{"id":811,"date":"2025-05-10T12:50:01","date_gmt":"2025-05-10T12:50:01","guid":{"rendered":"https:\/\/luth.obspm.fr\/~luthier\/corasaniti\/?page_id=811"},"modified":"2025-05-12T08:12:06","modified_gmt":"2025-05-12T08:12:06","slug":"publications-2","status":"publish","type":"page","link":"https:\/\/people-lux.obspm.fr\/corasaniti\/?page_id=811","title":{"rendered":"Publications"},"content":{"rendered":"\n<p>List of articles and bibliometrics: <a href=\"https:\/\/ui.adsabs.harvard.edu\/search\/fq=%7B!type%3Daqp%20v%3D%24fq_database%7D&amp;fq_database=database%3A%20astronomy&amp;q=author%3A(%22Corasaniti%2C%20P%22)&amp;sort=date%20desc%2C%20bibcode%20desc&amp;p_=0\" data-type=\"link\" data-id=\"https:\/\/ui.adsabs.harvard.edu\/search\/fq=%7B!type%3Daqp%20v%3D%24fq_database%7D&amp;fq_database=database%3A%20astronomy&amp;q=author%3A(%22Corasaniti%2C%20P%22)&amp;sort=date%20desc%2C%20bibcode%20desc&amp;p_=0\"><strong>ADS<\/strong><\/a> \/ <a href=\"https:\/\/inspirehep.net\/literature?sort=mostrecent&amp;size=25&amp;page=1&amp;q=find%20author%20corasaniti%2C%20p&amp;ui-citation-summary=true\" data-type=\"link\" data-id=\"https:\/\/inspirehep.net\/literature?sort=mostrecent&amp;size=25&amp;page=1&amp;q=find%20author%20corasaniti%2C%20p&amp;ui-citation-summary=true\"><strong>SPIRES<\/strong><\/a><\/p>\n\n\n\n<ol reversed class=\"wp-block-list\">\n<li><strong>P.S. Corasaniti <\/strong>et al., \u201c<em>The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project<\/em>&#8220;, A&amp;A 697, A33 (2025), <a href=\"https:\/\/arxiv.org\/abs\/2503.16379\">arXiv:2503.16379<\/a><\/li>\n\n\n\n<li>Y. Mellier et al., \u201c<em>Euclid. I. Overview of the Euclid mission<\/em>&#8220;, A&amp;A 697, A1 (2025), <a href=\"https:\/\/arxiv.org\/abs\/2405.13491\">arXiv:2405.13491<\/a><\/li>\n\n\n\n<li>G. Racz et al., \u201c<em>Euclid preparation LXIII. Simulations and nonlinearities beyond\u00a0\u039bCDM. 2. Results from non-standard simulations<\/em>&#8220;, A&amp;A 695, A232 (2025), <a href=\"https:\/\/arxiv.org\/abs\/2409.03523\">arXiv:2409.03523<\/a><\/li>\n\n\n\n<li>I. S\u00e1ez-Casares, Y. Rasera, T. R. G. Richardson,\u00a0<strong>P.-S. Corasaniti<\/strong>,\u201c<em>The e-MANTIS emulator: Fast and accurate predictions of the halo mass function in f(R)CDM and wCDM cosmologies<\/em>&#8221;, A&amp;A 691, A323 (2024), <a href=\"https:\/\/arxiv.org\/abs\/2410.05226\">arXiv:2410.05226<\/a><\/li>\n\n\n\n<li>C. Giocoli et al., \u201c<em>Euclid preparation. XXX. Evaluating the weak lensing cluster mass biases using the Three Hundred Project hydrodynamical simulations<\/em>\u201d, A&amp;A 681, A67 (2024),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2302.00687\">arXiv:2302.00687<\/a><\/li>\n\n\n\n<li>T. Richardson,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>A non-parametric approach to the relation between the halo mass function and internal dark matter structure of haloes<\/em>\u201d, A&amp;A 674, A173 (2023),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2212.03233\">arXiv:2212.03233<\/a><\/li>\n\n\n\n<li>L. Blot,&nbsp;<strong>P.S. Corasaniti<\/strong>, F. Schmidt,&nbsp;\u201c<em>Non-linear Eulerian Hydrodynamics of Dark Energy: Riemann problem and Finite Volume Schemes<\/em>\u201d, JCAP 05, 001 (2023),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2210.04800\">arXiv:2210.04800<\/a><\/li>\n\n\n\n<li>T. Castro et al.&nbsp;\u201c<em>Euclid preparation. XXIV. Calibration of the halo mass function in \u039b(\u03bd)CDM cosmologies<\/em>\u201d, A&amp;A 671, A100 (2023),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2208.02174\">arXiv:2208.02174<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, A.M.C. Le Brun, T. Richardson, Y. Rasera, S. Ettori, M. Arnaud, G.W. Pratt,&nbsp;\u201c<em>Forecasting cosmological parameter constraints using multiple sparsity measurements as tracers of the mass profiles of dark matter haloes<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 516, 437 (2022),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2204.06582\">arXiv:2204.06582<\/a><\/li>\n\n\n\n<li>T. Richardson,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Timing