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CONCERTO :
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Van Cuyck, M.
(författare)
CONCERTO : Extracting the power spectrum of the [CII] emission line
- Artikel/kapitelEngelska2023
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Nummerbeteckningar
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LIBRIS-ID:oai:DiVA.org:su-221072
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https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-221072URI
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https://doi.org/10.1051/0004-6361/202346270DOI
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Språk:engelska
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Sammanfattning på:engelska
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Ämneskategori:ref swepub-contenttype
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Ämneskategori:art swepub-publicationtype
Anmärkningar
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Context. CONCERTO is the first experiment to perform a [CII] line intensity mapping (LIM) survey on the COSMOS field to target z > 5.2. Measuring the [CII] angular power spectrum allows us to study the role of dusty star-forming galaxies in the star formation history during the epochs of Reionization and post-Reionization. The main obstacle to this measurement is the contamination by bright foregrounds: the dust continuum emission and atomic and molecular lines from foreground galaxies at z ≲ 3.Aims. We evaluate our ability to retrieve the [CII] signal in mock observations of the sky using the Simulated Infrared Dusty Extragalactic Sky (SIDES), which covers the mid-infrared to millimetre range. We also measure the impact of field-to-field variance on the residual foreground contamination.Methods. We compared two methods for dealing with the dust continuum emission from galaxies (i.e. the cosmic infrared background fluctuations): the standard principal component analysis (PCA) and the asymmetric re-weighted penalized least-squares (arPLS) method. For line interlopers, the strategy relies on masking low-redshift galaxies using the instrumental beam profile and external catalogues. As we do not have observations of CO or deep-enough classical CO proxies (such as LIR), we relied on the COSMOS stellar mass catalogue, which we demonstrate to be a reliable CO proxy for masking. To measure the angular power spectrum of masked data, we adapted the P of K EstimatoR (POKER) from cosmic infrared background studies and discuss its use on LIM data.Results. The arPLS method achieves a reduction in the cosmic infrared background fluctuations to a sub-dominant level of the [CII] power at z ∼ 7, a factor of > 70 below our fiducial [CII] model. When using the standard PCA, this factor is only 0.7 at this redshift. The masking lowers the power amplitude of line contamination down to 2 × 10−2 Jy2 sr−1. This residual level is dominated by faint undetected sources that are not clustered around the detected (and masked) sources. For our [CII] model, this results in a detection at z = 5.2 with a power ratio [CII]/(residual interlopers) = 62 ± 32 for a 22% area survey loss. However, at z = 7, [CII]/(residual interlopers) = 2.0 ± 1.4, due to the weak contrast between [CII] and the residual line contamination. Thanks to the large area covered by SIDES-Uchuu, we show that the power amplitude of line residuals varies by 12–15% for z = 5.2 − 7, which is less than the field-to-field variance affecting [CII] power spectra.Conclusions. We present an end-to-end simulation of the extragalactic foreground removal that we ran to detect the [CII] at high redshift via its angular power spectrum. We show that cosmic infrared background fluctuations are not a limiting foreground for [CII] LIM. On the contrary, the CO and [CI] line contamination severely limits our ability to accurately measure the [CII] angular power spectrum at z ≳ 7.
Ämnesord och genrebeteckningar
Biuppslag (personer, institutioner, konferenser, titlar ...)
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Ponthieu, N.
(författare)
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Lagache, G.
(författare)
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Beelen, A.
(författare)
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Béthermin, M.
(författare)
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Gkogkou, A.
(författare)
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Aravena, M.
(författare)
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Benoit, A.
(författare)
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Bounmy, J.
(författare)
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Calvo, M.
(författare)
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Catalano, A.
(författare)
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Désert, F. X.
(författare)
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Dupé, F. -X.
(författare)
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Fasano, A.
(författare)
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Ferrara, A.
(författare)
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Goupy, J.
(författare)
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Hoarau, C.
(författare)
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Hu, W.
(författare)
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Lambert, J. - C.
(författare)
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Macías-Pérez, J. F.
(författare)
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Marpaud, J.
(författare)
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Mellema, GarreltStockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)gmell
(författare)
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Monfardini, A.
(författare)
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Pallottini, A.
(författare)
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Stockholms universitetInstitutionen för astronomi
(creator_code:org_t)
Sammanhörande titlar
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Ingår i:Astronomy and Astrophysics6760004-63611432-0746
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- Av författaren/redakt...
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Van Cuyck, M.
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Ponthieu, N.
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Lagache, G.
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Beelen, A.
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Béthermin, M.
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Gkogkou, A.
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visa fler...
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Aravena, M.
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Benoit, A.
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Bounmy, J.
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Calvo, M.
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Catalano, A.
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Désert, F. X.
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Dupé, F. -X.
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Fasano, A.
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Ferrara, A.
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Goupy, J.
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Hoarau, C.
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Hu, W.
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Lambert, J. - C.
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Macías-Pérez, J. ...
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Marpaud, J.
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Mellema, Garrelt
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Monfardini, A.
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Pallottini, A.
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