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HIDDeN SIGNED

HIDDeN - Exploring the Hidden Dusty Nuclei of Galaxies

Total Cost €

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EC-Contrib. €

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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.

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

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 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.
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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