Psalm 22 LXX in Origen’s commentary on the Song of Songs

This article examines three distinct ways of reading Psalm 23(LXX 22), first in the Targum, then in the liturgy of early Christian initiation, and finally in Origen’s commentary on the Song of Songs. The Targum focuses on God’s protective presence in Israel’s history and looks forward to the salvation to come. Reading the psalm in the context of Christian initiation draws out the contextual possibilities of the text. In his interpretation of the Song of Songs, Origen seeks elements of spiritual progress after the stage of initiation. The “inebriating cup” points to a strongly affective dimension of this process

Philo’s De Decalogo: educating to respect the socially disadvantaged

Respect and care for the disadvantaged are firmly embedded in Philo’s interpretation of the Decalogue. In order to understand Philo’s teaching on this point within its proper perspective, this study highlights the following aspects of his interpretation of the Decalogue. The Ten Commandments are intended as a means of education, healing and transformation of people and their communities; they guide people to live in harmony with nature, reason and one another; in practice, this means to learn how to turn away from foolish pride and to live in gentleness, fellowship, simplicity, and equality. Such education will render people sensitive to the needs of those affected by bad fortune and inspire them to reach out to them

Pointing out persuasion in Philemon: Fifty readings of Paul’s rhetoric from the fourth to the eighteenth century

This informative and insightful work reveals the vast field of the history and life of the Letter to Philemon after it was written. This approach to biblical texts has received greater attention in recent years when the reader’s contribution to the meaning of textswas first recognised. This attention to the reception of biblical texts is the special subject of the Encyclopedia of the Bible and Its Reception (EBR), which started in 2009 and of which 20 volumes have already been published. This encyclopedia surveys not only sermons and commentaries, but also the various ways in which biblical texts have been received, such as in the creative arts, including paintings, sculptures, novels, films and music. Professor Tolmie’s study, however, focuses on how commentators and preachers have “pointed out persuasion” in this Pauline letter. He has selected, as the subtitle indicates, 50 readings of Philemon from three periods, the early church (starting with Ambrosiaster in chapter 1), the Middle Ages (chapter 2), and the period from the 16th to the 18th century (Chapter 3). For each of these interpreters, Tolmie offers a brief introduction and then focuses on the way they explain the rhetorical situation. He then focuses on the way each author explains the rhetorical strategy by moving through the letter, section by section. Chapter 4, the conclusion, is actually a synthesis, in which Tolmie looks for tendencies in the interpretation of Paul’s letter by focusing first on the way the rhetorical situation is imagined and then on Paul rhetorical strategies in the different literary units of Philemon

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta