JASMYN and the Need for LGBTQ+ Specific Organizations in Jacksonville, Florida

Nonprofit organizations receive a substantial amount of their funding from the federal government. In 2017, the current administration proposed cuts in areas of the federal budget that would negatively affect nonprofits and without this essential funding, such organizations may be unable to provide vital resources and services. LGBTQ+ specific organizations in northeast Florida, such as JASMYN, play a role fulfilling the health and social needs of LGBTQ+ youth that would otherwise not be addressed by non-LGBTQ+ specific organizations

Consent Is Not Enough: Why States Must Respect the Intensity Threshold in Transnational Conflict

It is widely accepted that a state cannot treat a struggle with an organized non-state actor as an armed conflict until the violence crosses a minimum threshold of intensity. For instance, during the recent standoff at the Oregon wildlife refuge, the US. government could have lawfully used force pursuant to its domestic law enforcement and human rights obligations, but President Obama could not have ordered a drone strike on the protesters. The reason for this uncontroversial rule is simple-not every riot or civil disturbance should be treated like a war. But what if President Obama had invited Canada to bomb the protestors-once the United States consented, would all bets be off? Can an intervening state use force that would be illegal for the host state to use itself? The silence on this issue is dangerous, in no small part because these once-rare conflicts are now commonplace. States are increasingly using force against organized non-state actors outside of the states\u27 own territories-usually, though not always, with the consent of the host state. What constrains the scope of the host state\u27s consent? And can the intervening state always presume that consent is valid? This Article argues that a host state\u27s authority to consent is limited and that intervening states cannot treat consent as a blank check. Accordingly, even in consent-based interventions, the logic andf oundational norms of the internationall egal order require both consent-giving and consent-receiving states to independently evaluate what legal regime governs-this will often turn on whether the intensity threshold has been met. Ifa non-international armed conflict exists, the actions of the intervening state are governed by international humanitarian law; if not, its actions are governed instead by its own and the host state\u27s human rights obligations

Characterizing Circumgalactic Gas around Massive Ellipticals at z~0.4 - II. Physical Properties and Elemental Abundances

We present a systematic investigation of the circumgalactic medium (CGM) within projected distances d<160 kpc of luminous red galaxies (LRGs). The sample comprises 16 intermediate-redshift (z=0.21-0.55) LRGs of stellar mass M_star>1e11 M_sun. Combining far-ultraviolet Cosmic Origin Spectrograph spectra from the Hubble Space Telescope and optical echelle spectra from the ground enables a detailed ionization analysis based on resolved component structures of a suite of absorption transitions, including the full HI Lyman series and various ionic metal transitions. By comparing the relative abundances of different ions in individually-matched components, we show that cool gas (T~1e4 K) density and metallicity can vary by more than a factor of ten in in an LRG halo. Specifically, metal-poor absorbing components with <1/10 solar metallicity are seen in 50% of the LRG halos, while gas with solar and super-solar metallicity is also common. These results indicate a complex multiphase structure and poor chemical mixing in these quiescent halos. We calculate the total surface mass density of cool gas, \Sigma_cool, by applying the estimated ionization fraction corrections to the observed HI column densities. The radial profile of \Sigma_cool is best-described by a projected Einasto profile of slope \alpha=1 and scale radius r_s=48 kpc. We find that typical LRGs at z~0.4 contain cool gas mass of M_cool= (1-2) x1e10 M_sun at d<160 kpc (or as much as 4x1e10 M_sun at d<500 kpc), comparable to the cool CGM mass of star-forming galaxies. Furthermore, we show that high-ionization OVI and low-ionization absorption species exhibit distinct velocity profiles, highlighting their different physical origins. We discuss the implications of our findings for the origin and fate of cool gas in LRG halos.Comment: Accepted for publication in MNRAS after a minor revision. 23 pages, 14 figures, and a 29-page Appendix with 27 additional figure

Consent Is Not Enough: Why States Must Respect the Intensity Threshold in Transnational Conflict

