0
Assigned ID: 4335
----- Attempting Submission 1 (Wed May 24 13:57:07 GMT 2023) -----
HST Phase I Proposal 4335 successfully submitted.
Receipt: # 4335-1
----- Attempting Submission 2 (Wed May 24 15:15:28 GMT 2023) -----
We resumbit our phase II proposal after the TTRB partially approved our HOPR request and awarded us 1 orbit to repeat the 2nd prbit of visit 16.
-1520670137
----- Attempting Submission 1 (Wed Sep 13 17:19:34 GMT 2023) -----
HST Phase II Proposal 17423 successfully submitted.
Receipt: # 17423-1
----- Attempting Submission 2 (Mon Oct 16 16:38:26 GMT 2023) -----
HST Phase II Proposal 17423 successfully submitted.
Receipt: # 17423-2
----- Attempting Submission 3 (Wed Jan 24 11:44:01 GMT 2024) -----
HST Phase II Proposal 17423 successfully submitted.
Receipt: # 17423-3
----- Attempting Submission 4 (Thu Mar 07 12:24:09 GMT 2024) -----
----- Attempting Submission 6 (Tue Aug 06 07:35:45 GMT 2024) -----
----- Attempting Submission 7 (Tue Aug 20 19:16:08 GMT 2024) -----
I only modified visits J2309+0027 - HOPR (Z6) and I ran both orbit and visit planners for this visit only, to avoid any change also to the other visits. However, it seems that the Orbits and Visit Planners should be run for the other completed/scheduled visits too.
Towards an unbiased sample of sub-arcsec dual AGN with HST/STIS
Hierarchical cosmological models predict the existence of dual active galactic nuclei (AGN) to in-spiral at the centre of the same host galaxy. They are the parent population of interacting supermassive black holes, which will eventually merge by emitting low-frequency gravitational waves. To date, only a handful of dual AGN (15) have been confirmed residing within the same host galaxy (separations < 7 kpc), preventing us to test fundamental predictions of galaxy formation and to conduct any statistical study on dual AGN properties (e.g. separation, black hole mass, luminosity ratio of the two AGN components). Hence, we propose to use HST/STIS to confirm the nature of an unprecedented unbiased sample of 16 multiple AGN, selected via the novel "GMP" technique based on Gaia observations. This method has proven to successfully select dual and lensed AGN at sub-arcsec separations. The proposed spectroscopic observations with HST/STIS will allow us: 1) to classify the targets as dual AGN or lensed systems, excluding cases of AGN/star pairs; 2) to collect a first large enough sample of confirmed dual AGN to conduct a statistical study on their key properties (e.g. separation, mass, luminosity ratio); 3) to confirm new strongly lensed AGN at sub-arcsec separations, the most compact regime ever probed, which will allow us to investigate the innermost region of the lens galaxy with future deep HST imaging.
This program will target binary systems of two AGN of similar luminosity (within a factor of ~5) and a separation between ~0.2" and ~0.8", to unveil their real nature as intrinsic dual AGN or lensed systems.
We will obtain STIS/G750L spectra of both sources our targets consist of. We will place the 2" slit covering both components at a random position angle for most targets, since we do not know the relative position and joining direction of the two sources. For the two targets with known relative position of the two sources, we will place the 2'' slit at a random position angle within a wide range which avoids slit orientations almost perpendicular to the joining direction of the two sources (i.e. we exclude slit orientations closer to the perpendicular direction of about +/- 25 deg, depending on the sources separation). In doing so, we will effectively obtain "slitless" spectra, whose spectral resolution will be determined by the angular size of the target, expected to be spatially unresolved. We will use the E1 aperture position to reduce problems with CTE.
The fainter component could be as faint as G=20.6, therefore we have set the exposure time for acquisition to 60 sec, to have a reasonable S/N also on the secondary object, useful during data analysis to define the position of each target and derive the wavelength calibration of each spectrum.
We will dedicate two orbits to each target, and use a 2-position STIS-ALONG-SLIT pattern with a 1.5'' spacing. The image acquired over each orbit will be split into two or three subexposures, depending on the available time, to optimise the CR correction. In case of two exposures, the Texp will be ~1000 sec each in the first orbit, and ~1300 sec each in the second orbit; in case of three exposures, Texp will be ~700 sec and ~900 sec in the first and second orbits, respectively.
We will obtain contemporary flat fields using a 52X2 aperture, as suggested for the 2" slit.
The team is composed of 8 staff astronomers at universities and public research institutes, two postdoc researchers, three PhD students and a Master's student. Several members of the team have extensive knowledge on both AGN in general and dual AGN in particular, and have published several papers on the topic. F. Mannucci, A. Marconi, and F. Belfiore have been PI of successful HST proposals, and most of the team members have been coIs of several proposals. F. Mannucci, G. Cresci and A. Ciurlo have large experience with analysing spatially resolved spectra obtained with HST and ground-based, AO-assisted telescopes. The team in perfectly equipped, in terms of hardware, software, and knowledge, to analyse HST/STIS spectra and to derive the expected physical information quickly and accurately.
Supermassive Black Holes and Active Galaxies
6
false
false
false
false
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SUPPORTED
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QSO
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QSO
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J2000
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QSO
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QSO
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false
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The scheduling data was generated by CASM 32.0.
CASM was run in Phase II mode.
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The scheduling data was generated by CASM 32.0.
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The scheduling data was generated by CASM 32.0.
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The scheduling data was generated by CASM 32.1.1.
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This is a HOPR partial repeat of failed visit 16
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