0
Assigned ID: 765
----- Attempting Submission 1 (Fri Apr 07 19:12:05 GMT 2017) -----
HST Phase I Proposal 765 (PaBetaGOALS_2017.apt) successfully submitted.
Receipt: # 765-1
----- Attempting Submission 2 (Fri Apr 07 23:19:50 GMT 2017) -----
----- Attempting Submission 3 (Fri Apr 07 23:23:24 GMT 2017) -----
----- Attempting Submission 4 (Fri Apr 07 23:24:58 GMT 2017) -----
----- Attempting Submission 6 (Fri Apr 07 23:43:51 GMT 2017) -----
HST Phase I Proposal 765 (PaBetaGOALS_2017.apt) successfully submitted.
Receipt: # 765-6
----- Attempting Submission 7 (Fri Apr 07 23:55:26 GMT 2017) -----
One of our high-priority targets, NGC0877, needed a second pointing to get both galaxies in the pair.
We therefore removed a lower priority target (NGC5331) in order to add this second pointing (NGC0877-S).
243851352
----- Attempting Submission 1 (Tue Aug 01 22:22:33 GMT 2017) -----
Clumpy Star Formation in Local LIRGS
Near IR PaBeta and PaAlpha imaging of Luminous Infrared Galaxies (LIRGs) have revealed that local LIRGs host many luminous clumpy star forming regions. These star forming regions range in SFR from (.001 to 10 Msun/yr) and span the range from local galaxies to those found at high redshift (1< z < 3);thus, bridging the gap between the local and the high-z universe. Star-formation in high-z galaxies is often concentrated in luminous star-forming `clumps' that are significantly larger and more luminous than those observed in normal galaxies in the local universe. These large clumps of star-formation are thought to be the product of high gas fractions in turbulent disks. We propose to obtain narrow-band PaBeta imaging of 20 local LIRGs with high molecular gas fractions (MGF > 20%) to study the key physical properties of star forming clumps in these high gas environments. We will measure the sizes, luminosities, and energy input of clumps of young massive stars that are currently being formed. The goals of this project are: (1) to investigate the role of star formation rate, MGF, and galaxy interactions on the clump luminosity function (2) to test if higher MGF LIRGs produce star forming clumps with higher SFR densities and (3) directly compare our results star forming clumps in local normal star forming galaxies, high redshift galaxies observed at the highest spatial resolution using gravitational lensing, and state of the art galaxy simulations.
description
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NGC0876 is a companion of NGC0877
NGC0876
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(Tic-Visit
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true
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
/Users/klarson/Dropbox/Proposals/HST2017/APT Phase2/OP-cache/klarson_15241-v14.xml
(Tic-Visit
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true
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
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(Tic-Visit
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
/Users/klarson/Dropbox/Proposals/HST2017/APT Phase2/OP-cache/klarson_15241-v16.xml
(Tic-Visit
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
/Users/klarson/Dropbox/Proposals/HST2017/APT Phase2/OP-cache/klarson_15241-v17.xml
(Tic-Visit
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(Tic-Orbit
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true
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
/Users/klarson/Dropbox/Proposals/HST2017/APT Phase2/OP-cache/klarson_15241-v18.xml
(Tic-Visit
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(Tic-Obset
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:low-sky "N"
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true
1
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
/Users/klarson/Dropbox/Proposals/HST2017/APT Phase2/OP-cache/klarson_15241-v19.xml
(Tic-Visit
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(Tic-Obset
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(Tic-Orbit
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true
1
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The scheduling data was generated by CASM 25.2.
CASM was run in Phase II mode.
/Users/klarson/Dropbox/Proposals/HST2017/APT Phase2/OP-cache/klarson_15241-v20.xml
(Tic-Visit
:proposal-id 15241
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(Tic-Obset
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true
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