It is widely accepted that a state cannot treat a struggle with an organized non-state actor as an armed conflict until the violence crosses a minimum threshold of intensity. For instance, during the recent standoff at the Oregon wildlife refuge, the US. government could have lawfully used force pursuant to its domestic law enforcement and human rights obligations, but President Obama could not have ordered a drone strike on the protesters. The reason for this uncontroversial rule is simple-not every riot or civil disturbance should be treated like a war. But what if President Obama had invited Canada to bomb the protestors-once the United States consented, would all bets be off? Can an intervening state use force that would be illegal for the host state to use itself? The silence on this issue is dangerous, in no small part because these once-rare conflicts are now commonplace. States are increasingly using force against organized non-state actors outside of the states\u27 own territories-usually, though not always, with the consent of the host state. What constrains the scope of the host state\u27s consent? And can the intervening state always presume that consent is valid? This Article argues that a host state\u27s authority to consent is limited and that intervening states cannot treat consent as a blank check. Accordingly, even in consent-based interventions, the logic andf oundational norms of the internationall egal order require both consent-giving and consent-receiving states to independently evaluate what legal regime governs-this will often turn on whether the intensity threshold has been met. Ifa non-international armed conflict exists, the actions of the intervening state are governed by international humanitarian law; if not, its actions are governed instead by its own and the host state\u27s human rights obligations

The SAGA Survey: I. Satellite Galaxy Populations Around Eight Milky Way Analogs

We present the survey strategy and early results of the "Satellites Around Galactic Analogs" (SAGA) Survey. The SAGA Survey's goal is to measure the distribution of satellite galaxies around 100 systems analogous to the Milky Way down to the luminosity of the Leo I dwarf galaxy ($M_r < -12.3$). We define a Milky Way analog based on $K$-band luminosity and local environment. Here, we present satellite luminosity functions for 8 Milky Way analog galaxies between 20 to 40 Mpc. These systems have nearly complete spectroscopic coverage of candidate satellites within the projected host virial radius down to $r_o < 20.75$ using low redshift $gri$ color criteria. We have discovered a total of 25 new satellite galaxies: 14 new satellite galaxies meet our formal criteria around our complete host systems, plus 11 additional satellites in either incompletely surveyed hosts or below our formal magnitude limit. Combined with 13 previously known satellites, there are a total of 27 satellites around 8 complete Milky Way analog hosts. We find a wide distribution in the number of satellites per host, from 1 to 9, in the luminosity range for which there are five Milky Way satellites. Standard abundance matching extrapolated from higher luminosities predicts less scatter between hosts and a steeper luminosity function slope than observed. We find that the majority of satellites (26 of 27) are star-forming. These early results indicate that the Milky Way has a different satellite population than typical in our sample, potentially changing the physical interpretation of measurements based only on the Milky Way's satellite galaxies.Comment: 22 pages, 19 figures, 2 tables. Updated to published version. Survey website: http://sagasurvey.org

Ccl5 Mediates Proper Wiring of Feedforward and Lateral Inhibition Pathways in the Inner Retina

The β-chemokine Ccl5 and its receptors are constitutively expressed in neurons of the murine inner retina. Here, we examined the functional and structural significance of this constitutive Ccl5 signaling on retinal development. We compared outcomes of electrophysiology, ocular imaging and retinal morphology in wild-type mice (WT) and mice with Ccl5 deficiency (Ccl5-/-). Assessment of retinal structure by ocular coherence tomography and histology revealed slight thinning of the inner plexiform layer (IPL) and inner nuclear layer (INL) in Ccl5-/- mice, compared to WT (p &lt; 0.01). Assessment of postnatal timepoints important for development of the INL (P7 and P10) revealed Ccl5-dependent alterations in the pattern and timing of apoptotic pruning. Morphological analyses of major inner retinal cell types in WT, Ccl5-/-, gustducingfp and gustducingfp/Ccl5-/- mice revealed Ccl5-dependent reduction in GNAT3 expression in rod bipolar cells as well as a displacement of their terminals from the IPL into the GCL. RGC dendritic organization and amacrine cell morphology in the IPL was similarly disorganized in Ccl5-/- mice. Examination of the intrinsic electrophysiological properties of RGCs revealed higher spontaneous activity in Ccl5-/- mice that was characterized by higher spiking frequency and a more depolarized resting potential. This hyperactive phenotype could be negated by current clamp and correlated with both membrane resistance and soma area. Overall, our findings identify Ccl5 signaling as a mediator of inner retinal circuitry during development of the murine retina. The apparent role of Ccl5 in retinal development further supports chemokines as trophic modulators of CNS development and function that extends far beyond the inflammatory contexts in which they were first characterized

