Author: "Trac, H." - Searchworks@Jio Institute Digital Library Search Results

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49 results on '"Trac, H."'

1. The Atacama Cosmology Telescope: A Catalog of > 4000 Sunyaev-Zel'dovich Galaxy Clusters

Author: Hilton, M., Sifón, C., Naess, S., Madhavacheril, M., Oguri, M., Rozo, E., Rykoff, E., Abbott, T. M. C., Adhikari, S., Aguena, M., Aiola, S., Allam, S., Amodeo, S., Amon, A., Annis, J., Ansarinejad, B., Aros-Bunster, C., Austermann, J. E., Avila, S., Bacon, D., Battaglia, N., Beall, J. A., Becker, D. T., Bernstein, G. M., Bertin, E., Bhandarkar, T., Bhargava, S., Bond, J. R., Brooks, D., Burke, D. L., Calabrese, E., Carretero, J., Choi, S. K., Choi, A., Conselice, C., da Costa, L. N., Costanzi, M., Crichton, D., Crowley, K. T., Dünner, R., Denison, E. V., Devlin, M. J., Dicker, S. R., Diehl, H. T., Dietrich, J. P., Doel, P., Duff, S. M., Duivenvoorden, A. J., Dunkley, J., Everett, S., Ferraro, S., Ferrero, I., Ferté, A., Flaugher, B., Frieman, J., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giles, P., Golec, J. E., Gralla, M. B., Grandis, S., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Han, D., Hartley, W. G., Hasselfield, M., Hill, J. C., Hilton, G. C., Hincks, A. D., Hinton, S. R., Ho, S-P. P., Honscheid, K., Hoyle, B., Hubmayr, J., Huffenberger, K. M., Hughes, J. P., Jaelani, A. T., Jain, B., James, D. J., Jeltema, T., Kent, S., Kind, M. Carrasco, Knowles, K., Koopman, B. J., Kuehn, K., Lahav, O., Lima, M., Lin, Y-T., Lokken, M., Loubser, S. I., MacCrann, N., Maia, M. A. G., Marriage, T. A., Martin, J., McMahon, J., Melchior, P., Menanteau, F., Miquel, R., Miyatake, H., Moodley, K., Morgan, R., Mroczkowski, T., Nati, F., Newburgh, L. B., Niemack, M. D., Nishizawa, A. J., Ogando, R. L. C., Orlowski-Scherer, J., Page, L. A., Palmese, A., Partridge, B., Paz-Chinchón, F., Phakathi, P., Plazas, A. A., Robertson, N. C., Romer, A. K., Rosell, A. Carnero, Salatino, M., Sanchez, E., Schaan, E., Schillaci, A., Sehgal, N., Serrano, S., Shin, T., Simon, S. M., Smith, M., Soares-Santos, M., Spergel, D. N., Staggs, S. T., Storer, E. R., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Trac, H., Ullom, J. N., Vale, L. R., Van Lanen, J., Vavagiakis, E. M., De Vicente, J., Wilkinson, R. D., Wollack, E. J., Xu, Z., and Zhang, Y.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a catalog of 4195 optically confirmed Sunyaev-Zel'dovich (SZ) selected galaxy clusters detected with signal-to-noise > 4 in 13,211 deg$^2$ of sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were selected by applying a multi-frequency matched filter to 98 and 150 GHz maps constructed from ACT observations obtained from 2008-2018, and confirmed using deep, wide-area optical surveys. The clusters span the redshift range 0.04 < z < 1.91 (median z = 0.52). The catalog contains 222 z > 1 clusters, and a total of 868 systems are new discoveries. Assuming an SZ-signal vs. mass scaling relation calibrated from X-ray observations, the sample has a 90% completeness mass limit of M500c > 3.8 x 10$^{14}$ MSun, evaluated at z = 0.5, for clusters detected at signal-to-noise ratio > 5 in maps filtered at an angular scale of 2.4'. The survey has a large overlap with deep optical weak-lensing surveys that are being used to calibrate the SZ-signal mass-scaling relation, such as the Dark Energy Survey (4566 deg$^2$), the Hyper Suprime-Cam Subaru Strategic Program (469 deg$^2$), and the Kilo Degree Survey (825 deg$^2$). We highlight some noteworthy objects in the sample, including potentially projected systems; clusters with strong lensing features; clusters with active central galaxies or star formation; and systems of multiple clusters that may be physically associated. The cluster catalog will be a useful resource for future cosmological analyses, and studying the evolution of the intracluster medium and galaxies in massive clusters over the past 10 Gyr., Comment: 35 pages, 27 figures, accepted for publication in ApJS; v1.0 catalogs will be available from LAMBDA https://lambda.gsfc.nasa.gov/product/act/actpol_prod_table.cfm; v1.0 catalogs available from https://astro.ukzn.ac.za/~mjh/ACTDR5/v1.0/ until then
Published: 2020
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2. Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos

Author: Schaan, E, Ferraro, S, Amodeo, S, Battaglia, N, Aiola, S, Austermann, JE, Beall, JA, Bean, R, Becker, DT, Bond, RJ, Calabrese, E, Calafut, V, Choi, SK, Denison, EV, Devlin, MJ, Duff, SM, Duivenvoorden, AJ, Dunkley, J, Dünner, R, Gallardo, PA, Guan, Y, Han, D, Hill, JC, Hilton, GC, Hilton, M, HloŽek, R, Hubmayr, J, Huffenberger, KM, Hughes, JP, Koopman, BJ, Macinnis, A, McMahon, J, Madhavacheril, MS, Moodley, K, Mroczkowski, T, Naess, S, Nati, F, Newburgh, LB, Niemack, MD, Page, LA, Partridge, B, Salatino, M, Sehgal, N, Schillaci, A, Sifón, C, Smith, KM, Spergel, DN, Staggs, S, Storer, ER, Trac, H, Ullom, JN, Van Lanen, J, Vale, LR, Van Engelen, A, Magaña, MV, Vavagiakis, EM, Wollack, EJ, and Xu, Z
Subjects: astro-ph.CO, astro-ph.GA
Abstract: The scattering of cosmic microwave background (CMB) photons off the free-electron gas in galaxies and clusters leaves detectable imprints on high resolution CMB maps: the thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ respectively). We use combined microwave maps from the Atacama Cosmology Telescope DR5 and Planck in combination with the CMASS (mean redshift ⟨z
Published: 2021

3. The Velocity Distribution Function of Galaxy Clusters as a Cosmological Probe

Author: Ntampaka, M., Trac, H., Cisewski, J., and Price, L. C.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a new approach for quantifying the abundance of galaxy clusters and constraining cosmological parameters using dynamical measurements. In the standard method, galaxy line-of-sight (LOS) velocities, $v$, or velocity dispersions are used to infer cluster masses, $M$, in order to quantify the halo mass function (HMF), $dn(M)/d\log(M)$, which is strongly affected by mass measurement errors. In our new method, the probability distribution of velocities for each cluster in the sample are summed to create a new statistic called the velocity distribution function (VDF), $dn(v)/dv$. The VDF can be measured more directly and precisely than the HMF and it can also be robustly predicted with cosmological simulations which capture the dynamics of subhalos or galaxies. We apply these two methods to mock cluster catalogs and forecast the bias and constraints on the matter density parameter $\Omega_m$ and the amplitude of matter fluctuations $\sigma_8$ in flat $\Lambda$CDM cosmologies. For an example observation of 200 massive clusters, the VDF with (without) velocity errors constrains the parameter combination $\sigma_8\Omega_m^{0.29\ (0.29)} = 0.587 \pm 0.011\ (0.583 \pm 0.011)$ and shows only minor bias. However, the HMF with dynamical mass errors is biased to low $\Omega_m$ and high $\sigma_8$ and the fiducial model lies well outside of the forecast constraints, prior to accounting for Eddington bias. When the VDF is combined with constraints from the cosmic microwave background (CMB), the degeneracy between cosmological parameters can be significantly reduced. Upcoming spectroscopic surveys that probe larger volumes and fainter magnitudes will provide a larger number of clusters for applying the VDF as a cosmological probe., Comment: 10 pages, 4 figures, accepted for publication at ApJ
Published: 2016
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4. The Atacama Cosmology Telescope: Two-season ACTPol spectra and parameters

Author: Louis, T, Grace, E, Hasselfield, M, Lungu, M, Maurin, L, Addison, GE, Ade, PAR, Aiola, S, Allison, R, Amiri, M, Angile, E, Battaglia, N, Beall, JA, De Bernardis, F, Bond, JR, Britton, J, Calabrese, E, Cho, HM, Choi, SK, Coughlin, K, Crichton, D, Crowley, K, Datta, R, Devlin, MJ, Dicker, SR, Dunkley, J, Dünner, R, Ferraro, S, Fox, AE, Gallardo, P, Gralla, M, Halpern, M, Henderson, S, Hill, JC, Hilton, GC, Hilton, M, Hincks, AD, Hlozek, R, Patty Ho, SP, Huang, Z, Hubmayr, J, Huffenberger, KM, Hughes, JP, Infante, L, Irwin, K, Kasanda, SM, Klein, J, Koopman, B, Kosowsky, A, Li, D, Madhavacheril, M, Marriage, TA, McMahon, J, Menanteau, F, Moodley, K, Munson, C, Naess, S, Nati, F, Newburgh, L, Nibarger, J, Niemack, MD, Nolta, MR, Nuñez, C, Page, LA, Pappas, C, Partridge, B, Rojas, F, Schaan, E, Schmitt, BL, Sehgal, N, Sherwin, BD, Sievers, J, Simon, S, Spergel, DN, Staggs, ST, Switzer, ER, Thornton, R, Trac, H, Treu, J, Tucker, C, Engelen, AV, Ward, JT, and Wollack, EJ
Subjects: CMBR experiments, CMBR polarisation, cosmological parameters from CMBR, astro-ph.CO, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: We present the temperature and polarization angular power spectra measured by the Atacama Cosmology Telescope Polarimeter (ACTPol). We analyze night-time data collected during 2013-14 using two detector arrays at 149 GHz, from 548 deg2 of sky on the celestial equator. We use these spectra, and the spectra measured with the MBAC camera on ACT from 2008-10, in combination with planck and wmap data to estimate cosmological parameters from the temperature, polarization, and temperature-polarization cross-correlations. We find the new ACTPol data to be consistent with the ΛCDM model. The ACTPol temperature-polarization cross-spectrum now provides stronger constraints on multiple parameters than the ACTPol temperature spectrum, including the baryon density, the acoustic peak angular scale, and the derived Hubble constant. The new ACTPol data provide information on damping tail parameters. The joint uncertainty on the number of neutrino species and the primordial helium fraction is reduced by 20% when adding ACTPol to Planck temperature data alone.
Published: 2017

5. Dynamical Mass Measurements of Contaminated Galaxy Clusters Using Machine Learning

Author: Ntampaka, M., Trac, H., Sutherland, D. J., Fromenteau, S., Poczos, B., and Schneider, J.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We study dynamical mass measurements of galaxy clusters contaminated by interlopers and show that a modern machine learning (ML) algorithm can predict masses by better than a factor of two compared to a standard scaling relation approach. We create two mock catalogs from Multidark's publicly available $N$-body MDPL1 simulation, one with perfect galaxy cluster membership information and the other where a simple cylindrical cut around the cluster center allows interlopers to contaminate the clusters. In the standard approach, we use a power-law scaling relation to infer cluster mass from galaxy line-of-sight (LOS) velocity dispersion. Assuming perfect membership knowledge, this unrealistic case produces a wide fractional mass error distribution, with a width of $\Delta\epsilon\approx0.87$. Interlopers introduce additional scatter, significantly widening the error distribution further ($\Delta\epsilon\approx2.13$). We employ the support distribution machine (SDM) class of algorithms to learn from distributions of data to predict single values. Applied to distributions of galaxy observables such as LOS velocity and projected distance from the cluster center, SDM yields better than a factor-of-two improvement ($\Delta\epsilon\approx0.67$) for the contaminated case. Remarkably, SDM applied to contaminated clusters is better able to recover masses than even the scaling relation approach applied to uncontaminated clusters. We show that the SDM method more accurately reproduces the cluster mass function, making it a valuable tool for employing cluster observations to evaluate cosmological models., Comment: 18 pages, 12 figures, accepted for publication at ApJ
Published: 2015
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6. The Atacama Cosmology Telescope: likelihood for small-scale CMB data

Author: Dunkley, J., Calabrese, E., Sievers, J., Addison, G. E., Battaglia, N., Battistelli, E. S., Bond, J. R., Das, S., Devlin, M. J., Dunner, R., Fowler, J. W., Gralla, M., Hajian, A., Halpern, M., Hasselfield, M., Hincks, A. D., Hlozek, R., Hughes, J. P., Irwin, K. D., Kosowsky, A., Louis, T., Marriage, T. A., Marsden, D., Menanteau, F., Moodley, K., Niemack, M., Nolta, M. R., Page, L. A., Partridge, B., Sehgal, N., Spergel, D. N., Staggs, S. T., Switzer, E. R., Trac, H., and Wollack, E.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Atacama Cosmology Telescope has measured the angular power spectra of microwave fluctuations to arcminute scales at frequencies of 148 and 218 GHz, from three seasons of data. At small scales the fluctuations in the primordial Cosmic Microwave Background (CMB) become increasingly obscured by extragalactic foregounds and secondary CMB signals. We present results from a nine-parameter model describing these secondary effects, including the thermal and kinematic Sunyaev-Zel'dovich (tSZ and kSZ) power; the clustered and Poisson-like power from Cosmic Infrared Background (CIB) sources, and their frequency scaling; the tSZ-CIB correlation coefficient; the extragalactic radio source power; and thermal dust emission from Galactic cirrus in two different regions of the sky. In order to extract cosmological parameters, we describe a likelihood function for the ACT data, fitting this model to the multi-frequency spectra in the multipole range 500
Published: 2013
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7. The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey

Author: Marriage, T. A., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., Burger, B., Chervenak, J., Das, S., Devlin, M. J., Dicker, S. R., Doriese, W. B., Dunkley, J., Dunner, R., Essinger-Hileman, T., Fisher, R. P., Fowler, J. W., Hajian, A., Halpern, M., Hasselfield, M., Hern'andez-Monteagudo, C., Hilton, G. C., Hilton, M., Hincks, A. D., Hlozek, R., Huffenberger, K. M., Hughes, D. H., Hughes, J. P., Infante, L., Irwin, K. D., Juin, J. B., Kaul, M., Klein, J., Kosowsky, A., Lau, J. M., Limon, M., Lin, Y. -T., Lupton, R. H., Marsden, D., Martocci, K., Mauskopf, P., Menanteau, F., Moodley, K., Moseley, H., Netterfield, C. B., Niemack, M. D., Nolta, M. R., Page, L. A., Parker, L., Partridge, B., Quintana, H., Reese, E. D., Reid, B., Sehgal, N., Sherwin, B. D., Sievers, J., Spergel, D. N., Staggs, S. T., Swetz, D. S., Switzer, E. R., Thornton, R., Trac, H., Tucker, C., Warne, R., Wilson, G., Wollack, E., and Zhao, Y.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We report on twenty-three clusters detected blindly as Sunyaev-Zel'dovich (SZ) decrements in a 148 GHz, 455 square-degree map of the southern sky made with data from the Atacama Cosmology Telescope 2008 observing season. All SZ detections announced in this work have confirmed optical counterparts. Ten of the clusters are new discoveries. One newly discovered cluster, ACT-CL J0102-4915, with a redshift of 0.75 (photometric), has an SZ decrement comparable to the most massive systems at lower redshifts. Simulations of the cluster recovery method reproduce the sample purity measured by optical follow-up. In particular, for clusters detected with a signal-to-noise ratio greater than six, simulations are consistent with optical follow-up that demonstrated this subsample is 100% pure. The simulations further imply that the total sample is 80% complete for clusters with mass in excess of 6x10^14 solar masses referenced to the cluster volume characterized by five hundred times the critical density. The Compton y -- X-ray luminosity mass comparison for the eleven best detected clusters visually agrees with both self-similar and non-adiabatic, simulation-derived scaling laws., Comment: 13 pages, 7 figures, Accepted for publication in ApJ
Published: 2010
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8. The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra

Author: Dunkley, J., Hlozek, R., Sievers, J., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., Burger, B., Chervenak, J., Das, S., Devlin, M. J., Dicker, S. R., Doriese, W. Bertrand, Dunner, R., Essinger-Hileman, T., Fisher, R. P., Fowler, J. W., Hajian, A., Halpern, M., Hasselfield, M., Hernandez-Monteagudo, C., Hilton, G. C., Hilton, M., Hincks, A. D., Huffenberger, K. M., Hughes, D. H., Hughes, J. P., Infante, L., Irwin, K. D., Juin, J. B., Kaul, M., Klein, J., Kosowsky, A., Lau, J. M, Limon, M., Lin, Y-T., Lupton, R. H., Marriage, T. A., Marsden, D., Mauskopf, P., Menanteau, F., Moodley, K., Moseley, H., Netterfield, C. B, Niemack, M. D., Nolta, M. R., Page, L. A., Parker, L., Partridge, B., Reid, B., Sehgal, N., Sherwin, B., Spergel, D. N., Staggs, S. T., Swetz, D. S., Switzer, E. R., Thornton, R., Trac, H., Tucker, C., Warne, R., Wollack, E., and Zhao, Y.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present cosmological parameters derived from the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over 296 deg^2 with the Atacama Cosmology Telescope (ACT) during its 2008 season. ACT measures fluctuations at scales 500
Published: 2010
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9. The Atacama Cosmology Telescope: Extragalactic Sources at 148 GHz in the 2008 Survey

