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HIDDeN SIGNED

HIDDeN - Exploring the Hidden Dusty Nuclei of Galaxies

Total Cost €

EC-Contrib. €

Partnership

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HIDDeN project word cloud

Explore the words cloud of the HIDDeN project. It provides you a very rough idea of what is the project "HIDDeN" about.

optical bolometric environments smbh connection regions central astrophysical discovered observations rapid heretofore nearby interconnected local 2 obscured dust alma duty complete co full spurts ground z agns context galactic galaxies starburst ray give luminous universe lirgs hst luminosity inflows connections emit powered active distant starbursts critical jvla advantage holes winds drive fraction wavelengths observational telescopes suggest largely lofar mm molecular curtain submm noema centres nature picture ir constraints accreting phases cold suspected supermassive compact cosmic infrared nuclei bursts deeply jwst breaking cons evolution unexplored 1 black extreme hidden star evolutionary takes interiors dusty galaxy near probing goals smbhs agn outflows unreachable cycle closest examples redshift host mainly

Project "HIDDeN" data sheet

The following table provides information about the project.

Coordinator	CHALMERS TEKNISKA HOEGSKOLA AB Organization address address: - city: GOETEBORG postcode: 41296 website: www.chalmers.se contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	Sweden [SE]
Total cost	2˙496˙320 €
EC max contribution	2˙496˙319 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2017-ADG
Funding Scheme	ERC-ADG
Starting year	2018
Duration (year-month-day)	from 2018-10-01 to 2023-09-30

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	CHALMERS TEKNISKA HOEGSKOLA AB CHALMERS TEKNISKA HOEGSKOLA AB Organization address address: - city: GOETEBORG postcode: 41296 website: www.chalmers.se contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	SE (GOETEBORG)	coordinator	2˙496˙319.00

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Project objective

Luminous infrared galaxies (LIRGs) emit most of their bolometric luminosity in the far-infrared. They are mainly powered by extreme bursts of star formation and/or Active Galactic Nuclei (AGNs; accreting supermassive black holes (SMBHs)) in their centres. LIRGs are the closest examples of rapid evolution in galaxies and a detailed study of LIRGs is critical for our understanding of the cosmic evolution of galaxies and SMBHs. Centres of some LIRGs are deeply obscured and unreachable at optical, IR and even X-ray wavelengths. These hidden nuclei therefore represent a largely unexplored phase of the growth of central regions with their SMBHs. Large growth spurts are suspected to occur when the SMBHs are deeply embedded. Obscured AGNs thus can provide new constraints on the AGN duty cycle, give the full range of environments and astrophysical processes that drive the growth of SMBHs, and help to complete the picture of connections between the host galaxy and SMBH. Many dust embedded AGNs are still to be discovered as studies suggest that a significant fraction of SMBHs may be obscured in the local and more distant Universe.â€¨In the HIDDeN project we use mm and submm observational methods to reach behind the curtain of dust in the most embedded centres of LIRGs, allowing us to undertake ground-breaking studies of heretofore hidden rapid evolutionary phases of nearby galaxy nuclei. HIDDeN takes advantage of emerging opportunities to address the nature of near-field, and redshift z=1-2, obscured AGNs/starbursts and their associated molecular inflows and outflows in the context of their evolution and the starburst-AGN connection. In particular we use the ALMA and NOEMA telescopes, supported by JVLA, LOFAR, HST and future JWST observations, to address four interconnected goals: A. Probing the Dusty Interiors of Compact Obscured Nuclei (CONs), B. The cold winds of change - Molecular Outflows from LIRGs and AGNs, C. The Co-Evolution of Starbursts and AGNs and D. Are there hidden CONs at z=1-2

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