About: Marian Douspis

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An Entity of Type : foaf:Person, within Data Space : data.idref.fr associated with source document(s)

Attributes	Values
type	Person
sameAs	Douspis, Marian (19..-....) Douspis, Marian (19..-....)
Life Event	http://www.idref.fr/063461498/birth
preferred label	Douspis, Marian (19..-....)
name	Marian Douspis
dbpedia-owl:citizenship	http://sws.geonames.org/3017382/
Language	http://lexvo.org/id/iso639-3/fra
Given name	Marian
familyName	Douspis
has biographical i...tion (Deprecated)	Co-directeur d'une thèse de : astronomie et astrophysique, Université Paris-Sud 11, Orsay (en 2010) Astronome à l'Institut d'Astrophysique Spatiale (Orsay) (en 2022)
note	Titulaire d'une thèse de doctorat en Astrophysique soutenue à l'Université Paul Sabatier à Toulouse (en 2000)
gender	male
ORCID iD	0000-0003-4203-3954
Scopus ID	6701702242
is sameAs of	Douspis, Marian (19..-....) Douspis, Marian (19..-....) Douspis, Marian (19..-....)
is Thesis advisor of	L'effet Sunyaev-Zel'dovich dans l'analyse du fond diffus cosmologique http://www.sudoc.fr/160132436/id http://www.sudoc.fr/194576884/id http://www.sudoc.fr/251848523/id http://www.sudoc.fr/274104474/id http://www.sudoc.fr/25405756X/id http://www.sudoc.fr/281211078/id
is Praeses of	http://www.sudoc.fr/221473297/id http://www.sudoc.fr/231943741/id
is Author of	http://www.sudoc.fr/063466139/id Archeops in-flight performance, data processing, and map making Planck intermediate results. XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE An alternative to the cosmological 'concordance model Euclid preparation. XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields Cosmological Parameter Estimation: Method Planck intermediate results. I. Further validation of new Planck clusters with XMM-Newton What can be learned about dark energy evolution? Planck 2013 results. XXX. Cosmic infrared background measurements and implications for star formation Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible Detection of intercluster gas in superclusters using the thermal Sunyaev–Zel’dovich effect Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects Planck intermediate results. XXIX. All-sky dust modelling with Planck, IRAS, and WISE observations Planck intermediate results. XXXII. The relative orientation between the magnetic field and structures traced by interstellar dust The Good, the Bad, and the Ugly: Statistical quality assessment of SZ detections Planck intermediate results. LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck Large-scale galaxy correlations as a test for dark energy Optical validation and characterization of Planck PSZ1 sources at the Canary Islands observatories. I. First year of ITP13 observations Star formation rates and stellar masses from machine learning Euclid: Fast two-point correlation function covariance through linear construction Constraints from thermal Sunyaev-Zel’dovich cluster counts and power spectrum combined with CMB Detectability of the 21-cm CMB cross-correlation from the epoch of reionization Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates https://hal.archives-ouvertes.fr/hal-02022168#id Planck 2018 results X. Constraints on inflation Planck intermediate results: XLVIII. Disentangling Galactic dust emission and cosmic infrared background anisotropies Evidence for new physics from clusters ? Small scale contributions to CMB: A coherent analysis Retrieving cosmological information from small-scale CMB foregrounds https://hal.archives-ouvertes.fr/hal-04700348#id Planck pre-launch status: The Planck mission Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories Euclid preparation. XIII. Forecasts for galaxy morphology with the Euclid Survey using deep generative models Euclid preparation X-ray galaxy clusters abundance and mass temperature scaling Planck 2015 results Planck 2015 results Planck 2015 results Biases on the cosmological parameters and thermal Sunyaev-Zel'dovich residuals Planck 2013 results. XXXI. Consistency of the Planck data Planck intermediate results X. Physics of the hot gas in the Coma cluster Planck early results. XIV. ERCSC validation and extreme radio sources https://hal.archives-ouvertes.fr/hal-02022192#id Planck early results. I. The Planck mission Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal Planck intermediate results. XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories The cross-correlation of the CMB polarization and the 21-cm line fluctuations from cosmic reionization Implications of bias evolution on measurements of the integrated Sachs-Wolfe effect: errors and biases in parameter estimation Planck 2015 results. XIV. Dark energy and modified gravity Comparison of Sunyaev-Zel’dovich measurements from Planck and from the Arcminute Microkelvin Imager for 99 galaxy clusters Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization Euclid preparation. X. The Euclid photometric-redshift challenge Goodness-of-fit statistics and CMB data sets X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38 http://www.sudoc.fr/246599987/id Planck intermediate results XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds A cross-correlation study between the cosmological 21 cm signal and the kinetic Sunyaev-Zel'dovich effect https://hal.archives-ouvertes.fr/in2p3-00556895#id PACT I: Combining ACT and Planck data for optimal detection of tSZ signal Planck 2018 results V. CMB power spectra and likelihoods Cosmological constraints from the observed angular cross-power spectrum between Sunyaev-Zel’dovich and X-ray surveys Cosmological implications from the observed properties of CMB. Gas and galaxies in filaments between clusters of galaxies - The study of A399-A401 Planck 2013 results . XX . Cosmology from Sunyaev-Zeldovich cluster counts A new parameterization of the reionisation history Planck intermediate results Planck 2015 results Planck 2015 results ATCA observations of the MACS-Planck Radio Halo Cluster Project https://hal.archives-ouvertes.fr/in2p3-00555658#id The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to z ∼ 5

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