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Assigned ID: 59
----- Attempting Submission 1 (Thu Aug 09 13:36:35 GMT 2018) -----
HST Phase I Proposal 59 (hd222925.apt) successfully submitted.
Receipt: # 59-1
The number of orbits used exceeds the number allocated
Updated orbit planner and visit planner with new guide star re-acquisition model, as per request received via email on 12/10/2018. --iur
Added one orbit to visit 03 (to replace the one that was lost in visit 02) and added a new two-orbit visit (58) to replace the two exposures that were lost in visit 08. See HOPR numbers 91643 and 91644. 10/17/2019. --iur
Added 5 new visits (51, 54, 55, 57, and 60) to replace exposures lost in previous visits (01, 04, 05, 07, 10+12). See HOPR 91692, 91693, 91694, 91695, and 91696). 01/09/2020. --iur
1933858128
----- Attempting Submission 1 (Sat Nov 17 05:04:47 GMT 2018) -----
HST Phase II Proposal 15657 (hd222925.apt) successfully submitted.
Receipt: # 15657-1
----- Attempting Submission 2 (Tue Dec 11 17:27:01 GMT 2018) -----
----- Attempting Submission 3 (Thu Oct 17 21:15:27 GMT 2019) -----
----- Attempting Submission 4 (Thu Jan 09 16:20:26 GMT 2020) -----
Only visits 03 and 58 have been modified here. The visit planner has been run for those two only.
The number of orbits (50) does not match the number allocated (47) because three additional orbits were granted to replace three failed exposures (see HOPR numbers 91643 and 91644).
The number of orbits (57) does not match the number allocated (47) because 10 additional orbits were granted to replace failed exposures (see HOPR numbers 91692 through 91696).
HD 222925: A unique opportunity to study the full range of nuclei produced by a single r-process event
The r-process is one of the fundamental ways nature produces heavy elements, but the specific physical characteristics of the r-process are not yet fully understood. HD 222925, the brightest and most highly r-process-enhanced star known, provides the first opportunity to test unexplored regimes of r-process models. New STIS/E230H observations are proposed to obtain a high-S/N, high-resolution UV spectrum of HD 222925, which will provide the most detailed census of elements produced by a single r-process event, such as a neutron star merger. Twenty-eight r-process elements have been detected in the optical spectrum of HD 222925; the proposed UV spectra would enable the detection of 13 additional elements produced by the r-process (Ge, Se, Cd, Sn, Sb, Te, Ta, W, Re, Pt, Au, Pb, and Bi) that cannot be detected in ground-based spectra of HD 222925 and are rarely, if ever, detected in optical/UV spectra of other r-process-enhanced stars. The proposed observations would yield the most complete and precise r-process abundance template beyond the Solar System, and it would be the only r-process pattern formed by a single r-process event where all three r-process peaks (Se, Te, and Os-Ir-Pt) are detected. Comparing the r-process abundance pattern derived from HD 222925 with model predictions links directly to the physics at the site of the r-process, including the level of neutron richness, the role played by mixing between the r-process peak production sites, and the importance of fission recycling. This approach to understanding the r-process complements and extends the approach informed by observations of the kilonovae associated with neutron star mergers.
The goal of this observing program is to collect E230H R=114,000 spectra of one star, HD 222925, with complete spectral coverage from 1924 to 3150 Angstroms. This is a non-variable, RHB, metal-poor Pop II star. Because the target is non-variable, spectra can be collected at any time with no constraints. Observations have been grouped into 2- or 3-orbit visits to minimize overhead and maximize scheduling flexibility.
For the 3-orbit visits, there should be five exposures. Orbit 1: ACQ, ACQ/PEAK, and SCIENCE. Orbit 2: SCIENCE. Orbit 3: SCIENCE.
For the 2-orbit visits, there should be four exposures. Orbit 1: ACQ, ACQ/PEAK, and SCIENCE. Orbit 2: SCIENCE.
Note to self: This sequence assumes that there are two guide stars available to minimize drift. If only one guide star is available, the drift could be enough to move the star off the 0.2x0.09 slit. (See STIS handbook, 8.1.4.) If that's the case, then use 2-orbit visits instead.
Setup 1: E230H/c3012 (2 orbits x 1 visit) = 2 orbits
STIS.sp.1178852
Setup 2: E230H/i2812: (2 orbits x 2 visits) = 4 orbits
STIS.sp.1178849
Setup 3: E230H/i2563: (3 orbits x 1 visit) + (2 orbits x 1 visit) = 5 orbits
STIS.sp.1178845
Setup 4: E230H/i2313: (3 orbits x 3 visits) = 9 orbits
STIS.sp.1178843
Setup 5: E230H/i2063: (3 orbits x 9 visits) = 27 orbits
STIS.sp.1182944
The ICRS coordinates, proper motions, and parallax values are taken from Gaia DR2. I have checked the target confirmation chart, and the crosshairs line up to within 1 DSS pixel of the stellar diffraction spikes on the image. This precision has been sufficient to correctly observe similar targets with the 0.2x0.09 slit in previous STIS observing runs.
The ETC gives a warning for the target acquisition steps: "WARNING MESSAGE: Partial overlap between instrument throughput band and target spectrum. Please doublecheck the wavelength range covered by the selected spectrum, and the instrument documentation for the selected filter." The STIS documentation does not clarify this warning, and when I used a nearly identical procedure for GO-14765 no warning was produced. (And now, when I try to reproduce the TA ETC for GO-14765, I get this warning; those observations were executed successfully.) An email from Dan Welty, via Tricia Royal, explained it as so: "I believe that this warning is triggered when the input spectrum used for the calculation does not fully cover the wavelength range over which the filter/aperture is defined. In this case, the input spectrum goes down to about 1300 A, but the F25ND3 is defined to below 1250 A. But since both the filter/CCD transmission and the input spectrum are both rapidly declining below 1300 A, it should not be a problem for the acq." Based on this information, I have disregarded this warning message.
Stellar Physics
6
false
false
true
false
false
false
false
SUPPORTED
STAR
G III-I
HORIZONTAL BRANCH STAR
POPULATION II
NO
This object was generated by the targetselector and retrieved from the SIMBAD database.
Star ID in Gaia DR2 catalog: Gaia DR2 6487799171512458624
J2000
J2000
STIS/NUV-MAMA
Spectroscopic
No
No
E230H
2063
STIS/NUV-MAMA
Spectroscopic
No
No
E230H
2313
STIS/NUV-MAMA
Spectroscopic
No
No
E230H
2563
STIS/NUV-MAMA
Spectroscopic
No
No
E230H
2563
STIS/NUV-MAMA
Spectroscopic
No
No
E230H
2812
STIS/NUV-MAMA
Spectroscopic
No
No
E230H
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This visit replaces three orbits lost in visits 10 and 12. See HOPR 91696.
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true
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This visit replaces the two exposures that were lost as part of visit 02.
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