the last major merger of galaxy clusters with large halo sparsity<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 513, 4951 (2022),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2112.04926\">arXiv:2112.04926<\/a><\/li>\n\n\n\n<li>Y. Rasera et al.,&nbsp;\u201c<em>The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: An application to lensing-matter clustering statistics<\/em>\u201d, A&amp;A 661, A90 (2022),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2111.08745\">arXiv:2111.08745<\/a><\/li>\n\n\n\n<li>J.P. Willis et al.,&nbsp;\u201c<em>Understanding X-ray and optical selection of galaxy clusters: A comparison of the XXL and CAMIRA cluster catalogues obtained in the common XXL-HSC SSP area<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 503, 5624 (2021),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2103.13434\">arXiv:2103.13434<\/a><\/li>\n\n\n\n<li>CHEX-MATE Collaboration: M. Arnaud et al.,&nbsp;\u201c<em>The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview<\/em>\u201d, A&amp;A 650, A104 (2021),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2010.11972\">arXiv:2010.11972<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, M. Sereno, S. Ettori,&nbsp;\u201c<em>Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data<\/em>\u201d, Astrophys. J. 911, 82 (2021),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2103.03283\">arXiv:2103.03283<\/a><\/li>\n\n\n\n<li>G. Parimbelli et al.,&nbsp;\u201c<em>The effects of massive neutrinos on the linear point of the correlation function<\/em>\u201d, JCAP 01, 009 (2021),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2007.10345\">arXiv:2007.10345<\/a><\/li>\n\n\n\n<li>L. Blot,&nbsp;<strong>P.S. Corasaniti<\/strong>, Y. Rasera, S. Agarwal,&nbsp;\u201c<em>Cosmological Model Parameter Dependence of the Matter Power Spectrum Covariance from the DEUS-PUR Cosmo Simulations<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 500, 2532 (2021),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2007.14984\">arXiv:2007.14984<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, C. Giocoli, M. Baldi,&nbsp;\u201c<em>Dark Matter Halo Sparsity of Modified Gravity Scenarios<\/em>\u201d, Phys. Rev. D 102, 043501 (2020),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/2005.13682\">arXiv:2005.13682<\/a><\/li>\n\n\n\n<li>M. O\u2019Dwyer, S. Anselmi, G. D. Starkman,&nbsp;<strong>P.S. Corasaniti<\/strong>, R.K. Sheth, I. Zehavi,&nbsp;\u201c<em>Linear Point and Sound Horizon as Purely Geometric standard rulers<\/em>\u201d, Phys. Rev. D 101, 083517 (2020),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/1910.10698\">arXiv:1910.10698<\/a><\/li>\n\n\n\n<li>J. Adamek, Y. Rasera,&nbsp;<strong>P.S. Corasaniti<\/strong>, J.-M. Alimi,&nbsp;\u201c<em>Ray tracing the ISW effect through the light cones of the DEUS-FUR simulations<\/em>\u201d, Phys. Rev. D 101, 023512 (2020),&nbsp;<a href=\"https:\/\/arxiv.org\/abs\/1910.03340\">arXiv:1910.03340<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, Y. Rasera,&nbsp;\u201c<em>Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples&nbsp;<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 487, 4382 (2019),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1906.02259\">arXiv:1906.02259<\/a><\/li>\n\n\n\n<li>S. Anselmi,&nbsp;<strong>P.S. Corasaniti<\/strong>, A.G. Sanchez, G.D. Starkman, R.K. Sheth, I. Zehavi,&nbsp;\u201c<em>Cosmic distance inference from purely geometric BAO methods: Linear Point standard ruler and Correlation Function Model Fitting<\/em>\u201d, Phys. Rev. D 99, 123515 (2019),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1811.12312\">arXiv:1811.12312<\/a><\/li>\n\n\n\n<li>I. Carucci,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Cosmic Reionization History and Dark Matter Scenarios<\/em>\u201d, Phys. Rev. D 99, 023518 (2019),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1811.07904\">arXiv:1811.07904<\/a><\/li>\n\n\n\n<li>S. Anselmi,&nbsp;<strong>P.S. Corasaniti<\/strong>, G. Starkman, R.K. Sheth, I. Zehavi,&nbsp;\u201c<em>The Linear Point Standard Ruler for galaxy survey data: validation with mock catalogues<\/em>\u201d, Phys. Rev. D 98, 023527 (2018),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1711.09063\">arXiv:1711.09063<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, S. Ettori, Y. Rasera, M. Sereno, S. Amodeo, M.