93 research outputs found
Rapid-response radio observations of short GRB 181123B with the Australia Telescope Compact Array
We introduce the Australia Telescope Compact Array (ATCA) rapid-response mode
by presenting the first successful trigger on the short-duration gamma-ray
burst (GRB) 181123B. Early-time radio observations of short GRBs may provide
vital insights into the radio afterglow properties of Advanced LIGO- and
Virgo-detected gravitational wave events, which will in turn inform follow-up
strategies to search for counterparts within their large positional
uncertainties. The ATCA was on target within 12.6 hr post-burst, when the
source had risen above the horizon. While no radio afterglow was detected
during the 8.3 hr observation, we obtained force-fitted flux densities of and Jy at 5.5 and 9 GHz, respectively. Afterglow
modelling of GRB 181123B showed that the addition of the ATCA force-fitted
radio flux densities to the Swift X-ray Telescope detections provided more
stringent constraints on the fraction of thermal energy in the electrons
(log rather than log derived without the inclusion of the ATCA values), which
is consistent with the range of typical derived from GRB afterglow
modelling. This allowed us to predict that the forward shock may have peaked in
the radio band days post-burst, producing detectable radio emission
days post-burst. Overall, we demonstrate the potential for
extremely rapid radio follow-up of transients and the importance of triggered
radio observations for constraining GRB blast wave properties, regardless of
whether there is a detection, via the inclusion of force-fitted radio flux
densities in afterglow modelling efforts.Comment: 15 pages, 7 figures, accepted for publication in MNRA
A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597-3704, in the Globular Cluster NGC 6256
We present Karl G. Jansky Very Large Array radio frequency observations of the new accreting millisecond X-ray pulsar (AMXP), IGR J16597-3704, located in the globular cluster NGC 6256. With these data, we detect a radio counterpart to IGR J16597-3704, and determine an improved source position. Pairing our radio observations with quasi-simultaneous Swift/XRT X-ray observations, we place IGR J16597-3704 on the radio-X-ray luminosity plane, where we find that IGR J16597-3704 is one of the more radio-quiet neutron star low-mass X-ray binaries known to date. We discuss the mechanisms that may govern radio luminosity (and in turn jet production and evolution) in AMXPs. Furthermore, we use our derived radio position to search for a counterpart in archival Hubble Space Telescope and Chandra X-ray Observatory data, and estimate an upper limit on the X-ray luminosity of IGR J16597-3704 during quiescence
From Analogical Proportion to Logical Proportions
International audienceGiven a 4-tuple of Boolean variables (a, b, c, d), logical proportions are modeled by a pair of equivalences relating similarity indicators ( a∧b and a¯∧b¯), or dissimilarity indicators ( a∧b¯ and a¯∧b) pertaining to the pair (a, b), to the ones associated with the pair (c, d). There are 120 semantically distinct logical proportions. One of them models the analogical proportion which corresponds to a statement of the form “a is to b as c is to d”. The paper inventories the whole set of logical proportions by dividing it into five subfamilies according to what they express, and then identifies the proportions that satisfy noticeable properties such as full identity (the pair of equivalences defining the proportion hold as true for the 4-tuple (a, a, a, a)), symmetry (if the proportion holds for (a, b, c, d), it also holds for (c, d, a, b)), or code independency (if the proportion holds for (a, b, c, d), it also holds for their negations (a¯,b¯,c¯,d¯)). It appears that only four proportions (including analogical proportion) are homogeneous in the sense that they use only one type of indicator (either similarity or dissimilarity) in their definition. Due to their specific patterns, they have a particular cognitive appeal, and as such are studied in greater details. Finally, the paper provides a discussion of the other existing works on analogical proportions
An overview of jets and outflows in stellar mass black holes
In this book chapter, we will briefly review the current empirical
understanding of the relation between accretion state and and outflows in
accreting stellar mass black holes. The focus will be on the empirical
connections between X-ray states and relativistic (`radio') jets, although we
are now also able to draw accretion disc winds into the picture in a systematic
way. We will furthermore consider the latest attempts to measure/order jet
power, and to compare it to other (potentially) measurable quantities, most
importantly black hole spin.Comment: Accepted for publication in Space Science Reviews. Also to appear in
the Space Sciences Series of ISSI - The Physics of Accretion on to Black
Holes (Springer Publisher
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