Author: Marriage, T. A., Juin, J. B., Lin, Y. -T., Marsden, D., Nolta, M. R., Partridge, B., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., Burger, B., Chervenak, J., Das, S., Devlin, M. J., Dicker, S. R., Doriese, W. B., Dunkley, J., Dunner, R., Essinger-Hileman, T., Fisher, R. P., Fowler, J. W., Hajian, A., Halpern, M., Hasselfield, M., Hernandez-Monteagudo, C., Hilton, G. C., Hilton, M., Hincks, A. D., Hlozek, R., Huffenberger, K. M., Hughes, D. H., Hughes, J. P., Infante, L., Irwin, K. D., Kaul, M., Klein, J., Kosowsky, A., Lau, J. M., Limon, M., Lupton, R. H., Martocci, K., Mauskopf, P., Menanteau, F., Moodley, K., Moseley, H., Netterfield, C. B., Niemack, M. D., Page, L. A., Parker, L., Quintana, H., Reid, B., Sehgal, N., Sherwin, B. D., Sievers, J., Spergel, D. N., Staggs, S. T., Swetz, D. S., Switzer, E. R., Thornton, R., Trac, H., Tucker, C., Warne, R., Wilson, G., Wollack, E., and Zhao, Y.
Subjects: Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract: We report on extragalactic sources detected in a 455 square-degree map of the southern sky made with data at a frequency of 148 GHz from the Atacama Cosmology Telescope 2008 observing season. We provide a catalog of 157 sources with flux densities spanning two orders of magnitude: from 15 to 1500 mJy. Comparison to other catalogs shows that 98% of the ACT detections correspond to sources detected at lower radio frequencies. Three of the sources appear to be associated with the brightest cluster galaxies of low redshift X-ray selected galaxy clusters. Estimates of the radio to mm-wave spectral indices and differential counts of the sources further bolster the hypothesis that they are nearly all radio sources, and that their emission is not dominated by re-emission from warm dust. In a bright (>50 mJy) 148 GHz-selected sample with complete cross-identifications from the Australia Telescope 20 GHz survey, we observe an average steepening of the spectra between 5, 20, and 148 GHz with median spectral indices of $\alpha_{\rm 5-20} = -0.07 \pm 0.06$, $\alpha_{\rm 20-148} = -0.39 \pm0.04$, and $\alpha_{\rm 5-148} = -0.20 \pm 0.03$. When the measured spectral indices are taken into account, the 148 GHz differential source counts are consistent with previous measurements at 30 GHz in the context of a source count model dominated by radio sources. Extrapolating with an appropriately rescaled model for the radio source counts, the Poisson contribution to the spatial power spectrum from synchrotron-dominated sources with flux density less than 20 mJy is $C^{\rm Sync} = (2.8 \pm 0.3) \times 10^{-6} \micro\kelvin^2$., Comment: Accepted to ApJ
Published: 2010
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10. The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz

Author: Fowler, J. W., Acquaviva, V., Ade, P. A. R., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., Burger, B., Chervenak, J., Das, S., Devlin, M. J., Dicker, S. R., Doriese, W. B., Dunkley, J., Dünner, R., Essinger-Hileman, T., Fisher, R. P., Hajian, A., Halpern, M., Hasselfield, M., Hernández-Monteagudo, C., Hilton, G. C., Hilton, M., Hincks, A. D., Hlozek, R., Huffenberger, K. M., Hughes, D. H., Hughes, J. P., Infante, L., Irwin, K. D., Jimenez, R., Juin, J. B., Kaul, M., Klein, J., Kosowsky, A., Lau, J. M., Limon, M., Lin, Y. -T., Lupton, R. H., Marriage, T. A., Marsden, D., Martocci, K., Mauskopf, P., Menanteau, F., Moodley, K., Moseley, H., Netterfield, C. B., Niemack, M. D., Nolta, M. R., Page, L. A., Parker, L., Partridge, B., Quintana, H., Reid, B., Sehgal, N., Sievers, J., Spergel, D. N., Staggs, S. T., Swetz, D. S., Switzer, E. R., Thornton, R., Trac, H., Tucker, C., Verde, L., Warne, R., Wilson, G., Wollack, E., Zhao, Y., and Collaboration, the ACT
Subjects: Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract: We present a measurement of the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz. The measurement uses maps with 1.4' angular resolution made with data from the Atacama Cosmology Telescope (ACT). The observations cover 228 square degrees of the southern sky, in a 4.2-degree-wide strip centered on declination 53 degrees South. The CMB at arcminute angular scales is particularly sensitive to the Silk damping scale, to the Sunyaev-Zel'dovich (SZ) effect from galaxy clusters, and to emission by radio sources and dusty galaxies. After masking the 108 brightest point sources in our maps, we estimate the power spectrum between 600 < \ell < 8000 using the adaptive multi-taper method to minimize spectral leakage and maximize use of the full data set. Our absolute calibration is based on observations of Uranus. To verify the calibration and test the fidelity of our map at large angular scales, we cross-correlate the ACT map to the WMAP map and recover the WMAP power spectrum from 250 < ell < 1150. The power beyond the Silk damping tail of the CMB is consistent with models of the emission from point sources. We quantify the contribution of SZ clusters to the power spectrum by fitting to a model normalized at sigma8 = 0.8. We constrain the model's amplitude ASZ < 1.63 (95% CL). If interpreted as a measurement of sigma8, this implies sigma8^SZ < 0.86 (95% CL) given our SZ model. A fit of ACT and WMAP five-year data jointly to a 6-parameter LCDM model plus terms for point sources and the SZ effect is consistent with these results., Comment: 15 pages, 8 figures. Accepted for publication in ApJ
Published: 2010
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11. The Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps

Author: Hincks, A. D., Acquaviva, V., Ade, P., Aguirre, P., Amiri, M., Appel, J. W., Barrientos, L. F., Battistelli, E. S., Bond, J. R., Brown, B., Burger, B., Chervenak, J., Das, S., Devlin, M. J., Dicker, S., Doriese, W. B., Dunkley, J., Dünner, R., Essinger-Hileman, T., Fisher, R. P., Fowler, J. W., Hajian, A., Halpern, M., Hasselfield, M., Hernández-Monteagudo, C., Hilton, G. C., Hilton, M., Hlozek, R., Huffenberger, K., Hughes, D., Hughes, J. P., Infante, L., Irwin, K. D., Jimenez, R., Juin, J. B., Kaul, M., Klein, J., Kosowsky, A., Lau, J. M., Limon, M., Lin, Y. -T., Lupton, R. H., Marriage, T., Marsden, D., Martocci, K., Mauskopf, P., Menanteau, F., Moodley, K., Moseley, H., Netterfield, C. B., Niemack, M. D., Nolta, M. R., Page, L. A., Parker, L., Partridge, B., Quintana, H., Reid, B., Sehgal, N., Sievers, J., Spergel, D. N., Staggs, S. T., Stryzak, O., Swetz, D., Switzer, E., Thornton, R., Trac, H., Tucker, C., Verde, L., Warne, R., Wilson, G., Wollack, E., and Zhao, Y.
Subjects: Astrophysics - Cosmology and Extragalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Atacama Cosmology Telescope (ACT) is currently observing the cosmic microwave background with arcminute resolution at 148 GHz, 218 GHz, and 277 GHz. In this paper, we present ACT's first results. Data have been analyzed using a maximum-likelihood map-making method which uses B-splines to model and remove the atmospheric signal. It has been used to make high-precision beam maps from which we determine the experiment's window functions. This beam information directly impacts all subsequent analyses of the data. We also used the method to map a sample of galaxy clusters via the Sunyaev-Zel'dovich (SZ) effect, and show five clusters previously detected with X-ray or SZ observations. We provide integrated Compton-y measurements for each cluster. Of particular interest is our detection of the z = 0.44 component of A3128 and our current non-detection of the low-redshift part, providing strong evidence that the further cluster is more massive as suggested by X-ray measurements. This is a compelling example of the redshift-independent mass selection of the SZ effect., Comment: 16 pages, 10 figures. Accepted for publication in ApJS. See Marriage et al. (arXiv:1010.1065) and Menanteau et al. (arXiv:1006.5126) for additional cluster results
Published: 2009
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12. Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect

Author: Moodley, K., Warne, R., Goheer, N., and Trac, H.
Subjects: Astrophysics
Abstract: Motivated by the observed shortfall of baryons in the local universe, we investigate the ability of high resolution cosmic microwave background (CMB) experiments to detect hot gas in the outer regions of nearby group halos. We construct hot gas models with the gas in hydrostatic equilibrium with the dark matter and described by a polytropic equation of state. We also consider models that add entropy to the gas in line with constraints from X-ray observations. We calculate the thermal Sunyaev-Zel'dovich (SZ) signal in these halos and compare it to the anticipated sensitivities of forthcoming SZ survey experiments such as ACT, PLANCK and SPT. Using a multi-frequency Wiener filter we derive SZ detectability limits as a function of halo mass and redshift in the presence of galactic and extragalactic foregrounds and the CMB. We find that group-sized halos with virial masses below 1e14 M_solar can be detected at z < 0.05 with the threshold mass dropping to 3-4e13 M_solar at z < 0.01. The SZ distortion of nearby group-sized halos can thus be mapped out to the virial radius by these CMB experiments, beyond the sensitivity limits of X-ray observations. These measurements will provide a unique probe of hot gas in the outer regions of group halos, shedding insight into the local census of baryons and the injection of entropy into the intragroup medium from non-gravitational feedback., Comment: 17 pages, 16 figures
Published: 2008
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13. The atacama cosmology telescope: A catalog of >4000 Sunyaev–Zel’dovich galaxy clusters

Author: Hilton, M, Sifon, C, Naess, S, Madhavacheril, M, Oguri, M, Rozo, E, Rykoff, E, Adhikari, S, Aguena, M, Aiola, S, Allam, S, Amodeo, S, Amon, A, Annis, J, Ansarinejad, B, Abbott, T, Aros-Bunster, C, Austermann, J, Avila, S, Bacon, D, Battaglia, N, Beall, J, Becker, D, Bernstein, G, Bertin, E, Bhandarkar, T, Bhargava, S, Bond, J, Brooks, D, Burke, D, Calabrese, E, Carrasco Kind, M, Carretero, J, Choi, S, Choi, A, Conselice, C, Da Costa, L, Costanzi, M, Crichton, D, Crowley, K, Dunner, R, Denison, E, Devlin, M, Dicker, S, Diehl, H, Dietrich, J, Doel, P, Duff, S, Duivenvoorden, A, Dunkley, J, Everett, S, Ferraro, S, Ferte, A, Flaugher, B, Frieman, J, Ferrero, I, Gallardo, P, Garcia-Bellido, J, Gaztanaga, E, Giles, P, Golec, J, Gralla, M, Grandis, S, Gruen, D, Gerdes, D, Gruendl, R, Gschwend, J, Gutierrez, G, Han, D, Hartley, W, Hasselfield, M, Hill, J, Hilton, G, Hincks, A, Hinton, S, Ho, S, Honscheid, K, Hoyle, B, Hubmayr, J, Huffenberger, K, Hughes, J, Jaelani, A, Jain, B, James, D, Jeltema, T, Kent, S, Knowles, K, Koopman, B, Kuehn, K, Lahav, O, Lima, M, Lin, Y, Lokken, M, Loubser, S, Maccrann, N, Maia, M, Marriage, T, Martin, J, Mcmahon, J, Melchior, P, Menanteau, F, Miquel, R, Moodley, K, Morgan, R, Mroczkowski, T, Nati, F, Newburgh, L, Niemack, M, Nishizawa, A, Miyatake, H, Ogando, R, Orlowski-Scherer, J, Page, L, Palmese, A, Partridge, B, Paz-Chinchon, F, Phakathi, P, Plazas, A, Robertson, N, Romer, A, Carnero Rosell, A, Sanchez, E, Schaan, E, Schillaci, A, Sehgal, N, Serrano, S, Shin, T, Simon, S, Smith, M, Salatino, M, Soares-Santos, M, Spergel, D, Staggs, S, Storer, E, Suchyta, E, Swanson, M, Tarle, G, Thomas, D, To, C, Trac, H, Ullom, J, Vale, L, Van Lanen, J, Vavagiakis, E, De Vicente, J, Wilkinson, R, Wollack, E, Xu, Z, Zhan, Y, Hilton M., Sifon C., Naess S., Madhavacheril M., Oguri M., Rozo E., Rykoff E., Adhikari S., Aguena M., Aiola S., Allam S., Amodeo S., Amon A., Annis J., Ansarinejad B., Abbott T. M. C., Aros-Bunster C., Austermann J. E., Avila S., Bacon D., Battaglia N., Beall J. A., Becker D. T., Bernstein G. M., Bertin E., Bhandarkar T., Bhargava S., Bond J. R., Brooks D., Burke D. L., Calabrese E., Carrasco Kind M., Carretero J., Choi S. K., Choi A., Conselice C., Da Costa L. N., Costanzi M., Crichton D., Crowley K. T., Dunner R., Denison E. V., Devlin M. J., Dicker S. R., Diehl H. T., Dietrich J. P., Doel P., Duff S. M., Duivenvoorden A. J., Dunkley J., Everett S., Ferraro S., Ferte A., Flaugher B., Frieman J., Ferrero I., Gallardo P. A., Garcia-Bellido J., Gaztanaga E., Giles P., Golec J. E., Gralla M. B., Grandis S., Gruen D., Gerdes D. W., Gruendl R. A., Gschwend J., Gutierrez G., Han D., Hartley W. G., Hasselfield M., Hill J. C., Hilton G. C., Hincks A. D., Hinton S. R., Ho S. -P. P., Honscheid K., Hoyle B., Hubmayr J., Huffenberger K. M., Hughes J. P., Jaelani A. T., Jain B., James D. J., Jeltema T., Kent S., Knowles K., Koopman B. J., Kuehn K., Lahav O., Lima M., Lin Y. -T., Lokken M., Loubser S. I., MacCrann N., Maia M. A. G., Marriage T. A., Martin J., McMahon J., Melchior P., Menanteau F., Miquel R., Moodley K., Morgan R., Mroczkowski T., Nati F., Newburgh L. B., Niemack M. D., Nishizawa A. J., Miyatake H., Ogando R. L. C., Orlowski-Scherer J., Page L. A., Palmese A., Partridge B., Paz-Chinchon F., Phakathi P., Plazas A. A., Robertson N. C., Romer A. K., Carnero Rosell A., Sanchez E., Schaan E., Schillaci A., Sehgal N., Serrano S., Shin T., Simon S. M., Smith M., Salatino M., Soares-Santos M., Spergel D. N., Staggs S. T., Storer E. R., Suchyta E., Swanson M. E. C., Tarle G., Thomas D., To C., Trac H., Ullom J. N., Vale L. R., Van Lanen J., Vavagiakis E. M., De Vicente J., Wilkinson R. D., Wollack E. J., Xu Z., Zhan Y., Hilton, M, Sifon, C, Naess, S, Madhavacheril, M, Oguri, M, Rozo, E, Rykoff, E, Adhikari, S, Aguena, M, Aiola, S, Allam, S, Amodeo, S, Amon, A, Annis, J, Ansarinejad, B, Abbott, T, Aros-Bunster, C, Austermann, J, Avila, S, Bacon, D, Battaglia, N, Beall, J, Becker, D, Bernstein, G, Bertin, E, Bhandarkar, T, Bhargava, S, Bond, J, Brooks, D, Burke, D, Calabrese, E, Carrasco Kind, M, Carretero, J, Choi, S, Choi, A, Conselice, C, Da Costa, L, Costanzi, M, Crichton, D, Crowley, K, Dunner, R, Denison, E, Devlin, M, Dicker, S, Diehl, H, Dietrich, J, Doel, P, Duff, S, Duivenvoorden, A, Dunkley, J, Everett, S, Ferraro, S, Ferte, A, Flaugher, B, Frieman, J, Ferrero, I, Gallardo, P, Garcia-Bellido, J, Gaztanaga, E, Giles, P, Golec, J, Gralla, M, Grandis, S, Gruen, D, Gerdes, D, Gruendl, R, Gschwend, J, Gutierrez, G, Han, D, Hartley, W, Hasselfield, M, Hill, J, Hilton, G, Hincks, A, Hinton, S, Ho, S, Honscheid, K, Hoyle, B, Hubmayr, J, Huffenberger, K, Hughes, J, Jaelani, A, Jain, B, James, D, Jeltema, T, Kent, S, Knowles, K, Koopman, B, Kuehn, K, Lahav, O, Lima, M, Lin, Y, Lokken, M, Loubser, S, Maccrann, N, Maia, M, Marriage, T, Martin, J, Mcmahon, J, Melchior, P, Menanteau, F, Miquel, R, Moodley, K, Morgan, R, Mroczkowski, T, Nati, F, Newburgh, L, Niemack, M, Nishizawa, A, Miyatake, H, Ogando, R, Orlowski-Scherer, J, Page, L, Palmese, A, Partridge, B, Paz-Chinchon, F, Phakathi, P, Plazas, A, Robertson, N, Romer, A, Carnero Rosell, A, Sanchez, E, Schaan, E, Schillaci, A, Sehgal, N, Serrano, S, Shin, T, Simon, S, Smith, M, Salatino, M, Soares-Santos, M, Spergel, D, Staggs, S, Storer, E, Suchyta, E, Swanson, M, Tarle, G, Thomas, D, To, C, Trac, H, Ullom, J, Vale, L, Van Lanen, J, Vavagiakis, E, De Vicente, J, Wilkinson, R, Wollack, E, Xu, Z, Zhan, Y, Hilton M., Sifon C., Naess S., Madhavacheril M., Oguri M., Rozo E., Rykoff E., Adhikari S., Aguena M., Aiola S., Allam S., Amodeo S., Amon A., Annis J., Ansarinejad B., Abbott T. M. C., Aros-Bunster C., Austermann J. E., Avila S., Bacon D., Battaglia N., Beall J. A., Becker D. T., Bernstein G. M., Bertin E., Bhandarkar T., Bhargava S., Bond J. R., Brooks D., Burke D. L., Calabrese E., Carrasco Kind M., Carretero J., Choi S. K., Choi A., Conselice C., Da Costa L. N., Costanzi M., Crichton D., Crowley K. T., Dunner R., Denison E. V., Devlin M. J., Dicker S. R., Diehl H. T., Dietrich J. P., Doel P., Duff S. M., Duivenvoorden A. J., Dunkley J., Everett S., Ferraro S., Ferte A., Flaugher B., Frieman J., Ferrero I., Gallardo P. A., Garcia-Bellido J., Gaztanaga E., Giles P., Golec J. E., Gralla M. B., Grandis S., Gruen D., Gerdes D. W., Gruendl R. A., Gschwend J., Gutierrez G., Han D., Hartley W. G., Hasselfield M., Hill J. C., Hilton G. C., Hincks A. D., Hinton S. R., Ho S. -P. P., Honscheid K., Hoyle B., Hubmayr J., Huffenberger K. M., Hughes J. P., Jaelani A. T., Jain B., James D. J., Jeltema T., Kent S., Knowles K., Koopman B. J., Kuehn K., Lahav O., Lima M., Lin Y. -T., Lokken M., Loubser S. I., MacCrann N., Maia M. A. G., Marriage T. A., Martin J., McMahon J., Melchior P., Menanteau F., Miquel R., Moodley K., Morgan R., Mroczkowski T., Nati F., Newburgh L. B., Niemack M. D., Nishizawa A. J., Miyatake H., Ogando R. L. C., Orlowski-Scherer J., Page L. A., Palmese A., Partridge B., Paz-Chinchon F., Phakathi P., Plazas A. A., Robertson N. C., Romer A. K., Carnero Rosell A., Sanchez E., Schaan E., Schillaci A., Sehgal N., Serrano S., Shin T., Simon S. M., Smith M., Salatino M., Soares-Santos M., Spergel D. N., Staggs S. T., Storer E. R., Suchyta E., Swanson M. E. C., Tarle G., Thomas D., To C., Trac H., Ullom J. N., Vale L. R., Van Lanen J., Vavagiakis E. M., De Vicente J., Wilkinson R. D., Wollack E. J., Xu Z., and Zhan Y.
Abstract: We present a catalog of 4195 optically confirmed Sunyaev–Zel’dovich (SZ) selected galaxy clusters detected with signal-to-noise ratio >4 in 13,211 deg2 of sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were selected by applying a multifrequency matched filter to 98 and 150 GHz maps constructed from ACT observations obtained from 2008 to 2018 and confirmed using deep, wide-area optical surveys. The clusters span the redshift range 0.04 < z < 1.91 (median z = 0.52). The catalog contains 222 z > 1 clusters, and a total of 868 systems are new discoveries. Assuming an SZ signal versus mass-scaling relation calibrated from X-ray observations, the sample has a 90% completeness mass limit of M500c > 3.8 × 1014 Me, evaluated at z = 0.5, for clusters detected at signal-to-noise ratio >5 in maps filtered at an angular scale of 2 4. The survey has a large overlap with deep optical weak-lensing surveys that are being used to calibrate the SZ signal mass-scaling relation, such as the Dark Energy Survey (4566 deg2), the Hyper Suprime-Cam Subaru Strategic Program (469 deg2), and the Kilo Degree Survey (825 deg2). We highlight some noteworthy objects in the sample, including potentially projected systems, clusters with strong lensing features, clusters with active central galaxies or star formation, and systems of multiple clusters that may be physically associated. The cluster catalog will be a useful resource for future cosmological analyses and studying the evolution of the intracluster medium and galaxies in massive clusters over the past 10 Gyr.
Published: 2021