-A. Breton, V. Ghirardini, D. Eckert,&nbsp;\u201c<em>Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements<\/em>\u201d, Astrophys. J. 862, 40 (2018)&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1711.00480\">arXiv:1711.00480<\/a><\/li>\n\n\n\n<li>C. Ma,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Statistical Test of Distance-Duality Relation with Type Ia Supernovae and Baryon Acoustic Oscillations<\/em>\u201d, Astrophys. J. 861, 124 (2018)&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1604.04631\">arXiv:1604.04631<\/a><\/li>\n\n\n\n<li>M. Chira, M. Plionis,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Environmental Dependence of the Abundance Function of Light-Cone Simulation Dark Matter Halos<\/em>\u201d, Astron. &amp; Astrophys. 616, 137 (2018),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1805.06397\">arXiv:1805.06397<\/a><\/li>\n\n\n\n<li>S. Anselmi, G. Starkman,&nbsp;<strong>P.S. Corasaniti<\/strong>, R.K. Sheth, I. Zehavi,&nbsp;\u201c<em>The Linear Point: A cleaner cosmological standard ruler<\/em>\u201d, Phys. Rev. Lett. 121, 021302 (2018)&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1703.01275\">arXiv:1703.01275<\/a><\/li>\n\n\n\n<li>I. Carucci,&nbsp;<strong>P.S. Corasaniti<\/strong>, M. Viel,&nbsp;\u201c<em>Imprints of non-standard Dark Energy and Dark Matter Models on the 21cm Intensity Map Power Spectrum<\/em>\u201d, JCAP 12, 018 (2017),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1706.09462\">arXiv:1706.09462<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, S. Agarwal, D.J.E. Marsh, S. Das,&nbsp;\u201c<em>Constraints on dark matter scenarios from measurements of the galaxy luminosity function at high redshifts<\/em>\u201d, Phys. Rev. D 95, 083512 (2017),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1611.05892\">arXiv:1611.05892<\/a><\/li>\n\n\n\n<li>L. Casarini, S.A. Bonometto, E. Tessarotto,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Extending the Coyote emulator to dark energy models with standard w_0-w_a parametrisation of the equation of state<\/em>\u201d, JCAP 1608, 008 (2016),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1601.07230\">arXiv:1601.07230<\/a><\/li>\n\n\n\n<li>C. Ma,&nbsp;<strong>P.S. Corasaniti<\/strong>, B. Bassett,&nbsp;\u201c<em>Application of Bayesian graphs to SN Ia data analysis and compression<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 463, 1651 (2016),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1603.08519\">arXiv:1603.08519<\/a><\/li>\n\n\n\n<li>L. Blot,&nbsp;<strong>P.S. Corasaniti<\/strong>, L. Amendola, T.D. Kitching,&nbsp;\u201c<em>Non-Linear Matter Power Spectrum Covariance Matrix Errors and Cosmological Parameter Uncertainties<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 458, 4462 (2016),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1512.05383\">arXiv:1512.05383<\/a><\/li>\n\n\n\n<li>M. Pierre et al.,&nbsp;\u201c<em>The XXL Survey: Scientific motivations \u2013 XMM-Newton observing plan \u2013 Follow-up observations and simulation programme<\/em>\u201d, Astron. &amp; Astrophys. 592, 16 (2016),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1512.04317\">arXiv:1512.04317<\/a><\/li>\n\n\n\n<li>S. Agarwal,&nbsp;<strong>P.S. Corasaniti<\/strong>, Y. Rasera, S. Das,&nbsp;\u201c<em>Small scale clustering of late forming dark matter<\/em>\u201d, Phys. Rev. D 92, 063502 (2015),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1412.1103\">arXiv:1412.1103<\/a><\/li>\n\n\n\n<li>S. Agarwal,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Structural properties of artificial halos in non-standard dark matter simulations<\/em>\u201d, Phys. Rev. D 91, 123509 (2015),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1503.03503\">arXiv:1503.03503<\/a><\/li>\n\n\n\n<li>V. Bouillot, J.M. Alimi,&nbsp;<strong>P.S. Corasaniti<\/strong>, Y. Rasera,&nbsp;\u201c<em>Probing