An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations

Ibarra-Medel, H.; Negrete, C. A.; Lacerna, I.; Hernández-Toledo, H. M.; Cortes-Suárez, E.; Sánchez, S. F.

doi:10.1093/mnras/stae2623

Title: An iterative method to deblend AGN-Host contributions for Integral Field spectroscopic observations

Journal Article · 22 November 2024 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stae2623 · OSTI ID:2480760

;

; Hernández-Toledo, H. M.; Cortes-Suárez, E.;

ABSTRACT We present a new iterative deblending method to separate the host galaxy (HG) and their Active Galactic Nuclei (AGNs) emission with the use of Integral Field spectroscopic (IFS) data. The method decomposes the resolved HG emission from the unresolved AGN emission by modelling the two-dimensional surface brightness (SB) profile of the point-spread function (PSF) and the two-dimensional SB HG continuum simultaneously per each monochromatic slide. Our method does not require any prior information about the observed SB profile or a detailed fitting of the PSF, making it ideal for the automatic analysis of large galaxy samples. In this work, we test the quality of our method, its advantages, and its disadvantages. We test our method by using a set of IFS mock data cubes to quantify the reliability of our deblending process and further compare our method with the qdblend3d analysis tool. Furthermore, we applied our method to three data cubes selected from the MaNGA survey according to the dominance of either its HG or its AGN. We show that our deblending method is capable of disengaging the bright, non-resolved AGN emission from the HG continuum and its narrow emission lines. However, the decoupling depends on how well the IFS spatially resolves the PSF, and on the relative flux intensity of the HG-AGN. Therefore, the method is ideal for disentangling the bright-flux contribution from AGN-dominated spectra.

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Sponsoring Organization:: USDOE

OSTI ID:: 2480760

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 536; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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Chemical Evolution History of MaNGA Galaxies Camps-Fariña, Artemi; Sánchez, Sebastián F.; Mejía-Narváez, Alfredo The Astrophysical Journal, Vol. 933, Issue 1 https://doi.org/10.3847/1538-4357/ac6cea	journal	July 2022
A Catalog of 71 Coronal Line Galaxies in MaNGA: [Ne v] Is an Effective AGN Tracer Negus, James; Comerford, Julia M.; Sánchez, Francisco Müller The Astrophysical Journal, Vol. 945, Issue 2 https://doi.org/10.3847/1538-4357/acb772	journal	March 2023
Active Galactic Nuclei Feedback in SDSS-IV MaNGA: AGNs Have Suppressed Central Star Formation Rates Lammers, Caleb; Iyer, Kartheik G.; Ibarra-Medel, Hector The Astrophysical Journal, Vol. 953, Issue 1 https://doi.org/10.3847/1538-4357/acdd57	journal	July 2023
The Sloan Digital Sky Survey Reverberation Mapping Project: The Black Hole Mass–Stellar Mass Relations at 0.2 ≲ z ≲ 0.8 Li, Jennifer I-Hsiu; Shen, Yue; Ho, Luis C. The Astrophysical Journal, Vol. 954, Issue 2 https://doi.org/10.3847/1538-4357/acddda	journal	September 2023
First Results from the JWST Early Release Science Program Q3D: The Warm Ionized Gas Outflow in z ∼ 1.6 Quasar XID 2028 and Its Impact on the Host Galaxy Veilleux, Sylvain; Liu, Weizhe; Vayner, Andrey The Astrophysical Journal, Vol. 953, Issue 1 https://doi.org/10.3847/1538-4357/ace10f	journal	August 2023
First Results from the JWST Early Release Science Program Q3D: Ionization Cone, Clumpy Star Formation, and Shocks in a z = 3 Extremely Red Quasar Host Vayner, Andrey; Zakamska, Nadia L.; Ishikawa, Yuzo The Astrophysical Journal, Vol. 955, Issue 2 https://doi.org/10.3847/1538-4357/ace784	journal	September 2023
The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release Lyke, Brad W.; Higley, Alexandra N.; McLane, J. N. The Astrophysical Journal Supplement Series, Vol. 250, Issue 1 https://doi.org/10.3847/1538-4365/aba623	journal	August 2020
Point-spread Function Deconvolution of the IFU Data and Restoration of Galaxy Stellar Kinematics Chung, Haeun; Park, Changbom; Park, Yong-Sun The Astrophysical Journal Supplement Series, Vol. 257, Issue 2 https://doi.org/10.3847/1538-4365/ac2828	journal	December 2021
The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data The Astrophysical Journal Supplement Series, Vol. 259, Issue 2, p. 35 https://doi.org/10.3847/1538-4365/ac4414	journal	March 2022
SDSS-IV MaNGA: pyPipe3D Analysis Release for 10,000 Galaxies Sánchez, S. F.; Barrera-Ballesteros, J. K.; Lacerda, E. The Astrophysical Journal Supplement Series, Vol. 262, Issue 2 https://doi.org/10.3847/1538-4365/ac7b8f	journal	September 2022
The Eighteenth Data Release of the Sloan Digital Sky Surveys: Targeting and First Spectra from SDSS-V Almeida, Andrés; Anderson, Scott F.; Argudo-Fernández, Maria The Astrophysical Journal Supplement Series, Vol. 267, Issue 2 https://doi.org/10.3847/1538-4365/acda98	journal	August 2023
Spatially Resolved star Formation main Sequence of Galaxies in the Califa Survey Cano-Díaz, M.; Sánchez, S. F.; Zibetti, S. The Astrophysical Journal, Vol. 821, Issue 2 https://doi.org/10.3847/2041-8205/821/2/L26	journal	April 2016
First Results from the JWST Early Release Science Program Q3D: Turbulent Times in the Life of a z ∼ 3 Extremely Red Quasar Revealed by NIRSpec IFU Wylezalek, Dominika; Vayner, Andrey; Rupke, David S. N. The Astrophysical Journal Letters, Vol. 940, Issue 1 https://doi.org/10.3847/2041-8213/ac98c3	journal	November 2022
Pipe3D, a pipeline to analyze Integral Field Spectroscopy data: I. New fitting phylosophy of FIT3D Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P. arXiv https://doi.org/10.48550/arXiv.1509.08552	preprint	January 2015
Pipe3D, a pipeline to analyse integral field spectroscopy data: II. Analysis sequence and CALIFA dataproducts Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P. arXiv https://doi.org/10.48550/arXiv.1602.01830	preprint	January 2016
The geometry of the quadruply imaged quasar PG 1115+080; implications for Ho Courbin, F.; Magain, P.; Keeton, C. R. arXiv https://doi.org/10.48550/arXiv.astro-ph/9705093	text	January 1997

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