Copied failed visits 6 and 7 and edited the new visit 6 (now visit 11) to be one orbit.
Visit 7 was copied directly into Visit 12 in order for it to be completely redone, as approved in the HOPR.
----- Attempting Submission 3 (Thu Jun 07 18:07:51 GMT 2007) -----
Phase II Proposal 11307 (11307) successfully submitted.
----- Attempting Submission 4 (Thu Jun 07 19:05:49 GMT 2007) -----
Phase II Proposal 11307 (11307) successfully submitted.
----- Attempting Submission 5 (Tue Jun 12 19:54:03 GMT 2007) -----
----- Attempting Submission 6 (Wed Jun 13 18:27:20 GMT 2007) -----
----- Attempting Submission 7 (Tue Jun 26 17:23:37 GMT 2007) -----
Phase II Proposal 11307 (11307_070620_3pt_crs) successfully submitted.
Submission failed communicating with the submission server:
java.rmi.ConnectException: Connection refused to host: 130.167.1.97; nested exception is:
java.net.ConnectException: Connection refused
Submission failed communicating with the submission server:
java.rmi.ConnectException: Connection refused to host: 130.167.1.97; nested exception is:
java.net.ConnectException: Connection refused
----- Attempting Submission 8 (Thu Jul 05 23:03:08 GMT 2007) -----
----- Attempting Submission 9 (Wed Aug 29 21:59:18 GMT 2007) -----
I only processed visits 11 and 12, as those were the ones I changed.
Completing the ACS Nearby Galaxy Survey with WFPC2
We are requesting 25 orbits of Director's Discretionary Time to complete the primary science goals of our highly-ranked ACS Nearby Galaxy Survey Treasury program (ANGST). Our program lost ~2/3 of its orbits due to the ACS failure. Roughly half of these were restored as a result of an appeal to the Telescope Time Review Board which re-scoped the program. The Board's response to our appeal was explicit in terms of which targets were to be observed and how. We were directed to request Director's discretionary time for the components of the appeal which were not granted by the Review Board, but which were vital to the success of the program.
The observing strategy for ANGST is two-fold: to obtain one deep field per galaxy which enables derivation of an accurate ancient star formation history, and to obtain radial tilings sufficient for recovering the full star formation history. The Review Board granted WFPC2 observations for deep fields in 7 galaxies, but no time for radial tilings. However, recovering the full star formation history of a galaxy is not possible without additional radial coverage. We have searched the archives for observations which may be used in place of the tilings (conceding some of the Treasury goals, but providing significant constraints on the full star formation history), and have identified suitable observations for all but two of the galaxies. Here we request DD time for radial tilings for those last two galaxies.
We will be tiling along the major axis of NGC 55 and NGC 3109. These observations will be used in concert with the deep observations (program 10915) to determine the history of star formation in these galaxies.
RESOLVED STELLAR POPULATIONS
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:saa-model "26"
:si-bright-earth-limb-angle 20.0
:data-volume 89632
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 11307
:visit-id "12"
:obset-id "12"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 11307
:visit-id "12"
:orbit-number 1
:pcs-time 355
:si-vis-utilization 2700
:al-overhead-at-end 180
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3159
:pcs-gap 0
)
true
1
0