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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.

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