arXiv - PHYS - Cosmology and Nongalactic Astrophysics最新文献

{"title":"Mass & Light in Galaxy Clusters: The case of Abell 370","authors":"M. Limousin, A. Niemiec, B. Beauchesne, J. Diego, M. Jauzac, K. Sharon, A. Acebron, D. Lagattuta, G. Mahler, L. Williams, J. Richard, E. Jullo, L. Furtak, A. Faisst, B. Frye, P. Hibon, P. Natarajan, M. Rich","doi":"arxiv-2409.04584","DOIUrl":"https://doi.org/arxiv-2409.04584","url":null,"abstract":"Parametric strong lensing studies of galaxy clusters often display\u0000\"misleading features\". This is the case in the galaxy cluster Abell 370. Using\u0000strong lensing techniques, it has been described parametrically by a four dark\u0000matter clumps model and galaxy scale perturbers, as well as a significant\u0000external shear component, which physical origin remains a challenge. The dark\u0000matter distribution features a mass clump with no stellar counterpart and a\u0000significant offset between one of the dark matter clumps and its associated\u0000stellar counterpart. In this paper, based on BUFFALO data, we begin by\u0000revisiting this mass model. We find a four dark matter clumps solution which\u0000does not require any external shear and provides a slightly better RMS compared\u0000to previous models. Investigating further this new solution, we present a class\u0000of models which can accurately reproduce the strong lensing data, but whose\u0000parameters for the dark matter component are poorly constrained. We then\u0000develop a model where each large scale dark matter component must be associated\u0000with a stellar counterpart. This model is unable to reproduce the observational\u0000constraints with an RMS smaller than 2.3\", and the parameters describing this\u0000dark matter component remain poorly constrained. Examining the total projected\u0000mass maps, we find a good agreement between the total mass and the stellar\u0000distribution, both being bimodal. We interpret the \"misleading features\" of the\u0000four dark matter clumps mass model and the failure of the three dark matter\u0000clumps mass model as being symptomatic of the lack of realism of a parametric\u0000description of the dark matter distribution, and encourage caution and\u0000criticism on the outputs of parametric strong lensing modelling. We briefly\u0000discuss the implications of our results for using Abell 370 as a gravitational\u0000telescope.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"32 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192597","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Abundance of Clustered Primordial Black Holes from Quasar Microlensing","authors":"Sven Heydenreich, Evencio Mediavilla, Jorge Jiménez-Vicente, Héctor Vives-Arias, Jose A. Muñoz","doi":"arxiv-2409.04534","DOIUrl":"https://doi.org/arxiv-2409.04534","url":null,"abstract":"While elementary particles are the favored candidate for the elusive dark\u0000matter, primordial black holes (PBHs) have also been considered to fill that\u0000role. Gravitational microlensing is a very well-suited tool to detect and\u0000measure the abundance of compact objects in galaxies. Previous studies based on\u0000quasar microlensing exclude a significant presence of substellar to\u0000intermediate-mass BHs ($lesssim 100,mathrm{M}_odot$). However, these\u0000studies were based on a spatially uniform distribution of BHs while, according\u0000to current theories of PBHs formation, they are expected to appear in clusters.\u0000We study the impact of clustering in microlensing flux magnification finding\u0000that at large scales clusters act like giant pseudo-particles, strongly\u0000affecting the emission coming from the Broad Line Region, which can no longer\u0000be used to define the zero microlensing baseline. As an alternative, we set\u0000this baseline from the intrinsic magnification ratios of quasar images\u0000predicted by macro lens models and compare them with the observed flux ratios\u0000in emission lines, infrared (IR), and radio. The (magnitude) differences are\u0000the flux-ratio anomalies attributable to microlensing, which we estimate for 35\u0000image pairs corresponding to 12 lens systems. A Bayesian analysis indicates\u0000that the observed anomalies are incompatible with the existence of a\u0000significant population of clustered PBHs. Furthermore, we find that more\u0000compact clusters exhibit a stronger microlensing impact. Consequently, we\u0000conclude that clustering makes the existence of a significant population of BHs\u0000in the substellar to intermediate mass range even more unlikely.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"53 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192593","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Dependence of Galaxy Stellar Properties on the Primordial Spin Factor","authors":"Jun-Sung MoonSeoul National University, Jounghun LeeSeoul National University","doi":"arxiv-2409.04017","DOIUrl":"https://doi.org/arxiv-2409.04017","url":null,"abstract":"We present a numerical discovery that the observable stellar properties of\u0000present galaxies retain significant dependences on the primordial density and\u0000tidal fields. Analyzing the galaxy catalogs from the IllustrisTNG 300-1\u0000simulations, we first compute the primordial spin factor, $tau$, defined as\u0000the mean degree of misalignments between the principal axes of the initial\u0000density and potential hessian tensors at the protogalactic sites. Then, we\u0000explore in the framework of Shannon's information theory if and how strongly\u0000each of six stellar properties of the present galaxies, namely the stellar\u0000sizes, ages, specific star formation rates, optical colors and metallicities,\u0000share mutual information with $tau$, measured at $z=127$. The TNG galaxy\u0000samples are deliberately controlled to have no differences in the mass,\u0000environmental density and shear distributions and to single out net effects of\u0000$tau$ on each of the galaxy stellar properties. In the higher stellar mass\u0000range of $M_{star}/(h^{-1},M_{odot})ge 10^{10}$, significant amounts of\u0000mutual information with $tau$ are exhibited by all of the six stellar\u0000properties, while in the lower range of $M_{star}/(h^{-1},M_{odot})<\u000010^{10}$ only four of the six properties except for the specific star formation\u0000rates and colors yield significant signals of $tau$-dependence. It is also\u0000shown that the galaxy stellar sizes, which turn out to be most robustly\u0000dependent on $tau$ regardless of $M_{star}$, follow a {it bimodal} Gamma\u0000distribution, the physical implication of which is discussed.