New Neighbours: Modelling the Growing Population of Gamma-ray Millisecond Pulsars

The Fermi Large Area Telescope, in collaboration with several groups from the radio community, have had marvellous success at uncovering new gamma-ray millisecond pulsars (MSPs). In fact, MSPs now make up a sizable fraction of the total number of known gamma-ray pulsars. The MSP population is characterized by a variety of pulse profile shapes, peak separations, and radio-to-gamma phase lags, with some members exhibiting nearly phase-aligned radio and gamma-ray light curves (LCs). The MSPs' short spin periods underline the importance of including special relativistic effects in LC calculations, even for emission originating from near the stellar surface. We present results on modelling and classification of MSP LCs using standard pulsar model geometries.Comment: 4 pages, 2 figures, proceedings of the ICREA Workshop on The High-Energy Emission from Pulsars and their Systems (HEEPS), Sant Cugat, Spai

Radio pulsar populations

The goal of this article is to summarize the current state of play in the field of radio pulsar statistics. Simply put, from the observed sample of objects from a variety of surveys with different telescopes, we wish to infer the properties of the underlying sample and to connect these with other astrophysical populations (for example supernova remnants or X-ray binaries). The main problem we need to tackle is the fact that, like many areas of science, the observed populations are often heavily biased by a variety of selection effects. After a review of the main effects relevant to radio pulsars, I discuss techniques to correct for them and summarize some of the most recent results. Perhaps the main point I would like to make in this article is that current models to describe the population are far from complete and often suffer from strong covariances between input parameters. That said, there are a number of very interesting conclusions that can be made concerning the evolution of neutron stars based on current data. While the focus of this review will be on the population of isolated Galactic pulsars, I will also briefly comment on millisecond and binary pulsars as well as the pulsar content of globular clusters and the Magellanic Clouds.Comment: 16 pages, 6 figures, to appear in Proceedings of ICREA Workshop on The High-Energy Emission from Pulsars and their Systems, Sant Cugat, Spain, 2010 April 12-16 (Springer

Effects of Antiepileptic Drugs on GABA Responses and on Reduction of GABA Responses by PTZ and DMCM on Mouse Neurons in Cell Culture

