Design and use of a large-format CCD instrument for the identification and study of distant galaxy clusters by Luppino, Gerard Anthony

Get full text

THE REDSHIFT EVOLUTION OF THE MEAN TEMPERATURE, PRESSURE, AND ENTROPY PROFILES IN 80 SPT-SELECTED GALAXY CLUSTERS by McDonald, Michael A., Bautz, Marshall W., Miller, Eric D

“…We present the results of an X-ray analysis of 80 galaxy clusters selected in the 2500 deg[superscript 2] South Pole Telescope survey and observed with the Chandra X-ray Observatory. …”
Get full text
Get full text

X-RAY SIGNATURES OF NON-EQUILIBRIUM IONIZATION EFFECTS IN GALAXY CLUSTER ACCRETION SHOCK REGIONS by Wong, Ka-Wah, Sarazin, Craig L., Ji, Li

Get full text

GALAXY CLUSTERS IN THE SWIFT /BURST ALERT TELESCOPE ERA: HARD X-RAYS IN THE INTRACLUSTER MEDIUM by Ajello, M., Rebusco, Paola, Cappelluti, N., Reimer, O., Böhringer, H., Greiner, J., Gehrels, N., Tueller, J., Moretti, A.

“…We also derive the first log N-log S and luminosity function distributions of galaxy clusters above 15 keV.…”
Get full text
Get full text

The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type by Norberg, P, Baugh, C, Hawkins, E, Maddox, S, Madgwick, D, Lahav, O, Cole, S, Frenk, C, Baldry, I, Bland-Hawthorn, J, Bridges, T, Cannon, R, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, S, Efstathiou, G, Ellis, R, Glazebrook, K, Jackson, C, Lewis, I, Lumsden, S, Peacock, J

Surveying the sky with the Arcminute MicroKelvin Imager: expected constraints on galaxy cluster evolution and cosmology by Kneissl, R, Jones, M, Saunders, R, Eke, V, Lasenby, A, Grainge, K, Cotter, G

Planck Intermediate Results. IV. The XMM-Newton validation programme for new Planck galaxy clusters by Collaboration, P, Ade, P, Aghanim, N, Arnaud, M, Ashdown, M, Aumont, J, Baccigalupi, C, Balbi, A, Banday, A, Barreiro, R, Bartlett, J, Battaner, E, Benabed, K, Benoît, A, Bernard, J, Bersanelli, M, Bikmaev, I, Böhringer, H, Bonaldi, A, Bond, JR, Borgani, S, Borrill, J, Bouchet, F, Brown, M, Burigana, C

“…We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios between 4.0 and 6.1 in the 15.5-month nominal Planck survey. …”

Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters by Hurley-Walker, N, Bridle, S, Cypriano, E, Davies, M, Erben, T, Feroz, F, Franzen, T, Grainge, K, Hobson, M, Lasenby, A, Marshall, P, Olamaie, M, Pooley, G, Rodriguez-Gonzalvez, C, Saunders, R, Scaife, A, Schammel, M, Scott, P, Shimwell, T, Titterington, D, Waldram, E, Zwart, J, Consortium, AMI

Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters by Hurley-Walker, N, Bridle, S, Cypriano, E, Davies, M, Erben, T, Feroz, F, Franzen, T, Grainge, K, Hobson, M, Lasenby, A, Marshall, P, Olamaie, M, Pooley, G, Rodríguez-Gonzálvez, C, Saunders, R, Scaife, A, Schammel, M, Scott, P, Shimwell, T, Titterington, D, Waldram, E, Zwart, J

“…We present an analysis of observations made with the Arcminute Microkelvin Imager (AMI) and the Canada-France-Hawaii Telescope (CFHT) of six galaxy clusters in a redshift range of 0.16-0.41. The cluster gas is modelled using the Sunyaev-Zel'dovich (SZ) data provided by AMI, while the total mass is modelled using the lensing data from the CFHT. …”

Physics of cosmic plasmas from high angular resolution X-ray imaging of galaxy clusters by Markevitch, M, Bulbul, E, Churazov, E, Giacintucci, S, Kraft, R, Kunz, M, Nagai, D, Roediger, E, Ruszkowski, M, Schekochihin, A, Weeren, RV, Vikhlinin, A, Walker, SA, Wang, QHS, Werner, N, Wik, D, Zhuravleva, I, Zuhone, J

“…Galaxy clusters are massive dark matter-dominated systems filled with X-ray emitting, optically thin plasma. …”

Ultraviolet imaging of the galaxy cluster CL 0939+4713 (Abell 851) at z=0.41 by Buson, L, Bertola, F, Cappellari, M, Chiosi, C, Dressler, A, Oemler, A

Planck Intermediate Results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect by Collaboration, P, Ade, P, Aghanim, N, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Balbi, A, Banday, A, Barreiro, R, Bartlett, J, Battaner, E, Benabed, K, Benoit, A, Bernard, J, Bersanelli, M, Bhatia, R, Bikmaev, I, Boehringer, H, Bonaldi, A, Bond, JR, Borgani, S, Borrill, J, Bouchet, F

Smoothed Particle Inference: A Kilo‐Parametric Method for X‐Ray Galaxy Cluster Modeling by Peterson, JR, Marshall, P, Andersson, K

Tomographic galaxy clustering with the Subaru Hyper Suprime-Cam first year public data release by Nicola, A, Alonso, D, Sánchez, J, Slosar, A, Awan, H, Broussard, A, Dunkley, J, Gawiser, E, Gomes, Z, Mandelbaum, R, Miyatake, H, Newman, JA, Sevilla, I, Skinner, S, Wagoner, E

“…In terms of photometric redshift systematics, we show that additional care is needed in order to marginalize over uncertainties in the redshift distribution in galaxy clustering, even for samples of this small size, and that these uncertainties can be significantly constrained by including cross-bin correlations. …”

Surveying the sky with the Arcminute MicroKelvin Imager: expected constraints on galaxy cluster evolution and cosmology by Kneissl, R, Jones, M, Saunders, R, Eke, V, Lasenby, A, Grainge, K, Cotter, G

Evidence for a Redshifted Excess in the Intracluster Light Fractions of Merging Clusters at z ∼ 0.8 by Yolanda Jiménez-Teja, Renato A. Dupke, Paulo A. A. Lopes, Paola Dimauro

Subjects: “…Galaxy clusters…”
Get full text

Generating galaxy clusters mass density maps from mock multiview images via deep learning by de Andres Daniel, Cui Weiguang, Yepes Gustavo, De Petris Marco, Aversano Gianmarco, Ferragamo Antonio, De Luca Federico, Muñoz A. Jiménez

“…Galaxy clusters are composed of dark matter, gas and stars. …”
Get full text

UPCluster-SZ: The Updated Catalog of Galaxy Clusters from the List of Planck Sunyaev–Zel’dovich Sources by Hyeonguk Bahk, Ho Seong Hwang

Subjects: “…Galaxy clusters…”
Get full text

Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters by Wicker R., Douspis M., Salvati L., Aghanim N.

“…The gas mass fraction in galaxy clusters is a quantity which can be used as a robust cosmological probe. …”
Get full text

Constraining Baryon Loading Efficiency of Active Galactic Nuclei with Diffuse Neutrino Flux from Galaxy Clusters by Xin-Yue Shi, Ruo-Yu Liu, Chong Ge, Xiang-Yu Wang

Subjects: Get full text