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"57 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192604","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: II. Anisotropic large-scale coherence in hot gas, galaxies, and dark matter","authors":"M. Lokken, A. van Engelen, M. Aguena, S. S. Allam, D. Anbajagane, D. Bacon, E. Baxter, J. Blazek, S. Bocquet, J. R. Bond, D. Brooks, E. Calabrese, A. Carnero Rosell, J. Carretero, M. Costanzi, L. N. da Costa, W. R. Coulton, J. De Vicente, S. Desai, P. Doel, C. Doux, A. J. Duivenvoorden, J. Dunkley, Z. Huang, S. Everett, I. Ferrero, J. Frieman, J. García-Bellido, M. Gatti, E. Gaztanaga, G. Giannini, V. Gluscevic, D. Gruen, R. A. Gruendl, Y. Guan, G. Gutierrez, S. R. Hinton, R. Hložek, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, O. Lahav, S. Lee, Z. Li, M. Madhavacheril, G. A. Marques, J. L. Marshall, J. Mena-Fernández, F. Menanteau, R. Miquel, J. Myles, M. D. Niemack, S. Pandey, M. E. S. Pereira, A. Pieres, A. A. Plazas Malagón, A. Porredon, M. Rodríguez-Monroy, A. Roodman, S. Samuroff, E. Sanchez, D. Sanchez Cid, B. Santiago, M. Schubnell, I. Sevilla-Noarbe, C. Sifón, M. Smith, S. Staggs, E. Suchyta, M. E. C. Swanson, G. Tarle, C-H. To, N. Weaverdyck, P. Wiseman, E. J. Wollack","doi":"arxiv-2409.04535","DOIUrl":"https://doi.org/arxiv-2409.04535","url":null,"abstract":"Statistics that capture the directional dependence of the baryon distribution\u0000in the cosmic web enable unique tests of cosmology and astrophysical feedback.\u0000We use constrained oriented stacking of thermal Sunyaev-Zel'dovich (tSZ) maps\u0000to measure the anisotropic distribution of hot gas $2.5-40$ Mpc away from\u0000galaxy clusters embedded in massive filaments and superclusters. The cluster\u0000selection and orientation (at a scale of $sim15$ Mpc) use Dark Energy Survey\u0000(DES) Year 3 data, while expanded tSZ maps from the Atacama Cosmology Telescope\u0000Data Release 6 enable a $sim3times$ more significant measurement of the\u0000extended gas compared to the technique's proof-of-concept. Decomposing stacks\u0000into cosine multipoles of order $m$, we detect a dipole ($m=1$) and quadrupole\u0000($m=2$) at $8-10sigma$, as well as evidence for $m=4$ signal at up to\u0000$6sigma$, indicating sensitivity to late-time non-Gaussianity. We compare to\u0000the Cardinal simulations with spherical gas models pasted onto dark matter\u0000halos. The fiducial tSZ data can discriminate between two models that deplete\u0000pressure differently in low-mass halos (mimicking astrophysical feedback),\u0000preferring higher average pressure in extended structures. However, uncertainty\u0000in the amount of cosmic infrared background contamination reduces the\u0000constraining power. Additionally, we apply the technique to DES galaxy density\u0000and weak lensing to study for the first time their oriented relationships with\u0000tSZ. In the tSZ-to-lensing relation, averaged on 7.5 Mpc (transverse) scales,\u0000we observe dependence on redshift but not shape or radial distance. Thus, on\u0000large scales, the superclustering of gas pressure, galaxies, and total matter\u0000is coherent in shape and extent.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"53 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192592","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Diffuse Satellite Population of Local Volume Hosts","authors":"A. Bianca Davis, Christopher T. Garling, Anna M. Nierenberg, Annika H. G. Peter, Amy Sardone, Christopher S. Kochanek, Adam K. Leroy, Kirsten J. Casey, Richard W. Pogge, Daniella M. Roberts, David J. Sand, Johnny P. Greco","doi":"arxiv-2409.03999","DOIUrl":"https://doi.org/arxiv-2409.03999","url":null,"abstract":"We present the results of the Large Binocular Telescope Satellites Of Nearby\u0000Galaxies Survey (LBT-SONG) ``Far Sample,'' including survey completeness\u0000estimates. We find 10 satellite candidates in the inner virial regions of 13\u0000star-forming galaxies outside the Local Group. The hosts are at distances\u0000between $sim 5-11$ Mpc and have stellar masses in the little explored range of\u0000$sim 5 times 10^8 - 5times 10^{10}~text{M}_{odot}$. Among the 10 satellite\u0000candidates, 3 are new discoveries in this survey. In this paper, we\u0000characterize the properties of 8 low-mass satellite candidates, including the 3\u0000new discoveries but excluding 2 well-studied massive satellites. Of the 8\u0000low-mass dwarfs, optical colors from the LBT imaging and measurements in the\u0000ultraviolet with GALEX suggest that 2 show signs of active star formation, and\u00006 are likely quenched (although some may still have Htextsc{i} gas\u0000reservoirs). Notably, we report the discovery of an ultrafaint dwarf candidate,\u0000NGC 672 dwD, with $text{M}_{text{V}} = -6.6$ and an estimated stellar mass of\u0000$5.6 times 10^4 ~text{M}_{odot}$ if its association with the host is\u0000confirmed. It is spatially coincident with a weak detection of Htextsc{i},\u0000with $text{M}_{text{HI}}/text{M}_{text{*}} sim 1$. If confirmed, it would\u0000be the least luminous known ultrafaint satellite to be so gas-rich. The\u0000prevalence of quenched satellites in our sample suggests there are\u0000environmental effects at work in lower mass hosts that are similar to those at\u0000play in Milky Way-size hosts, although the preponderance of Htextsc{i}\u0000detections is at odds with the paucity of Htextsc{i} detections in Milky Way\u0000satellites. By robustly measuring our survey completeness function, we are able\u0000to compare our observational results to predictions from theory, finding good\u0000agreement with the Cold Dark Matter galaxy evolution paradigm.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"75 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192605","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"A Stochastic Approach to Reconstructing the Speed of Light in Cosmology","authors":"Cheng-Yu Zhang, Wei Hong, Yu-Chen Wang, Tong-Jie Zhang","doi":"arxiv-2409.03248","DOIUrl":"https://doi.org/arxiv-2409.03248","url":null,"abstract":"The Varying Speed of Light (VSL) model describes how the speed of light in a\u0000vacuum changes with cosmological redshift. Despite numerous models, there is\u0000little observational evidence for this variation. While the speed of light can\u0000be accurately measured by physical means, cosmological methods are rarely used.