The mechanisms of action of antiepileptic drugs effective against generalized absence seizures (antiabsence AEDs) remain uncertain. Antiabsence AEDs are generally effective against seizures induced in experimental animals by pentylenÉtÉtrazol (PTZ) and methyl-6,7-dimethoxy-4-ethyl-Β-carboline-3-carboxylate (DMCM), drugs which reduce GABAergic inhibition. Thus, antiabsence AEDs have been suggested to enhance GABAergic inhibition. We studied the effects of several AEDs on GABA responses recorded from mouse spinal cord neurons grown in primary dissociated cell culture. Four antiabsence AEDs were included: ethosuximide (ESM), dimethadione (DMO), sodium valproate (VPA), and diazepam (DZP). Two experimental AEDs, CGS 9896 and ZK 91296, with anticonvulsant action against PTZ- or DMCM-induced seizures were also included. Possible effects of the antiabsence and experimental AEDS on PTZ- and DMCM-induced inhibition of GABA responses were also evaluated. PTZ and DMCM revers-ibly reduced GABA responses in a concentration-dependent manner. PTZ complÉtÉly inhibited GABA responses at 10 mM (IC 50 of 1.1 mM), whereas DMCM-induced inhibition of GABA responses reached a plateau level of 39% of control values at 1 p.M (IC 50 of 33 nM). ESM (1,200 ΜM), DMO (6 mM), VPA (200 u.M), CGS 9896 (2 ΜM), and ZK 98% (2 Μ M ) did not alter GABA responses. DZP enhanced GABA responses in a concentration-dependent manner. The inhibition of GABA responses produced by PTZ 1 mM was unaltered by ESM (600 Μ M ), DMO (6 mM), CGS 9896 (1 Μ M), or ZK 9896 (1 ΜM)- Coapplication of VPA (200 ΜM) and PTZ (1 mM) slightly enhanced the PTZ effect. DZP (> 10 nM), however, reversed the PTZ-induced reduction of GABA responses. The DMCM (250 nM) inhibition of GABA-responses was unaltered by ESM (600 Μ.M), DMO (2 mM), or VPA (200 ΜM). CGS 9896 (2 Μ M ) and ZK 91296 (2 ΜM), however, antagonized the DMCM effect. DZP (> 10 nM) significantly reversed the DMCM-induced inhibition of GABA responses. The lack of effect of VPA, ESM, and DMO on postsynaptic GABA responses suggests that direct enhancement of postsynaptic GABA action is not a common mechanism of action of antiabsence AEDs. The AEDs DZP, CGS 98%, and ZK 912% all reversed DMCM, but not PTZ, reduction of GABA responses, suggesting that these AEDs blocked DMCM seizures by acting at benzodiazepine receptors. However, since only DZP enhanced GABA responses, it is unclear how CGS 98% and ZK 912% blocked PTZ seizures. Key Words: Anticonvulsants–GABA–Neuron culture–Cell culture–Spinal cord neurons–Convulsants. RESUMEN Los mecanismos de accidn de las medicaciones antiepilÉpticas eficaces contra los ataques generalizados de ausencia (AEDs antiausencia) permanecen inciertos. Los AEDs antiausencia son, generalmente, eficaces contra ataques experimentales inducidos por el pentilentetrazol (PTZ) y el metil-6,7-dimetoxy-4-etil-Pcarbolina-3-carboxilato (DMCM) en animates, medicaciones que reducen la inhibiciÓn GABAÉrgica. Hemos estudiado los efectos de varios AEDs sobre respuestas-GABA registradas en las neuronas de la mÉdula espinal de ratones que habian crecido en cultivos de cÉlulas primarieas disociadas. Cuatro AEDs antiausencia fueron incluidos: etoxusimida (ESM), dimetadiona (DMO), valproato sÓdico (VPA) y diazepan (DZP). TambtÉn se incluyeron dos AEDs experimentales, CGS 9896 y ZK 912%, con acciÓn anticonvulsiva contra los ataques inducidos por PTZ o DMCM. TambiÓn se valoraron los posibles efectos de los AEDs antiausencia y experimentales sobre el PTZ y la inhibiciÓn de las respuestas-GABA inducidas por el DMCM. El PTZ y el DMCM redujeron las respuestas-GABA de modo reversible y dependiendo de sus concentraciones. El PTZ inhibiÓ cmpleta-mente las respuestas-GABA a 10 mM (IC 50 de 1.1 mM) mientras que la inhibitiÓn de las respuestas GABA inducida por el DMCM alcanzÓ un nivel estable del 39% de los valores control con 1 Μ. M (IC 50 de 33 mM). La ESM (1200 