#	Pagina
attuale pagina	/open-h2020/projects/216529/index.html
-1	/open-h2020/per-topic/sensefinity/list/index.html
-2	/open-h2020/projects/225323/index.html
-3	/open-h2020/projects/213269/index.html
-4	/open-h2020/projects/214169/index.html
-5	/open-h2020/projects/218056/index.html
-6	/open-h2020/per-topic/designdevelopment/list/index.html
-7	/open-consip/fornitori/2015/profilo-03818720249/index.html
-8	/open-h2020/projects/197562/index.html
-9	/open-h2020/projects/222179/index.html
-10	/open-h2020/per-topic/snapshot/list/index.html

Opendata, web and dolomites

CONCERTO SIGNED

Intensity mapping of the atomic carbon CII line: the promise of a new observational probe of dusty star-formation in post-reionization and reionization epoch

Total Cost €

EC-Contrib. €

Partnership

Views

CONCERTO project word cloud

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

redshifts degrees dust instead perform square individual population universe cosmic capitalizing apex millimeter construct line frequency sources emission few forefront star straight 5 valuable topology faint era outstanding alternative answer galaxies cross redshift technique fundamental world inductance unexplored lies instruments methodology mapping concerto probes kinetic building questions galaxy detecting map first team dusty instrument install sensitivity 360 lt tracers experiment correlation ideas touching cii flourishing breakthrough band extremely spectra probing regions contributes martin signals spectrometer puplett combined evolution detectors music observe reionization signal fluctuations intensity shaping play interferometer sky capture 200 arrays fast z ghz antenna

Project "CONCERTO" data sheet

The following table provides information about the project.

Coordinator	UNIVERSITE D'AIX MARSEILLE Organization address address: Boulevard Charles Livon 58 city: Marseille postcode: 13284 website: n.a. 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	France [FR]
Total cost	3˙499˙942 €
EC max contribution	3˙499˙942 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2017-ADG
Funding Scheme	ERC-ADG
Starting year	2019
Duration (year-month-day)	from 2019-01-01 to 2023-12-31

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	UNIVERSITE D'AIX MARSEILLE UNIVERSITE D'AIX MARSEILLE Organization address address: Boulevard Charles Livon 58 city: Marseille postcode: 13284 website: n.a. contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	FR (Marseille)	coordinator	2˙214˙437.00
2	CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS Organization address address: RUE MICHEL ANGE 3 city: PARIS postcode: 75794 website: www.cnrs.fr contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	FR (PARIS)	participant	1˙285˙505.00

Map

Project objective

I propose for funding to construct a spectrometer to map in 3-D the intensity due to line emission, a technique known as Intensity Mapping. Instead of detecting individual galaxies, this emerging technique measures signal fluctuations produced by the combined emission of the galaxy population on large regions of the sky in a wide frequency (i.e. redshift) band, and thus increases sensitivity to faint sources. Capitalizing on a recent technology breakthrough, our intensity mapping experiment will measure the 3-D fluctuations of the [CII] line at redshifts 4.5<z<8.5. [CII] is one of the most valuable star formation tracers at high redshift. My project will answer the outstanding questions of whether dusty star-formation contributes to early galaxy evolution, and whether dusty galaxies play an important role in shaping cosmic reionization. My team will first build, test, and finally install the instrument on the APEX antenna following an agreement with APEX partners. The spectrometer will be based on the state-of-the-art development of new arrays in the millimeter using Kinetic Inductance Detectors. Spectra (200-360 GHz) will be obtained by a fast Martin-Puplett interferometer. Then, we will observe with CONCERTO a few square degrees and offer a straight forward alternative for probing star formation and dust build-up in the early Universe. Finally, CONCERTO will set to music the various cosmic evolution probes. Cross-correlation of the signals will be used in particular to capture the topology of the end of reionization era. CONCERTO will be one of two instruments in the world to perform intensity mapping of the [CII] line in the short term. The novel methodology is extremely promising as it targets an unexplored observable touching on some of the fundamental processes building the early universe. In the flourishing of new ideas in the intensity-mapping field, CONCERTO lies at the forefront.

Deliverables

List of deliverables.
Data Management Plan (DMP)	Open Research Data Pilot	2019-08-29 13:09:43

Take a look to the deliverables list in detail: detailed list of CONCERTO deliverables.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "CONCERTO" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

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