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Opendata, web and dolomites

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.

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

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

Map

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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The information about "HIDDEN" are provided by the European Opendata Portal: CORDIS opendata.