\u0000Previous studies quantified the speed of light at specific redshifts using\u0000Gaussian processes and reconstructed the redshift-dependent function $c(z)$. It\u0000is crucial to quantify the speed of light across varying redshifts. We use the\u0000latest data on angular diameter distances $D_A(z)$ and Hubble parameters $H(z)$\u0000from baryon acoustic oscillation (BAO) and cosmic chronometer measurements in\u0000the redshift interval $zin[0.07,1.965]$. The speed of light $c(z)$ is\u0000determined using Gaussian and deep Gaussian processes to reconstruct $H(z)$,\u0000$D_A(z)$, and $D^{prime}_A(z)$. Furthermore, we conduct comparisons across\u0000three distinct models, encompassing two renowned VSL models. We get the result\u0000of the parameters constraints in the models (1) for the ``$c$-c\" model,\u0000$c_0=29492.6 pm^{6.2}_{5.3} mathrm{~km} mathrm{~s}^{-1}$. (2) For the\u0000``$c$-cl\" model, $c_0=29665.5 pm^{11.2}_{11.4}mathrm{~km} mathrm{~s}^{-1}$\u0000and $n=0.05535 pm^{0.00008}_{0.00007}$. (3) For the ``$c$-CPL\" model,\u0000$c_0=29555.7 pm^{13.3}_{13.2} mathrm{~km} mathrm{~s}^{-1}$ and $n=-0.0607\u0000pm 0.0001$. Based on our findings, it may be inferred that Barrow's classical\u0000VSL model is not a suitable fit for our data. In contrast, the widely\u0000recognized Chevallier-Polarski-Linder (CPL) VSL model, under some\u0000circumstances, as well as the universal ``c is constant\" model, demonstrate a\u0000satisfactory ability to account for our findings.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"396 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192610","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Ageing and dynamics of the tailed radio galaxies in Abell 2142","authors":"L. Bruno, T. Venturi, D. Dallacasa, M. Brienza, A. Ignesti, G. Brunetti, C. J. Riseley, M. Rossetti, F. Gastaldello, A. Botteon, L. Rudnick, R. J. van Weeren, A. Shulevski, D. V. Lal","doi":"arxiv-2409.03453","DOIUrl":"https://doi.org/arxiv-2409.03453","url":null,"abstract":"Context. Tailed radio galaxies are shaped by ram pressure owing to the\u0000high-velocity motion of their host through the intracluster medium (ICM).\u0000Recent works have reported on the increasing complexity of the phenomenology of\u0000tailed galaxies, with departures from theoretical ageing models and evidence of\u0000re-energising mechanisms, which are yet unclear. Aims. The nearby (z = 0.0894)\u0000galaxy cluster Abell 2142 hosts two tailed galaxies, namely T1 and T2, which\u0000exhibit peculiar morphological features. We aim to investigate the properties\u0000of T1 and T2 and constrain their spectral evolution, dynamics, and interactions\u0000with the ICM. Methods. We combined LOw Frequency Array (LOFAR), upgraded Giant\u0000Metrewave Radio Telescope (uGMRT), Very Large Array (VLA), and MeerKAT data\u0000(from 30 MHz to 6.5 GHz) to carry out a detailed spectral analysis of T1 and\u0000T2. We analysed surface brightness profiles, measured integrated and\u0000spatially-resolved spectral indices, and performed a comparison with single\u0000injection ageing models. Chandra X-ray data were used to search for\u0000discontinuities in the ICM properties in the direction of the targets. Results.\u0000The spectral properties of T1 at low frequencies are predicted by ageing\u0000models, and provide constraints on the 3D dynamics of the host by assuming a\u0000constant velocity. However, sharp transitions along sub-regions of the tail,\u0000local surface brightness enhancements, and a spectral shape at high frequencies\u0000that is not predicted by models suggest a more complex scenario, possibly\u0000involving hydrodynamical instabilities and particle mixing. T2 exhibits unusual\u0000morphological and surface brightness features, and its spectral behaviour is\u0000not predicted by standard models. Two AGN outburst events during the infall of\u0000T2 towards the cluster centre could explain its properties.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"46 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192615","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $ρ$,Ophiuchi, Perseus and W43","authors":"R. González-González, R. T. Génova-Santos, J. A. Rubiño-Martín, M. W. Peel, F. Guidi, C. H. López-Caraballo, M. Fernández-Torreiro, R. Rebolo, C. Hernández-Monteagudo, D. Adak, E. Artal, M. Ashdown, R. B. Barreiro, F. J. Casas, E. de la Hoz, A. Fasano, D. Herranz, R. J. Hoyland, E. Martínez-González, G. Pascual-Cisneros, L. Piccirillo, F. Poidevin, B. Ruiz-Granados, D. Tramonte, F. Vansyngel, P. Vielva, R. A. Watson","doi":"arxiv-2409.03418","DOIUrl":"https://doi.org/arxiv-2409.03418","url":null,"abstract":"This work focuses on the study of the AME, an important emission mechanism\u0000between 10 and 60 GHz whose polarization properties are not yet fully\u0000understood, and is therefore a potential contaminant for future CMB\u0000polarization observations. We use new QUIJOTE-MFI maps 11, 13, 17 and 19 GHz,\u0000together with other public ancillary data including WMAP and Planck, to study\u0000the polarization properties of the AME in three Galactic regions: rho-Ophiuchi,\u0000Perseus and W43. We have obtained the SEDs for those three regions over the frequency range\u00000.4-3000 GHz, both in intensity and polarization. The intensity SEDs are well\u0000described by a combination of free-free emission, thermal dust, AME and CMB\u0000anisotropies. In polarization, we extracted the flux densities using all\u0000available data between 11 and 353 GHz. We implemented an improved\u0000intensity-to-polarization leakage correction that has allowed for the first\u0000time to derive reliable polarization constraints well below the 1% level from\u0000Planck-LFI data. A frequency stacking of maps in the range 10-60 GHz has\u0000allowed us to reduce the statistical noise and to push the upper limits on the\u0000AME polarization level. We have obtained upper limits on the AME polarization fraction of order <1%\u0000(95% confidence level) for the three regions. In particular we get Pi_AME <\u00001.1% (at 28.4 GHz), Pi_AME < 1.1% (at 22.8 GHz) and Pi_AME < 0.28% (at 33 GHz)\u0000in rho-Ophiuchi, Perseus and W43 respectively. At the QUIJOTE 17 GHz frequency\u0000band, we get Pi_AME< 5.1% for rho-Ophiuchi, Pi_AME< 3.5% for Perseus and\u0000Pi_AME< 0.85% for W43. Our final upper limits derived using the stacking\u0000procedure are Pi_AME < 0.58% for rho-Ophiuchi, Pi_AME < 1.64% for Perseus and\u0000Pi_AME < 0.31% for W43. Altogether, these are the most stringent constraints to\u0000date on the AME polarization fraction of these three star-forming regions.