dark energy models with extreme pairwise velocities of galaxy clusters from the DEUS-FUR simulations<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 450, 145 (2015),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1405.6679\">arXiv:1405.6679<\/a><\/li>\n\n\n\n<li>L. Blot,&nbsp;<strong>P.S. Corasaniti<\/strong>, J.M. Alimi, Y. Rasera, V. Reverdy,&nbsp;\u201c<em>Matter Power Spectrum Covariance Matrix from the DEUS-PUR \u039bCDM simulations: Mass Resolution and non-Gaussian Errors<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 446, 1756 (2015),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1406.2713\">arXiv:1406.2713<\/a><\/li>\n\n\n\n<li>D. Munshi,&nbsp;<strong>P.S. Corasaniti<\/strong>, P. Coles, A. Heavens, S. Pandolfi,&nbsp;\u201c<em>Reionization &amp; CMB non-Gaussianity<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 442, 3427 (2014),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1403.1531\">arXiv:1403.1531<\/a><\/li>\n\n\n\n<li>Y. Rasera,&nbsp;<strong>P.S. Corasaniti<\/strong>, J.M. Alimi, V. Bouillot, V. Reverdy, I. Balmes,&nbsp;\u201c<em>Cosmic variance limited Baryon Acoustic Oscillations from the DEUS-FUR \u039bCDM simulation<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 440, 1420 (2014),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1311.5662\">arXiv:1311.5662<\/a><\/li>\n\n\n\n<li>I. Balmes, Y. Rasera,&nbsp;<strong>P.S. Corasaniti<\/strong>, J.M. Alimi,&nbsp;\u201c<em>Imprints of Dark Energy on Cosmic Structure Formation: III) Sparsity of Dark Matter Halos<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 437, 2328 (2014),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1307.2922\">arXiv:1307.2922<\/a><\/li>\n\n\n\n<li>I. Achitouv, Y. Rasera, R.K. Sheth,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Testing the self-consistency of the excursion set approach to predicting the dark matter halo mass function<\/em>\u201d, Phys. Rev. Lett. 111, 231303 (2013),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1212.1166\">arXiv:1212.1166<\/a><\/li>\n\n\n\n<li>I. Balmes,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Bayesian approach to gravitational lens model selection: constraining H0 with a selected sample of strong lenses<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 431, 1528 (2013),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1206.5801\">arXiv:1206.5801<\/a><\/li>\n\n\n\n<li>I. Achitouv,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Primordial bispectrum and trispectrum contributions to the non-Gaussian excursion set halo mass function with diffusive drifting barrier<\/em>\u201d, Phys. Rev. D 86, 083011 (2012),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1207.4796\">arXiv:1207.4796<\/a><\/li>\n\n\n\n<li>I. Achitouv,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Non-Gaussian Halo Mass Function and Non-Spherical Halo Collapse: Theory vs. Simulations<\/em>\u201d, JCAP, 02, 002 (2012),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1109.3196\">arXiv:1109.3196<\/a>; Erratum, JCAP 07, E01 (2012)<\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, I. Achitouv,&nbsp;\u201c<em>Excursion set halo mass function and bias in a stochastic barrier model of ellipsoidal collapse<\/em>\u201d, Phys. Rev. D 84, 023009 (2011),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1107.1251\">arXiv:1107.1251<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, I. Achitouv,&nbsp;\u201c<em>Toward a Universal Formulation of the Halo Mass Function<\/em>\u201d, Phys. Rev. Lett. 106, 241302 (2011),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1012.3468\">arXiv:1012.3468<\/a><\/li>\n\n\n\n<li>M. Pierre, F. Pacaud, J.B. Juin, J.B. Melin, P. Valageas, N. Clerc,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Precision cosmology with a wide area XMM cluster survey<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 414, 1732 (2011),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1009.3182\">arXiv:1009.3182<\/a><\/li>\n\n\n\n<li>J. Courtin, Y. Rasera, J.M. Alimi,&nbsp;<strong>P.S. Corasaniti<\/strong>, V. Boucher, A. F\u00fczfa,&nbsp;\u201c<em>Imprints of dark energy on cosmic structure formation \u2013 II. Non-universality of the halo mass function<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 410, 1911 (2011),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/1001.3425\">arXiv:1001.3425<\/a><\/li>\n\n\n\n<li>J.M. Alimi, A. Fuzfa, V. Boucher, Y. Rasera, J. Courtin,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Imprints of Dark Energy on Cosmic Structure Formation: I) Realistic Quintessence Models<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 401, 775 (2010),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/0903.5490\">arXiv:0903.5490<\/a><\/li>\n\n\n\n<li>P.D. Meerburg, J.P. van der Schaar,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Signatures of Initial State Modifications on Bispectrum Statistics<\/em>\u201d, JCAP 0905, 018 (2009),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/0901.4044\">arXiv:0901.4044<\/a><\/li>\n\n\n\n<li>J. Larena, J.-M. Alimi, T. Buchert, M. Kunz,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Testing backreaction effects with observations<\/em>\u201d, Phys. Rev. D 79, 083011 (2009),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/0808.1161\">arXiv:0808.1161<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Slow-roll suppression of adiabatic instabilities in coupled scalar field-dark matter models<\/em>\u201d, Phys. Rev. D 78, 083538 (2008),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/0808.1646\">arXiv:0808.1646<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, A. Melchiorri,&nbsp;\u201c<em>Testing Cosmology with Cosmic Sound Waves<\/em>\u201d, Phys. Rev. D 77, 103507 (2008),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/0711.4119\">arXiv:0711.4119<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, D. Huterer, A. Melchiorri,&nbsp;\u201c<em>Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test<\/em>\u201d, Phys. Rev. D 75, 062001 (2007),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0701433\">astro-ph\/0701433<\/a><\/li>\n\n\n\n<li>P. Zhang,&nbsp;<strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>Cosmic Dust Induced Fluctuations: Bad and Good Aspects<\/em>\u201d, Astrophys. J. 657, 1 (2007),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0607635\">astro-ph\/0607635<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>,&nbsp;\u201c<em>The impact of cosmic dust on supernova cosmology<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 372, 191 (2006),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0603833\">astro-ph\/0603833<\/a><\/li>\n\n\n\n<li>P. Mukherjee, D. Parkinson,&nbsp;<strong>P.S. Corasaniti<\/strong>, A.R. Liddle, M. Kunz,&nbsp;\u201c<em>Model selection as a science driver for dark energy surveys<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 369, 1725 (2006),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0512484\">astro-ph\/0512484<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, M. Loverde, A. Crotts, C. Blake,&nbsp;\u201c<em>Testing dark energy with the advanced liquid-mirror probe of asteroids, cosmology and astrophysics<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 369, 798 (2006),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0511632\">astro-ph\/0511632<\/a><\/li>\n\n\n\n<li>S. Das,&nbsp;<strong>P.S. Corasaniti<\/strong>, J. Khoury,&nbsp;\u201c<em>Super-acceleration as signature of dark sector interaction<\/em>\u201d, Phys. Rev. D 73, 083509 (2006),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0510628\">astro-ph\/0510628<\/a><\/li>\n\n\n\n<li>L. Pogosian,&nbsp;<strong>P.S. Corasaniti<\/strong>. C. Stephan-Otto, R. Crittenden, R. Nichol,&nbsp;\u201c<em>Tracking dark energy with the ISW effect: short and long-term predictions<\/em>\u201d, Phys. Rev. D 72 (2005), 103519,&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0506396\">astro-ph\/0506396<\/a><\/li>\n\n\n\n<li>C. Ungarelli,&nbsp;<strong>P.S. Corasaniti<\/strong>, R.A. Mercer and A. Vecchio,&nbsp;\u201c<em>Gravitational