14. Hydrodynamical Simulations of the IGM at High Mach Numbers

Author: Trac, H., Zhang, P., Pen, U., Rosenberg, Jessica L., editor, and Putman, Mary E., editor
Published: 2003
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15. The Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev–Zel’dovich Galaxy Clusters

Author: Hilton, M., primary, Sifón, C., additional, Naess, S., additional, Madhavacheril, M., additional, Oguri, M., additional, Rozo, E., additional, Rykoff, E., additional, Abbott, T. M. C., additional, Adhikari, S., additional, Aguena, M., additional, Aiola, S., additional, Allam, S., additional, Amodeo, S., additional, Amon, A., additional, Annis, J., additional, Ansarinejad, B., additional, Aros-Bunster, C., additional, Austermann, J. E., additional, Avila, S., additional, Bacon, D., additional, Battaglia, N., additional, Beall, J. A., additional, Becker, D. T., additional, Bernstein, G. M., additional, Bertin, E., additional, Bhandarkar, T., additional, Bhargava, S., additional, Bond, J. R., additional, Brooks, D., additional, Burke, D. L., additional, Calabrese, E., additional, Carrasco Kind, M., additional, Carretero, J., additional, Choi, S. K., additional, Choi, A., additional, Conselice, C., additional, Costa, L. N. da, additional, Costanzi, M., additional, Crichton, D., additional, Crowley, K. T., additional, Dünner, R., additional, Denison, E. V., additional, Devlin, M. J., additional, Dicker, S. R., additional, Diehl, H. T., additional, Dietrich, J. P., additional, Doel, P., additional, Duff, S. M., additional, Duivenvoorden, A. J., additional, Dunkley, J., additional, Everett, S., additional, Ferraro, S., additional, Ferrero, I., additional, Ferté, A., additional, Flaugher, B., additional, Frieman, J., additional, Gallardo, P. A., additional, García-Bellido, J., additional, Gaztanaga, E., additional, Gerdes, D. W., additional, Giles, P., additional, Golec, J. E., additional, Gralla, M. B., additional, Grandis, S., additional, Gruen, D., additional, Gruendl, R. A., additional, Gschwend, J., additional, Gutierrez, G., additional, Han, D., additional, Hartley, W. G., additional, Hasselfield, M., additional, Hill, J. C., additional, Hilton, G. C., additional, Hincks, A. D., additional, Hinton, S. R., additional, Ho, S-P. P., additional, Honscheid, K., additional, Hoyle, B., additional, Hubmayr, J., additional, Huffenberger, K. M., additional, Hughes, J. P., additional, Jaelani, A. T., additional, Jain, B., additional, James, D. J., additional, Jeltema, T., additional, Kent, S., additional, Knowles, K., additional, Koopman, B. J., additional, Kuehn, K., additional, Lahav, O., additional, Lima, M., additional, Lin, Y-T., additional, Lokken, M., additional, Loubser, S. I., additional, MacCrann, N., additional, Maia, M. A. G., additional, Marriage, T. A., additional, Martin, J., additional, McMahon, J., additional, Melchior, P., additional, Menanteau, F., additional, Miquel, R., additional, Miyatake, H., additional, Moodley, K., additional, Morgan, R., additional, Mroczkowski, T., additional, Nati, F., additional, Newburgh, L. B., additional, Niemack, M. D., additional, Nishizawa, A. J., additional, Ogando, R. L. C., additional, Orlowski-Scherer, J., additional, Page, L. A., additional, Palmese, A., additional, Partridge, B., additional, Paz-Chinchón, F., additional, Phakathi, P., additional, Plazas, A. A., additional, Robertson, N. C., additional, Romer, A. K., additional, Rosell, A. Carnero, additional, Salatino, M., additional, Sanchez, E., additional, Schaan, E., additional, Schillaci, A., additional, Sehgal, N., additional, Serrano, S., additional, Shin, T., additional, Simon, S. M., additional, Smith, M., additional, Soares-Santos, M., additional, Spergel, D. N., additional, Staggs, S. T., additional, Storer, E. R., additional, Suchyta, E., additional, Swanson, M. E. C., additional, Tarle, G., additional, Thomas, D., additional, To, C., additional, Trac, H., additional, Ullom, J. N., additional, Vale, L. R., additional, Lanen, J. Van, additional, Vavagiakis, E. M., additional, Vicente, J. De, additional, Wilkinson, R. D., additional, Wollack, E. J., additional, Xu, Z., additional, and Zhang, Y., additional
Published: 2021
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16. A Computational Study on the Redox Reactions of Ammonia and Methylamine with Nitrogen Tetroxide

Author: Trac, H. Phuong, primary, Le Huyen, Trinh, additional, and Lin, Ming-Chang, additional
Published: 2020
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17. The Simons Observatory: science goals and forecasts