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"24 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192609","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Map-level baryonification: Efficient modelling of higher-order correlations in the weak lensing and thermal Sunyaev-Zeldovich fields","authors":"Dhayaa Anbajagane, Shivam Pandey, Chihway Chang","doi":"arxiv-2409.03822","DOIUrl":"https://doi.org/arxiv-2409.03822","url":null,"abstract":"Semi-analytic methods can generate baryon-corrected fields from N-body\u0000simulations (``baryonification'') and are rapidly becoming a ubiquitous tool in\u0000modeling structure formation on non-linear scales. We extend this formalism to\u0000consistently model the weak lensing and thermal Sunyaev-Zeldovich (tSZ) fields\u0000directly on the full-sky, with an emphasis on higher-order correlations. We use\u0000the auto- and cross- $N$th-order moments, with $N in {2, 3, 4}$, as a\u0000summary statistic of the lensing and tSZ fields, and show that our model can\u0000jointly fit these statistics measured in IllustrisTNG to within measurement\u0000uncertainties, for scales above $gtrsim 1 {rm Mpc}$ and across multiple\u0000redshifts. The model predictions change only minimally when including\u0000additional information from secondary halo properties, such as halo\u0000concentration and ellipticity. Each individual moment is dependent on halos of\u0000different mass ranges and has different sensitivities to the model parameters.\u0000A simulation-based forecast on the ULAGAM simulation suite shows that the\u0000combination of all moments, measured from current and upcoming lensing and tSZ\u0000surveys, can jointly constrain cosmology and baryons to high precision. The\u0000lensing and tSZ field are sensitive to different combinations of the\u0000baryonification parameters, with degeneracy directions that are often\u0000orthogonal, and the combination of the two fields leads to significantly better\u0000constraints on both cosmology and astrophysics. Our pipeline for map-level\u0000baryonification is publicly available at\u0000https://github.com/DhayaaAnbajagane/Baryonification.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"2 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192601","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Euclid preparation. Simulations and nonlinearities beyond $Λ$CDM. 2. Results from non-standard simulations","authors":"Euclid Collaboration, G. RáczJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USADepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, M. -A. BretonInstitute of Space SciencesInstitut de Ciencies de l'EspaiLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, B. FioriniInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UKSchool of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UK, A. M. C. Le BrunLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, FranceInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, H. -A. WintherInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, Z. SakrInstitut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, GermanyInstitut de Recherche en Astrophysique et PlanétologieUniversité St Joseph, Faculty of Sciences, Beirut, Lebanon, L. PizzutiDipartimento di Fisica \"G. Occhialini\", Università degli Studi di Milano Bicocca, Piazza della Scienza 3, 20126 Milano, Italy, A. RagagninINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, T. GayouxLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, E. AltamuraJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, E. CarellaINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, ItalyDipartimento di Fisica \"Aldo Pontremoli\", Università degli Studi di Milano, Via Celoria 16, 20133 Milano, Italy, K. PardedeINFN Gruppo Collegato di Parma, Viale delle Scienze 7/A 43124 Parma, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyInternational Centre for Theoretical PhysicsIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, G. VerzaCenter for Cosmology and Particle Physics, Department of Physics, New York University, New York, NY 10003, USACenter for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, 10010, New York, NY, USA, K. KoyamaInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, M. BaldiDipartimento di Fisica e Astronomia, Università di Bologna, Via Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, A. PourtsidouInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UKHiggs Centre for Theoretical Physics, School of Physics and Astronomy, The University of Edinburgh, Edinburgh EH9 3FD, UK, F. VernizziInstitut de Physique Théorique, CEA, CNRS, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France, A. G. AdameDepartamento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, SpainInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, SpainCentro de Investigación Avanzada en Física Fundamental, J. AdamekDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, S. AvilaInstitut de Física d'Altes Energies, C. CarboneINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, G. DespaliDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, C. GiocoliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Bologna, Via Irnerio 46, 40126 Bologna, Italy, C. Hernández-AguayoMax-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str.~1, 85748 Garching, Germany, F. HassaniInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, M. KunzUniversité de Genève, Département de Physique Théorique and Centre for Astroparticle Physics, 24 quai Ernest-Ansermet, CH-1211 Genève 4, Switzerland, B. LiDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, DH1 3LE, UK, Y. RaseraLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, FranceInstitut universitaire de France, G. YepesDepartamento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, SpainCentro de Investigación Avanzada en Física Fundamental, V. Gonzalez-PerezDepartamento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid, 28049 Cantoblanco, Madrid, Spain, P. -S. CorasanitiLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, J. García-BellidoInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, Spain, N. HamausUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyExcellence Cluster ORIGINS, Boltzmannstrasse 2, 85748 