• No se han encontrado resultados

Southern cosmology survey ii massive optically selected clusters from 70 square degrees of the sunyaev zel'dovich effect common survey area

N/A
N/A
Protected

Academic year: 2020

Share "Southern cosmology survey ii massive optically selected clusters from 70 square degrees of the sunyaev zel'dovich effect common survey area"

Copied!
12
0
0

Texto completo

Loading

Figure

Figure 1. Computed likelihood density map images centered at z = 0.3 and width Δz = 0.1 over the 23 hr (top panel) and the 5 hr (bottom panel) field
Figure 2. E(B − V ) dust extinction maps created for the 5 hr (left) and 23 hr (right) fields in magnitudes using the Schlegel et al
Figure 3. Composite gri color image for nine newly discovered massive SCS clusters in the 5 hr field
Figure 4. Composite gri color image for nine newly discovered massive SCS clusters in the 23 hr field
+3

Referencias

Documento similar

No obstante, como esta enfermedad afecta a cada persona de manera diferente, no todas las opciones de cuidado y tratamiento pueden ser apropiadas para cada individuo.. La forma

The luminosity function of the former method is derived by summing membership probabilities of all stars fitted to distribution functions in the vector point diagram, whereas

In the previous sections we have shown how astronomical alignments and solar hierophanies – with a common interest in the solstices − were substantiated in the

Finally, experiments with solar [17–34], atmospheric [35–45], reactor [46–50], and long-baseline accelerator [51–59] neutrinos indicate that neutrino flavor change through

Díaz Soto has raised the point about banning religious garb in the ―public space.‖ He states, ―for example, in most Spanish public Universities, there is a Catholic chapel

teriza por dos factores, que vienen a determinar la especial responsabilidad que incumbe al Tribunal de Justicia en esta materia: de un lado, la inexistencia, en el

Relationship between the total cluster stellar mass and the photometric blue fraction for the ALHAMBRA cluster and group sample stacked into different redshift bins. The galaxy

As a means to probe the possible fractal structure of the galaxy distribution we have studied the scaling of the num- ber density and angular correlation function of galaxies