Author: Ade, P, Aguirre, J, Ahmed, Z, Aiola, S, Ali, A, Alonso, D, Alvarez, M, Arnold, K, Ashton, P, Austermann, J, Awan, H, Baccigalupi, C, Baildon, T, Barron, D, Battaglia, N, Battye, R, Baxter, E, Bazarko, A, Beall, J, Bean, R, Beck, D, Beckman, S, Beringue, B, Bianchini, F, Boada, S, Boettger, D, Bond, J, Borrill, J, Brown, M, Bruno, S, Bryan, S, Calabrese, E, Calafut, V, Calisse, P, Carron, J, Challinor, A, Chesmore, G, Chinone, Y, Chluba, J, Cho, H, Choi, S, Coppi, G, Cothard, N, Coughlin, K, Crichton, D, Crowley, K, Cukierman, A, D'Ewart, J, Dünner, R, de Haan, T, Devlin, M, Dicker, S, Didier, J, Dobbs, M, Dober, B, Duell, C, Duff, S, Duivenvoorden, A, Dunkley, J, Dusatko, J, Errard, J, Fabbian, G, Feeney, S, Ferraro, S, Fluxà, P, Freese, K, Frisch, J, Frolov, A, Fuller, G, Fuzia, B, Galitzki, N, Gallardo, P, Ghersi, J, Gao, J, Gawiser, E, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Golec, J, Gordon, S, Gralla, M, Green, D, Grigorian, A, Groh, J, Groppi, C, Guan, Y, Gudmundsson, J, Han, D, Hargrave, P, Hasegawa, M, Hasselfield, M, Hattori, M, Haynes, V, Hazumi, M, He, Y, Healy, E, Henderson, S, Hervias-Caimapo, C, Hill, C, Hill, J, Hilton, G, Hilton, M, Hincks, A, Hinshaw, G, Hložek, R, Ho, S, Howe, L, Huang, Z, Hubmayr, J, Huffenberger, K, Hughes, J, Ijjas, A, Ikape, M, Irwin, K, Jaffe, A, Jain, B, Jeong, O, Kaneko, D, Karpel, E, Katayama, N, Keating, B, Kernasovskiy, S, Keskitalo, R, Kisner, T, Kiuchi, K, Klein, J, Knowles, K, Koopman, B, Kosowsky, A, Krachmalnicoff, N, Kuenstner, S, Kuo, C, Kusaka, A, Lashner, J, Lee, A, Lee, E, Leon, D, Leung, J, Lewis, A, Li, Y, Li, Z, Limon, M, Linder, E, Lopez-Caraballo, C, Louis, T, Lowry, L, Lungu, M, Madhavacheril, M, Mak, D, Maldonado, F, Mani, H, Mates, B, Matsuda, F, Maurin, L, Mauskopf, P, May, A, Mccallum, N, Mckenney, C, Mcmahon, J, Meerburg, P, Meyers, J, Miller, A, Mirmelstein, M, Moodley, K, Munchmeyer, M, Munson, C, Naess, S, Nati, F, Navaroli, M, Newburgh, L, Nguyen, H, Niemack, M, Nishino, H, Orlowski-Scherer, J, Page, L, Partridge, B, Peloton, J, Perrotta, F, Piccirillo, L, Pisano, G, Poletti, D, Puddu, R, Puglisi, G, Raum, C, Reichardt, C, Remazeilles, M, Rephaeli, Y, Riechers, D, Rojas, F, Roy, A, Sadeh, S, Sakurai, Y, Salatino, M, Rao, M, Schaan, E, Schmittfull, M, Sehgal, N, Seibert, J, Seljak, U, Sherwin, B, Shimon, M, Sierra, C, Sievers, J, Sikhosana, P, Silva-Feaver, M, Simon, S, Sinclair, A, Siritanasak, P, Smith, K, Smith, S, Spergel, D, Staggs, S, Stein, G, Stevens, J, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Teply, G, Thomas, D, Thorne, B, Thornton, R, Trac, H, Tsai, C, Tucker, C, Ullom, J, Vagnozzi, S, Engelen, A, Lanen, J, Winkle, D, Vavagiakis, E, Vergès, C, Vissers, M, Wagoner, K, Walker, S, Ward, J, Westbrook, B, Whitehorn, N, Williams, J, Wollack, E, Xu, Z, Yu, B, Yu, C, Zago, F, Zhang, H, Zhu, N, Ade, Peter, Aguirre, James, Ahmed, Zeeshan, Aiola, Simone, Ali, Aamir, Alonso, David, Alvarez, Marcelo A., Arnold, Kam, Ashton, Peter, Austermann, Jason, Awan, Humna, Baccigalupi, Carlo, Baildon, Taylor, Barron, Darcy, Battaglia, Nick, Battye, Richard, Baxter, Eric, Bazarko, Andrew, Beall, James A., Bean, Rachel, Beck, Dominic, Beckman, Shawn, Beringue, Benjamin, Bianchini, Federico, Boada, Steven, Boettger, David, Bond, J. Richard, Borrill, Julian, Brown, Michael L., Bruno, Sarah Marie, Bryan, Sean, Calabrese, Erminia, Calafut, Victoria, Calisse, Paolo, Carron, Julien, Challinor, Anthony, Chesmore, Grace, Chinone, Yuji, Chluba, Jens, Cho, Hsiao-Mei Sherry, Choi, Steve, Coppi, Gabriele, Cothard, Nicholas F., Coughlin, Kevin, Crichton, Devin, Crowley, Kevin D., Crowley, Kevin T., Cukierman, Ari, D'Ewart, John M., Dünner, Rolando, de Haan, Tijmen, Devlin, Mark, Dicker, Simon, Didier, Joy, Dobbs, Matt, Dober, Bradley, Duell, Cody J., Duff, Shannon, Duivenvoorden, Adri, Dunkley, Jo, Dusatko, John, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Ferraro, Simone, Fluxà, Pedro, Freese, Katherine, Frisch, Josef C., Frolov, Andrei, Fuller, George, Fuzia, Brittany, Galitzki, Nicholas, Gallardo, Patricio A., Ghersi, Jose Tomas Galvez, Gao, Jiansong, Gawiser, Eric, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Golec, Joseph, Gordon, Sam, Gralla, Megan, Green, Daniel, Grigorian, Arpi, Groh, John, Groppi, Chris, Guan, Yilun, Gudmundsson, Jon E., Han, Dongwon, Hargrave, Peter, Hasegawa, Masaya, Hasselfield, Matthew, Hattori, Makoto, Haynes, Victor, Hazumi, Masashi, He, Yizhou, Healy, Erin, Henderson, Shawn W., Hervias-Caimapo, Carlos, Hill, Charles A., Hill, J. Colin, Hilton, Gene, Hilton, Matt, Hincks, Adam D., Hinshaw, Gary, Hložek, Renée, Ho, Shirley, Ho, Shuay-Pwu Patty, Howe, Logan, Huang, Zhiqi, Hubmayr, Johannes, Huffenberger, Kevin, Hughes, John P., Ijjas, Anna, Ikape, Margaret, Irwin, Kent, Jaffe, Andrew H., Jain, Bhuvnesh, Jeong, Oliver, Kaneko, Daisuke, Karpel, Ethan D., Katayama, Nobuhiko, Keating, Brian, Kernasovskiy, Sarah S., Keskitalo, Reijo, Kisner, Theodore, Kiuchi, Kenji, Klein, Jeff, Knowles, Kenda, Koopman, Brian, Kosowsky, Arthur, Krachmalnicoff, Nicoletta, Kuenstner, Stephen E., Kuo, Chao-Lin, Kusaka, Akito, Lashner, Jacob, Lee, Adrian, Lee, Eunseong, Leon, David, Leung, Jason S. -Y., Lewis, Antony, Li, Yaqiong, Li, Zack, Limon, Michele, Linder, Eric, Lopez-Caraballo, Carlos, Louis, Thibaut, Lowry, Lindsay, Lungu, Marius, Madhavacheril, Mathew, Mak, Daisy, Maldonado, Felipe, Mani, Hamdi, Mates, Ben, Matsuda, Frederick, Maurin, Loïc, Mauskopf, Phil, May, Andrew, McCallum, Nialh, McKenney, Chris, McMahon, Jeff, Meerburg, P. Daniel, Meyers, Joel, Miller, Amber, Mirmelstein, Mark, Moodley, Kavilan, Munchmeyer, Moritz, Munson, Charles, Naess, Sigurd, Nati, Federico, Navaroli, Martin, Newburgh, Laura, Nguyen, Ho Nam, Niemack, Michael, Nishino, Haruki, Orlowski-Scherer, John, Page, Lyman, Partridge, Bruce, Peloton, Julien, Perrotta, Francesca, Piccirillo, Lucio, Pisano, Giampaolo, Poletti, Davide, Puddu, Roberto, Puglisi, Giuseppe, Raum, Chris, Reichardt, Christian L., Remazeilles, Mathieu, Rephaeli, Yoel, Riechers, Dominik, Rojas, Felipe, Roy, Anirban, Sadeh, Sharon, Sakurai, Yuki, Salatino, Maria, Rao, Mayuri Sathyanarayana, Schaan, Emmanuel, Schmittfull, Marcel, Sehgal, Neelima, Seibert, Joseph, Seljak, Uros, Sherwin, Blake, Shimon, Meir, Sierra, Carlos, Sievers, Jonathan, Sikhosana, Precious, Silva-Feaver, Maximiliano, Simon, Sara M., Sinclair, Adrian, Siritanasak, Praween, Smith, Kendrick, Smith, Stephen R., Spergel, David, Staggs, Suzanne T., Stein, George, Stevens, Jason R., Stompor, Radek, Suzuki, Aritoki, Tajima, Osamu, Takakura, Satoru, Teply, Grant, Thomas, Daniel B., Thorne, Ben, Thornton, Robert, Trac, Hy, Tsai, Calvin, Tucker, Carole, Ullom, Joel, Vagnozzi, Sunny, Engelen, Alexander van, Lanen, Jeff Van, Winkle, Daniel D. Van, Vavagiakis, Eve M., Vergès, Clara, Vissers, Michael, Wagoner, Kasey, Walker, Samantha, Ward, Jon, Westbrook, Ben, Whitehorn, Nathan, Williams, Jason, Williams, Joel, Wollack, Edward J., Xu, Zhilei, Yu, Byeonghee, Yu, Cyndia, Zago, Fernando, Zhang, Hezi, Zhu, Ningfeng, Ade, P, Aguirre, J, Ahmed, Z, Aiola, S, Ali, A, Alonso, D, Alvarez, M, Arnold, K, Ashton, P, Austermann, J, Awan, H, Baccigalupi, C, Baildon, T, Barron, D, Battaglia, N, Battye, R, Baxter, E, Bazarko, A, Beall, J, Bean, R, Beck, D, Beckman, S, Beringue, B, Bianchini, F, Boada, S, Boettger, D, Bond, J, Borrill, J, Brown, M, Bruno, S, Bryan, S, Calabrese, E, Calafut, V, Calisse, P, Carron, J, Challinor, A, Chesmore, G, Chinone, Y, Chluba, J, Cho, H, Choi, S, Coppi, G, Cothard, N, Coughlin, K, Crichton, D, Crowley, K, Cukierman, A, D'Ewart, J, Dünner, R, de Haan, T, Devlin, M, Dicker, S, Didier, J, Dobbs, M, Dober, B, Duell, C, Duff, S, Duivenvoorden, A, Dunkley, J, Dusatko, J, Errard, J, Fabbian, G, Feeney, S, Ferraro, S, Fluxà, P, Freese, K, Frisch, J, Frolov, A, Fuller, G, Fuzia, B, Galitzki, N, Gallardo, P, Ghersi, J, Gao, J, Gawiser, E, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Golec, J, Gordon, S, Gralla, M, Green, D, Grigorian, A, Groh, J, Groppi, C, Guan, Y, Gudmundsson, J, Han, D, Hargrave, P, Hasegawa, M, Hasselfield, M, Hattori, M, Haynes, V, Hazumi, M, He, Y, Healy, E, Henderson, S, Hervias-Caimapo, C, Hill, C, Hill, J, Hilton, G, Hilton, M, Hincks, A, Hinshaw, G, Hložek, R, Ho, S, Howe, L, Huang, Z, Hubmayr, J, Huffenberger, K, Hughes, J, Ijjas, A, Ikape, M, Irwin, K, Jaffe, A, Jain, B, Jeong, O, Kaneko, D, Karpel, E, Katayama, N, Keating, B, Kernasovskiy, S, Keskitalo, R, Kisner, T, Kiuchi, K, Klein, J, Knowles, K, Koopman, B, Kosowsky, A, Krachmalnicoff, N, Kuenstner, S, Kuo, C, Kusaka, A, Lashner, J, Lee, A, Lee, E, Leon, D, Leung, J, Lewis, A, Li, Y, Li, Z, Limon, M, Linder, E, Lopez-Caraballo, C, Louis, T, Lowry, L, Lungu, M, Madhavacheril, M, Mak, D, Maldonado, F, Mani, H, Mates, B, Matsuda, F, Maurin, L, Mauskopf, P, May, A, Mccallum, N, Mckenney, C, Mcmahon, J, Meerburg, P, Meyers, J, Miller, A, Mirmelstein, M, Moodley, K, Munchmeyer, M, Munson, C, Naess, S, Nati, F, Navaroli, M, Newburgh, L, Nguyen, H, Niemack, M, Nishino, H, Orlowski-Scherer, J, Page, L, Partridge, B, Peloton, J, Perrotta, F, Piccirillo, L, Pisano, G, Poletti, D, Puddu, R, Puglisi, G, Raum, C, Reichardt, C, Remazeilles, M, Rephaeli, Y, Riechers, D, Rojas, F, Roy, A, Sadeh, S, Sakurai, Y, Salatino, M, Rao, M, Schaan, E, Schmittfull, M, Sehgal, N, Seibert, J, Seljak, U, Sherwin, B, Shimon, M, Sierra, C, Sievers, J, Sikhosana, P, Silva-Feaver, M, Simon, S, Sinclair, A, Siritanasak, P, Smith, K, Smith, S, Spergel, D, Staggs, S, Stein, G, Stevens, J, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Teply, G, Thomas, D, Thorne, B, Thornton, R, Trac, H, Tsai, C, Tucker, C, Ullom, J, Vagnozzi, S, Engelen, A, Lanen, J, Winkle, D, Vavagiakis, E, Vergès, C, Vissers, M, Wagoner, K, Walker, S, Ward, J, Westbrook, B, Whitehorn, N, Williams, J, Wollack, E, Xu, Z, Yu, B, Yu, C, Zago, F, Zhang, H, Zhu, N, Ade, Peter, Aguirre, James, Ahmed, Zeeshan, Aiola, Simone, Ali, Aamir, Alonso, David, Alvarez, Marcelo A., Arnold, Kam, Ashton, Peter, Austermann, Jason, Awan, Humna, Baccigalupi, Carlo, Baildon, Taylor, Barron, Darcy, Battaglia, Nick, Battye, Richard, Baxter, Eric, Bazarko, Andrew, Beall, James A., Bean, Rachel, Beck, Dominic, Beckman, Shawn, Beringue, Benjamin, Bianchini, Federico, Boada, Steven, Boettger, David, Bond, J. Richard, Borrill, Julian, Brown, Michael L., Bruno, Sarah Marie, Bryan, Sean, Calabrese, Erminia, Calafut, Victoria, Calisse, Paolo, Carron, Julien, Challinor, Anthony, Chesmore, Grace, Chinone, Yuji, Chluba, Jens, Cho, Hsiao-Mei Sherry, Choi, Steve, Coppi, Gabriele, Cothard, Nicholas F., Coughlin, Kevin, Crichton, Devin, Crowley, Kevin D., Crowley, Kevin T., Cukierman, Ari, D'Ewart, John M., Dünner, Rolando, de Haan, Tijmen, Devlin, Mark, Dicker, Simon, Didier, Joy, Dobbs, Matt, Dober, Bradley, Duell, Cody J., Duff, Shannon, Duivenvoorden, Adri, Dunkley, Jo, Dusatko, John, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Ferraro, Simone, Fluxà, Pedro, Freese, Katherine, Frisch, Josef C., Frolov, Andrei, Fuller, George, Fuzia, Brittany, Galitzki, Nicholas, Gallardo, Patricio A., Ghersi, Jose Tomas Galvez, Gao, Jiansong, Gawiser, Eric, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Golec, Joseph, Gordon, Sam, Gralla, Megan, Green, Daniel, Grigorian, Arpi, Groh, John, Groppi, Chris, Guan, Yilun, Gudmundsson, Jon E., Han, Dongwon, Hargrave, Peter, Hasegawa, Masaya, Hasselfield, Matthew, Hattori, Makoto, Haynes, Victor, Hazumi, Masashi, He, Yizhou, Healy, Erin, Henderson, Shawn W., Hervias-Caimapo, Carlos, Hill, Charles A., Hill, J. Colin, Hilton, Gene, Hilton, Matt, Hincks, Adam D., Hinshaw, Gary, Hložek, Renée, Ho, Shirley, Ho, Shuay-Pwu Patty, Howe, Logan, Huang, Zhiqi, Hubmayr, Johannes, Huffenberger, Kevin, Hughes, John P., Ijjas, Anna, Ikape, Margaret, Irwin, Kent, Jaffe, Andrew H., Jain, Bhuvnesh, Jeong, Oliver, Kaneko, Daisuke, Karpel, Ethan D., Katayama, Nobuhiko, Keating, Brian, Kernasovskiy, Sarah S., Keskitalo, Reijo, Kisner, Theodore, Kiuchi, Kenji, Klein, Jeff, Knowles, Kenda, Koopman, Brian, Kosowsky, Arthur, Krachmalnicoff, Nicoletta, Kuenstner, Stephen E., Kuo, Chao-Lin, Kusaka, Akito, Lashner, Jacob, Lee, Adrian, Lee, Eunseong, Leon, David, Leung, Jason S. -Y., Lewis, Antony, Li, Yaqiong, Li, Zack, Limon, Michele, Linder, Eric, Lopez-Caraballo, Carlos, Louis, Thibaut, Lowry, Lindsay, Lungu, Marius, Madhavacheril, Mathew, Mak, Daisy, Maldonado, Felipe, Mani, Hamdi, Mates, Ben, Matsuda, Frederick, Maurin, Loïc, Mauskopf, Phil, May, Andrew, McCallum, Nialh, McKenney, Chris, McMahon, Jeff, Meerburg, P. Daniel, Meyers, Joel, Miller, Amber, Mirmelstein, Mark, Moodley, Kavilan, Munchmeyer, Moritz, Munson, Charles, Naess, Sigurd, Nati, Federico, Navaroli, Martin, Newburgh, Laura, Nguyen, Ho Nam, Niemack, Michael, Nishino, Haruki, Orlowski-Scherer, John, Page, Lyman, Partridge, Bruce, Peloton, Julien, Perrotta, Francesca, Piccirillo, Lucio, Pisano, Giampaolo, Poletti, Davide, Puddu, Roberto, Puglisi, Giuseppe, Raum, Chris, Reichardt, Christian L., Remazeilles, Mathieu, Rephaeli, Yoel, Riechers, Dominik, Rojas, Felipe, Roy, Anirban, Sadeh, Sharon, Sakurai, Yuki, Salatino, Maria, Rao, Mayuri Sathyanarayana, Schaan, Emmanuel, Schmittfull, Marcel, Sehgal, Neelima, Seibert, Joseph, Seljak, Uros, Sherwin, Blake, Shimon, Meir, Sierra, Carlos, Sievers, Jonathan, Sikhosana, Precious, Silva-Feaver, Maximiliano, Simon, Sara M., Sinclair, Adrian, Siritanasak, Praween, Smith, Kendrick, Smith, Stephen R., Spergel, David, Staggs, Suzanne T., Stein, George, Stevens, Jason R., Stompor, Radek, Suzuki, Aritoki, Tajima, Osamu, Takakura, Satoru, Teply, Grant, Thomas, Daniel B., Thorne, Ben, Thornton, Robert, Trac, Hy, Tsai, Calvin, Tucker, Carole, Ullom, Joel, Vagnozzi, Sunny, Engelen, Alexander van, Lanen, Jeff Van, Winkle, Daniel D. Van, Vavagiakis, Eve M., Vergès, Clara, Vissers, Michael, Wagoner, Kasey, Walker, Samantha, Ward, Jon, Westbrook, Ben, Whitehorn, Nathan, Williams, Jason, Williams, Joel, Wollack, Edward J., Xu, Zhilei, Yu, Byeonghee, Yu, Cyndia, Zago, Fernando, Zhang, Hezi, and Zhu, Ningfeng
Abstract: The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its performance. SO will measure the temperature and polarization anisotropy of the cosmic microwave background in six frequency bands centered at: 27, 39, 93, 145, 225 and 280 GHz. The initial con figuration of SO will have three small-aperture 0.5-m telescopes and one large-aperture 6-m telescope, with a total of 60,000 cryogenic bolometers. Our key science goals are to characterize the primordial perturbations, measure the number of relativistic species and the mass of neutrinos, test for deviations from a cosmological constant, improve our understanding of galaxy evolution, and constrain the duration of reionization. The small aperture telescopes will target the largest angular scales observable from Chile, mapping approximate to 10% of the sky to a white noise level of 2 mu K-arcmin in combined 93 and 145 GHz bands, to measure the primordial tensor-to-scalar ratio, r, at a target level of sigma(r) = 0.003. The large aperture telescope will map approximate to 40% of the sky at arcminute angular resolution to an expected white noise level of 6 mu K-arcmin in combined 93 and 145 GHz bands, overlapping with the majority of the Large Synoptic Survey Telescope sky region and partially with the Dark Energy Spectroscopic Instrument. With up to an order of magnitude lower polarization noise than maps from the Planck satellite, the high-resolution sky maps will constrain cosmological parameters derived from the damping tail, gravitational lensing of the microwave background, the primordial bispectrum, and the thermal and kinematic Sunyaev-Zel'dovich effects, and will aid in delensing the large-angle polarization signal to measure the tensor-to-scalar ratio. The survey will also provide a legacy catalog of 16,000 galaxy clusters and
Published: 2019

18. THE VELOCITY DISTRIBUTION FUNCTION OF GALAXY CLUSTERS AS A COSMOLOGICAL PROBE

Author: Ntampaka, M., primary, Trac, H., additional, Cisewski, J., additional, and Price, L. C., additional
Published: 2017
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19. Comparison of reionization models: radiative transfer simulations and approximate, seminumeric models

Author: Zahn O, McQuinn M, Trac H, Cen R, Hernquist LE, MESINGER, ANDREI ALBERT, Zahn, O, Mesinger, ANDREI ALBERT, Mcquinn, M, Trac, H, Cen, R, and Hernquist, Le
Published: 2011

20. DYNAMICAL MASS MEASUREMENTS OF CONTAMINATED GALAXY CLUSTERS USING MACHINE LEARNING

Author: Ntampaka, M., primary, Trac, H., additional, Sutherland, D. J., additional, Fromenteau, S., additional, Póczos, B., additional, and Schneider, J., additional
Published: 2016
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21. Dense Sampling and Large Volume: The Structure of the Intergalactic Medium from 50,000 SDSS3 BOSS Quasar Absorption Spectra

Author: Croft, Rupert A., Arnau, E., Aubourg, E., Bailey, S., Bechtold, J., Bhardwaj, V., Bolton, A., Borde, A., Brinkmann, J., Busca, N., Carithers, W., Cen, R., Charlassier, R., Cortes, M., Dall Aglio, A., Stefano Cristiani, Dawson, K., Delubac, T., Font-Ribera, A., Hamilton, J., Ho, S., Lee, K., Legoff, J., Kirkby, D., Lundgren, B., Menard, B., Miralda-Escude, J., Palanque-Delabrouille, N., Myers, A., Paris, I., Peirani, S., Petitjean, P., Pieri, M., Rich, J., Rollinde, E., Ross, N., Schlegel, D., Skibba, R., Slosar, A., Suzuki, N., Trac, H., Vikas, S., Viel, M., Wake, D., Weinberg, D., White, M., Yeche, C., APC - Cosmologie, Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie (APC (UMR_7164)), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), SDSS-III, Hamilton, Jean-Christophe, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: International audience; The BOSS quasar spectra analyzed so far contain over a quarter billion pixels of information on the intervening intergalactic medium. The statistical power of BOSS has previously enabled 10% of the eventual full dataset to yield the first measurements of three dimensional large-scale structure in the Lya forest (Slosar et al 2011). Here we present results from a sample several times larger, covering several topics in cosmology and intergalactic medium science which are qualitatively transformed by the dense sampling (20 quasars per square degree) and enormous sky area. These include new constraints on cosmology and the neutrino mass from a Lya forest power spectrum measurement using 20 times more spectra than the largest previously published analysis (from SDSS), a new catalog of metal absorbers and a stacking analysis which has uncovered many metal species never before seen in the intergalactic medium. Cross-correlations of quasars, galaxies, metal lines and Lyman series absorption provide us with a wide variety of probes, including of cosmology, quasar host masses, lifetimes, and absorber galaxy masses. We show several of these results. We also show through correlation function analysis that the prime task, of making a BAO detection from Lya forest clustering, (the first BAO constraint between z=1 and the CMB) is well on the way to completion.
Published: 2012

22. A MACHINE LEARNING APPROACH FOR DYNAMICAL MASS MEASUREMENTS OF GALAXY CLUSTERS

Author: Ntampaka, M., primary, Trac, H., additional, Sutherland, D. J., additional, Battaglia, N., additional, Póczos, B., additional, and Schneider, J., additional
Published: 2015
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23. REIONIZATION ON LARGE SCALES. IV. PREDICTIONS FOR THE 21 cm SIGNAL INCORPORATING THE LIGHT CONE EFFECT

Author: La Plante, P., primary, Battaglia, N., additional, Natarajan, A., additional, Peterson, J. B., additional, Trac, H., additional, Cen, R., additional, and Loeb, A., additional
Published: 2014
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24. The cosmic code comparison project

Author: Heitmann, K, Lukić, Z, Fasel, P, Habib, S, Warren, M S, White, M, Ahrens, J, Ankeny, L, Armstrong, R, O'Shea, B, Ricker, P M, Springel, V, Stadel, J, Trac, H, Heitmann, K, Lukić, Z, Fasel, P, Habib, S, Warren, M S, White, M, Ahrens, J, Ankeny, L, Armstrong, R, O'Shea, B, Ricker, P M, Springel, V, Stadel, J, and Trac, H
Abstract: Current and upcoming cosmological observations allow us to probe structures on smaller and smaller scales, entering highly nonlinear regimes. In order to obtain theoretical predictions in these regimes, large cosmological simulations have to be carried out. The promised high accuracy from observations makes the simulation task very demanding: the simulations have to be at least as accurate as the observations. This requirement can only be fulfilled by carrying out an extensive code verification program. The first step of such a program is the comparison of different cosmology codes including gravitational interactions only. In this paper, we extend a recently carried out code comparison project to include five more simulation codes. We restrict our analysis to a small cosmological volume which allows us to investigate properties of halos. For the matter power spectrum and the mass function, the previous results hold, with the codes agreeing at the 10% level over wide dynamic ranges. We extend our analysis to the comparison of halo profiles and investigate the halo count as a function of local density. We introduce and discuss ParaView as a flexible analysis tool for cosmological simulations, the use of which immensely simplifies the code comparison task.
Published: 2008

