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Please specify your scheduling constraints or 'No Constraints' on all Observation forms.0Assigned ID: 1187
----- Attempting Submission 1 (Sun Jan 05 19:02:18 GMT 2020) -----Joint XMM-HSTPOS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.
POS TARG & PATTERN should be used carefully with ACS ramp filters as central wavelengths & transmission efficiencies vary within the apertures.Chiaberge was added as co-I. Chiaberge is in fact co-PI of the original XMM/HST proposal and for unknown reasons (possibly because his JHU affiliation was listed in the XMM proposal?) was not transferred to the associated HST observation. Chiaberge also acts as phase 2 contact.
Submission #2
Removed scheduling link between Visits 1 and 2. Visit 1 is still required to be scheduled whithin a specific time window, while Visit 2 is now unconstrained.
SCHED 100 is used to visit 1 to facilitate scheduling
04/28/2020 - ROYLE - removed BETWEEN from visit 01 to open up windows.1391741956----- Attempting Submission 1 (Wed Feb 19 22:39:28 GMT 2020) -----
----- Attempting Submission 2 (Wed Mar 18 19:36:37 GMT 2020) -----
----- Attempting Submission 3 (Tue Apr 28 15:56:46 GMT 2020) -----
HST Phase II Proposal 16062 successfully submitted.
Receipt: # 16062-3See sumbission comments for explanation of the added co-I.
POS-TARGs for ramp filters are ok since the target is relatively smallQuasi-Periodic Eruptions (QPEs) in GSN 069We have recently reported on the discovery of a new X-ray variability pattern from the nucleus of the galaxy GSN~069, dubbed as Quasi-Periodic Eruptions, or QPEs (Miniutti et al. 2019, Nature, 573, 381). We propose here for further XMM-Newton observations to better characterize this newly-discovered variability pattern. Ideally, our observations will be complemented with 2 HST orbits with the goals of: i) deriving the optical to X-ray SED of GSN~069; ii) search for possible blue point sources other than the galactic nucleus in comparison with our Chandra data; iii) study the morphology of the poorly known host galaxy; iv) study the spatially-resolved structure of the narrow-line-region in [O~III].We ask for exposures with the following camera/filters: i) ACS/SBC exposures in the FUV with lters 140LP and 165LP (the second needed to get rid of red leaks) to look for potentially blue sources other than the nucleus, and to contribute
to build the SED of GSN 069, in this case in the FUV; ii) ACS/WFC with lter F606W for spatially-
resolved imaging of the host galaxy and to look for possible disturbances/merger; iii) ACS/WFC with filters
FR647M (continuum) and FR505N (for the [O III] region) to search for signatures of recurrent/intermittent
nuclear activity reflected in the narrow line region spatially-resolved structure (e.g. rings/arcs).
The HST observations should be scheduled quasi-simultaneously with the XMM observations (within a few weeks).
At the time the phase 2 is submitted, we only know that the XMM observations could be scheduled between May 30 2020 and July 17 2020. We temporarily set the BETWEEN dates accordingly and we will update them when the XMM schedule is made public, if needed.
Visit 1 and 2 should be grouped within about 5 days but the order does not matter.None RequiredMassive Black Holes And Their Host Galaxies6falsefalsefalsefalsefalsefalsefalseSUPPORTEDGALAXYSEYFERTYESGalaxy magnitude from GaiaJ2000J2000ACS/SBCImagingNoNoF140LPACS/SBCImagingNoNoF165LPACS/WFCImagingNoNoF606WACS/WFCRampFilterNoNoFR647MACS/WFCRampFilterNoNoFR505NPOS-TARGDITHER0.472LINEfalsefalse244.4ACS-SBC-DITHER-LINE1falsePOS-TARGDITHER3.034LINEfalsefalse285.29ACS-WFC-DITHER-LINE2false/private/var/folders/8t/mg1bkfyj20xf2vfc_9vyhfs80006z1/T/OPVisit16907536023828474659.xmlThe scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 16062
:visit-id "01"
:proposal-version -1
:trans-version "20191203"
:date "28-Apr-2020 11:51:34.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "28"
:si-bright-earth-limb-angle 20.0
:data-volume 74064
:tdrss-contact-duration 0
:coron NIL
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(Tic-Obset
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(Tic-Orbit
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:orbit-number 1
:pcs-time 333
:si-vis-utilization 2303
:al-overhead-at-end 0
:internal-dur-at-end 117
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
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)true10The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.(Tic-Visit
:proposal-id 16062
:visit-id "02"
:proposal-version -1
:trans-version "20191203"
:date "18-Mar-2020 15:31:36.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "27"
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:data-volume 852752
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:coron NIL
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(Tic-Obset
:proposal-id 16062
:visit-id "02"
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(Tic-Orbit
:proposal-id 16062
:visit-id "02"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2847
:al-overhead-at-end 0
:internal-dur-at-end 347
:dark-offset NIL
:dark-utilization 0
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:low-sky "N"
:pcs-visibility 3180
:pcs-gap 0
)true10