNoNoFR931NACS/WFCRampFilterNoNoFR505NACS/WFCRampFilterNoNoFR647MACS/WFCRampFilterNoNoFR656NACS/WFCRampFilterNoNoFR716NACS/WFCRampFilterNoNoFR914MACS/WFCRampFilterNoNoFR931NThe scheduling data was generated by CASM 33.0.CASM was run in Phase II mode./private/var/folders/tn/vrvc8r7n4yz1j60w20cdvr2c0000gp/T/OPVisit13898609050292905202.xml(Tic-Visit
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)
(Tic-Orbit
:proposal-id 17913
:visit-id "07"
:orbit-number 2
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:si-vis-utilization 2718
:al-overhead-at-end 0
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:pcs-gap 0
)
(Tic-Orbit
:proposal-id 17913
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:pcs-gap 0
)
(Tic-Orbit
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:pcs-gap 0
)true40