25. REIONIZATION ON LARGE SCALES. III. PREDICTIONS FOR LOW-ℓ COSMIC MICROWAVE BACKGROUND POLARIZATION AND HIGH-ℓ KINETIC SUNYAEV-ZEL'DOVICH OBSERVABLES

Author: Battaglia, N., primary, Natarajan, A., additional, Trac, H., additional, Cen, R., additional, and Loeb, A., additional
Published: 2013
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26. REIONIZATION ON LARGE SCALES. I. A PARAMETRIC MODEL CONSTRUCTED FROM RADIATION-HYDRODYNAMIC SIMULATIONS

Author: Battaglia, N., primary, Trac, H., additional, Cen, R., additional, and Loeb, A., additional
Published: 2013
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27. REIONIZATION ON LARGE SCALES. II. DETECTING PATCHY REIONIZATION THROUGH CROSS-CORRELATION OF THE COSMIC MICROWAVE BACKGROUND

Author: Natarajan, A., primary, Battaglia, N., additional, Trac, H., additional, Pen, U.-L., additional, and Loeb, A., additional
Published: 2013
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28. The Atacama Cosmology Telescope: likelihood for small-scale CMB data

Author: Dunkley, J, primary, Calabrese, E, additional, Sievers, J, additional, Addison, G.E, additional, Battaglia, N, additional, Battistelli, E.S, additional, Bond, J.R, additional, Das, S, additional, Devlin, M.J, additional, Dünner, R, additional, Fowler, J.W, additional, Gralla, M, additional, Hajian, A, additional, Halpern, M, additional, Hasselfield, M, additional, Hincks, A.D, additional, Hlozek, R, additional, Hughes, J.P, additional, Irwin, K.D, additional, Kosowsky, A, additional, Louis, T, additional, Marriage, T.A, additional, Marsden, D, additional, Menanteau, F, additional, Moodley, K, additional, Niemack, M, additional, Nolta, M.R, additional, Page, L.A, additional, Partridge, B, additional, Sehgal, N, additional, Spergel, D.N, additional, Staggs, S.T, additional, Switzer, E.R, additional, Trac, H, additional, and Wollack, E, additional
Published: 2013
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29. THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM

Author: Dunkley, J., primary, Hlozek, R., additional, Sievers, J., additional, Acquaviva, V., additional, Ade, P. A. R., additional, Aguirre, P., additional, Amiri, M., additional, Appel, J. W., additional, Barrientos, L. F., additional, Battistelli, E. S., additional, Bond, J. R., additional, Brown, B., additional, Burger, B., additional, Chervenak, J., additional, Das, S., additional, Devlin, M. J., additional, Dicker, S. R., additional, Doriese, W. Bertrand, additional, Dünner, R., additional, Essinger-Hileman, T., additional, Fisher, R. P., additional, Fowler, J. W., additional, Hajian, A., additional, Halpern, M., additional, Hasselfield, M., additional, Hernández-Monteagudo, C., additional, Hilton, G. C., additional, Hilton, M., additional, Hincks, A. D., additional, Huffenberger, K. M., additional, Hughes, D. H., additional, Hughes, J. P., additional, Infante, L., additional, Irwin, K. D., additional, Juin, J. B., additional, Kaul, M., additional, Klein, J., additional, Kosowsky, A., additional, Lau, J. M, additional, Limon, M., additional, Lin, Y-T., additional, Lupton, R. H., additional, Marriage, T. A., additional, Marsden, D., additional, Mauskopf, P., additional, Menanteau, F., additional, Moodley, K., additional, Moseley, H., additional, Netterfield, C. B, additional, Niemack, M. D., additional, Nolta, M. R., additional, Page, L. A., additional, Parker, L., additional, Partridge, B., additional, Reid, B., additional, Sehgal, N., additional, Sherwin, B., additional, Spergel, D. N., additional, Staggs, S. T., additional, Swetz, D. S., additional, Switzer, E. R., additional, Thornton, R., additional, Trac, H., additional, Tucker, C., additional, Warne, R., additional, Wollack, E., additional, and Zhao, Y., additional
Published: 2011
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30. THE ATACAMA COSMOLOGY TELESCOPE (ACT): BEAM PROFILES AND FIRST SZ CLUSTER MAPS

Author: Hincks, A. D., primary, Acquaviva, V., additional, Ade, P. A. R., additional, Aguirre, P., additional, Amiri, M., additional, Appel, J. W., additional, Barrientos, L. F., additional, Battistelli, E. S., additional, Bond, J. R., additional, Brown, B., additional, Burger, B., additional, Chervenak, J., additional, Das, S., additional, Devlin, M. J., additional, Dicker, S. R., additional, Doriese, W. B., additional, Dunkley, J., additional, Dünner, R., additional, Essinger-Hileman, T., additional, Fisher, R. P., additional, Fowler, J. W., additional, Hajian, A., additional, Halpern, M., additional, Hasselfield, M., additional, Hernández-Monteagudo, C., additional, Hilton, G. C., additional, Hilton, M., additional, Hlozek, R., additional, Huffenberger, K. M., additional, Hughes, D. H., additional, Hughes, J. P., additional, Infante, L., additional, Irwin, K. D., additional, Jimenez, R., additional, Juin, J. B., additional, Kaul, M., additional, Klein, J., additional, Kosowsky, A., additional, Lau, J. M., additional, Limon, M., additional, Lin, Y.-T., additional, Lupton, R. H., additional, Marriage, T. A., additional, Marsden, D., additional, Martocci, K., additional, Mauskopf, P., additional, Menanteau, F., additional, Moodley, K., additional, Moseley, H., additional, Netterfield, C. B., additional, Niemack, M. D., additional, Nolta, M. R., additional, Page, L. A., additional, Parker, L., additional, Partridge, B., additional, Quintana, H., additional, Reid, B., additional, Sehgal, N., additional, Sievers, J., additional, Spergel, D. N., additional, Staggs, S. T., additional, Stryzak, O., additional, Swetz, D. S., additional, Switzer, E. R., additional, Thornton, R., additional, Trac, H., additional, Tucker, C., additional, Verde, L., additional, Warne, R., additional, Wilson, G., additional, Wollack, E., additional, and Zhao, Y., additional
Published: 2010
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31. THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE 600 < ℓ < 8000 COSMIC MICROWAVE BACKGROUND POWER SPECTRUM AT 148 GHz

Author: Fowler, J. W., primary, Acquaviva, V., additional, Ade, P. A. R., additional, Aguirre, P., additional, Amiri, M., additional, Appel, J. W., additional, Barrientos, L. F., additional, Battistelli, E. S., additional, Bond, J. R., additional, Brown, B., additional, Burger, B., additional, Chervenak, J., additional, Das, S., additional, Devlin, M. J., additional, Dicker, S. R., additional, Doriese, W. B., additional, Dunkley, J., additional, Dünner, R., additional, Essinger-Hileman, T., additional, Fisher, R. P., additional, Hajian, A., additional, Halpern, M., additional, Hasselfield, M., additional, Hernández-Monteagudo, C., additional, Hilton, G. C., additional, Hilton, M., additional, Hincks, A. D., additional, Hlozek, R., additional, Huffenberger, K. M., additional, Hughes, D. H., additional, Hughes, J. P., additional, Infante, L., additional, Irwin, K. D., additional, Jimenez, R., additional, Juin, J. B., additional, Kaul, M., additional, Klein, J., additional, Kosowsky, A., additional, Lau, J. M., additional, Limon, M., additional, Lin, Y.-T., additional, Lupton, R. H., additional, Marriage, T. A., additional, Marsden, D., additional, Martocci, K., additional, Mauskopf, P., additional, Menanteau, F., additional, Moodley, K., additional, Moseley, H., additional, Netterfield, C. B., additional, Niemack, M. D., additional, Nolta, M. R., additional, Page, L. A., additional, Parker, L., additional, Partridge, B., additional, Quintana, H., additional, Reid, B., additional, Sehgal, N., additional, Sievers, J., additional, Spergel, D. N., additional, Staggs, S. T., additional, Swetz, D. S., additional, Switzer, E. R., additional, Thornton, R., additional, Trac, H., additional, Tucker, C., additional, Verde, L., additional, Warne, R., additional, Wilson, G., additional, Wollack, E., additional, and Zhao, Y., additional
Published: 2010
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32. DETECTION OF HOT GAS IN GALAXY GROUPS VIA THE THERMAL SUNYAEV-ZEL'DOVICH EFFECT

Author: Moodley, K., primary, Warne, R., additional, Goheer, N., additional, and Trac, H., additional
Published: 2009
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33. A comparison of hydrodynamic techniques for modelling collisions between main-sequence stars

Author: Trac, H., primary, Sills, A., additional, and Pen, U.-L., additional
Published: 2007
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34. Galaxy catalogs and the diffuse warm gas phase.

Author: Hernandez-Monteagudo, Carlos, primary, Trac, H., additional, Jimenez, Raul, additional, and Verde, Licia, additional
Published: 2007
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35. Dependence of the non-linear mass power spectrum on the equation of state of dark energy

Author: McDonald, P., primary, Trac, H., additional, and Contaldi, C., additional
Published: 2006
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36. A moving frame algorithm for high Mach number hydrodynamics

Author: TRAC, H, primary
Published: 2004
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37. Precision era of the kinetic Sunyaev-Zel'dovich effect: simulations, analytical models and observations and the power to constrain reionization

Author: Zhang, P., primary, Pen, U.-L., additional, and Trac, H., additional
Published: 2004
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38. REIONIZATION ON LARGE SCALES. IV. PREDICTIONS FOR THE 21 cm SIGNAL INCORPORATING THE LIGHT CONE EFFECT.

Author: Plante, P. La, Battaglia, N., Natarajan, A., Peterson, J. B., Trac, H., Cen, R., and Loeb, A.
Subjects: LIGHT cones, BRIGHTNESS temperature, POWER spectra, ANISOTROPY, GALACTIC redshift, METAPHYSICAL cosmology, INTERSTELLAR medium
Abstract: We present predictions for the 21 cm brightness temperature power spectrum during the Epoch of Reionization (EoR). We discuss the implications of the “light cone” effect, which incorporates evolution of the neutral hydrogen fraction and 21 cm brightness temperature along the line of sight. Using a novel method calibrated against radiation-hydrodynamic simulations, we model the neutral hydrogen density field and 21 cm signal in large volumes (L = 2 Gpc h–1). The inclusion of the light cone effect leads to a relative decrease of about 50% in the 21 cm power spectrum on all scales. We also find that the effect is more prominent at the midpoint of reionization and later. The light cone effect can also introduce an anisotropy along the line of sight. By decomposing the 3D power spectrum into components perpendicular to and along the line of sight, we find that in our fiducial reionization model, there is no significant anisotropy. However, parallel modes can contribute up to 40% more power for shorter reionization scenarios. The scales on which the light cone effect is relevant are comparable to scales where one measures the baryon acoustic oscillation. We argue that due to its large comoving scale and introduction of anisotropy, the light cone effect is important when considering redshift space distortions and future application to the Alcock-Paczyński test for the determination of cosmological parameters. [ABSTRACT FROM AUTHOR]
Published: 2014
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39. Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev–Zel’dovich Galaxy Clusters

Author: Eli S. Rykoff, Jo Dunkley, E. Bertin, Ofer Lahav, Nick Battaglia, M. Soares-Santos, Hironao Miyatake, Shannon M. Duff, R. D. Wilkinson, Adriaan J. Duivenvoorden, L. N. da Costa, Joel N. Ullom, Robert Morgan, D. L. Burke, Devin Crichton, Kavilan Moodley, Peter Doel, Alexandra Amon, Edward J. Wollack, N. C. Robertson, H. T. Diehl, Joseph E. Golec, Sunayana Bhargava, Samuel Hinton, Emmanuel Schaan, Enrique Gaztanaga, Megan Gralla, David N. Spergel, Johannes Hubmayr, Simon Dicker, David Bacon, S. Allam, Robert A. Gruendl, Simone Ferraro, C. Aros-Bunster, Felipe Menanteau, G. Gutierrez, Kevin M. Huffenberger, Daniel Thomas, Ramon Miquel, Michael D. Niemack, I. Ferrero, Mathew S. Madhavacheril, J. P. Dietrich, Niall MacCrann, Juan Garcia-Bellido, Tesla E. Jeltema, David J. James, Yanxi Zhang, A. K. Romer, Ben Hoyle, Hy Trac, Mark J. Devlin, Patricio A. Gallardo, J. Gschwend, A. A. Plazas, Brian J. Koopman, Rolando Dünner, Zhilei Xu, Simone Aiola, Behzad Ansarinejad, A. Choi, Jeff McMahon, Eduardo Rozo, Gary Bernstein, K. Honscheid, Michel Aguena, Tanay Bhandarkar, Dan Becker, C. Sifon, Neelima Sehgal, Bhuvnesh Jain, Laura Newburgh, Dongwon Han, F. Paz-Chinchón, J. R. Bond, Kyler Kuehn, Peter Melchior, M. Carrasco Kind, Eve M. Vavagiakis, Steve K. Choi, Suzanne T. Staggs, Paul Giles, R. L. C. Ogando, J. C. Hill, Federico Nati, M. E. C. Swanson, E. V. Denison, Kevin T. Crowley, Tony Mroczkowski, W. G. Hartley, Antonella Palmese, Martine Lokken, S. Kent, Alessandro Schillaci, Masamune Oguri, John P. Hughes, M. A. G. Maia, Maria Salatino, S. Amodeo, T. Shin, S. Adhikari, M. Hasselfield, M. Costanzi, S. I. Loubser, J. Van Lanen, B. Partridge, Sigurd Naess, Adam D. Hincks, J. A. Beall, B. Flaugher, S. M. Simon, Jason E. Austermann, S. P. Ho, John Orlowski-Scherer, M. Smith, Daniel Gruen, J. Martin, D. W. Gerdes, J. Annis, Kenda Knowles, David J. Brooks, Erminia Calabrese, Emilie R. Storer, Gene C. Hilton, Leila R. Vale, Salcedo Romero de Ávila, Phumlani Phakathi, Josh Frieman, Yen-Ting Lin, T. M. C. Abbott, Chun-Hao To, E. J. Sanchez, J. Carretero, E. Suchyta, Matt Hilton, Christopher J. Conselice, Tobias A. Marriage, Sebastian Grandis, A. Carnero Rosell, Agnès Ferté, Anton T. Jaelani, Marcos Lima, S. Everett, S. Serrano, Lyman A. Page, J. De Vicente, Atsushi J. Nishizawa, G. Tarle, UAM. Departamento de Física Teórica, Hilton, M, Sifon, C, Naess, S, Madhavacheril, M, Oguri, M, Rozo, E, Rykoff, E, Adhikari, S, Aguena, M, Aiola, S, Allam, S, Amodeo, S, Amon, A, Annis, J, Ansarinejad, B, Abbott, T, Aros-Bunster, C, Austermann, J, Avila, S, Bacon, D, Battaglia, N, Beall, J, Becker, D, Bernstein, G, Bertin, E, Bhandarkar, T, Bhargava, S, Bond, J, Brooks, D, Burke, D, Calabrese, E, Carrasco Kind, M, Carretero, J, Choi, S, Choi, A, Conselice, C, Da Costa, L, Costanzi, M, Crichton, D, Crowley, K, Dunner, R, Denison, E, Devlin, M, Dicker, S, Diehl, H, Dietrich, J, Doel, P, Duff, S, Duivenvoorden, A, Dunkley, J, Everett, S, Ferraro, S, Ferte, A, Flaugher, B, Frieman, J, Ferrero, I, Gallardo, P, Garcia-Bellido, J, Gaztanaga, E, Giles, P, Golec, J, Gralla, M, Grandis, S, Gruen, D, Gerdes, D, Gruendl, R, Gschwend, J, Gutierrez, G, Han, D, Hartley, W, Hasselfield, M, Hill, J, Hilton, G, Hincks, A, Hinton, S, Ho, S, Honscheid, K, Hoyle, B, Hubmayr, J, Huffenberger, K, Hughes, J, Jaelani, A, Jain, B, James, D, Jeltema, T, Kent, S, Knowles, K, Koopman, B, Kuehn, K, Lahav, O, Lima, M, Lin, Y, Lokken, M, Loubser, S, Maccrann, N, Maia, M, Marriage, T, Martin, J, Mcmahon, J, Melchior, P, Menanteau, F, Miquel, R, Moodley, K, Morgan, R, Mroczkowski, T, Nati, F, Newburgh, L, Niemack, M, Nishizawa, A, Miyatake, H, Ogando, R, Orlowski-Scherer, J, Page, L, Palmese, A, Partridge, B, Paz-Chinchon, F, Phakathi, P, Plazas, A, Robertson, N, Romer, A, Carnero Rosell, A, Sanchez, E, Schaan, E, Schillaci, A, Sehgal, N, Serrano, S, Shin, T, Simon, S, Smith, M, Salatino, M, Soares-Santos, M, Spergel, D, Staggs, S, Storer, E, Suchyta, E, Swanson, M, Tarle, G, Thomas, D, To, C, Trac, H, Ullom, J, Vale, L, Van Lanen, J, Vavagiakis, E, De Vicente, J, Wilkinson, R, Wollack, E, Xu, Z, Zhan, Y, Hilton, M., Sifón, C., Naess, S., Madhavacheril, M., Oguri, M., Rozo, E., Rykoff, E., Abbott, T. M. C., Adhikari, S., Aguena, M., Aiola, S., Allam, S., Amodeo, S., Amon, A., Annis, J., Ansarinejad, B., Aros-Bunster, C., Austermann, J. E., Avila, S., Bacon, D., Battaglia, N., Beall, J. A., Becker, D. T., Bernstein, G. M., Bertin, E., Bhandarkar, T., Bhargava, S., Bond, J. R., Brooks, D., Burke, D. L., Calabrese, E., Carretero, J., Choi, S. K., Choi, A., Conselice, C., da Costa, L. N., Costanzi, M., Crichton, D., Crowley, K. T., Dünner, R., Denison, E. V., Devlin, M. J., Dicker, S. R., Diehl, H. T., Dietrich, J. P., Doel, P., Duff, S. M., Duivenvoorden, A. J., Dunkley, J., Everett, S., Ferraro, S., Ferrero, I., Ferté, A., Flaugher, B., Frieman, J., Gallardo, P. A., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giles, P., Golec, J. E., Gralla, M. B., Grandis, S., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Han, D., Hartley, W. G., Hasselfield, M., Hill, J. C., Hilton, G. C., Hincks, A. D., Hinton, S. R., S-P. P., Ho, Honscheid, K., Hoyle, B., Hubmayr, J., Huffenberger, K. M., Hughes, J. P., Jaelani, A. T., Jain, B., James, D. J., Jeltema, T., Kent, S., Carrasco Kind, M., Knowles, K., Koopman, B. J., Kuehn, K., Lahav, O., Lima, M., Lin, Y-T., Lokken, M., Loubser, S. I., Maccrann, N., Maia, M. A. G., Marriage, T. A., Martin, J., Mcmahon, J., Melchior, P., Menanteau, F., Miquel, R., Miyatake, H., Moodley, K., Morgan, R., Mroczkowski, T., Nati, F., Newburgh, L. B., Niemack, M. D., Nishizawa, A. J., Ogando, R. L. C., Orlowski-Scherer, J., Page, L. A., Palmese, A., Partridge, B., Paz-Chinchón, F., Phakathi, P., Plazas, A. A., Robertson, N. C., Romer, A. K., Carnero Rosell, A., Salatino, M., Sanchez, E., Schaan, E., Schillaci, A., Sehgal, N., Serrano, S., Shin, T., Simon, S. M., Smith, M., Soares-Santos, M., Spergel, D. N., Staggs, S. T., Storer, E. R., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Trac, H., Ullom, J. N., Vale, L. R., Van Lanen, J., Vavagiakis, E. M., De Vicente, J., Wilkinson, R. D., Wollack, E. J., Xu, Z., and Zhang, Y.
Subjects: Galaxy clusters, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Cosmology, Large-scale structure of the universe, Astrophysics - Cosmology and Nongalactic Astrophysics, Intracluster medium, 0103 physical sciences, Cluster (physics), Sunyaev-Zeldovich Effect, 010303 astronomy & astrophysics, Cosmology, Galaxy clusters, Galaxy cluster, Astrophysics::Galaxy Astrophysics, AGLOMERADOS (GALÁXIA), Physics, 010308 nuclear & particles physics, Star formation, Física, Astronomy and Astrophysics, XMM-newton Telescope, Galaxies, Galaxy, Redshift, Space and Planetary Science, Atacama Cosmology Telescope
Abstract: Hilton, M., et al., We present a catalog of 4195 optically confirmed Sunyaev–Zel’dovich (SZ) selected galaxy clusters detected with signal-to-noise ratio >4 in 13,211 deg of sky surveyed by the Atacama Cosmology Telescope (ACT). Cluster candidates were selected by applying a multifrequency matched filter to 98 and 150 GHz maps constructed from ACT observations obtained from 2008 to 2018 and confirmed using deep, wide-area optical surveys. The clusters span the redshift range 0.04 < z < 1.91 (median z = 0.52). The catalog contains 222 z > 1 clusters, and a total of 868 systems are new discoveries. Assuming an SZ signal versus mass-scaling relation calibrated from X-ray observations, the sample has a 90% completeness mass limit of M > 3.8 × 10 M, evaluated at z = 0.5, for clusters detected at signal-to-noise ratio >5 in maps filtered at an angular scale of 2 4. The survey has a large overlap with deep optical weak-lensing surveys that are being used to calibrate the SZ signal mass-scaling relation, such as the Dark Energy Survey (4566 deg), the Hyper Suprime-Cam Subaru Strategic Program (469 deg), and the Kilo Degree Survey (825 deg). We highlight some noteworthy objects in the sample, including potentially projected systems, clusters with strong lensing features, clusters with active central galaxies or star formation, and systems of multiple clusters that may be physically associated. The cluster catalog will be a useful resource for future cosmological analyses and studying the evolution of the intracluster medium and galaxies in massive clusters over the past 10 Gyr., The DES Data Management System is supported by the NSF under Grant Nos. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Unionʼs Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2).
Published: 2021

