Pornography Isn\u27t the Problem: A Feminist Theoretical Perspective on the War Against Pornhub

Over the last year, Pornhub and its parent company, MindGeek, ignited public outcry against the prevalence of content users posted to their sites featuring sexual violence, nonconsensual pornography, and sex trafficking. Activists, journalists, and legislators allege that Pornhub and similar pornography sites are apathetic toward the victims in these videos and photos while profiting from the ad revenue such content brings to their sites. In December 2021, Senator Josh Hawley proposed the Survivors of Human Trafficking Fight Back Act, proposing to add criminal penalties and a federal cause of action against websites that either post or refuse to remove criminal pornography from their sites. This Note examines the arguments for and against legislation penalizing pornography websites for posting or hosting content of featuring sexual violence through a feminist lens. This style of legislation, which nobly aims to protect survivors of sexual violence, will likely appear again in Congress. This Note argues that Congress should not pass these bills because they subject transactional sex workers and pornography performers to economic and physical harm, making it an ineffective and misguided method to address the core harms of digital sexual exploitation

No Child Was Harmed in the Making of This Video: Morphed Child Pornography and the First Amendment

On February 13, 2020, the Fifth Circuit Court of Appeals held, in United States v. Mecham, that the First Amendment does not protect morphed child pornography as a form of speech. The Fifth Circuit found that “morphed child pornography” is like “real child pornography” because the content harms the emotional health and reputation of a child. Thus, the Fifth Circuit held that the First Amendment excludes both forms of child pornography from protection. The Sixth and Second Circuits follow this rule, emphasizing that the government has a strong imperative to intervene in situations that harm children. In contrast, the Eighth Circuit has held that, under the Supreme Court’s recent opinion in United States v. Stevens, the First Amendment protects morphed child pornography unless it depicts an underlying crime. Therefore, in the Eighth Circuit, the First Amendment protects morphed child pornography that does not capture the real sexual abuse of a child. The Supreme Court denied Mecham certiorari, and the Court has not addressed the treatment of morphed child pornography under the First Amendment substantively. This Comment argues that the Fifth Circuit correctly decided Mecham by holding that the First Amendment does not protect morphed child pornography. It also argues that the Eighth Circuit minority holding is erroneous because it fails to show judicial restraint and disregards policy

A detailed statistical analysis of the mass profiles of galaxy clusters

The distribution of mass in the halos of galaxies and galaxy clusters has been probed observationally, theoretically, and in numerical simulations. Yet there is still confusion about which of several suggested parameterized models is the better representation, and whether these models are universal. We use the temperature and density profiles of the intracluster medium as measured by X-ray observations of 11 relaxed galaxy clusters to investigate mass models for the halo using a thorough Bayesian statistical analysis. We make careful comparisons between two- and three-parameter models, including the issue of a universal third parameter. We find that, of the two-parameter models, the NFW is the best representation, but we also find moderate statistical evidence that a generalized three-parameter NFW model with a freely varying inner slope is preferred, despite penalizing against the extra degree of freedom. There is a strong indication that this inner slope needs to be determined for each cluster individually, i.e. some clusters have central cores and others have steep cusps. The mass-concentration relation of our sample is in reasonable agreement with predictions based on numerical simulations.Comment: 10 pages, 5 figures, accepted by ApJ. Matches accepted versio

Galaxy and Mass Assembly (GAMA): merging galaxies and their properties

We derive the close pair fractions and volume merger rates for galaxies in the Galaxy and Mass Assembly (GAMA) survey with −23 < Mr < −17 (ΩM = 0.27, ΩΛ = 0.73, H0 = 100 km s−1 Mpc−1) at 0.01 < z < 0.22 (look-back time of <2 Gyr). The merger fraction is approximately 1.5 per cent Gyr−1 at all luminosities (assuming 50 per cent of pairs merge) and the volume merger rate is ≈3.5 × 10−4 Mpc−3 Gyr−1. We examine how the merger rate varies by luminosity and morphology. Dry mergers (between red/spheroidal galaxies) are found to be uncommon and to decrease with decreasing luminosity. Fainter mergers are wet, between blue/discy galaxies. Damp mergers (one of each type) follow the average of dry and wet mergers. In the brighter luminosity bin (−23 < Mr < −20), the merger rate evolution is flat, irrespective of colour or morphology, out to z ∼ 0.2. The makeup of the merging population does not appear to change over this redshift range. Galaxy growth by major mergers appears comparatively unimportant and dry mergers are unlikely to be significant in the buildup of the red sequence over the past 2 Gyr. We compare the colour, morphology, environmental density and degree of activity (BPT class, Baldwin, Phillips & Terlevich) of galaxies in pairs to those of more isolated objects in the same volume. Galaxies in close pairs tend to be both redder and slightly more spheroid dominated than the comparison sample. We suggest that this may be due to ‘harassment’ in multiple previous passes prior to the current close interaction. Galaxy pairs do not appear to prefer significantly denser environments. There is no evidence of an enhancement in the AGN fraction in pairs, compared to other galaxies in the same volume

