0
Assigned ID: 900
----- Attempting Submission 1 (Fri Apr 08 22:09:29 GMT 2016) -----
HST Phase I Proposal 900 (cycle24_targets.apt) successfully submitted.
Receipt: # 900-1
0
----- Attempting Submission 1 (Fri Jul 08 08:50:20 GMT 2016) -----
The detailed properties of star-forming regions at high redshift: a matched-resolution HST-Halpha-ALMA study
Star-formation in high redshift galaxies takes place in very different conditions to those locally: high-redshift star-forming galaxies are dominated by gas-rich (f_gas ~ 20-80%) turbulent disks, have a highly pressured interstellar medium, and contain star-forming complexes orders of magnitude larger than those nearby. To understand quantitative the physical conditions and processes in these galaxies requires spatially-resolved studies of their properties and dynamics. We have been addressing this using adaptive-optics-assisted integral field spectroscopy of the H-alpha line emission of 'typical' galaxies at z=1.47 and 2.23, coupled with ALMA imaging of the thermal dust emission at matched 0.1-arcsec resolution. Here we propose to obtain two-filter HST images of 9 of these galaxies to delineate the old and young stellar populations on the same kpc-scales. Using these data we will: (i) measure spatially-resolved dust attenuation by accurately mapping the H-alpha to ultraviolet star-formation rate ratio across the galaxies; (ii) derive corrected star-formation rates, quantify the properties of the star-forming clumps, and investigate their scaling relations; (iii) critically test numerical simulations of the properties and lifetimes of these clumps; (iv) determine the morphological properties of the galaxies: evidence for mergers, disk scale-lengths, Sersic indices; (v) provide the first spatially-resolved comparison of the three classic star-formation tracers (UV, H-alpha, far-IR) at high redshift. This matched-resolution HST-Halpha-ALMA dataset will be a uniquely powerful resource for understanding the physical conditions within high-redshift star-forming galaxies.
We will observe the 9 targets from our HiZELS-SINFONI/NIFS-ALMA sample at z=1.47 and z=2.23, using the WFC3/UVIS F606W filter and the WFC3/IR F140W filter.
HiZELS is a wide-field near-infrared narrow-band survey which has selected H-alpha emitting galaxies in four narrow redshift slices, over large sky areas. The large HiZELS samples have allowed the selection of galaxies close enough to bright stars to enable adaptive-optics-assisted integral field spectroscopy of the H-alpha emission with VLT-SINFONI and Gemini-NIFS at ~0.1 arcsec resolution. For the 9 targets in this proposal we also have ALMA time to study their dust continuum emission, also at 0.1 arcsec resolution. These HST observations will obtain matched resolution observations of the rest-frame near-UV emission (~2400 Ang and ~1900 Ang using the F606W filter at z=1.47 and z=2.23 respectively) and optical (~5500 Ang and 4350 Ang using the F140W filter), spanning the 4000 Ang break, and so tracing the young and old stellar populations. Importantly, at both redshifts these filters cover line-free regions of the spectrum.
The targets all have AB magnitudes in the range 23.0 < F606W < 24.0 and 20.5 < F140W < 22.0. The angular sizes of the galaxies are typically 1-1.5 arcsec. We require accurate morphological information, and therefore target an integrated signal-to-noise ratio of at least ~50, and ideally >100, within a 1.5 arcsec diameter aperture. This is achievable with one orbit integrations through each filter.
We will split each orbit into a 3-point dither pattern in the UVIS channel, as this offers the best compromise between maximising sensitivity and sub-sampling the PSF. In the IR channel, angular resolution is of higher priority than sensitivity, and so a 4-point dither pattern will be adopted to fully recover the PSF.
Galaxies
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