We report results from 21-cm intensity maps acquired from the Parkes radio telescope and cross-correlated with galaxy maps from the 2dF galaxy survey. The data span the redshift range 0.057 < z < 0.098 and cover approximately 1,300 square degrees over two long fields. Cross correlation is detected at a significance of 5.18 σ. The amplitude of the cross-power spectrum is low relative to the expected dark matter power spectrum, assuming a neutral hydrogen (HI) bias and mass density equal to measurements from the ALFALFA survey. The decrement is pronounced and statistically significant at small scales. At k ∼ 1.5 h Mpc −1 , the cross power spectrum is more than a factor of 6 lower than expected, with a significance of 14.8 σ. This decrement indicates either a lack of clustering of neutral hydrogen (HI) , a small correlation coefficient between optical galaxies and HI , or some combination of the two. Separating 2dF into red and blue galaxies, we find that red galaxies are much more weakly correlated with HI on k ∼ 1.5 h Mpc −1 scales, suggesting that HI is more associated with blue star-forming galaxies and tends to avoid red galaxies.

We present a new measurement of the kinetic Sunyaev-Zeldovich effect (kSZ) using Planck cosmic microwave background (CMB) and Baryon Oscillation Spectroscopic Survey (BOSS) data. Using the "LowZ North/South" galaxy catalogue from BOSS DR12, and the group catalogue from BOSS DR13, we evaluate the mean pairwise kSZ temperature associated with BOSS galaxies. We construct a "Central Galaxies Catalogue" (CGC) which consists of isolated galaxies from the original BOSS data set, and apply the aperture photometry (AP) filter to suppress the primary CMB contribution. By constructing a halo model to fit the pairwise kSZ function, we constrain the mean optical depth to beτ ¼ ð0.53 AE 0.32Þ × 10 −4 ð1.65σÞ for LowZ North CGC,τ ¼ ð0.30 AE 0.57Þ × 10 −4 ð0.53σÞ for LowZ South CGC, andτ ¼ ð0.43 AE 0.28Þ × 10 −4 ð1.53σÞ for DR13 Group. In addition, we vary the radius of the AP filter and find that the AP size of 7 arcmin gives the maximum detection forτ. We also investigate the dependence of the signal with halo mass and findτ ¼ ð0.32 AE 0.36Þ × 10 −4 ð0.8σÞ andτ ¼ ð0.67 AE 0.46Þ × 10 −4 ð1.4σÞ for DR13 Group with halo mass restricted to, respectively, less and greater than its median halo mass, 10 12 h −1 M ⊙ . For the LowZ North CGC sample restricted to M h ≳ 10 14 h −1 M ⊙ there is no detection of the kSZ signal because these high mass halos are associated with the high-redshift galaxies of the LowZ North catalogue, which have limited contribution to the pairwise kSZ signals.

Understanding visual signal processing can benefit from simultaneous measurement of different types of retinal neurons working together. In this paper we demonstrate that intrinsic optical signal (IOS) imaging of frog retina slices allows simultaneous observation of stimulus-evoked responses propagating from the photoreceptors to inner neurons. High resolution imaging revealed robust IOSs at the photoreceptor, inner plexiform and ganglion cell layers. While IOSs of the photoreceptor layer were mainly confined to the area directly stimulated by the visible light; IOSs of inner retinal layers spread from the stimulus site into relatively large areas with a characteristic near to far time course.

Functional measurement is important for retinal study and disease diagnosis. Transient intrinsic optical signal (IOS) response, tightly correlated with functional stimulation, has been previously detected in normal retinas. In this paper, comparative IOS imaging of wild-type (WT) and rod-degenerated mutant mouse retinas is reported. Both 2-month and 1-year-old mice were measured. In 2-month-old mutant mice, time course and peak value of the stimulus-evoked IOS were significantly delayed (relative to stimulus onset) and reduced, respectively, compared to age matched WT mice. In 1-year-old mutant mice, stimulus-evoked IOS was totally absent. However, enhanced spontaneous IOS responses, which might reflect inner neural remodeling in diseased retina, were observed in both 2-month and 1-year-old mutant retinas. Our experiments demonstrate the potential of using IOS imaging for noninvasive and high resolution identification of disease-associated retinal dysfunctions. Moreover, high spatiotemporal resolution IOS imaging may also lead to advanced understanding of disease-associated neural remodeling in the retina.