Aloha TMT

In a long awaited announcement, America’s largest optical telescope project unveiled the chosen site for its new observatory. After a long and extensive campaign of site testing and comparison, and, more importantly perhaps, much politicking, the Thirty Meter Telescope board have reached an agreement to build their telescope on the Mauna Kea in Hawaii.

The TMT, a collaboration of US, Canadian and Japanese institutes, is one of three projects in the so-called class of extremely large telescopes, or ELTs. In the last year, two potenial sites were studied in a final run-off: the well known Hawaiian mountain Mauna Kea, and Cerro Armazones, an as yet undeveloped site in the Chilean Andes. As both sites are excellent from the astroclimatological perspective, it is rumoured that the Japanese involvement was at least partly responsible for the final choice. All three of the partner countries already have telescopes and infastructure on Mauna Kea.

With the smallest of the ELTs, the 24-m
Giant Magellan Telescope confirmed to be sited at Las Campanas, also in Chile, and ESO’s strong ties with the country, TMT will ensure that an ELT will also be watching the Northern skies. In addition seems sensible to question the sanity of locating three of the world’s most powerful telescopes in a relatively small area – and one with substantial seismic activity at that.

All eyes are now on ESO, whose 42-m ELT project, the imaginatively named European ELT, is the last in the trio to be found a home. While ESO are running an extensive testing campaign at 5 sites around the world, there is much speculation that TMT’s second-choice site, Armazones, could now be in the running for the E-ELT. An announcement from ESO is expected in the next year.

.Astronomy 2009: More info on registration

dotastro_banner

[Cross-posted from the .Astronomy blog]

Over at .Astronomy HQ we’re excited that the registration for the 2009 workshop in Leiden is under way. However I wanted to put here a little more info on the registration process, the form and the format of the workshop – so that we can learn more about you, the participants.

The workshop will be relatively small, with the number of participants limited to 50. This will allow us to make optimal use of the excellent Lorentz Center facilities. We’ve had a lot of interest and we expect that the workshop will fill up well before the starting date – so if you’d like to join us, please don’t wait to register.

Between us, the organisers, we know lots of people who are involved in great initiatives and projects in web-based science and astronomy. Some of these people will have received invites from the Lorentz Center to register for .Astronomy but there are plenty of places left for those who weren’t invited. If you didn’t get an invitation, this doesn’t mean we don’t want you to attend. In fact, we want you to attend more. This is why we’re advertising the workshop widely via Twitter and our blogs.

[Read more...]

Grand tour

Welcome to my blog’s new home. I decided to move to my own domain because WordPress’ free hosting, while it’s amazingly efficient and user friendly, is a little more restrictive than the standalone version (e.g. no javascript).

“Grand tour” is really only meant ironically as there is not much difference between this and the old site. But take a look round, grab a beer and play with the cat. Thanks for the visit.

Image: Betsy Malloy (2006)

More success for Herschel

After the early sneak preview from the PACS instrument on board the recently launched Herschel infrared space telescope, more images have now been released from its other instruments, SPIRE and HIFI. The above image shows images taken with the IR imager and spectrometer SPIRE of nearby galaxy M74 at 250 micron. The amount of detail visible in the images is really great, particularly as all the image reconstruction software hasn’t even been optimised yet. We may be very used to seeing spectacularly detailed images from Hubble, but achieving these resolutions at Herschel’s far-infrared wavelengths is very new. [Read more...]

NTT snaps the Omega Nebula

This beautiful picture of the Omega Nebula (M17) was released today by ESO. It’s a three-colour composite image taken with the 3.6-m New Technology Telescope at ESO’s La Silla site in Chile. The nebula is a region of active star formation, one of the youngest and nearest to our solar system. A recent paper by Matthew Povich and collaborators reported over 90 candidate newborn stars in the region at varying stages of starbirth. Energetic radiation from hot young stars is exciting and lighting up the gas in the nebula.

The Povich paper contains a complete description of this hotbed of star formation at wavelengths from the radio to X-ray and is an excellent reference if you wold like to learn more.

Image credit: ESO