round 1
round 2
round 3
484297676
Assigned ID: 5954
----- Attempting Submission 1 (Mon Nov 04 21:12:05 GMT 2024) -----
HST Phase I Proposal 5954 successfully submitted.
Receipt: # 5954-1
----- Attempting Submission 2 (Wed Nov 06 15:06:19 GMT 2024) -----
HST Phase I Proposal 5954 successfully submitted.
Receipt: # 5954-2
----- Attempting Submission 3 (Thu Nov 07 14:11:46 GMT 2024) -----
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Orbit number missing (probably due to addition of this sub-exposure after previous Orbit Planner processing). To learn more about orbit numbers, please read the full error text in the Diagnostic Report.
tweaked visits 4,14,25 to add a direct expoures in F098M and removed a scan in F606W
added visit 30, 31 per HOPR and put 2 on hold, 11 and 19
revised 19 and 50
211447905
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 2 (Mon Feb 10 14:24:38 GMT 2025) -----
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 3 (Fri Mar 14 17:00:57 GMT 2025) -----
----- Attempting Submission 4 (Tue May 20 22:19:18 GMT 2025) -----
----- Attempting Submission 5 (Mon Mar 02 16:43:17 GMT 2026) -----
tweaked visit 4,14,25
added visits 30,31 per HOPR and put 11 and 19 on hold
revised 19 and 51
Completing the HST+Gaia Reference Sample to Optimize the Measurement of the Hubble Constant
The Hubble tension, a >5 sigma discrepancy between the measured and cosmologically-predicted value of the Hubble constant (H0), is one of the most exciting developments in cosmology in decades. Having withstood scrunity and crosschecks, it is a clue we must now pursue with maximum signal-to-noise while establishing a route to future improvements. The leading determination of H0 relies on photometric observations collected over 10 years and 5 WFC3-IR programs of Milky Way Cepheids geometrically calibrated by parallaxes from Gaia. These are used to calibrate Cepheids in the hosts of 42 local SN Ia, canceling zeropoint errors through consistent use of WFC3-IR. The best MW Cepheids for this purpose have good Gaia parallax solutions (i.e., non-binaries), high parallax SNR (>10), are unsaturated in Gaia (G>6 mag), have low reddening (V-I < 2) and long periods (P>5 days), a modest-sized sample of 115 objects. In this last opportunity to use WFC3-IR, we propose two goals to both optimize the HST measurement of H0 now and simultaneously calibrate the developing effort from JWST: (1) Complete the sample of ``high-leverage'' MW Cepheid calibrators by observing the last 25 with WFC3-IR, (2) obtain WFC3-IR NIR grism spectrophotometry of these MW Cepheids at 0.8-1.7 microns to synthesize their magnitudes in the JWST filter system (F090W,F115W,F150W) to empirically calibrate JWST's developing distance ladder. This data will optimize the measurement of H0 from Gaia now and in future releases. Collecting these observations will lay a cornerstone for a 1% determination of H0 and continue to steadily advance our knowledge of what appears to be a new feature in the cosmological model.
tbd
Adam Riess: Has been leading the SH0ES Team. Extensive experience in leading large cosmological
measurements, including with HST, experience in measuring supernovae, Cepheids, parallaxes, photometry,
and astrometry. Is also a member of the WFC3 Team at STScI and is very familiar with its workings, etc.
Stefano Casertano: Deep knowledge of measurements and capabilities related to HST, Gaia parallax,
photometry and astrometry. Observatory Scientist at STScI.
Lucas Macri: An expert in Cepheids and measurements of Cepheids. Broad experience with telescopic
observations, large data sets and the near-IR.
Wenlong Yuan: An expert in Cepheids and measurements of Cepheids. Experience in ground-based
measurements of Cepheid light curves.
Louise Breuval: Experienced with measuring Cepheids, distance scale.
Javier Minniti: Expert on Cepheids, spectroscopy
Large Scale Structure of the Universe
Stellar Physics and Stellar Types
6
false
false
false
false
false
false
false
AVAILABLE
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
STAR
CEPHEID
This object was generated by the targetselector and retrieved from the SIMBAD database.
SIMBAD listed proper motion for this target. When retrieving targets with PM from SIMBAD, APT requests the coordinates be calculated with an epoch of the year 2000. Do not modify this epoch. Always review coordinates using the Target Confirmation tool, which graphically displays the PM.
J2000
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
WFC3/IR
Spectroscopic
No
No
G102
WFC3/IR
Spectroscopic
No
No
G141
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F098M
WFC3/IR
Imaging
No
No
F153M
WFC3/IR
Imaging
No
No
F127M
WFC3/IR
Imaging
No
No
F139M
WFC3/UVIS
Imaging
No
No
F555W
WFC3/UVIS
Imaging
No
No
F814W
WFC3/UVIS
Imaging
No
No
F390W
WFC3/UVIS
Imaging
No
No
F438W
The scheduling data was generated by CASM 33.0.
CASM was run in Phase II mode.
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(Tic-Obset
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IR scan, Cepheid moves across field, reverse
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
The scheduling data was generated by CASM 33.0.
CASM was run in Phase II mode.
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IR scan, Cepheid moves across field, reverse
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
The scheduling data was generated by CASM 33.0.
CASM was run in Phase II mode.
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IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
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The scheduling data was generated by CASM 33.0.
CASM was run in Phase II mode.
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staring mode
IR scan, Cepheid moves across field
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IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
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scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
The scheduling data was generated by CASM 33.0.
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scan, keep Cepheid within frame
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The scheduling data was generated by CASM 33.0.
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IR scan, Cepheid moves across field
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IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
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/System/Volumes/Data/solaris/user1/williamj/hst/work/cycle32/OP-cache/17915-v29.xml
HOPR repeat of visit 06
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remove for LMC guys
IR scan, Cepheid moves across field
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The scheduling data was generated by CASM 33.0.
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IR scan, Cepheid moves across field
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The scheduling data was generated by CASM 33.0.
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The scheduling data was generated by CASM 33.0.
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The scheduling data was generated by CASM 33.1.
CASM was run in Phase II mode.
HOPR repeat of visit 11.
(Tic-Visit
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direct image
direct image
The scheduling data was generated by CASM 33.1.
CASM was run in Phase II mode.
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IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
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direct image
direct image
The scheduling data was generated by CASM 33.0.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 33.0.
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:data-volume 582896
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:coron NIL
)
(Tic-Obset
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(Tic-Obset
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(Tic-Orbit
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)
false
1
0
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field, reverse
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
The scheduling data was generated by CASM 33.0.
CASM was run in Phase II mode.
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288.2181741027124
(Tic-Visit
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false
1
0
staring mode
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field, reverse
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
The scheduling data was generated by CASM 33.1.
CASM was run in Phase II mode.
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81.05555049120949
(Tic-Visit
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:saa-model "29"
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(Tic-Obset
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(Tic-Obset
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)
false
1
0
staring mode
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field, reverse
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
The scheduling data was generated by CASM 33.1.
CASM was run in Phase II mode.
1765562435000
19.978635222849306
(Tic-Visit
:proposal-id 17915
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:trans-errors '(:WARNINGS 12 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
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(Tic-Obset
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(Tic-Obset
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:dark-offset NIL
:dark-utilization 0
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:low-sky "N"
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false
1
0
staring mode
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field, reverse
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
IR scan, Cepheid moves across field
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame
scan, keep Cepheid within frame,reverse
scan, keep Cepheid within frame