For G160M observations, please consult Chapter 9 of the COS Instrument Handbook to estimate overheads and the number of exposures per orbit, and consequently the correct lifetime position. Use of LP4 with G160M requires justification in the "Special Requirements" section of the Phase I PDF. Use of the default LP6 with G160M requires no justification. Proposals can be submitted with the warning present. This is to be coordinated with XMM and that is not yet scheduled -857567776 Assigned ID: 6048 ----- Attempting Submission 1 (Wed Dec 18 21:10:53 GMT 2024) ----- HST Phase I Proposal 6048 successfully submitted. Receipt: # 6048-1 Warning not relevant for Phase I submission COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE COORDINATES SHOULD BE IN THE ICRS REFERENCE SYSTEM FOR A SMALL APERTURE 0 ----- Attempting Submission 1 (Tue Jan 07 17:49:20 GMT 2025) ----- ----- Attempting Submission 2 (Mon Jan 13 00:07:11 GMT 2025) ----- Have conferred with contact scientist to determine proposal is OK We propose a 220 ks XMM exposure with 150 ks of NuSTAR and 4 orbits of HST in support of a 150 ks approved cycle 1 XRISM observation of NGC 4051. Together these will reveal reprocessing signatures over a broad range of xi, NH and velocity. The tightly-constrained black hole mass in NGC 4051 will facilitate translation of measurements to accurate radial and geometric constraints, elucidating contributions from the accretion disk, BLR and torus. The proposed campaign will provide a major step toward a complete model for the reprocessor. We propose a 220 ks XMM exposure with 150 ks of NuSTAR and 4 orbits of HST in support of a 150 ks approved cycle 1 XRISM observation of NGC 4051. Dr. Turner has extensive experience in the analysis, interpretation and publication of X-ray spectral and timing data has authored 200 publications in refereed journals and discovered the first case of anomalous unidentified lines redward of Fe Kalpha. Dr. Reeves has extensive experience in analysis, interpretation and publication of X-ray spectral data including modeling of fast outflowing X-ray winds. Dr. Reeves has extensive experience with high-resolution spectra. Dr. Reeves is also a XRISM Guest Scientist and is working on PV phase observations of PDS 456. Dr. Braito has extensive experience in analysis, interpretation and publication of X-ray spectral data and experience with high resolution X-ray imaging. Dr. Braito has extensive experience with high-resolution spectra. Dr. Anna Trindade Falcao has experience in analysis, interpretation and publication of HST COS and STIS data. Dr Trindada Falcao also has experience with X-ray data analysis and modeling. Dr Shoji Ogawa has experience with X-ray data, in particular Dr Ogawa has worked extensively with data from the new XRISM satellite, covering a range of source categories. Satoshi Yamada has experience with X-ray data and has worked extensively with data from the new XRISM satellite, acquiring expertise in the analysis of Resolve and Xtend data, and in the particulars of both instruments. Dr Yamada has expertise in AGN and other fields. Supermassive Black Holes and Active Galaxies 6 false false false false false false false true SECONDARY XMM_NEWTON 096015 false SUPPORTED GALAXY ACCRETION DISK SEYFERT NO This object was generated by the targetselector and retrieved from the NED database. J2000 J2000 COS/FUV Spectroscopic No No G130M 1222 COS/FUV Spectroscopic No No G160M 1533 /private/var/folders/4n/tsz7xr8d6y3d6dlqybjwz6j80000gn/T/OPVisit6021993039509900250.xml 1736726694547 The scheduling data was generated by CASM 32.1.3. CASM was run in Phase II mode. (Tic-Visit :proposal-id 17896 :visit-id "01" :proposal-version -1 :trans-version "20240604" :date "12-Jan-2025 19:04:53.0" :trans-errors '(:WARNINGS 9 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 4 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 852768 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17896 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17896 :visit-id "01" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2669 :al-overhead-at-end 0 :internal-dur-at-end 57 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3049 :pcs-gap 0 ) (Tic-Orbit :proposal-id 17896 :visit-id "01" :orbit-number 2 :pcs-time 380 :si-vis-utilization 2669 :al-overhead-at-end 0 :internal-dur-at-end 2261 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3049 :pcs-gap 0 ) (Tic-Orbit :proposal-id 17896 :visit-id "01" :orbit-number 3 :pcs-time 380 :si-vis-utilization 2669 :al-overhead-at-end 0 :internal-dur-at-end 2256 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3049 :pcs-gap 0 ) (Tic-Orbit :proposal-id 17896 :visit-id "01" :orbit-number 4 :pcs-time 380 :si-vis-utilization 2669 :al-overhead-at-end 0 :internal-dur-at-end 546 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3049 :pcs-gap 0 ) true 4 0 Schedule with XMM