Un succes (explications ci dessous)
Les premieres franges d’interferences
obtenues en recombinant la lumiere venant des 2 telescopes
Keck1 et Keck2,
a l’aide de fibres optiques monomodes.
This is the first time that
fibers are successfully used
as a replacement for mirrors to bring the light from
different telescopes to a
common interferometric focus.
C’est une premiere
this feels like a wonderful achievement right now,
these first fringes are also the start of an
exciting and promising
experimental adventure.
Les premieres franges,
Sujet: Premieres franges
De: Guy Perrin
<guy.perrin@obspm.fr>
A: ….
Date: Sam, 18
Juin 2005, 17:12
Chers tous,
nous avons enfin obtenu ces premieres franges 'OHANA. Et
dans des
conditions une nouvelle fois difficiles. Ciel quasi
totalement couvert.
Plus un florilege de petits problemes.
Les premieres franges ont ete obtenues sur une etoile de
magnitude 4,6
en K, 107 Hercule (voir ci-dessous). La sensibilite
n'etait pas
mauvaise compte-tenu des conditions. La dispersion visible
dans les
franges n'est pas due aux fibres 'OHANA mais aux deux dichroiques de
Keck 1 et Keck 2 de nature differentes !
Il est pour nous temps d'aller dormir apres cette tres
tres longue
journee.
Merci a tous ceux qui ont travaille et apporte leur
soutien a 'OHANA.
C'est une premiere etape qui en verra d'autres.
Guy et toute l'equipe 'OHANA.
………………….
Sujet: `Ohana fringes at
Keck!
De: "Olivier Lai <Olivier Lai" <lai@cfht.hawaii.edu>
A: ohana@cfht.hawaii.edu
Date: Mar, 21 Juin 2005, 23:38
Dear OHANA Committee and
extended `Ohana,
It is with great pleasure that I am
writing to you on behalf of the
entire `Ohana team on this
happy and important occasion. Indeed on
Saturday June 18th, at 00:26 am, fringes were obtained with the OHANA
fibers at the Keck
Interferometer: these were obtained on
a K = 4.61
star (we picked a star bright enough to ensure a
high SNR to maximise
our chances to find the fringes,
of course!), 107 Hercules, and the
sensitivity was very
encouraging (more quantitative details
forthcoming
once we all get some
rest!). This is the first time
that fibers are
successfully used as a replacement for mirrors to bring the light from
different telescopes to a
common interferometric focus.
The preceding two
weeks were filled with alignment, internal
fringes,
vibration damping, more alignement and beautiful
weather. Once again,
`Ohana suffered from clouds
on Mauna Kea, but for once these were cirrus
rolling in on the second half of the night, so
this is an improvement
over our last 4 runs! We did loose some time to varying absorption (at
4:00am, the moon was completely hidden), and with the usual unexpected
problems that had to be
solved in real time.
We learnt many things in
one short night, both on our injection
modules
and ways to improve our
observing efficiency but also on the Keck AO and
interferometer systems. As
can be duly expected, our efficiency
was not
very high during the beginning of this very first night of
operation
(but it did improve towards the end). The prototpype OHANA
requires a
lot of
operations with two injection
modules, two AOs,
and an
interferometer. The
injection modules had to be realigned to a very high
level of precision on a regular basis to ensure maximum
coupling into
the fibers. Slight temperature drifts in
the interferometric lab
required the OHANA fibers to be recentered with respect to the Keck
system. These are normal procedures that would need
to be streamlined
and improved during a
commissioning phase.
Dispersion is present in these very first fringes due
to different
dichroics in the two Keck
AO systems (the internal fringes showed
none)
thus reducing the fringe contrast; however, this did
not prevent from
finding them which is
encouraging. In any case, we see clear ways on how
to improve our subsystems, and so while
this feels like a wonderful
achievement right now,
these first fringes are
also the start of an
exciting and promising
experimental adventure.
Aloha,
Olivier on behalf of the
entire `Ohana team