Detection of maturity and ligament injury using magic angle directional imaging

Purpose: To investigate whether magnetic field–related anisotropies of collagen may be correlated with postmortem findings in animal models. Methods: Optimized scan planning and new MRI data‐processing methods were proposed and analyzed using Monte Carlo simulations. Six caprine and 10 canine knees were scanned at various orientations to the main magnetic field. Image intensities in segmented voxels were used to compute the orientation vectors of the collagen fibers. Vector field and tractography plots were computed. The Alignment Index was defined as a measure of orientation distribution. The knees were subsequently assessed by a specialist orthopedic veterinarian, who gave a pathological diagnosis after having dissected and photographed the joints. Results: Using 50% less scans than reported previously can lead to robust calculation of fiber orientations in the presence of noise, with much higher accuracy. The 6 caprine knees were found to range from very immature ( 3 years). Mature specimens exhibited significantly more aligned collagen fibers in their patella tendons compared with the immature ones. In 2 of the 10 canine knees scanned, partial cranial caudal ligament tears were identified from MRI and subsequently confirmed with encouragingly high consistency of tractography, Alignment Index, and dissection results. Conclusion: This method can be used to detect injury such as partial ligament tears, and to visualize maturity‐related changes in the collagen structure of tendons. It can provide the basis for new, noninvasive diagnostic tools in combination with new scanner configurations that allow less‐restricted field orientations

Normal black holes in bulge-less galaxies: the largely quiescent, merger-free growth of black holes over cosmic time

© 2018 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).Understanding the processes that drive the formation of black holes (BHs) is a key topic in observational cosmology. While the observed M BH-M Bulge correlation in bulge-dominated galaxies is thought to be produced by major mergers, the existence of an M BH-M* relation, across all galaxy morphological types, suggests that BHs may be largely built by secular processes. Recent evidence that bulge-less galaxies, which are unlikely to have had significant mergers, are offset from the M BH-M Bulge relation, but lie on the M BH-M* relation, has strengthened this hypothesis. Nevertheless, the small size and heterogeneity of current data sets, coupled with the difficulty in measuring precise BH masses, make it challenging to address this issue using empirical studies alone. Here, we use Horizon-AGN, a cosmological hydrodynamical simulation to probe the role of mergers in BH growth over cosmic time. We show that (1) as suggested by observations, simulated bulge-less galaxies lie offset from the main M BH-M Bulge relation, but on the M BH-M* relation, (2) the positions of galaxies on the M BH-M* relation are not affected by their merger histories, and (3) only ~35 per cent of the BH mass in today's massive galaxies is directly attributable to merging - the majority (~65 per cent) of BH growth, therefore, takes place gradually, via secular processes, over cosmic time.Peer reviewedFinal Published versio

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete release of the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, which reached its goal of surveying over 10,000 nearby galaxies. The complete release of the MaNGA Stellar Library (MaStar) accompanies this data, providing observations of almost 30,000 stars through the MaNGA instrument during bright time. DR17 also contains the complete release of the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) survey which publicly releases infra-red spectra of over 650,000 stars. The main sample from the Extended Baryon Oscillation Spectroscopic Survey (eBOSS), as well as the sub-survey Time Domain Spectroscopic Survey (TDSS) data were fully released in DR16. New single-fiber optical spectroscopy released in DR17 is from the SPectroscipic IDentification of ERosita Survey (SPIDERS) sub-survey and the eBOSS-RM program. Along with the primary data sets, DR17 includes 25 new or updated Value Added Catalogs (VACs). This paper concludes the release of SDSS-IV survey data. SDSS continues into its fifth phase with observations already underway for the Milky Way Mapper (MWM), Local Volume Mapper (LVM) and Black Hole Mapper (BHM) surveys