40. The Atacama Cosmology Telescope: DR4 maps and cosmological parameters

Author: Simone Aiola, Suzanne T. Staggs, C. Sifon, J. Richard Bond, Martine Lokken, Bruce Partridge, Brittany Fuzia, Giampaolo Pisano, Matthew Hasselfield, Vincent Lakey, Shannon M. Duff, H. M. Cho, Naomi Robertson, Brandon S. Hensley, Laura Newburgh, Alexander van Engelen, Jesus Rivera, Kirsten Hall, Matt Hilton, Susan E. Clark, Kavilan Moodley, Rachel Bean, Kent D. Irwin, David Alonso, Andrina Nicola, Edward J. Wollack, Mathew S. Madhavacheril, Dhaneshwar D. Sunder, Brian J. Koopman, David N. Spergel, Rolando Dünner, Jakob M. Helton, Toshiya Namikawa, Zhilei Xu, Sigurd Naess, Leopoldo Infante, Adam D. Hincks, Emily Grace, Renée Hložek, Ningfeng Zhu, Felipe Rojas, Jeff McMahon, Grace E. Chesmore, Jacob Klein, Max Fankhanel, Frank J. Qu, Heather Prince, S. Henderson, Yaqiong Li, Timothy D. Morton, Dale Li, Jason E. Austermann, E. V. Denison, Jason R. Stevens, Robert Thornton, Kenda Knowles, Christine G. Pappas, Amanda MacInnis, Yuhan Wang, Joseph E. Golec, Precious Sikhosana, Adriaan J. Duivenvoorden, Neelima Sehgal, John P. Hughes, Felipe Maldonado, Eve M. Vavagiakis, Peter Charles Hargrave, Sarah Marie Bruno, Michael R. Nolta, Zack Li, Dongwon Han, John P. Nibarger, Sara M. Simon, Jon Sievers, Kasey Wagoner, Blake D. Sherwin, J. Colin Hill, Lyman A. Page, Thibaut Louis, John Orlowski-Sherer, Fernando Zago, Arthur Kosowsky, Benjamin L. Schmitt, Carlos Sierra, Felipe Menanteau, Loïc Maurin, B. Thorne, Vera Gluscevic, Eric R. Switzer, Kevin M. Huffenberger, Marius Lungu, Jo Dunkley, Emilie R. Storer, Felipe Carrero, Gene C. Hilton, Maya Mallaby-Kay, Steve K. Choi, Roberto Puddu, Phumlani Phakathi, Jeff Van Lanen, Jonathan T. Ward, Omar Darwish, Yilun Guan, Maria Salatino, Daniel T. Becker, Anna E. Fox, James A. Beall, Kevin T. Crowley, Federico Nati, Carole Tucker, Alessandro Schillaci, Graeme E. Addison, Shuay-Pwu Patty Ho, Elio Angile, S. Amodeo, Erminia Calabrese, Leila R. Vale, Megan Gralla, Mandana Amiri, Nick Battaglia, Rahul Datta, Peter A. R. Ade, Devin Crichton, Michael D. Niemack, Nicholas F. Cothard, Victoria Calafut, Jesse Treu, Thomas Essinger-Hileman, Cody J. Duell, Luis E. Campusano, Danica Marsden, Rebecca Jackson, Emmanuel Schaan, Johannes Hubmayr, Mark Halpern, Simone Ferraro, Hy Trac, Mark J. Devlin, Patricio A. Gallardo, Maximilian H. Abitbol, Taylor Baildon, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), ACT, Aiola, S, Calabrese, E, Maurin, L, Naess, S, Schmitt, B, Abitbol, M, Addison, G, Ade, P, Alonso, D, Amiri, M, Amodeo, S, Angile, E, Austermann, J, Baildon, T, Battaglia, N, Beall, J, Bean, R, Becker, D, Richard Bond, J, Bruno, S, Calafut, V, Campusano, L, Carrero, F, Chesmore, G, Cho, H, Choi, S, Clark, S, Cothard, N, Crichton, D, Crowley, K, Darwish, O, Datta, R, Denison, E, Devlin, M, Duell, C, Duff, S, Duivenvoorden, A, Dunkley, J, Dunner, R, Essinger-Hileman, T, Fankhanel, M, Ferraro, S, Fox, A, Fuzia, B, Gallardo, P, Gluscevic, V, Golec, J, Grace, E, Gralla, M, Guan, Y, Hall, K, Halpern, M, Han, D, Hargrave, P, Hasselfield, M, Helton, J, Henderson, S, Hensley, B, Colin Hill, J, Hilton, G, Hilton, M, Hincks, A, Hlozek, R, Ho, S, Hubmayr, J, Huffenberger, K, Hughes, J, Infante, L, Irwin, K, Jackson, R, Klein, J, Knowles, K, Koopman, B, Kosowsky, A, Lakey, V, Li, D, Li, Y, Li, Z, Lokken, M, Louis, T, Lungu, M, Macinnis, A, Madhavacheril, M, Maldonado, F, Mallaby-Kay, M, Marsden, D, Mcmahon, J, Menanteau, F, Moodley, K, Morton, T, Namikawa, T, Nati, F, Newburgh, L, Nibarger, J, Nicola, A, Niemack, M, Nolta, M, Orlowski-Sherer, J, Page, L, Pappas, C, Partridge, B, Phakathi, P, Pisano, G, Prince, H, Puddu, R, Qu, F, Rivera, J, Robertson, N, Rojas, F, Salatino, M, Schaan, E, Schillaci, A, Sehgal, N, Sherwin, B, Sierra, C, Sievers, J, Sifon, C, Sikhosana, P, Simon, S, Spergel, D, Staggs, S, Stevens, J, Storer, E, Sunder, D, Switzer, E, Thorne, B, Thornton, R, Trac, H, Treu, J, Tucker, C, Vale, L, van Engelen, A, van Lanen, J, Vavagiakis, E, Wagoner, K, Wang, Y, Ward, J, Wollack, E, Xu, Z, Zago, F, and Zhu, N
Subjects: CMBR polarisation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmic microwave background, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Cosmology, symbols.namesake, 0103 physical sciences, CMBR experiments, Planck, Physics, Spectral index, 010308 nuclear & particles physics, Spectral density, Astronomy and Astrophysics, CMB cold spot, Baryon, Cosmological parameters from CMBR, 13. Climate action, Atacama Cosmology Telescope, symbols, CMBR experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present new arcminute-resolution maps of the Cosmic Microwave Background temperature and polarization anisotropy from the Atacama Cosmology Telescope, using data taken from 2013-2016 at 98 and 150 GHz. The maps cover more than 17,000 deg$^2$, the deepest 600 deg$^2$ with noise levels below 10 $\mu$K-arcmin. We use the power spectrum derived from almost 6,000 deg$^2$ of these maps to constrain cosmology. The ACT data enable a measurement of the angular scale of features in both the divergence-like polarization and the temperature anisotropy, tracing both the velocity and density at last-scattering. From these one can derive the distance to the last-scattering surface and thus infer the local expansion rate, $H_0$. By combining ACT data with large-scale information from WMAP we measure $H_0 = 67.6 \pm 1.1$ km/s/Mpc, at 68% confidence, in excellent agreement with the independently-measured Planck satellite estimate (from ACT alone we find $H_0 = 67.9 \pm 1.5$ km/s/Mpc). The $\Lambda$CDM model provides a good fit to the ACT data, and we find no evidence for deviations: both the spatial curvature, and the departure from the standard lensing signal in the spectrum, are zero to within 1$\sigma$; the number of relativistic species, the primordial Helium fraction, and the running of the spectral index are consistent with $\Lambda$CDM predictions to within $1.5 - 2.2\sigma$. We compare ACT, WMAP, and Planck at the parameter level and find good consistency; we investigate how the constraints on the correlated spectral index and baryon density parameters readjust when adding CMB large-scale information that ACT does not measure. The DR4 products presented here will be publicly released on the NASA Legacy Archive for Microwave Background Data Analysis., Comment: 33 pages, 24 figures, products available on the NASA LAMBDA website, version accepted for publication in JCAP
Published: 2020
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41. A Model-Insensitive Baryon Acoustic Oscillation Feature in the 21 cm Signal from Reionization

Author: Matthew McQuinn, Vid Iršič, Anson D'Aloisio, Christopher Cain, Hy Trac, Cain, C [0000-0001-9420-7384], Iršič, V [0000-0002-5445-461X], Trac, H [0000-0001-6778-3861], and Apollo - University of Cambridge Repository
Subjects: Observational cosmology, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010504 meteorology & atmospheric sciences, Population, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Reionization, 0103 physical sciences, education, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Intergalactic medium, Physics, education.field_of_study, Star formation, Spectral density, Astronomy and Astrophysics, Baryon, Amplitude, Orders of magnitude (time), Space and Planetary Science, Intergalactic travel, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We examine the impact of baryon-dark matter relative velocities on intergalactic small-scale structure and the 21 cm signal during reionization. Streaming velocities reduced clumping in the intergalactic medium (IGM) on mass scales of $\sim 10^4 - 10^8$ M$_{\odot}$. This effect produced a distinct baryon acoustic oscillation (BAO) feature in the 21 cm power spectrum at wave numbers $k\sim 0.1$ h/Mpc, near which forthcoming surveys will be most sensitive. In contrast to the highly uncertain impact of streaming velocities on star formation, the effect on clumping is better constrained because it is set mainly by cosmology and straightforward gas dynamics. We quantify the latter using coupled radiation-hydrodynamic simulations that capture the Jeans scale of pre-reionization gas. The clumping factor of ionized gas is reduced by 5-10\% in regions with RMS streaming velocities. The suppression peaks $\approx 5$ Myr after a region is reionized, but disappears within 200 Myr due to pressure smoothing. We model the corresponding impact on the 21 cm signal and find that the BAO feature is most likely to appear at $\approx$ 10 \% ionization. During this phase, the feature may appear at the 1 \% (5 \%) level at $k \sim 0.1 (0.06)$ h/Mpc with an amplitude that varies by a factor of $< 10$ across a range of reionization histories. We also provide a model for the signal originating from streaming velocity's impact on ionizing sources, which can vary by 4 orders of magnitude depending on highly uncertain source properties. We find that the clumping signal probably dominates the source one unless Population III star formation in $10^6 - 10^8$ M$_{\odot}$ halos contributed significantly to the first 10\% of reionization., 28 pages, 12 figures
Published: 2020