Μ.M), la DMO (6 mM), el VPA (200 Μ M ), el CGS 98% (2 Μ M) y el ZK 98% (2 Μ M) no alteraron las respuestas-GABA. El DZP aumentÓ las respuestas GABA de una manera concentraciÓn-dependiente. La inhibition de las respuestas-GABA producidas por el PTZ (1 mM), no se altero con las ESM (600 Μ M), la DMO (6 mM), el CGS 98% (1 Μ M) o el ZK 98% (1 Μ .M). La co-aplicacion de VPA (200 Μ M) y el PTZ (1 mM) aument6 ligeramente los efectos del PTZ. Sin embargo el DZP (10 nM) revirtiÓ significativamente la inhibition de las respuestas GABA inducidas por el DMCM. La falta de efectos de CPA, ESM y DMO sobre las respuestas GABA post-sinÁpticas sugiere que el incremento de la acciÓn GABA post-sinÁptica no es un mecanismo comÚn de actuatiÓn de las AEDs antiausencia. Todas las AEDs DZP, CGS 98% y ZK 912% revirtieron la reduction de las respuestas GABA producidas por el DMCM pero no las inducidas por el PTZ lo que sugiere que estos AEDs bloquean los ataques DMCM actuando sobre los receptores de la benzodiazepina. Sin embargo, puesto que el incremento de las respuestas GABA sÓlÓ se produce por el DZP, permanece todavia sin aclarar el por quÉ el CGS 98% y el ZK 912% bloquean los ataques producidos por el PTZ. ZUSAMMENFASSUNG Der Wirkmechansimus von Antiepileptika gegen generalisierte Absencen ist unklar. Antiabsencemittel sind generell wirkungs-voll gegen PTZ- und Methyl-6,7-Dimethoxy-4-Äthyl-P-Carbolin-Β-Carboxylat (DMCM) induzierte tierexperimentelle AnfÄlle, also von Medikamenten, die die GABA-erge Inhibition reduzieren. Es wurde vermutet, daß Antiabsencemittel die GABA-erge Inhibition verstÄrken. Wir untersuchten die Wirkung von verschiedenen Antiepileptika auf GABA-Antworten in spinalen MÄuseneuronen, die in Zellkulturen gew-achsen waren. Es wurden 4 Absencemittel untersucht: Ethosux-imid (ESM), Dimethadion (DMD), Sodium Valproat (VPA) und Diazepam (DZP). ZusÄtzlich wurden 2 experimentelle Antiepileptika, CGS 98% und ZK 912%, die gegen PTZ0 oder DMCM-induzierte AnfÄlle wirkungsvoll sind, eingeschlossen. Mogliche Wirkungen der Antiabsence- und experimentellen Antiepileptika auf PTZ- und DMCM-induzierte Hemmung der GABA-Antworten wurden ebenfalls ausgewertet. PTZ und DMCM zeigten eine konzentrationsabhÄngige reversible Reduktion der GABA-Antworten. PTZ zeigte eine komplette Hemmung der GABA-Antworten bei 10 mM (IC 50 1,1 mM), DMCM-Hemmung der GABA-Antworten zeigte ein Plateau von 39% der Kontroll-werte bei 1 uJtf (ICJO von 33 mAfl. ESM (1200 uJtf), DMD (6 mM), VPA (200 Μ M), CGS 98% (2 Μ M) und ZK 98% (2 Μ M) anderten nicht die GABA-Antworten. DZP verstarkte die GABA-Antworten konzentrationsabhangig. Die durch PTZ (1 mM) hervorgerufene Hemmung der GABA-Antworten war bei ESM (600 Μ M), DMD (6 mM), CGS 98% (1 mAO und ZK 3836 (1 mM) unverÄndert. ZusÄtliche Anwendung von VPA (200 mM) und PTZ (1 mM) verstÄrkten geringfÜgig den PTZ-Effekt. DZP (10 nM) kehrte die durch PTZ hervorgerufene Reduktion der GABA-Antworten um. Die durch DMCM (250 nM) hervorgerufene Hemmung der GABA-Antworten war durch ESM (600 Μ .M), DMD (2 mM) und VPA (200 Μ M ) unbeeinflusst. CGS 98% (2 Μ M) und ZK 912% (2 Μ M ) antagonisierten die DMCM-Wirkung. DZP (>10 nM) kehrte die durch DMCM-induzierte Hemmung der GABA-Antworten um. Das Fehlen einer Wirkung von VPA. ESM und DMD auf die postsynaptischen GABA-Antworten legen nahe, daß eine direkte VerstÄrkung der postsynaptischen GABA-Aktion kein gemeinsamer Mechanis-mus der Antiabsencemittel darstellt. Die Antiepileptika DZP, CGS 98% und ZK 912% kehrten die DMCM-Wirkung auf die GABA-Antworten um, jedoch nicht die von PTZ, was vermuten lapt, daß diese Antiepileptika die DMCM-AnfÄlle Über die Wirkung an den Benzodiazipin-Rezeptoren verhinderte. Da jedoch nur DZP GABA-Antworten verstarkte, ist unklar, in welcher Weise CGS 98% und ZK 912% die PTZ-AnfaUe ver-hinderten.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/65188/1/j.1528-1157.1989.tb05275.x.pd

