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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.

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

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

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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.
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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