42. The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz

Author: Kavilan Moodley, Emilie R. Storer, Simone Aiola, Phumlani Phakathi, Jeff Van Lanen, E. Grace, Stefania Amodeo, Felipe Rojas, Yaqiong Li, Nick Battaglia, Precious Sikhosana, Suzanne T. Staggs, Vera Gluscevic, Robert Thornton, Benjamin L. Schmitt, Christine G. Pappas, Rolando Dünner, Danica Marsden, Yilun Guan, Felipe Carrero, Blake D. Sherwin, Sigurd Naess, Leopoldo Infante, Adam D. Hincks, Toshiya Namikawa, Zhilei Xu, Brittany Fuzia, Graeme E. Addison, Kasey Wagoner, Daniel T. Becker, J. Richard Bond, Jason E. Austermann, Sarah Marie Bruno, Matthew Hasselfield, Naomi Robertson, Jesse Treu, Vincent Lakey, John P. Nibarger, Timothy D. Morton, Sara M. Simon, David N. Spergel, Jesus Rivera, Michael R. Nolta, Zack Li, Shawn W. Henderson, Max Fankhanel, Martine Lokken, B. Thorne, Mark J. Devlin, Thomas Essinger-Hileman, James A. Beall, Yuhan Wang, Kevin T. Crowley, John Orlowski-Sherer, Bruce Partridge, Adriaan J. Duivenvoorden, Laura Newburgh, Grace E. Chesmore, Alessandro Schillaci, Jon Sievers, Dhaneshwar D. Sunder, Federico Nati, Rahul Datta, Dale Li, Shuay-Pwu Patty Ho, Shannon M. Duff, Edward V. Denison, Peter A. R. Ade, Mathew S. Madhavacheril, Maya Mallaby-Kay, Erminia Calabrese, Roberto Puddu, J. Colin Hill, Elio Angile, Jo Dunkley, Omar Darwish, Kenda Knowles, Marius Lungu, Megan Gralla, Susan E. Clark, Jeff Klein, Fernando Zago, Dongwon Han, Brandon S. Hensley, Devin Crichton, Renée Hložek, Peter Charles Hargrave, Frank J. Qu, Neelima Sehgal, Leila R. Vale, Matt Hilton, Gene C. Hilton, Joseph E. Golec, Heather Prince, Mandana Amiri, Alexander van Engelen, Maria Salatino, Loïc Maurin, Andrina Nicola, Lyman A. Page, Thibaut Louis, Steve K. Choi, Michael D. Niemack, Eve M. Vavagiakis, Nicholas F. Cothard, Victoria Calafut, Jonathan T. Ward, Carole Tucker, Arthur Kosowsky, Kevin M. Huffenberger, Kent D. Irwin, Hsiao-Mei Cho, Edward J. Wollack, Anna E. Fox, Ningfeng Zhu, Amanda MacInnis, Felipe Maldonado, Brian J. Koopman, Jeff McMahon, Cristóbal Sifón, Emmanuel Schaan, Johannes Hubmayr, Mark Halpern, Simone Ferraro, Hy Trac, Patricio A. Gallardo, Maximilian H. Abitbol, Taylor Baildon, Luis E. Campusano, Rebecca Jackson, Carlos Sierra, Felipe Menanteau, Jason R. Stevens, John P. Hughes, Cody J. Duell, Eric R. Switzer, Kirsten Hall, Rachel Bean, David Alonso, Choi, S, Hasselfield, M, Ho, S, Koopman, B, Lungu, M, Abitbol, M, Addison, G, Ade, P, Aiola, S, Alonso, D, Amiri, M, Amodeo, S, Angile, E, Austermann, J, Baildon, T, Battaglia, N, Beall, J, Bean, R, Becker, D, Richard Bond, J, Bruno, S, Calabrese, E, Calafut, V, Campusano, L, Carrero, F, Chesmore, G, Cho, H, Clark, S, Cothard, N, Crichton, D, Crowley, K, Darwish, O, Datta, R, Denison, E, Devlin, M, Duell, C, Duff, S, Duivenvoorden, A, Dunkley, J, Dunner, R, Essinger-Hileman, T, Fankhanel, M, Ferraro, S, Fox, A, Fuzia, B, Gallardo, P, Gluscevic, V, Golec, J, Grace, E, Gralla, M, Guan, Y, Hall, K, Halpern, M, Han, D, Hargrave, P, Henderson, S, Hensley, B, Colin Hill, J, Hilton, G, Hilton, M, Hincks, A, Hlozek, R, Hubmayr, J, Huffenberger, K, Hughes, J, Infante, L, Irwin, K, Jackson, R, Klein, J, Knowles, K, Kosowsky, A, Lakey, V, Li, D, Li, Y, Li, Z, Lokken, M, Louis, T, Macinnis, A, Madhavacheril, M, Maldonado, F, Mallaby-Kay, M, Marsden, D, Maurin, L, Mcmahon, J, Menanteau, F, Moodley, K, Morton, T, Naess, S, Namikawa, T, Nati, F, Newburgh, L, Nibarger, J, Nicola, A, Niemack, M, Nolta, M, Orlowski-Sherer, J, Page, L, Pappas, C, Partridge, B, Phakathi, P, Prince, H, Puddu, R, Qu, F, Rivera, J, Robertson, N, Rojas, F, Salatino, M, Schaan, E, Schillaci, A, Schmitt, B, Sehgal, N, Sherwin, B, Sierra, C, Sievers, J, Sifon, C, Sikhosana, P, Simon, S, Spergel, D, Staggs, S, Stevens, J, Storer, E, Sunder, D, Switzer, E, Thorne, B, Thornton, R, Trac, H, Treu, J, Tucker, C, Vale, L, van Engelen, A, van Lanen, J, Vavagiakis, E, Wagoner, K, Wang, Y, Ward, J, Wollack, E, Xu, Z, Zago, F, Zhu, N, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), and ACT
Subjects: Physics, CMBR polarisation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010308 nuclear & particles physics, Cosmic microwave background, Library science, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Cosmological parameters from CMBR, 0103 physical sciences, Atacama Cosmology Telescope, CMBR experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the temperature and polarization angular power spectra of the CMB measured by the Atacama Cosmology Telescope (ACT) from 5400 deg$^2$ of the 2013-2016 survey, which covers $>$15000 deg$^2$ at 98 and 150 GHz. For this analysis we adopt a blinding strategy to help avoid confirmation bias and, related to this, show numerous checks for systematic error done before unblinding. Using the likelihood for the cosmological analysis we constrain secondary sources of anisotropy and foreground emission, and derive a "CMB-only" spectrum that extends to $\ell=4000$. At large angular scales, foreground emission at 150 GHz is $\sim$1% of TT and EE within our selected regions and consistent with that found by Planck. Using the same likelihood, we obtain the cosmological parameters for $\Lambda$CDM for the ACT data alone with a prior on the optical depth of $\tau=0.065\pm0.015$. $\Lambda$CDM is a good fit. The best-fit model has a reduced $\chi^2$ of 1.07 (PTE=0.07) with $H_0=67.9\pm1.5$ km/s/Mpc. We show that the lensing BB signal is consistent with $\Lambda$CDM and limit the celestial EB polarization angle to $\psi_P =-0.07^{\circ}\pm0.09^{\circ}$. We directly cross correlate ACT with Planck and observe generally good agreement but with some discrepancies in TE. All data on which this analysis is based will be publicly released., Comment: 44 pages, 27 figures, products available on the NASA LAMBDA website, version accepted for publication in JCAP
Published: 2020
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43. Hydrodynamic Response of the Intergalactic Medium to Reionization

Author: Christopher Cain, Andrei Mesinger, Hy Trac, Anson D'Aloisio, Matthew McQuinn, D'Aloisio, A., Mcquinn, M., Trac, H., Cain, C., and Mesinger, A.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Photon, Cosmic web, 010504 meteorology & atmospheric sciences, Mean free path, FOS: Physical sciences, Hydrodynamical simulation, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Approx, 01 natural sciences, Reionization, Radiative transfer simulation, Settore FIS/05 - Astronomia e Astrofisica, Ionization, 0103 physical sciences, Astrophysics - Cosmology and Nongalactic Astrophysic, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Intergalactic medium, 0105 earth and related environmental sciences, Physics, Astronomy and Astrophysics, Plasma, Astrophysics - Astrophysics of Galaxies, Redshift, 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Intensity (heat transfer), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The intergalactic medium is expected to clump on scales down to $10^4-10^8$ M$_{\odot}$ before the onset of reionization. The impact of these small-scale structures on reionization is poorly understood despite the modern understanding that gas clumpiness limits the growth of H II regions. We use a suite of radiation-hydrodynamics simulations that capture the $\sim 10^4$ $M_\odot$ Jeans mass of unheated gas to study density fluctuations during reionization. Our simulations track the complex ionization and hydrodynamical response of gas in the wake of ionization fronts. The clumping factor of ionized gas (proportional to the recombination rate) rises to a peak value of $5-20$ approximately $\Delta t = 10$ Myr after ionization front passage, depending on the incident intensity, redshift, and degree to which the gas had been pre-heated by the first X-ray sources. The clumping factor reaches its relaxed value of $\approx 3$ by $\Delta t = 300$ Myr. The mean free path of Lyman-limit photons evolves in unison, being up to several times shorter in un-relaxed, recently reionized regions compared to those that were reionized much earlier. Assessing the impact of this response on the global reionizaton process, we find that un-relaxed gaseous structures boost the total number of recombinations by $\approx 50$ % and lead to spatial fluctuations in the mean free path that persist appreciably for several hundred million years after the completion of reionization., Comment: Matches published version
Published: 2020
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44. The Atacama Cosmology Telescope: The Two-season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog

Author: Kavilan Moodley, David N. Spergel, Rolando Dünner, Simone Aiola, Kevin M. Huffenberger, Federico Nati, Mathew S. Madhavacheril, Laura Newburgh, Eve M. Vavagiakis, Sigurd Naess, Adam D. Hincks, Thibaut Louis, Loïc Maurin, Tobias A. Marriage, Matthew Hasselfield, Suzanne T. Staggs, Benjamin L. Schmitt, Bruce Partridge, S. P. Ho, Megan Gralla, Brian J. Koopman, Edward J. Wollack, Nicholas Battaglia, Jeff McMahon, J. Richard Bond, Joanna Dunkley, V. Bharadwaj, Lyman A. Page, Masamune Oguri, Michael D. Niemack, Rahul Datta, Devin Crichton, Steve K. Choi, Matt Hilton, Alexander van Engelen, John P. Hughes, Arthur Kosowsky, Hironao Miyatake, Johannes Hubmayr, Hy Trac, Mark J. Devlin, Patricio A. Gallardo, Cristóbal Sifón, Jon Sievers, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), ACT, Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Hilton, M, Hasselfield, M, Sifón, C, Battaglia, N, Aiola, S, Bharadwaj, V, Bond, J, Choi, S, Crichton, D, Datta, R, Devlin, M, Dunkley, J, Dünner, R, Gallardo, P, Gralla, M, Hincks, A, Ho, S, Hubmayr, J, Huffenberger, K, Hughes, J, Koopman, B, Kosowsky, A, Louis, T, Madhavacheril, M, Marriage, T, Maurin, L, Mcmahon, J, Miyatake, H, Moodley, K, Næss, S, Nati, F, Newburgh, L, Niemack, M, Oguri, M, Page, L, Partridge, B, Schmitt, B, Sievers, J, Spergel, D, Staggs, S, Trac, H, Engelen, A, Vavagiakis, E, and Wollack, E
Subjects: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), 010308 nuclear & particles physics, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Cosmic Microwave Background, Atacama Cosmology Telescope, Sunyaev–Zel’dovich Effect, Cluster Catalog, cosmology: large-scale structure of universe, FOS: Physical sciences, Library science, Astronomy and Astrophysics, 01 natural sciences, Square kilometre array, Space and Planetary Science, galaxies: clusters: general, cosmology: observations, 0103 physical sciences, Atacama Cosmology Telescope, Christian ministry, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a catalog of 182 galaxy clusters detected through the Sunyaev-Zel'dovich effect by the Atacama Cosmology Telescope in a contiguous 987.5 deg$^{2}$ field. The clusters were detected as SZ decrements by applying a matched filter to 148 GHz maps that combine the original ACT equatorial survey with data from the first two observing seasons using the ACTPol receiver. Optical/IR confirmation and redshift measurements come from a combination of large public surveys and our own follow-up observations. Where necessary, we measured photometric redshifts for clusters using a pipeline that achieves accuracy $��z/(1 + z)=0.015$ when tested on SDSS data. Under the assumption that clusters can be described by the so-called Universal Pressure Profile and its associated mass-scaling law, the full signal-to-noise > 4 sample spans the mass range $1.6 < M^{\rm UPP}_{\rm 500c}/10^{14}{\rm M}_{\odot} 4 \times 10^{14}$ M$_{\odot}$ is consistent with the number of such clusters found in the South Pole Telescope SZ survey., Accepted for publication in ApJS; 38 pages, 31 figures; a .fits table that combines tables A1-A3 is available from https://acru.ukzn.ac.za/~mjh/ACTPol_E-D56Catalog (and will be posted on LAMBDA soon)
Published: 2018
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45. The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters

Author: Brian J. Koopman, Jeff McMahon, Kavilan Moodley, Joanna Dunkley, Felipe Menanteau, David N. Spergel, Simon Muya Kasanda, Jesse Treu, Graeme E. Addison, J. Richard Bond, Shawn W. Henderson, Sara M. Simon, Simone Aiola, John P. Hughes, Matt Hilton, Joseph W. Britton, Alexander van Engelen, Tobias A. Marriage, Jonathan T. Ward, Robert Thornton, Michael R. Nolta, Christine G. Pappas, Rahul Datta, Peter A. R. Ade, Gene C. Hilton, Jeff Klein, Nicholas Battaglia, Mathew S. Madhavacheril, Matthew Hasselfield, Arthur Kosowsky, Benjamin L. Schmitt, Devin Crichton, Charles Munson, Thibaut Louis, Zhiqi Huang, Erminia Calabrese, Kevin Coughlin, Francesco De Bernardis, Neelima Sehgal, Megan Gralla, Kent D. Irwin, Hsiao-Mei Cho, J. Colin Hill, Edward J. Wollack, Michael D. Niemack, Steve K. Choi, Loïc Maurin, Lyman A. Page, Suzanne T. Staggs, S. P. Patty Ho, Federico Nati, Mandana Amiri, Kevin M. Huffenberger, Emmanuel Schaan, Johannes Hubmayr, Eric R. Switzer, Elio Angile, Mark Halpern, Simone Ferraro, James A. Beall, Kevin T. Crowley, Hy Trac, Mark J. Devlin, Patricio A. Gallardo, R. Allison, Simon Dicker, Sigurd Naess, Leopoldo Infante, Laura Newburgh, Dale Li, Adam D. Hincks, Carole Tucker, Bruce Partridge, Anna E. Fox, Jon Sievers, Renée Hlozek, E. Grace, Felipe Rojas, Rolando Dünner, John P. Nibarger, Marius Lungu, Carolina Núñez, Blake D. Sherwin, Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), ACTPol, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Louis, T, Grace, E, Hasselfield, M, Lungu, M, Maurin, L, Addison, G, Ade, P, Aiola, S, Allison, R, Amiri, M, Angile, E, Battaglia, N, Beall, J, De Bernardis, F, Bond, J, Britton, J, Calabrese, E, Cho, H, Choi, S, Coughlin, K, Crichton, D, Crowley, K, Datta, R, Devlin, M, Dicker, S, Dunkley, J, Dünner, R, Ferraro, S, Fox, A, Gallardo, P, Gralla, M, Halpern, M, Henderson, S, Hill, J, Hilton, G, Hilton, M, Hincks, A, Hlozek, R, Patty Ho, S, Huang, Z, Hubmayr, J, Huffenberger, K, Hughes, J, Infante, L, Irwin, K, Kasanda, S, Klein, J, Koopman, B, Kosowsky, A, Li, D, Madhavacheril, M, Marriage, T, Mcmahon, J, Menanteau, F, Moodley, K, Munson, C, Naess, S, Nati, F, Newburgh, L, Nibarger, J, Niemack, M, Nolta, M, Nuñez, C, Page, L, Pappas, C, Partridge, B, Rojas, F, Schaan, E, Schmitt, B, Sehgal, N, Sherwin, B, Sievers, J, Simon, S, Spergel, D, Staggs, S, Switzer, E, Thornton, R, Trac, H, Treu, J, Tucker, C, Engelen, A, Ward, J, and Wollack, E
Subjects: cosmological model, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astrophysics, 7. Clean energy, 01 natural sciences, Atomic, Particle and Plasma Physics, CMBR experiments, 010303 astronomy & astrophysics, QC, media_common, QB, helium: primordial, Physics, Hubble constant, Celestial equator, Astrophysics::Instrumentation and Methods for Astrophysics, cosmological parameters from CMBR, Planck temperature, CMB cold spot, Nuclear & Particles Physics, Atacama Cosmology Telescope, symbols, astro-ph.CO, power spectrum: angular dependence, Astrophysics::Earth and Planetary Astrophysics, Neutrino, CMBR experiment, Astronomical and Space Sciences, Astrophysics - Cosmology and Nongalactic Astrophysics, CMBR polarisation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), satellite: Planck, media_common.quotation_subject, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, symbols.namesake, 0103 physical sciences, Nuclear, Planck, Astrophysics::Galaxy Astrophysics, beam: polarization, 010308 nuclear & particles physics, baryon: density, Molecular, Astronomy and Astrophysics, 13. Climate action, Sky, WMAP, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Hubble's law
Abstract: We present the temperature and polarization angular power spectra measured by the Atacama Cosmology Telescope Polarimeter (ACTPol). We analyze night-time data collected during 2013-14 using two detector arrays at 149 GHz, from 548 deg$^2$ of sky on the celestial equator. We use these spectra, and the spectra measured with the MBAC camera on ACT from 2008-10, in combination with Planck and WMAP data to estimate cosmological parameters from the temperature, polarization, and temperature-polarization cross-correlations. We find the new ACTPol data to be consistent with the LCDM model. The ACTPol temperature-polarization cross-spectrum now provides stronger constraints on multiple parameters than the ACTPol temperature spectrum, including the baryon density, the acoustic peak angular scale, and the derived Hubble constant. Adding the new data to planck temperature data tightens the limits on damping tail parameters, for example reducing the joint uncertainty on the number of neutrino species and the primordial helium fraction by 20%., 23 pages, 25 figures
Published: 2017
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46. Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel’dovich measurements from BOSS CMASS and LOWZ halos

Author: Schaan, Emmanuel, Ferraro, Simone, Amodeo, Stefania, Battaglia, Nick, Aiola, Simone, Austermann, Jason E., Beall, James A., Bean, Rachel, Becker, Daniel T., Bond, Richard J., Calabrese, Erminia, Calafut, Victoria, Choi, Steve K., Denison, Edward V., Devlin, Mark J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Gallardo, Patricio A., Guan, Yilun, Han, Dongwon, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hložek, Renée, Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Koopman, Brian J., MacInnis, Amanda, McMahon, Jeff, Madhavacheril, Mathew S., Moodley, Kavilan, Mroczkowski, Tony, Naess, Sigurd, Nati, Federico, Newburgh, Laura B., Niemack, Michael D., Page, Lyman A., Partridge, Bruce, Salatino, Maria, Sehgal, Neelima, Schillaci, Alessandro, Sifón, Cristóbal, Smith, Kendrick M., Spergel, David N., Staggs, Suzanne, Storer, Emilie R., Trac, Hy, Page, A., Ullom, Joel N., Van Lanen, Jeff, R. Vale, Leila, van Engelen, Alexander, Vargas Magaña, Mariana, M. Vavagiakis, Eve, Wollack, Edward J., Xu, Zhilei, Schaan, E, Ferraro, S, Amodeo, S, Battaglia, N, Aiola, S, Austermann, J, Beall, J, Bean, R, Becker, D, Bond, R, Calabrese, E, Calafut, V, Choi, S, Denison, E, Devlin, M, Duff, S, Duivenvoorden, A, Dunkley, J, Dunner, R, Gallardo, P, Guan, Y, Han, D, Hill, J, Hilton, G, Hilton, M, Hlozek, R, Hubmayr, J, Huffenberger, K, Hughes, J, Koopman, B, Macinnis, A, Mcmahon, J, Madhavacheril, M, Moodley, K, Mroczkowski, T, Naess, S, Nati, F, Newburgh, L, Niemack, M, Page, L, Partridge, B, Salatino, M, Sehgal, N, Schillaci, A, Sifon, C, Smith, K, Spergel, D, Staggs, S, Storer, E, Trac, H, Ullom, J, Van Lanen, J, Vale, L, Van Engelen, A, Magana, M, Vavagiakis, E, Wollack, E, and Xu, Z
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.GA, Cosmic microwave background, FOS: Physical sciences, High resolution, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, CMB, 01 natural sciences, Atomic, symbols.namesake, Particle and Plasma Physics, 0103 physical sciences, Nuclear, Planck, 010306 general physics, Astrophysics::Galaxy Astrophysics, Physics, Quantum Physics, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Molecular, Astrophysics - Astrophysics of Galaxies, Nuclear & Particles Physics, Redshift, Galaxy, 13. Climate action, Astrophysics of Galaxies (astro-ph.GA), Atacama Cosmology Telescope, symbols, astro-ph.CO, Halo, Astronomical and Space Sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The scattering of cosmic microwave background (CMB) photons off the free-electron gas in galaxies and clusters leaves detectable imprints on high resolution CMB maps: the thermal and kinematic Sunyaev-Zel'dovich effects (tSZ and kSZ respectively). We use combined microwave maps from the Atacama Cosmology Telescope (ACT) DR5 and Planck in combination with the CMASS and LOWZ galaxy catalogs from the Baryon Oscillation Spectroscopic Survey (BOSS DR10 and DR12), to study the gas associated with these galaxy groups. Using individual reconstructed velocities, we perform a stacking analysis and reject the no-kSZ hypothesis at 6.5$\sigma$, the highest significance to date. This directly translates into a measurement of the electron number density profile, and thus of the gas density profile. Despite the limited signal to noise, the measurement shows at high significance that the gas density profile is more extended than the dark matter density profile, for any reasonable baryon abundance (formally $>90\sigma$ for the cosmic baryon abundance). We simultaneously measure the tSZ signal, i.e. the electron thermal pressure profile of the same CMASS objects, and reject the no-tSZ hypothesis at 10$\sigma$. We combine tSZ and kSZ measurements to estimate the electron temperature to 20% precision in several aperture bins, and find it comparable to the virial temperature. In a companion paper, we analyze these measurements to constrain the gas thermodynamics and the properties of feedback inside galaxy groups. We present the corresponding LOWZ measurements in this paper, ruling out a null kSZ (tSZ) signal at 2.9 (13.9)$\sigma$, and leave their interpretation to future work. Our stacking software ThumbStack is publicly available at https://github.com/EmmanuelSchaan/ThumbStack and directly applicable to future Simons Observatory and CMB-S4 data., Comment: Accepted in Physical Review D, Editors' Suggestion
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47. The Simons Observatory: science goals and forecasts