Characterizing Circumgalactic Gas around Massive Ellipticals at z ~ 0.4 I. Initial Results

We present a new Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) absorption-line survey to study halo gas around 16 luminous red galaxies (LRGs) at z=0.21-0.55. The LRGs are selected uniformly with stellar mass Mstar>1e11 Msun and no prior knowledge of the presence/absence of any absorption features. Based on observations of the full Lyman series, we obtain accurate measurements of neutral hydrogen column density N(HI) and find that high-N(HI) gas is common in these massive quiescent halos with a median of <log N(HI)> = 16.6 at projected distances d<~160 kpc. We measure a mean covering fraction of optically-thick gas with log N(HI)>~17.2 of LLS=0.44^{+0.12}_{-0.11} at d<~160 kpc and LLS=0.71^{+0.11}_{-0.20} at d<~100 kpc. The line-of-sight velocity separations between the HI absorbing gas and LRGs are characterized by a mean and dispersion of =29 km/s and \sigma_v_{gas-gal}=171 km/s. Combining COS FUV and ground-based echelle spectra provides an expanded spectral coverage for multiple ionic transitions, from low-ionization MgII and SiII, to intermediate ionization SiIII and CIII, and to high-ionization OVI absorption lines. We find that intermediate ions probed by CIII and SiIII are the most prominent UV metal lines in LRG halos with a mean covering fraction of _{0.1}=0.75^{+0.08}_{-0.13} for W(977)>=0.1 Ang at d<160 kpc, comparable to what is seen for CIII in L* and sub-L* star-forming and red galaxies but exceeding MgII or OVI in quiescent halos. The COS-LRG survey shows that massive quiescent halos contain widespread chemically-enriched cool gas and that little distinction between LRG and star-forming halos is found in their HI and CIII content.Comment: 19 pages, 6 figures, accepted by MNRA

Constraints on the Universal CIV Mass Density at z~6 from Early IR Spectra Obtained with the Magellan FIRE Spectrograph

We present a new determination of the intergalactic CIV mass density at 4.3 < z < 6.3. Our constraints are derived from high signal-to-noise spectra of seven quasars at z > 5.8 obtained with the newly commissioned FIRE spectrograph on the Magellan Baade telescope, coupled with six observations of northern objects taken from the literature. We confirm the presence of a downturn in the CIV abundance at =5.66 by a factor of 4.1 relative to its value at =4.96, as measured in the same sightlines. In the FIRE sample, a strong system previously reported in the literature as CIV at z=5.82 is re-identified as MgII at z=2.78, leading to a substantial downward revision in $\Omega_{CIV}$ for these prior studies. Additionally we confirm the presence of at least two systems with low-ionization CII, SiII, and OI absorption but relatively weak signal from CIV. The latter systems systems may be of interest if the downward trend in $\Omega_{CIV}$ at high redshift is driven in part by ionization effects.Comment: 14 pages, 6 figures, 2 tables. Submitted to Ap

1999-2000 Tribute - Music by Women Composers

This concert is presented by Palm Beach County Music Teacher\u27s Association.https://spiral.lynn.edu/conservatory_otherseasonalconcerts/1109/thumbnail.jp