Garching, Germany, A. KiesslingJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, M. MarinucciDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, C. MorettiSISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, D. F. MotaInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, L. PigaDipartimento di Scienze Matematiche, Fisiche e Informatiche, Università di Parma, Viale delle Scienze 7/A 43124 Parma, ItalyINFN Gruppo Collegato di Parma, Viale delle Scienze 7/A 43124 Parma, ItalyINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, A. PisaniAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, FranceDepartment of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USACenter for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, 10010, New York, NY, USAThe Cooper Union for the Advancement of Science and Art, 41 Cooper Square, New York, NY 10003, USA, I. SzapudiInstitute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA, P. Tallada-CrespíCentro de Investigaciones Energéticas, Medioambientales y TecnológicasPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, N. AghanimUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, S. AndreonINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, C. BaccigalupiIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, Italy, S. BardelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, D. BoninoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, E. BranchiniDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINAF-Osservatorio Astronomico di Brera, Via Brera 28, 20122 Milano, Italy, M. BresciaDepartment of Physics \"E. Pancini\", University Federico II, Via Cinthia 6, 80126, Napoli, ItalyINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, J. BrinchmannInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, PortugalFaculdade de Ciências da Universidade do Porto, Rua do Campo de Alegre, 4150-007 Porto, Portugal, S. CameraDipartimento di Fisica, Università degli Studi di Torino, Via P. Giuria 1, 10125 Torino, ItalyINFN-Sezione di Torino, Via P. Giuria 1, 10125 Torino, ItalyINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, V. CapobiancoINAF-Osservatorio Astrofisico di Torino, Via Osservatorio 20, 10025 Pino Torinese, V. F. CardoneINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, ItalyINFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy, J. CarreteroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 Bellaterra, S. CasasInstitute for Theoretical Particle Physics and Cosmology, M. CastellanoINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, G. CastignaniINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. CavuotiINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, ItalyINFN section of Naples, Via Cinthia 6, 80126, Napoli, Italy, A. CimattiDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, C. Colodro-CondeInstituto de Astrofísica de Canarias, Calle Vía Láctea s/n, 38204, San Cristóbal de La Laguna, Tenerife, Spain, G. CongedoInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, C. J. ConseliceJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, L. ConversiEuropean Space Agency/ESRIN, Largo Galileo Galilei 1, 00044 Frascati, Roma, ItalyESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, Y. CopinUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, F. CourbinInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne, H. M. CourtoisUCB Lyon 1, CNRS/IN2P3, IUF, IP2I Lyon, 4 rue Enrico Fermi, 69622 Villeurbanne, France, A. Da SilvaDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Campo Grande, 1749-016 Lisboa, Portugal, H. DegaudenziDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, G. De LuciaINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. DouspisUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, F. DubathDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. A. J. DuncanJodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK, X. DupacESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, S. DusiniINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, A. EaletUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, M. FarinaINAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy, S. FarrensUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, S. FerriolUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, P. FosalbaInstitut d'Estudis Espacials de CatalunyaInstitut de Ciencies de l'Espai, M. FrailisINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, E. FranceschiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. FumanaINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, S. GaleottaINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, B. GillisInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, P. Gómez-AlvarezFRACTAL S.L.N.E., calle Tulipán 2, Portal 13 1A, 28231, Las Rozas de Madrid, SpainESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, Spain, A. GrazianINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, Italy, F. GruppMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, GermanyUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, Germany, S. V. H. HauganInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, W. HolmesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, F. HormuthFelix Hormuth Engineering, Goethestr. 17, 69181 Leimen, Germany, A. HornstrupTechnical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, DenmarkCosmic Dawn Center, S. IlićUniversité Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, FranceInstitut de Recherche en Astrophysique et Planétologie, K. JahnkeMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, M. JhabvalaNASA Goddard Space Flight Center, Greenbelt, MD 20771, USA, B. JoachimiDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK, E. KeihänenDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland, S. KermicheAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, M. KilbingerUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, T. KitchingMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK, B. KubikUniversité Claude Bernard Lyon 1, CNRS/IN2P3, IP2I Lyon, UMR 5822, Villeurbanne, F-69100, France, H. Kurki-SuonioDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, P. B. LiljeInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, V. LindholmDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, I. LloroNOVA optical infrared instrumentation group at ASTRON, Oude Hoogeveensedijk 4, 7991PD, Dwingeloo, The Netherlands, G. MainettiCentre de Calcul de l'IN2P3/CNRS, 21 avenue Pierre de Coubertin 69627 Villeurbanne