Scientific Category is a required field. Science Keywords is a required field. Science Keywords: Select from 3 to 5 items. Wavelength is a required field. Period, Zero phase, Phase start and Phase end are all required for the Period requirement. Wavelength is a required field. Period, Zero phase, Phase start and Phase end are all required for the Period requirement. Wavelength is a required field. Period, Zero phase, Phase start and Phase end are all required for the Period requirement. 0 Assigned ID: 5 ----- Attempting Submission 1 (Wed Mar 05 16:33:27 GMT 2014) ----- Submitting for XMM Early Cycle 22 Execution The total number of Primary Orbits used in all Cycles must equal the total number of Primary Orbits specified on all the Observations. (Compare totals reported on the first and second pages of the PDF Preview.) Scientific Category is a required field. Science Keywords is a required field. Science Keywords: Select from 3 to 5 items. At least one target must be specified in Phase I At least one observation must be specified 0 0 ----- Attempting Submission 1 (Mon Mar 24 08:42:56 GMT 2014) ----- I've run the BOT, GSCII says it's safe, and the target is not in GALEX - I don't know why I got this error at submission... Characterizing the high-energy properties of a highly magnetized star CPD-28 2561 is the only known magnetic O-star without high-energy observations. However, because of the particular geometry of this object, it represents a crucial step towards a full understanding of the dynamic magnetospheres of high-mass stars. We propose to fill this gap by observing it in X-rays as well as in UV, both with high-resolution and with a monitoring to sample crucial phases. These complementary data will help us constrain the energetics, shock physics and 3D structure of the magnetosphere of this unique object. This program is designed to obtain UV spectroscopy of the magnetic massive star CPD-28D2561 with HST/STIS in order to diagnose the density and velocity structure of the cooler material trapped in its magnetosphere. This information will provide the context required to interpret contemporaneously acquired X-ray spectra from XMM-Newton correctly, and to model both the hot and cool components of the star's circumstellar enviroment completely. STIS/E140M observations are planned at 3 phases of the 73.41-day rotation period in order to constrain the magnetospheric structure at 3 different orientations. The phases correspond to two maxima (as defined by the variation of Halpha equivalent width; these are phases 0.0 and 0.5) and one minimum (either 0.25 or 0.75). The E140M grating provides optimal wavelength coverage and resolution of the resonance lines that are key to the analysis. Adequate S/N (about 50) can be obtained for each of the 3 visits in a single orbit. The target does not violate health or safety limits in this configuration. N/A N/A N/A HOT STARS Default false false 65 false false false SUPPORTED STAR OF This object was generated by the targetselector and retrieved from the SIMBAD database. CD-28D5104 J2000 B-V=0.04 STIS/FUV-MAMA Spectroscopic No No E140M STIS/FUV-MAMA Spectroscopic No No E140M STIS/FUV-MAMA Spectroscopic No No E140M Timing link suitability includes constraints ([Group (01 02 03) Within 73.4 days]) The scheduling data was generated by CASM 22.0. CASM was run in Phase II mode. This exposure should be taken at phase=0. +- 0.02 We would prefer to have all data taken within the same 73d period and simultaneously with XMM if possible (i.e. either the 73.4d cycle in May-June or the 73.4d cycle in Nov-Dec 2014). 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CASM was run in Phase II mode. This exposure should be taken at phase=0.5 +- 0.02 We would prefer to have all data taken within the same 73d period and simultaneously with XMM if possible (i.e. either the 73.4d cycle in May-June or the 73.4d cycle in Nov-Dec 2014). 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CASM was run in Phase II mode. This exposure should be taken at phase=0.25 or 0.75 +- 0.02. We would prefer to have all data taken within the same 73d period and simultaneously with XMM if possible (i.e. either the 73.4d cycle in May-June or the 73.4d cycle in Nov-Dec 2014). (Tic-Visit :proposal-id 13629 :visit-id "03" :proposal-version -1 :trans-version "20131031" :date "27-Mar-2014 08:37:57.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 87424 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13629 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Obset :proposal-id 13629 :visit-id "03" :obset-id "A3" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13629 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2810 :al-overhead-at-end 0 :internal-dur-at-end 394 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3253 :pcs-gap 0 ) true 1 0