Toward the measurement of neutrino masses: Performance of cosmic magnification with submillimeter galaxies

Home

All issues

Volume 687 (July 2024)

A&A, 687 (2024) A300

Full HTML

Open Access

Table 2.

MCMC results from each considered case.

	σ₈ CUE24a	A_s CUE24a	A_sPlanck	A_sPlanck (σ = 0.1)	A_s CUE24a (no G15)
α	$0 . 69_{- 0.46}^{+ 0.30} (0.60)$ $0.69^{+0.30}_{-0.46}\,(0.60)$	> 0.79 (−)	> 1.17 (−)	> 1.09 (−)	$0 . 89_{- 0.26}^{+ 0.18} (0.81)$ $0.89^{+0.18}_{-0.26}\,(0.81)$
log M_min	$11 . 64_{- 0.12}^{+ 0.17} (11.68)$ $11.64^{+0.17}_{-0.12}\,(11.68)$	$11 . 47_{- 0.11}^{+ 0.14} (11.50)$ $11.47^{+0.14}_{-0.11}\,(11.50)$	$11 . 49_{- 0.16}^{+ 0.14} (11.50)$ $11.49^{+0.14}_{-0.16}\,(11.50)$	$11 . 53_{- 0.14}^{+ 0.15} (11.54)$ $11.53^{+0.15}_{-0.14}\,(11.54)$	$11 . 46_{- 0.16}^{+ 0.27} (11.53)$ $11.46^{+0.27}_{-0.16}\,(11.53)$
log M₁	$13 . 39_{- 0.92}^{+ 0.71} (13.34)$ $13.39^{+0.71}_{-0.92}\,(13.34)$	$12 . 89_{- 0.41}^{+ 0.56} (13.01)$ $12.89^{+0.56}_{-0.41}\,(13.01)$	$12 . 52_{- 0.25}^{+ 0.36} (12.61)$ $12.52^{+0.36}_{-0.25}\,(12.61)$	$12 . 59_{- 0.34}^{+ 0.50} (12.71)$ $12.59^{+0.50}_{-0.34}\,(12.71)$	$12 . 43_{- 0.46}^{+ 0.70} (12.68)$ $12.43^{+0.70}_{-0.46}\,(12.68)$
Ω_m	$0 . 28_{- 0.08}^{+ 0.04} (0.25)$ $0.28^{+0.04}_{-0.08}\,(0.25)$	$0 . 18_{- 0.02}^{+ 0.02} (0.18)$ $0.18^{+0.02}_{-0.02}\,(0.18)$	$0 . 16_{- 0.02}^{+ 0.01} (0.16)$ $0.16^{+0.01}_{-0.02}\,(0.16)$	$0 . 17_{- 0.03}^{+ 0.01} (0.16)$ $0.17^{+0.01}_{-0.03}\,(0.16)$	$0 . 34_{- 0.03}^{+ 0.02} (0.33)$ $0.34^{+0.02}_{-0.03}\,(0.33)$
h	< 0.70 (−)	> 0.77 (−)	> 0.82 (−)	> 0.83 (−)	$0 . 72_{- 0.06}^{+ 0.07} (0.73)$ $0.72^{+0.07}_{-0.06}\,(0.73)$
∑m_ν (eV)	− (−)	< 0.22 (−)	< 0.36 (−)	< 0.46 (−)	− (−)
β	$2 . 91_{- 0.04}^{+ 0.04} (2.91)$ $2.91^{+0.04}_{-0.04}\,(2.91)$	$2 . 91_{- 0.02}^{+ 0.03} (2.91)$ $2.91^{+0.03}_{-0.02}\,(2.91)$	$2 . 92_{- 0.04}^{+ 0.04} (2.92)$ $2.92^{+0.04}_{-0.04}\,(2.92)$	$2 . 92_{- 0.04}^{+ 0.04} (2.92)$ $2.92^{+0.04}_{-0.04}\,(2.92)$	$2 . 90_{- 0.03}^{+ 0.04} (2.90)$ $2.90^{+0.04}_{-0.03}\,(2.90)$

Notes. The mean and 68% credible intervals for each parameter are stated, along with the marginalized maximum a posteriori value in parenthesis. Dashes indicate unconstrained distributions or unmeaningful maximum a posteriori values. Halo masses are expressed in M_⊙/h.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.