Cedex, France, E. MaioranoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, O. MansuttiINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, O. MarggrafUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, K. MarkovicJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, M. MartinelliINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, ItalyINFN-Sezione di Roma, Piazzale Aldo Moro, 2 - c/o Dipartimento di Fisica, Edificio G. Marconi, 00185 Roma, Italy, N. MartinetAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, F. MarulliDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, R. MasseyDepartment of Physics, Institute for Computational Cosmology, Durham University, South Road, DH1 3LE, UK, E. MedinaceliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. MeiUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, Y. MellierInstitut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, FranceInstitut d'Astrophysique de Paris, UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, M. MeneghettiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, G. MeylanInstitute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fédérale de Lausanne, M. MorescoDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, L. MoscardiniDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, S. -M. NiemiEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, C. PadillaInstitut de Física d'Altes Energies, S. PaltaniDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, F. PasianINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, K. PedersenDepartment of Physics and Astronomy, University of Aarhus, Ny Munkegade 120, DK-8000 Aarhus C, Denmark, W. J. PercivalWaterloo Centre for Astrophysics, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaPerimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada, V. PettorinoEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, S. PiresUniversité Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France, G. PolentaSpace Science Data Center, Italian Space Agency, via del Politecnico snc, 00133 Roma, Italy, M. PoncetCentre National d'Etudes Spatiales -- Centre spatial de Toulouse, 18 avenue Edouard Belin, 31401 Toulouse Cedex 9, France, L. A. PopaInstitute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania, F. RaisonMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, R. ReboloInstituto de Astrofísica de Canarias, Calle Vía Láctea s/n, 38204, San Cristóbal de La Laguna, Tenerife, SpainDepartamento de Astrofísica, Universidad de La Laguna, 38206, La Laguna, Tenerife, Spain, A. RenziDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, J. RhodesJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA, G. RiccioINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, E. RomelliINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. RoncarelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, R. SagliaUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, J. -C. SalvignolEuropean Space Agency/ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands, A. G. SánchezMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, D. SaponeDepartamento de Física, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile, B. SartorisUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. SchirmerMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, T. SchrabbackUniversität Innsbruck, Institut für Astro- und Teilchenphysik, Technikerstr. 25/8, 6020 Innsbruck, Austria, A. SecrounAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, G. SeidelMax-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany, S. SerranoInstitut d'Estudis Espacials de CatalunyaSatlantis, University Science Park, Sede Bld 48940, Leioa-Bilbao, SpainInstitute of Space Sciences, C. SirignanoDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, G. SirriINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, L. StancoINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, J. SteinwagnerMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, A. N. TaylorInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, I. TerenoDepartamento de Física, Faculdade de Ciências, Universidade de Lisboa, Edifício C8, Campo Grande, PT1749-016 Lisboa, PortugalInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal, R. Toledo-MoreoUniversidad Politécnica de Cartagena, Departamento de Electrónica y Tecnología de Computadoras, Plaza del Hospital 1, 30202 Cartagena, Spain, F. TorradeflotPort d'Informació Científica, Campus UAB, C. Albareda s/n, 08193 BellaterraCentro de Investigaciones Energéticas, Medioambientales y Tecnológicas, I. TutusausInstitut de Recherche en Astrophysique et Planétologie, L. ValenzianoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, T. VassalloUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, G. Verdoes KleijnKapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands, Y. WangInfrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA, J. WellerUniversitäts-Sternwarte München, Fakultät für Physik, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 München, GermanyMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, E. ZuccaINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, A. BivianoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, A. BoucaudUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, E. BozzoDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. BuriganaINAF, Istituto di Radioastronomia, Via Piero Gobetti 101, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, M. CalabreseAstronomical Observatory of the Autonomous Region of the Aosta ValleyINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, D. Di FerdinandoINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, J. A. Escartin VigoMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, G. FabbianInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UKSchool of Physics and Astronomy, Cardiff University, The Parade, Cardiff, CF24 3AA, UKCenter for Computational Astrophysics, Flatiron Institute, 162 5th Avenue, 10010, New York, NY, USA, F. FinelliINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, J. Gracia-CarpioMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, S. MatthewInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, N. MauriDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, A. PezzottaMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, M. PöntinenDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, C. PorcianiUniversität Bonn, Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany, V. ScottezInstitut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, FranceJunia, EPA department, 41 Bd