Binary and Millisecond Pulsars at the New Millennium

We review the properties and applications of binary and millisecond pulsars. Our knowledge of these exciting objects has greatly increased in recent years, mainly due to successful surveys which have brought the known pulsar population to over 1300. There are now 56 binary and millisecond pulsars in the Galactic disk and a further 47 in globular clusters. This review is concerned primarily with the results and spin-offs from these surveys which are of particular interest to the relativity community.Comment: 59 pages, 26 figures, 5 tables. Accepted for publication in Living Reviews in Relativity (http://www.livingreviews.org

Fermi Large Area Telescope observations of PSR J1836+5925

The discovery of the gamma-ray pulsar PSR J1836+5925, powering the formerly unidentified EGRET source 3EG J1835+5918, was one of the early accomplishments of the Fermi Large Area Telescope (LAT). Sitting 25 degrees off the Galactic plane, PSR J1836+5925 is a 173 ms pulsar with a characteristic age of 1.8 million years, a spindown luminosity of 1.1$\times10^{34}$ erg s$^{-1}$, and a large off-peak emission component, making it quite unusual among the known gamma-ray pulsar population. We present an analysis of one year of LAT data, including an updated timing solution, detailed spectral results and a long-term light curve showing no indication of variability. No evidence for a surrounding pulsar wind nebula is seen and the spectral characteristics of the off-peak emission indicate it is likely magnetospheric. Analysis of recent XMM observations of the X-ray counterpart yields a detailed characterization of its spectrum, which, like Geminga, is consistent with that of a neutron star showing evidence for both magnetospheric and thermal emission.Comment: Accepted to Astrophysical Journa

Binary and Millisecond Pulsars

We review the main properties, demographics and applications of binary and millisecond radio pulsars. Our knowledge of these exciting objects has greatly increased in recent years, mainly due to successful surveys which have brought the known pulsar population to over 1700. There are now 80 binary and millisecond pulsars associated with the disk of our Galaxy, and a further 103 pulsars in 24 of the Galactic globular clusters. Recent highlights have been the discovery of the first ever double pulsar system and a recent flurry of discoveries in globular clusters, in particular Terzan 5.Comment: 77 pages, 30 figures, available on-line at http://www.livingreviews.org/lrr-2005-

Relativistic Binaries in Globular Clusters

Galactic globular clusters are old, dense star systems typically containing 10\super{4}--10\super{7} stars. As an old population of stars, globular clusters contain many collapsed and degenerate objects. As a dense population of stars, globular clusters are the scene of many interesting close dynamical interactions between stars. These dynamical interactions can alter the evolution of individual stars and can produce tight binary systems containing one or two compact objects. In this review, we discuss theoretical models of globular cluster evolution and binary evolution, techniques for simulating this evolution that leads to relativistic binaries, and current and possible future observational evidence for this population. Our discussion of globular cluster evolution will focus on the processes that boost the production of hard binary systems and the subsequent interaction of these binaries that can alter the properties of both bodies and can lead to exotic objects. Direct {\it N}-body integrations and Fokker--Planck simulations of the evolution of globular clusters that incorporate tidal interactions and lead to predictions of relativistic binary populations are also discussed. We discuss the current observational evidence for cataclysmic variables, millisecond pulsars, and low-mass X-ray binaries as well as possible future detection of relativistic binaries with gravitational radiation.Comment: 88 pages, 13 figures. Submitted update of Living Reviews articl

Functional annotation of the cattle genome through systematic discovery and characterization of chromatin states and butyrate-induced variations

The functional annotation of genomes, including chromatin accessibility and modifications, is important for understanding and effectively utilizing the increased amount of genome sequences reported. However, while such annotation has been well explored in a diverse set of tissues and cell types in human and model organisms, relatively little data are available for livestock genomes, hindering our understanding of complex trait variation, domestication, and adaptive evolution. Here, we present the first complete global landscape of regulatory elements in cattle and explore the dynamics of chromatin states in rumen epithelial cells induced by the rumen developmental regulator—butyrate.https://doi.org/10.1186/s12915-019-0687-