!
Welcome!
Welcome to the new e-MERLIN
newsletter. Every quarter we will
be publishing e-MERLIN-related
news and science highlights,
including calls for proposals,
adverts for summer schools and
links to e-MERLIN partners like
the EVN and ORP. If you would
like to contribute to the e-MERLIN
newsletter, please get in touch at:
emerlin.support@jb.man.ac.uk "
If you have any suggestions for
additions or topics, please don’t
hesitate to get in touch too!"
Detecting the BOAT
with e-MERLIN
On 9th October 2022, the
brightest gamma ray burst of all
time (i.e. the “BOAT”) was
detected with the Neil Gehrels
Swift Observatory. At a redshift of
z~0.15, it is one of the nearest
GRBs ever recorded and was so
bright that it caused disturbances
in the Earth’s ionosphere. e-
MERLIN joined in as part of rapid
response time (RRT) observations,
detecting the source and
providing precise co-ordinates for
EVN observations to follow up.
This work is published as a GCN
here (Rhodes et al., 2022,
GCN.32700).
STFC and RADIOBLOCKS funding
streams announced
e-MERLIN is funded by UKRI-STFC and the e-MERLIN
team submitted a substantial proposal to STFC's
Projects Peer Review Panel (PPRP) last year requesting
operational funding for the period 2023-28 as well as a
'technical refresh' to replace much of the digital
equipment from the telescopes and data links to the
correlator. We are pleased to report that the PPRP
review was very positive about current and future
science with e-MERLIN and fully supported the
continuation of operations and the technical upgrade,
which also includes the start of a programme to develop
a new 8-16 GHz receiver band. STFC have now
awarded funding for the 2023-28 period and we have
started the initial design work on the key digital
upgrades. Future newsletter issues will provide updates
on the progress of this work."
Separate to the STFC funding above, e-MERLIN and
Jodrell Bank Centre for Astrophysics personnel will be
playing significant roles in the ‘RADIOBLOCKS’ Horizon
Europe project, which was recently awarded 10 million
of funding to develop new beyond-state-of-the-art
technologies and infrastructure for radio and sub-mm
telescopes for the next decades. Launching in April
2023 and lasting for four years, this project will develop
state-of-the-art receivers and correlators for radio
telescopes, as well as new data processing and imaging
methods. Prof Rob Beswick, the project lead at The
University of Manchester commented, “The project
brings together leading academic research and industry
experts from across the world to co-develop new
technologies”. A full description of the RADIOBLOCKS
project can be found here."
User Newsletter
Issue 1 24 January 2023!
A PRECISE
measurement of a
repeating FRB
The study of repeating fast radio
bursts (FRBs) has increased
exponentially in recent years
with the discovery that some
FRBs show repeat bursts.
Recently the FRB source FRB
20220912A was found to be a
very active repeater and as part
of the PRECISE project, e-
MERLIN joined other EVN
stations to observe the source
and localise the emission on
milliarcsecond scales. These
data are now being correlated
and analysis is still ongoing, but
over 150 bursts found in the
Eelsberg data were already
published as an ATel here
(Kirsten et al., 2022, ATel
15727). "
Resolving the Serpens radio jet
Young Stellar Objects (YSOs) are known to produce
radio jets, though how they are collimated and
launched is not well understood. The collimation of
these jets happens on au-scales, necessitating high-
resolution radio interferometers to reveal the relative
contributions of these dierent processes. "
As part of the Thermal Jets e-MERLIN legacy
programme, the Serpens radio jet was observed over
multiple epochs with e-MERLIN and the VLA. For the
first time for an intermediate-mass protostar, motions
on scales less than 100 au were detected, owing to
the resolving power of e-MERLIN. In fact, the central
region of the Serpens jet was resolved at ~15 au
resolution into several components, enabling the
calculation of the jet velocity which was found to be
highly variable over 10 years of observations. This
variability points to episodic variations of the accretion
rate. The inferred ~100 km/s jet velocity suggests that
it was launched from the innermost regions of the
accretion disc."
Read the full paper here (Rodríguez-Kamenetzky
et al. 2022, ApJL, 931, 2, L26).
The Mark 2 telescope
peering out through the
mist one November
morning. Credit to Anthony
Holloway (twitter: @aj_h)
The variable and evolving Serpens radio jet
e-MERLIN Cycle 15
results announced
The results for cycle 15 of the e-
MERLIN call for proposals have
now been released to PIs. The
successful programmes are
listed here.
EVN + e-MERLIN probe the recurrent
nova RS Ophiuchi
The symbiotic binary and recurrent nova RS Ophiuchi
(RS Oph) went into outburst in August 2021, the third
such outburst in the last 40 years which e-MERLIN
and its predecessors have followed at centimetre
wavelengths. EVN + e-MERLIN observations taken 34
days post-outburst showed lobes of emission
expanding outwards into the CSM at milliarcsecond
scales. The radio emission is bi-polar as the outburst
sweeps up the red giant wind. The eastern side of this
bi-polar structure is thought to be obscured due to a
density enhancement near the binary position. Using
the new GAIA position of RS Oph, the lobes were
found to be moving with velocities of ~7500 km/s and
matches optical spectroscopic data. Analysis of
additional%observations is underway and is expected
to reveal the details of the expansion%of the ejecta. "
Read the full paper here (Munari et al. 2022, A&A
Letters, 666, L6)
RS Oph’s radio structure 34 days post-outburst
Announcements
EVN Call for Proposals.
Deadline 1 February 2023.
Click here for further information"
Eelsberg Call for Proposals.
Deadline 2 February 2023.
Click here for further information"
INAF Call for Proposals
Deadline expected in April 2023.
Click here for further information"
Meetings/Workshops
ORP Proposal Writing School
On-line on 20/27 February and
6/20 March 2023. Deadline 27
January. See here for more."
IAU Symposium 378: Black
hole winds at all scales 12-16
March 2023, Haifa, Israel, Click
here for more details
Bologna VLBI: Life begins at
40! Bologna, Italy, 22-26 May
2023. Abstract submission TBC.
Click here for more details"
CASA-VLBI Workshop
Dwingeloo, Netherlands, 5-9
June 2023, Click here for more"
Get in touch
To get in touch with the e-
MERLIN support team, email:
emerlin.support@jb.man.ac.uk"