Vauban, 59800 Lille, France, M. TentiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, M. VielIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalySISSA, International School for Advanced Studies, Via Bonomea 265, 34136 Trieste TS, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, M. WiesmannInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, Y. AkramiInstituto de Física Teórica UAM-CSIC, Campus de Cantoblanco, 28049 Madrid, SpainCERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, OH 44106, USA, V. AllevatoINAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, 80131 Napoli, Italy, S. AnselmiINFN-Padova, Via Marzolo 8, 35131 Padova, ItalyDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, M. ArchidiaconoDipartimento di Fisica \"Aldo Pontremoli\", Università degli Studi di Milano, Via Celoria 16, 20133 Milano, ItalyINFN-Sezione di Milano, Via Celoria 16, 20133 Milano, Italy, F. Atrio-BarandelaDepartamento de Física Fundamental. Universidad de Salamanca. Plaza de la Merced s/n. 37008 Salamanca, Spain, A. Balaguera-AntolinezInstituto de Astrofísica de Canarias, Calle Vía Láctea s/n, 38204, San Cristóbal de La Laguna, Tenerife, SpainDepartamento de Astrofísica, Universidad de La Laguna, 38206, La Laguna, Tenerife, Spain, M. BallardiniDipartimento di Fisica e Scienze della Terra, Università degli Studi di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyIstituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Via Giuseppe Saragat 1, 44122 Ferrara, Italy, D. BertaccaDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINAF-Osservatorio Astronomico di Padova, Via dell'Osservatorio 5, 35122 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, L. BlotKavli Institute for the Physics and Mathematics of the UniverseLaboratoire Univers et Théorie, Observatoire de Paris, Université PSL, Université Paris Cité, CNRS, 92190 Meudon, France, S. BorganiDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, Italy, S. BrutonMinnesota Institute for Astrophysics, University of Minnesota, 116 Church St SE, Minneapolis, MN 55455, USA, R. CabanacInstitut de Recherche en Astrophysique et Planétologie, A. CalabroINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, B. Camacho QuevedoInstitut d'Estudis Espacials de CatalunyaInstitute of Space Sciences, A. CappiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Bd de l'Observatoire, CS 34229, 06304 Nice cedex 4, France, F. CaroINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, C. S. CarvalhoInstituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências, Universidade de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal, T. CastroINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, ItalyICSC - Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, Via Magnanelli 2, Bologna, Italy, K. C. ChambersInstitute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA, S. ContariniMax Planck Institute for Extraterrestrial Physics, Giessenbachstr. 1, 85748 Garching, Germany, A. R. CoorayDepartment of Physics & Astronomy, University of California Irvine, Irvine CA 92697, USA, B. De CaroINAF-IASF Milano, Via Alfonso Corti 12, 20133 Milano, Italy, S. de la TorreAix-Marseille Université, CNRS, CNES, LAM, Marseille, France, G. DesprezDepartment of Astronomy & Physics and Institute for Computational Astrophysics, Saint Mary's University, 923 Robie Street, Halifax, Nova Scotia, B3H 3C3, Canada, A. Díaz-SánchezDepartamento Física Aplicada, Universidad Politécnica de Cartagena, Campus Muralla del Mar, 30202 Cartagena, Murcia, Spain, J. J. DiazInstituto de Astrofísica de Canarias, S. Di DomizioDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, H. DoleUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, S. EscoffierAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, A. G. FerrariDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, P. G. FerreiraDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, I. FerreroInstitute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, 0315 Oslo, Norway, A. FontanaINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, F. FornariINFN-Bologna, Via Irnerio 46, 40126 Bologna, Italy, L. GabarraDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, K. GangaUniversité Paris Cité, CNRS, Astroparticule et Cosmologie, 75013 Paris, France, T. GasparettoINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, E. GaztanagaInstitute of Space SciencesInstitut d'Estudis Espacials de CatalunyaInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, F. GiacominiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, F. GianottiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, G. GozaliaslDepartment of Computer Science, Aalto University, PO Box 15400, Espoo, FI-00 076, FinlandDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, Finland, C. M. GutierrezInstituto de Astrofí sica de Canarias, c/ Via Lactea s/n, La Laguna E-38200, Spain. Departamento de Astrofí sica de la Universidad de La Laguna, Avda. Francisco Sanchez, La Laguna, E-38200, Spain, A. HallInstitute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, H. HildebrandtRuhr University Bochum, Faculty of Physics and Astronomy, Astronomical Institute, J. HjorthDARK, Niels Bohr Institute, University of Copenhagen, Jagtvej 155, 2200 Copenhagen, Denmark, A. Jimenez MuñozUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France, J. J. E. KajavaDepartment of Physics and Astronomy, Vesilinnantie 5, 20014 University of Turku, FinlandSerco for European Space Agency, V. KansalARC Centre of Excellence for Dark Matter Particle Physics, Melbourne, AustraliaCentre for Astrophysics & Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122, Australia, D. KaragiannisSchool of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UKDepartment of Physics and Astronomy, University of the Western Cape, Bellville, Cape Town, 7535, South Africa, C. C. KirkpatrickDepartment of Physics and Helsinki Institute of Physics, Gustaf Hällströmin katu 2, 00014 University of Helsinki, Finland, F. LacasaUniversité Libre de BruxellesUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, J. Le GraetAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, L. LegrandICTP South American Institute for Fundamental Research, Instituto de Física Teórica, Universidade Estadual Paulista, São Paulo, Brazil, J. LesgourguesInstitute for Theoretical Particle Physics and Cosmology, T. I. LiaudatIRFU, CEA, Université Paris-Saclay 91191 Gif-sur-Yvette Cedex, France, A. LoureiroOskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, Stockholm, SE-106 