Author: Ade, Peter, Aguirre, James, Ahmed, Zeeshan, Aiola, Simone, Ali, Aamir, Alonso, David, Alvarez, Marcelo A., Arnold, Kam, Ashton, Peter, Austermann, Jason, Awan, Humna, Baccigalupi, Carlo, Baildon, Taylor, Barron, Darcy, Battaglia, Nick, Battye, Richard, Baxter, Eric, Bazarko, Andrew, Beall, James A., Bean, Rachel, Beck, Dominic, Beckman, Shawn, Beringue, Benjamin, Bianchini, Federico, Boada, Steven, Boettger, David, Richard Bond, J., Borrill, Julian, Brown, Michael L., Bruno, Sarah Marie, Bryan, Sean, Calabrese, Erminia, Calafut, Victoria, Calisse, Paolo, Carron, Julien, Challinor, Anthony, Chesmore, Grace, Chinone, Yuji, Chluba, Jens, Cho, Hsiao-Mei Sherry, Choi, Steve, Coppi, Gabriele, Cothard, Nicholas F., Coughlin, Kevin, Crichton, Devin, Crowley, Kevin D., Crowley, Kevin T., Cukierman, Ari, D`Ewart, Mitch, Dünner, Rolando, de Haan, Tijmen, Devlin, Mark, Dicker, Simon, DIDIER, JOY, Dobbs, Matt, Dober, Bradley, Duell, Cody, Duff, Shannon, Duivenvoorden, Adri, Dunkley, Jo, Dusatko, John, Errard, Josquin, Fabbian, Giulio, Feeney, Stephen, Ferraro, Simone, Fluxà, Pedro, Freese, Katherine, Frisch, Josef, Frolov, Andrei, Fuller, George, Fuzia, Brittany, Galitzki, Nicholas, Gallardo, Patricio A., Galvez Ghersi, Jose Tomas, Gao, Jiansong, Gawiser, Eric, Gerbino, Martina, Gluscevic, Vera, Goeckner-Wald, Neil, Golec, Joseph, Gordon, Sam, Gralla, Megan, Green, Daniel, Grigorian, Arpi, Groh, John, Groppi, Chris, Guan, Yilun, Gudmundsson, Jon E., Han, Dongwon, Hargrave, Peter, Hasegawa, Masaya, Hasselfield, Matthew, Hattori, Makoto, Haynes, Victor, Hazumi, Masashi, He, Yizhou, Healy, Erin, Henderson, Shawn, Hervias-Caimapo, Carlos, Hill, Charles A., Colin Hill, J., HILTON, GENE, Hilton, Matt, Hincks, Adam D., Hinshaw, Gary, Hložek, Renée, Ho, Shirley, Ho, Shuay-Pwu Patty, Howe, Logan, Huang, Zhiqi, Hubmayr, Johannes, Huffenberger, Kevin, Hughes, John P., Ijjas, Anna, Ikape, Margaret, Irwin, Kent, Jaffe, Andrew H., Jain, Bhuvnesh, Jeong, Oliver, Kaneko, Daisuke, Karpel, Ethan, Katayama, Nobuhiko, Keating, Brian, Kernasovski, Sarah, Keskitalo, Reijo, Kisner, Theodore, Kiuchi, Kenji, Klein, Jeff, Knowles, Kenda, Koopman, Brian, Kosowsky, Arthur, Krachmalnicoff, Nicoletta, Kuenstner, Stephen, Kuo, Chao-Lin, Kusaka, Akito, Lashner, Jacob, Lee, Adrian, Lee, Eunseong, Leon, David, Leung, Jason S.-Y., Lewis, Antony, Li, Yaqiong, Li, Zack, Limon, Michele, Linder, Eric, Lopez-Caraballo, Carlos, Louis, Thibaut, Lowry, Lindsay, Lungu, Marius, Madhavacheril, Mathew, Mak, Daisy, Maldonado, Felipe, Mani, Hamdi, Mates, Ben, Matsuda, Frederick, Maurin, Loïc, Mauskopf, Phil, May, Andrew, McCallum, Nialh, McKenney, Chris, McMahon, Jeff, Daniel Meerburg, P., Meyers, Joel, Miller, Amber, Mirmelstein, Mark, Moodley, Kavilan, Munchmeyer, Moritz, Munson, Charles, Naess, Sigurd, Nati, Federico, Navaroli, Martin, Newburgh, Laura, Nguyen, Ho Nam, Niemack, Mike, Nishino, Haruki, Orlowski-Scherer, John, Page, Lyman, Partridge, Bruce, Peloton, Julien, Perrotta, Francesca, Piccirillo, Lucio, Pisano, Giampaolo, Poletti, Davide, Puddu, Roberto, Puglisi, Giuseppe, Raum, Chris, Reichardt, Christian L., Remazeilles, Mathieu, Rephaeli, Yoel, Riechers, Dominik, Rojas, Felipe, Roy, Anirban, Sadeh, Sharon, Sakurai, Yuki, Salatino, Maria, Rao, Mayuri Sathyanarayana, Schaan, Emmanuel, Schmittfull, Marcel, Sehgal, Neelima, Seibert, Joseph, Seljak, Uros, Sherwin, Blake, Shimon, Meir, Sierra, Carlos, Sievers, Jonathan, Sikhosana, Precious, Silva-Feaver, Max, Simon, Sara M., Sinclair, Adrian, Siritanasak, Praween, Smith, Kendrick, Smith, Steve, Spergel, David, Staggs, Suzanne, Stein, George, Stevens, Jason R., Stompor, Radek, Suzuki, Aritoki, Tajima, Osamu, Takakura, Satoru, Teply, Grant, Thomas, Daniel B., Thorne, Ben, Thornton, Robert, Trac, Hy, Tsai, Calvin, Tucker, Carole, Ullom, Joel, Vagnozzi, Sunny, van Engelen, Alexander, Van Lanen, Jeff, van Winkle, Dan, Vavagiakis, Eve M., Vergès, Clara, Vissers, Michael, Wagoner, Kasey, Walker, Samantha, Ward, Jon, WESTBROOK, BEN, Whitehorn, Nathan, Williams, Jason, Williams, Joel, Wollack, Edward J., Xu, Zhilei, Ye, Jiani, Yu, Byeonghee, Yu, Cyndria, Zago, Fernando, Zhang, Hezi, Zhu, Ningfeng, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Simons Observatory, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), ANR-17-CE31-0022,BxB,Champs B interstellaires et modes B de l'inflation(2017), Ade, P, Aguirre, J, Ahmed, Z, Aiola, S, Ali, A, Alonso, D, Alvarez, M, Arnold, K, Ashton, P, Austermann, J, Awan, H, Baccigalupi, C, Baildon, T, Barron, D, Battaglia, N, Battye, R, Baxter, E, Bazarko, A, Beall, J, Bean, R, Beck, D, Beckman, S, Beringue, B, Bianchini, F, Boada, S, Boettger, D, Bond, J, Borrill, J, Brown, M, Bruno, S, Bryan, S, Calabrese, E, Calafut, V, Calisse, P, Carron, J, Challinor, A, Chesmore, G, Chinone, Y, Chluba, J, Cho, H, Choi, S, Coppi, G, Cothard, N, Coughlin, K, Crichton, D, Crowley, K, Cukierman, A, D'Ewart, J, Dünner, R, de Haan, T, Devlin, M, Dicker, S, Didier, J, Dobbs, M, Dober, B, Duell, C, Duff, S, Duivenvoorden, A, Dunkley, J, Dusatko, J, Errard, J, Fabbian, G, Feeney, S, Ferraro, S, Fluxà, P, Freese, K, Frisch, J, Frolov, A, Fuller, G, Fuzia, B, Galitzki, N, Gallardo, P, Ghersi, J, Gao, J, Gawiser, E, Gerbino, M, Gluscevic, V, Goeckner-Wald, N, Golec, J, Gordon, S, Gralla, M, Green, D, Grigorian, A, Groh, J, Groppi, C, Guan, Y, Gudmundsson, J, Han, D, Hargrave, P, Hasegawa, M, Hasselfield, M, Hattori, M, Haynes, V, Hazumi, M, He, Y, Healy, E, Henderson, S, Hervias-Caimapo, C, Hill, C, Hill, J, Hilton, G, Hilton, M, Hincks, A, Hinshaw, G, Hložek, R, Ho, S, Howe, L, Huang, Z, Hubmayr, J, Huffenberger, K, Hughes, J, Ijjas, A, Ikape, M, Irwin, K, Jaffe, A, Jain, B, Jeong, O, Kaneko, D, Karpel, E, Katayama, N, Keating, B, Kernasovskiy, S, Keskitalo, R, Kisner, T, Kiuchi, K, Klein, J, Knowles, K, Koopman, B, Kosowsky, A, Krachmalnicoff, N, Kuenstner, S, Kuo, C, Kusaka, A, Lashner, J, Lee, A, Lee, E, Leon, D, Leung, J, Lewis, A, Li, Y, Li, Z, Limon, M, Linder, E, Lopez-Caraballo, C, Louis, T, Lowry, L, Lungu, M, Madhavacheril, M, Mak, D, Maldonado, F, Mani, H, Mates, B, Matsuda, F, Maurin, L, Mauskopf, P, May, A, Mccallum, N, Mckenney, C, Mcmahon, J, Meerburg, P, Meyers, J, Miller, A, Mirmelstein, M, Moodley, K, Munchmeyer, M, Munson, C, Naess, S, Nati, F, Navaroli, M, Newburgh, L, Nguyen, H, Niemack, M, Nishino, H, Orlowski-Scherer, J, Page, L, Partridge, B, Peloton, J, Perrotta, F, Piccirillo, L, Pisano, G, Poletti, D, Puddu, R, Puglisi, G, Raum, C, Reichardt, C, Remazeilles, M, Rephaeli, Y, Riechers, D, Rojas, F, Roy, A, Sadeh, S, Sakurai, Y, Salatino, M, Rao, M, Schaan, E, Schmittfull, M, Sehgal, N, Seibert, J, Seljak, U, Sherwin, B, Shimon, M, Sierra, C, Sievers, J, Sikhosana, P, Silva-Feaver, M, Simon, S, Sinclair, A, Siritanasak, P, Smith, K, Smith, S, Spergel, D, Staggs, S, Stein, G, Stevens, J, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Teply, G, Thomas, D, Thorne, B, Thornton, R, Trac, H, Tsai, C, Tucker, C, Ullom, J, Vagnozzi, S, Engelen, A, Lanen, J, Winkle, D, Vavagiakis, E, Vergès, C, Vissers, M, Wagoner, K, Walker, S, Ward, J, Westbrook, B, Whitehorn, N, Williams, J, Wollack, E, Xu, Z, Yu, B, Yu, C, Zago, F, Zhang, H, Zhu, N, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and High-Energy Frontier
Subjects: CMBR polarisation, Cosmology and Nongalactic Astrophysics (astro-ph.CO), media_common.quotation_subject, Cosmic microwave background, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, law.invention, Telescope, symbols.namesake, Settore FIS/05 - Astronomia e Astrofisica, Observatory, law, 0103 physical sciences, CMBR experiments, Cosmological parameters from CMBR, Astronomy and Astrophysics, Planck, Reionization, QC, Astrophysics::Galaxy Astrophysics, media_common, Physics, 010308 nuclear & particles physics, Settore FIS/05, Astrophysics::Instrumentation and Methods for Astrophysics, cosmological parameters from CMBR, Nuclear & Particles Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Gravitational lens, 13. Climate action, Sky, symbols, astro-ph.CO, Neutrino, Cosmology and Nongalactic Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astronomical and Space Sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Simons Observatory (SO) is a new cosmic microwave background experiment being built on Cerro Toco in Chile, due to begin observations in the early 2020s. We describe the scientific goals of the experiment, motivate the design, and forecast its performance. SO will measure the temperature and polarization anisotropy of the cosmic microwave background in six frequency bands: 27, 39, 93, 145, 225 and 280 GHz. The initial configuration of SO will have three small-aperture 0.5-m telescopes (SATs) and one large-aperture 6-m telescope (LAT), with a total of 60,000 cryogenic bolometers. Our key science goals are to characterize the primordial perturbations, measure the number of relativistic species and the mass of neutrinos, test for deviations from a cosmological constant, improve our understanding of galaxy evolution, and constrain the duration of reionization. The SATs will target the largest angular scales observable from Chile, mapping ~10% of the sky to a white noise level of 2 $\mu$K-arcmin in combined 93 and 145 GHz bands, to measure the primordial tensor-to-scalar ratio, $r$, at a target level of $\sigma(r)=0.003$. The LAT will map ~40% of the sky at arcminute angular resolution to an expected white noise level of 6 $\mu$K-arcmin in combined 93 and 145 GHz bands, overlapping with the majority of the LSST sky region and partially with DESI. With up to an order of magnitude lower polarization noise than maps from the Planck satellite, the high-resolution sky maps will constrain cosmological parameters derived from the damping tail, gravitational lensing of the microwave background, the primordial bispectrum, and the thermal and kinematic Sunyaev-Zel'dovich effects, and will aid in delensing the large-angle polarization signal to measure the tensor-to-scalar ratio. The survey will also provide a legacy catalog of 16,000 galaxy clusters and more than 20,000 extragalactic sources., Comment: This paper presents an overview of the Simons Observatory science goals, details about the instrument will be presented in a companion paper. The author contribution to this paper is available at https://simonsobservatory.org/publications.php (Abstract abridged) -- matching version published in JCAP
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48. Evidence of galaxy cluster motions with the kinematic Sunyaev-Zel'dovich effect.

Author: Hand N, Addison GE, Aubourg E, Battaglia N, Battistelli ES, Bizyaev D, Bond JR, Brewington H, Brinkmann J, Brown BR, Das S, Dawson KS, Devlin MJ, Dunkley J, Dunner R, Eisenstein DJ, Fowler JW, Gralla MB, Hajian A, Halpern M, Hilton M, Hincks AD, Hlozek R, Hughes JP, Infante L, Irwin KD, Kosowsky A, Lin YT, Malanushenko E, Malanushenko V, Marriage TA, Marsden D, Menanteau F, Moodley K, Niemack MD, Nolta MR, Oravetz D, Page LA, Palanque-Delabrouille N, Pan K, Reese ED, Schlegel DJ, Schneider DP, Sehgal N, Shelden A, Sievers J, Sifón C, Simmons A, Snedden S, Spergel DN, Staggs ST, Swetz DS, Switzer ER, Trac H, Weaver BA, Wollack EJ, Yeche C, and Zunckel C
Abstract: Using high-resolution microwave sky maps made by the Atacama Cosmology Telescope, we for the first time present strong evidence for motions of galaxy clusters and groups via microwave background temperature distortions due to the kinematic Sunyaev-Zel'dovich effect. Galaxy clusters are identified by their constituent luminous galaxies observed by the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. We measure the mean pairwise momentum of clusters, with a probability of the signal being due to random errors of 0.002, and the signal is consistent with the growth of cosmic structure in the standard model of cosmology.
Published: 2012
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49. Can sterile neutrinos be the dark matter?

Author: Seljak U, Makarov A, McDonald P, and Trac H
Abstract: We use the Ly-alpha forest power spectrum measured by the Sloan Digital Sky Survey and high-resolution spectroscopy observations in combination with cosmic microwave background and galaxy clustering constraints to place limits on a sterile neutrino as a dark matter candidate in the warm dark matter scenario. Such a neutrino would be created in the early Universe through mixing with an active neutrino and would suppress structure on scales smaller than its free-streaming scale. We ran a series of high-resolution hydrodynamic simulations with varying neutrino masses to describe the effect of a sterile neutrino on the Ly-alpha forest power spectrum. We find that the mass limit is m(s) >13 keV at 95% C.L. (9 keV at 99.9%), which is above the upper limit allowed by x-ray constraints, excluding this candidate from being all of the dark matter in this model.
Published: 2006
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