waves, inflation and the cosmic microwave background: towards testing the slow-roll paradigm<\/em>\u201d, Class. Quant. Grav. 22, S964 (2005),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0504294\">astro-ph\/0504294<\/a><\/li>\n\n\n\n<li>A. Cooray,&nbsp;<strong>P.S. Corasaniti<\/strong>, T. Giannantonio and A. Melchiorri,&nbsp;\u201c<em>An indirect limit on the amplitude of primordial gravitational wave background from the CMB-galaxy cross correlation<\/em>\u201d, Phys. Rev. D 72, 023514 (2005),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0504290\">astro-ph\/0504290<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, T. Giannantonio, A. Melchiorri,&nbsp;\u201c<em>Constraining dark energy with cross-correlated CMB and large scale structure data<\/em>\u201d, Phys. Rev. D 71, 123521 (2005),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0504115\">astro-ph\/0504115<\/a><\/li>\n\n\n\n<li>B.A. Bassett,&nbsp;<strong>P.S. Corasaniti<\/strong>, M. Kunz,&nbsp;\u201c<em>The essence of quintessence and the cost of compression<\/em>\u201d, Astrophys. J. 617, L1 (2004),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0407364\">astro-ph\/0407364<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, M. Kunz, D. Parkinson, E.J. Copeland, B.A. Bassett,&nbsp;\u201c<em>The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe<\/em>\u201c, Phys. Rev. D 70, 083006 (2004),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0406608\">astro-ph\/0406608<\/a><\/li>\n\n\n\n<li>N. Bartolo,&nbsp;<strong>P.S. Corasaniti<\/strong>, A. Liddle, M. Malquarti,&nbsp;\u201c<em>Perturbations in cosmologies with a scalar field and a perfect fluid<\/em>\u201d, Phys. Rev. D 70, 043532 (2004),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0311503\">astro-ph\/0311503<\/a><\/li>\n\n\n\n<li>M. Kunz,&nbsp;<strong>P.S. Corasaniti<\/strong>, D. Parkinson, E.J. Copeland, B.A. Bassett,&nbsp;\u201c<em>Model-independent dark energy test with sigma(8) using results from the Wilkinson Microwave Anisotropy Probe<\/em>\u201c, Phys. Rev. D 70, 041301 (2004),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0307346\">astro-ph\/0307346<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, B.A. Bassett, C. Ungarelli, E.J. Copeland,&nbsp;\u201c<em>Model-independent dark energy differentiation with the ISW effect<\/em>\u201c, Phys. Rev. Lett. 90, 091303 (2003),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0210209\">astro-ph\/0210209<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, E.J. Copeland,&nbsp;\u201c<em>A model independent approach to the dark energy equation of state<\/em>\u201d, Phys. Rev. D 67, 063521 (2003),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0205544\">astro-ph\/0205544<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, E.J. Copeland,&nbsp;\u201c<em>Constraining the quintessence equation of state with SNIa data and CMB peaks<\/em>\u201d, Phys. Rev. D 65, 043004 (2002),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0107378\">astro-ph\/0107378<\/a><\/li>\n\n\n\n<li><strong>P.S. Corasaniti<\/strong>, L. Amendola and F. Occhionero,&nbsp;\u201c<em>Present limits to cosmic bubbles from the COBE-DMR three point correlation function<\/em>\u201d, Mont. Not. Roy. Astron. Soc. 323, 677 (2001),&nbsp;<a href=\"http:\/\/arxiv.org\/abs\/astro-ph\/0005575\">astro-ph\/0005575<\/a><\/li>\n<\/ol>\n","protected":false},"excerpt":{"rendered":"<p>List of articles and bibliometrics: ADS \/ SPIRES<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-811","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=\/wp\/v2\/pages\/811","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=811"}],"version-history":[{"count":8,"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=\/wp\/v2\/pages\/811\/revisions"}],"predecessor-version":[{"id":822,"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=\/wp\/v2\/pages\/811\/revisions\/822"}],"wp:attachment":[{"href":"https:\/\/people-lux.obspm.fr\/corasaniti\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=811"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}