Science Keywords: Select from 2 to 5 items. Science Keywords is a required field. US Admin CoI is a required field. Wavelength is a required field. Wavelength is a required field. 0 Assigned ID: 1623 ----- Attempting Submission 1 (Mon Dec 11 15:56:29 GMT 2017) ----- Joint XMM/HST For the best data quality, it is strongly recommended that the maximum number of allowed FP-POS positions is used when observing at a given COS CENWAVE setting. See full description for details. REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE adjusted exposure time to fit orbits with schedulability = 100 291372565 ----- Attempting Submission 1 (Thu Jan 11 23:25:09 GMT 2018) ----- Your proposal could not be saved. Submission aborted. ----- Attempting Submission 2 (Fri Jan 12 19:52:12 GMT 2018) ----- ----- Attempting Submission 3 (Fri Jul 06 19:01:52 GMT 2018) ----- ----- Attempting Submission 4 (Fri Jul 06 21:11:53 GMT 2018) ----- The only warning now is the one associated with the "Extended" parameter which is not used anymore. The deep minimum state of AGNs is characterized by a strongly suppressed or even absent primary continuum. As the continuum disappears weak spectral features like relativistic iron lines or narrow soft X-ray emission lines from ionised plasmas become highly significant and their parameters can be determined. Therefore deep minimum states offer unique possibilities to investigate in detail the physics of the reprocessed components in AGN, including the immediate vicinity of the supermassive black hole. Applying our experience (several deep minimum observations) we propose 2 triggered 10ks XMM snapshot, one 80ks XMM follow-up simultaneous with one 80ks NuSTAR one 2-orbit HST observation of an AGN in deep minimum state. We will identify deep minimum states mainly based on Swift and XMM-Newton slews. During the first orbit we need a 30s aquisition image (MIRRORB ACQ/Image PSA) and then a 1800s exposure with G130M centered at 1291A. During the second orbit we need a 1800s exposure with G160M at 1623A Massive Black Holes And Their Host Galaxies 6 false false false false false false 80 false SUPPORTED GALAXY QUASAR NO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 COS/FUV Spectroscopic No No G160M COS/FUV Spectroscopic No No G130M 1530911420833 /private/var/folders/f8/jhfklx8j2jn082w2wqr5s47r0000gr/T/OPVisit1321511731994714933.xml The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. (Tic-Visit :proposal-id 15439 :visit-id "01" :proposal-version -1 :trans-version "20180409" :date "06-Jul-2018 17:10:20.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 278464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15439 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15439 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2652 :al-overhead-at-end 0 :internal-dur-at-end 114 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2989 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15439 :visit-id "01" :orbit-number 2 :pcs-time 222 :si-vis-utilization 2758 :al-overhead-at-end 0 :internal-dur-at-end 350 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2989 :pcs-gap 0 ) true 2 0