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----- Attempting Submission 1 (Thu Dec 09 12:35:58 GMT 2021) -----
HST Phase I Proposal 2649 successfully submitted.
Receipt: # 2649-1
----- Attempting Submission 2 (Thu Dec 09 12:44:56 GMT 2021) -----Joint XMM/HST ProposalCOS ACQ/PEAKD exposure should be preceded by an ACQ/PEAKXD exposure in the Visit.Dear colleagues,
this is a further resubmission of my Phase II Proposal 16899.
I set the SCHEDULABILITY to 100.
Best regards, Wolfram Kollatschny-1903633701----- Attempting Submission 1 (Tue Jan 11 09:27:59 GMT 2022) -----
HST Phase II Proposal 16899 successfully submitted.
Receipt: # 16899-1
----- Attempting Submission 2 (Mon Jan 17 17:16:04 GMT 2022) -----
----- Attempting Submission 3 (Tue Apr 12 13:11:51 GMT 2022) -----
HST Phase II Proposal 16899 successfully submitted.
Receipt: # 16899-3
----- Attempting Submission 4 (Thu Apr 14 09:37:30 GMT 2022) -----I do not understand the warning: COS ACQ/PEAKD exposure should be preceded by an ACQ/PEAKXD
exposure in the Visit.
I made this.The extreme X-ray weakness of PG 0043+039PG 0043+039 is the most X-ray weak quasar known to date. Marginally detected in 2005, an XMM- Newton observation in 2013 set a clear detection im- plying a flux increase of at least a factor 3.8. Simulta- neous observations at other wavelengths showed the quasar still extreme X-ray weak, with a peculiar spec- tral energy distribution (SED) and unique features in the UV spectrum. We propose that PG 0043+039 is a genuine X-ray weak quasar. To probe this hy- pothesis and to test alternative emission scenarios (ADAFs, missing corona (Ricci et al., 2020 ApJ 898, L1), cyclotron-emission (Kollatschny et al. 2015, A&A, 577, L1)) this unique source deserves further, deeper, observations, aiming to establish its X-ray spectrum, its optical to hard X-ray SED and new con- straints on its variability. Our proposal is to observe PG 0043+039 quasi-simultaneously (2 days) with XMM-Newton (100ks + 20ks), NuSTAR (60ks) and HST (2 orbits). We will arrange quasi-simultaneous observations with the ground 10m Hobby-Eberly Telescope in Texas and with the 10m SALT Telescope in South Africa.PG 0043+039 is the most X-ray weak quasar known. We plan to observe PG0043+039 quasi-simultaneously with HST and XMM. We intend to take a FUV spectrum with COS/FUV G140L(1105) for the first orbit. The second orbit is devoted to a NUV spectrum with COS/NUV G230L.
We observed this quasar before with COS/FUV G140L(1105) on July 18, 2013. See the publication: Kollatschny+ 2016, A&A585, A18.n/aSupermassive Black Holes and Active Galaxies6falsefalsefalsefalsefalsefalsefalseSUPPORTEDGALAXYQUASARNOJ2000J2000COS/FUVSpectroscopicNoNoG140L1280COS/NUVSpectroscopicNoNoG230L2635COS/NUVSpectroscopicNoNoG230L2635/users/wkollat/Propos/HST/Schartelpg0043_2021/OP-cache/wk_Ph2_16899_20220412-v01.xmlThe scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.(Tic-Visit
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