91, SwedenAstrophysics Group, Blackett Laboratory, Imperial College London, London SW7 2AZ, UK, J. Macias-PerezUniv. Grenoble Alpes, CNRS, Grenoble INP, LPSC-IN2P3, 53, Avenue des Martyrs, 38000, Grenoble, France, G. MaggioINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, Italy, M. MagliocchettiINAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere, 100, 00100 Roma, Italy, F. MannucciINAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy, R. MaoliDipartimento di Fisica, Sapienza Università di Roma, Piazzale Aldo Moro 2, 00185 Roma, ItalyINAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00078 Monteporzio Catone, Italy, C. J. A. P. MartinsCentro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, PortugalInstituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal, L. MaurinUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, R. B. MetcalfDipartimento di Fisica e Astronomia \"Augusto Righi\" - Alma Mater Studiorum Università di Bologna, via Piero Gobetti 93/2, 40129 Bologna, ItalyINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, M. MiluzioESAC/ESA, Camino Bajo del Castillo, s/n., Urb. Villafranca del Castillo, 28692 Villanueva de la Cañada, Madrid, SpainHE Space for European Space Agency, P. MonacoDipartimento di Fisica - Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, 34131 Trieste, ItalyINAF-Osservatorio Astronomico di Trieste, Via G. B. Tiepolo 11, 34143 Trieste, ItalyINFN, Sezione di Trieste, Via Valerio 2, 34127 Trieste TS, ItalyIFPU, Institute for Fundamental Physics of the Universe, via Beirut 2, 34151 Trieste, Italy, A. MontoroInstitute of Space SciencesInstitut d'Estudis Espacials de Catalunya, A. MoraAurora Technology for European Space Agency, G. MorganteINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, S. NadathurInstitute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK, Nicholas A. WaltonInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, L. PatriziiINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, V. PopaInstitute of Space Science, Str. Atomistilor, nr. 409 Măgurele, Ilfov, 077125, Romania, D. PotterDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, P. ReimbergInstitut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014, Paris, France, I. RissoDipartimento di Fisica, Università degli studi di Genova, and INFN-Sezione di Genova, via Dodecaneso 33, 16146, Genova, Italy, P. -F. RocciUniversité Paris-Saclay, CNRS, Institut d'astrophysique spatiale, 91405, Orsay, France, M. SahlénTheoretical astrophysics, Department of Physics and Astronomy, Uppsala University, Box 515, 751 20 Uppsala, Sweden, A. SchneiderDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, M. SerenoINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, ItalyINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, A. SilvestriInstitute Lorentz, Leiden University, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands, A. Spurio ManciniDepartment of Physics, Royal Holloway, University of London, TW20 0EX, UKMullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK, J. StadelDepartment of Astrophysics, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland, K. TanidisDepartment of Physics, Oxford University, Keble Road, Oxford OX1 3RH, UK, C. TaoAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France, N. TessoreDepartment of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK, G. TesteraINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, R. TeyssierDepartment of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ 08544, USA, S. ToftCosmic Dawn CenterCosmic Dawn CenterNiels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200 Copenhagen, Denmark, S. TosiDipartimento di Fisica, Università di Genova, Via Dodecaneso 33, 16146, Genova, ItalyINFN-Sezione di Genova, Via Dodecaneso 33, 16146, Genova, Italy, A. TrojaDipartimento di Fisica e Astronomia \"G. Galilei\", Università di Padova, Via Marzolo 8, 35131 Padova, ItalyINFN-Padova, Via Marzolo 8, 35131 Padova, Italy, M. TucciDepartment of Astronomy, University of Geneva, ch. d'Ecogia 16, 1290 Versoix, Switzerland, C. ValieriINFN-Sezione di Bologna, Viale Berti Pichat 6/2, 40127 Bologna, Italy, J. ValiviitaDepartment of Physics, P.O. Box 64, 00014 University of Helsinki, FinlandHelsinki Institute of Physics, Gustaf Hällströmin katu 2, University of Helsinki, Helsinki, Finland, D. VerganiINAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Via Piero Gobetti 93/3, 40129 Bologna, Italy, P. VielzeufAix-Marseille Université, CNRS/IN2P3, CPPM, Marseille, France","doi":"arxiv-2409.03523","DOIUrl":"https://doi.org/arxiv-2409.03523","url":null,"abstract":"The Euclid mission will measure cosmological parameters with unprecedented\u0000precision. To distinguish between cosmological models, it is essential to\u0000generate realistic mock observables from cosmological simulations that were run\u0000in both the standard $Lambda$-cold-dark-matter ($Lambda$CDM) paradigm and in\u0000many non-standard models beyond $Lambda$CDM. We present the scientific results\u0000from a suite of cosmological N-body simulations using non-standard models\u0000including dynamical dark energy, k-essence, interacting dark energy, modified\u0000gravity, massive neutrinos, and primordial non-Gaussianities. We investigate\u0000how these models affect the large-scale-structure formation and evolution in\u0000addition to providing synthetic observables that can be used to test and\u0000constrain these models with Euclid data. We developed a custom pipeline based\u0000on the Rockstar halo finder and the nbodykit large-scale structure toolkit to\u0000analyse the particle output of non-standard simulations and generate mock\u0000observables such as halo and void catalogues, mass density fields, and power\u0000spectra in a consistent way. We compare these observables with those from the\u0000standard $Lambda$CDM model and quantify the deviations. We find that\u0000non-standard cosmological models can leave significant imprints on the\u0000synthetic observables that we have generated. Our results demonstrate that\u0000non-standard cosmological N-body simulations provide valuable insights into the\u0000physics of dark energy and dark matter, which is essential to maximising the\u0000scientific return of Euclid.","PeriodicalId":501207,"journal":{"name":"arXiv - PHYS - Cosmology and Nongalactic Astrophysics","volume":"74 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142192607","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}