Welcome!
Welcome to the issue 4 of the e-
MERLIN newsletter. 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 !
First e-MERLIN Data
school held at JBCA
Last week at JBCA (23-25
October), we held the first e-
MERLIN data school. Participants
learnt about using the e-MERLIN
CASA Pipeline (eMCP) to
calibrate and image e-MERLIN
data. The ORP sponsored event
enabled students from across the
world to bring their own e-
MERLIN data to get expert help
from the in-house operations
team at Jodrell Bank.!
Missed the data school? We’ve
placed all of the documentation
online here. We will also be
holding similar events in the
future, including hybrid versions
so that more people can attend.
Please get in touch if you are
interested in in-person or hybrid
events such as this in the future.
e-MERLIN detections of oset dual-
SMBH candidates proves fruitful
Dual super massive black holes (SMBH) may appear in
the post-merger stage of galaxies and as the system
evolves the two SMBHs would get closer to each other
and coalesce. Such dual SMBHs may appear as a dual
AGN (active galactic nuclei) if both SMBHs are
accreting, or an o-nucleus AGN, if only one SMBH is
active. However dual and o-nucleus AGN were
previously found mostly at low redshifts or large
separations (> 10 kpc).!
One promising technique is that of varstrometry, which
uses the astrometric jitter of the photocenter in Gaia
observations to identify candidate dual AGNs. In this
study, five such sources were selected for e-MERLIN
follow-up and four of them showed significant radio-
optical osets, suggesting an oset radio-loud nucleus
and the optical photocenter of the dual SMBH system.
This large oset is not normally seen in quasars, further
favouring the dual or o-nucleus scenario. Thus, e-
MERLIN observations of such systems could be a
potentially fruitful probe of dual-SMBHs in the future.!
Read the full paper here (Wang et al. 2023, MNRAS
Letters, Volume 524, Issue 1, p.L38)!
User Newsletter
Issue 4 3 November 2023"
Radio-optical offsets of five dual-SMBH
candidates
Announcements
EVN Call for Proposals.
Deadline 1 February 2023. Click
here for further information!
VLBI observations of Palomar-Green
quasars, including EVN+e-MERLIN
Very long baseline interferometry can be a powerful
tool for providing insights into the origins of the
nuclear radio emission in quasars. In radio-quiet
quasars (RQQs), it is especially important as a high-
brightness temperature core at sub-arcsecond
resolution can be attributed to the presence of jets or
coronae from an accreting AGN, rather than star
formation or winds. By combining multiple VLBI
datasets, from VLA, VLBA, e-MERLIN and EVN, 20
Palomar-Green quasars at low redshift (z<0.5) were
studied with unequivocal detections on 10 of them.
For the source with combined EVN + e-MERLIN data,
it was possible to recover diuse emissions from an
intricate jet structure at a noise level of 9 µJy per
beam.!
Read the full papers here (Wang et al. 2023a,
MNRAS, Volume 518, Issue 1, p 39) and here (Wang
et al 2023b, MNRAS, Volume 525, Issue 4, p 6064).!
e-MERLIN Cycle 17 call for proposals
The e-MERLIN cycle 17 call for proposals has now
closed. Cycle 18 will be announced in Spring 2024.
Please see the e-MERLIN observe page for more
details.
A new frequency flexibility system
has been developed by JBO
engineers to enable rapid
swapping between L and C band
on the Lovell telescope. It is
pictured above in the workshops
being tested. It has recently been
installed onto the Lovell and after
some further checks will be ready
for use later this year.
www.e-merlin.ac.uk
52nd YERAC a success at JBCA/JBO
The Jodrell Bank Centre for Astrophysics hosted more
than 30 young astronomers to continue the long
tradition of the Young European Radio Astronomer’s
Conference (YERAC). YERAC gives early career
researchers working across Europe (and more broadly
worldwide) a fun and welcoming atmosphere to meet
their peers, present their own research and learn
about all aspects of radio astronomy. This year,
YERAC participants gave talks on a wide variety of
fields, including pulsars, AGNs, galaxy evolution,
masers and much more. Participants also had a day
out at the observatory, hearing from SKA director
general Phil Diamond and exploring the First Light
Pavilion at Jodrell Bank’s visitor centre. The next
YERAC will be held at Yebes in 2024, but you can
reminisce about previous YERACs on the JIVE
webpages here.
52nd YERAC conference photo in front of the Lovell
Meetings/Workshops
Breakthrough Listen UK Kick-
O SKAO HQ, UK, 13-15
November 2023, Click here for
more details !
SPINS-UK 2023 Oxford, UK,
22-24 November 2023, Click
here for more details !
7th LOFAR Data School
Dwingeloo, Netherlands, 15-19
April 2024, Registration
deadline: 30 November 2023.
Click here for more details !
AGN across continents
conference Durham, UK, 8-12
July 2024. Abstract submission
deadline: 3 November 2023.
Click here for more details!
European ALMA School
Manchester, UK, 10-14 June
2024, Registration deadline: 31
December 2023. Click here for
more details!
SPARCS XII Bologna, Italy, 6-10
May 2024, Registration
deadline: TBC. Click here for
more details