Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys

Large scale filaments, with lengths that can reach tens of Mpc, are the most prominent features in the cosmic web. These filaments have only been observed indirectly through the positions of galaxies in large galaxy surveys or through absorption features in the spectra of high redshift sources. In this study we propose to go one step further and directly detect intergalactic medium filaments through their emission in the HI 21cm line. We make use of high resolution cosmological simulations to estimate the intensity of this emission in low redshift filaments and use it to make predictions for the direct detectability of specific filaments previously inferred from galaxy surveys, in particular the Sloan Digital Sky Survey. Given the expected signal of these filaments our study shows that HI emission from large filaments can be observed by current and next generation radio telescopes. We estimate that gas in filaments of length $l \gtrsim$ 15 $h^{-1}$Mpc with relatively small inclinations to the line of sight ($\lesssim 10^\circ$) can be observed in $\sim40-100$ hours with telescopes such as GMRT or EVLA, potentially providing large improvements over our knowledge of the astrophysical properties of these filaments. Due to their large field of view and sufficiently long integration times, upcoming HI surveys with the Apertif and ASKAP instruments will be able to detect large filaments independently of their orientation and curvature. Furthermore, our estimates indicate that a more powerful future radio telescope like SKA-2 can be used to map most of these filaments, which will allow them to be used as a strong cosmological probe.Comment: 16 pages, 11 figures, Accepted for publication in MNRA

Tomographic Intensity Mapping versus Galaxy Surveys: Observing the Universe in H-alpha emission with new generation instruments

The H-alpha line emission is an important probe for a number of fundamental quantities in galaxies, including their number density, star formation rate (SFR) and overall gas content. A new generation of low-resolution intensity mapping probes, e.g. SPHEREx and CDIM, will observe galaxies in H-alpha emission over a large fraction of the sky from the local Universe till a redshift of z ~ 6 to 10, respectively. This will also be the target line for observations by the high-resolution Euclid and WFIRST instruments in the z ~ 0.7 - 2 redshift range. In this paper, we estimate the intensity and power spectra of the H-alpha line in the z ~ 0 - 5 redshift range using observed line luminosity functions (LFs), when possible, and simulations, otherwise. We estimate the significance of our predictions by accounting for the modelling uncertainties (e.g. SFR, extinction, etc.) and observational contamination. We find that Intensity Mapping (IM) surveys can make a statistical detection of the full H-alpha emission between z ~ 0.8 - 5. Moreover, we find that the high-frequency resolution and the sensitivity of the planned CDIM surveys allow for the separation of H-alpha emission from several interloping lines. We explore ways to use the combination of these line intensities to probe galaxy properties. As expected, our study indicates that galaxy surveys will only detect bright galaxies that contribute up to a few percent of the overall H-alpha intensity. However, these surveys will provide important constraints on the high end of the H-alpha LF and put strong constraints on the AGN LF.Comment: Submitted to MNRA

Object identification and characterization with hyperspectral imagery to identify structure and function of Natura 2000 habitats

Habitat monitoring of designated areas under the EU Habitats Directive requires every 6 years information on area, range, structure and function for the protected (Annex I) habitat types. First results from studies on heathland areas in Belgium and the Netherlands show that hyperspectral imagery can be an important source of information to assist the evaluation of the habitat conservation status. Hyperspectral imagery can provide continuous maps of habitat quality indicators (e.g., life forms or structure types, management activities, grass, shrub and tree encroachment) at the pixel level. At the same time, terrain managers, nature conservation agencies and national authorities responsible for the reporting to the EU are not directly interested in pixels, but rather in information at the level of vegetation patches, groups of patches or the protected site as a whole. Such local level information is needed for management purposes, e.g., exact location of patches of habitat types and the sizes and quality of these patches within a protected site. Site complexity determines not only the classification success of remote sensing imagery, but influences also the results of aggregation of information from the pixel to the site level. For all these reasons, it is important to identify and characterize the vegetation patches. This paper focuses on the use of segmentation techniques to identify relevant vegetation patches in combination with spectral mixture analysis of hyperspectral imagery from the Airborne Hyperspectral Scanner (AHS). Comparison with traditional vegetation maps shows that the habitat or vegetation patches can be identified by segmentation of hyperspectral imagery. This paper shows that spectral mixture analysis in combination with segmentation techniques on hyperspectral imagery can provide useful information on processes such as grass encroachment that determine the conservation status of Natura 2000 heathland areas to a large extent. A limitation is that both advanced remote sensing approaches and traditional field based vegetation surveys seem to cause over and underestimations of grass encroachment for specific categories, but the first provides a better basis for monitoring if specific species are not directly considered

Erratum:Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys [MNRAS, (2019)] DOI: 10.1093/mnras/stx509

This is an erratum to the paper' Filament Hunting: Integrated HI 21cm Emission From Filaments Inferred by Galaxy Surveys' that was published in MNRAS, 468, 857. Due to the use of an incorrect equation to calculate the thermal noise of an observation, the noise was underestimated in the paper, affecting some of our conclusions

Recellularization of Porcine Internal Thoracic Arteries as a Tissue Engineered Small-Diameter Vascular Graft Alternative

Small-diameter vascular grafts are the leading treatment for myocardial infarctions resulting from atherosclerosed coronary vasculature. A potential alternative to using patient-derived grafts is the use of tissue engineered vessels. The removal of native cells from xenogenic vessels allows for recellularization with human cells types; however, the decellularization process depends on the use of cytotoxic reagents that must be removed prior to recellularization. The recellularization process must produce a functional graft that contains the multiple cell types found within arteries. We hypothesized that porcine internal thoracic arteries decellularized using a combination of detergents could be processed to support human endothelial and smooth muscle cell growth. We also hypothesized that in order to optimize in vitro co-culture conditions during recellularization, a mix of media types would be necessary to simultaneously support endothelial and smooth muscle cell growth. A cytotoxicity assay was performed to assess the effects of residual detergents on endothelial cells seeded onto the scaffolds. A relationship between the degree of detergent rinsing and cellular viability was identified via a resazurin reduction assay with more extensive rinsing significantly enhancing cell viability. This same cell viability assay was used to identify media combinations that supported growth of both endothelial and smooth muscle cells. Both cell types were able to grow in a 50:50 mixture of their media types without any loss of viability or effect on morphology. Furthermore, endothelial cells grown in the mixed medium maintained their characteristic CD31 expression. Taken together, these results show that human cells native to arteries can remain viable within the extracellular matrix of porcine internal thoracic artery scaffolds after thorough scaffold detoxification. Additionally, the co-culture conditions established can support the growth of both endothelial and smooth muscle cell types found within arteries. Future work will focus on simultaneously culturing the cells within scaffolds to build toward the goal of tissue engineering small-diameter vascular graft alternatives.https://digitalcommons.winthrop.edu/sureposters/1005/thumbnail.jp