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Assigned ID: 666
----- Attempting Submission 1 (Fri Mar 06 19:03:38 GMT 2020) -----
ORBIT PLANNER SERVER INTERNAL ERROR
In this version, we have increased the exptime for ACQs for the remaining visits (including repeated HOPR visits) to ensure proper acquisition of the target. We also duplicated the failed visit 12 (approved HOPR request) in visit ZA.
1966785126
----- Attempting Submission 1 (Tue Jun 23 03:16:32 GMT 2020) -----
----- Attempting Submission 2 (Thu Nov 05 17:13:16 GMT 2020) -----
----- Attempting Submission 3 (Wed Jan 05 17:21:07 GMT 2022) -----
I accidently changed the exptime for ACQ exposure for visit 07, which is being scheduled. This caused a technical problem with the APT file, but should not affect the rest of the visits.
Understanding the offset in the broad-line region size-luminosity relation with UV spectroscopy
Nearly two decades of reverberation mapping (RM) studies on nearby AGN have revealed a tight correlation between the size of the Hbeta broad-line region and the optical luminosity of the AGN, designated the R-L relation. This correlation is the foundation for the so-called "single-epoch virial black hole mass estimators" that have been widely applied to distant quasars to estimate their black hole masses without dedicated RM measurements. Recent RM measurements for quasars beyond the nearby Universe and for a subset of nearby AGN with estimated high accretion rates have independently revealed a systematic offset from the canonical R-L relation based on the nearby RM AGN sample. The most likely explanation of this offset is that these new RM samples explore AGN that have different accretion rates and therefore different shapes of the continuum spectral energy distribution (SED), responsible for ionizing the line-emitting gas, than the nearby RM AGN sample. We propose STIS UV spectroscopy for a sample of 18 quasars at z~0.4 from one of these recent RM samples to test this hypothesis and to develop empirical corrections to the R-L relation based on additional AGN parameters. We will model the UV spectra with detailed photoionization calculations to constrain the ionizing continuum directly incident on the broad-line region gas. The combination of UV and (existing) optical spectroscopy for a unique non-local AGN sample with direct RM-based black hole masses also will enable better SED-fitting to constrain accretion parameters and better calibrations of single-epoch mass recipes based on UV broad emission lines.
This program will observe 18 low-redshift (0.2<z<0.6) broad-line quasars with STIS NUV-MAMA G230L in spectroscopic mode. These targets have GALEX NUV mag ~ 19-21 and SDSS r-band mag ~ 19~20.
We will use the 52"x0.2" slit, and observe with 1 orbit for 12 targets, 2 orbits for 5 targets and 3 orbits for 1 target (RM301). Our targets are largely point-sources (bright quasars) so we will use the point-source mode for acqusition. Our targets are the brightest source within 5x5 arcsecond area, and there is no need for peakup acquisition.
Each visit consists of acquisition with the F28x50LP CCD aperture, with typical exposure time of 30 seconds, followed by a single (or multiple in case of more than one orbit for the visit) MAMA exposure. We do not require special slit orientations for these observations.
The proposing team includes experts on reverberation mapping (RM), AGN physics, and photoionization modeling. Team memebers have access to the multi-wavelength data already collected and future data (in particular the quasi-simultaneous optical spectroscopy) for the target sample.
Specifically, PI Shen works on RM and AGN science, and is leading the SDSS-RM project and its extension into the SDSS-V survey (2020-2025). Co-I Jennifer Li is a PhD student at PI's institution and works on the SDSS-RM data. Co-I Hengxiao Guo is a postdoc at PI's institution and is an expert on photoionization modeling of AGN spectra. Co-Is Brad Peterson, Keith Horne and Luis Ho are long-time experts on RM and AGN science. Co-Is Kate Grier, Niel Brandt, Patrick Hall, Yasaman Homayouni, Don Schneider, and Scott Anderson are core members of the SDSS-RM team, and are experienced with RM, AGN variability and related science.
Supermassive Black Holes and Active Galaxies
6
false
false
true
false
false
false
false
false
SUPPORTED
GALAXY
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STIS/NUV-MAMA
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