Category Archives: Profesional

AAT Outreach Exercise: “LMC Little Gems with CACTI”

Today, Thursday 24th November I’m the scheduled support astronomer at the Anglo-Australian Telescope (AAT). It is a “2dF+AAOmega service night”, meaning that I’ll be observing “service programs”, that is, science projects that require less than 6 hours in total to be completed, using the 2dF+AAOmega instruments at the 3.9m AAT.

Additionally, I’ve requested additional ~30 minutes to try to use the new CACTI camera to get a new, nice outreach image of an interesting object. As I did last May I’m asking the public to please provide feedback and help us to decide.

What do you want the AAT observes tonight?

For today’s observations I have chosen 4 objects located in the Large Magellanic Cloud (LMC),  that is why I’ve called the experiment “LMC Little Gems using CACTI”.

The chosen 4 objects are these:

1. Stellar cluster + Nebula NGC 1949
2. Globular cluster NGC 2121
3. Supernova remnant NGC 2018
4. Stellar cluster + Nebula NGC 1850

Objects chosen for the "LMC Little Gems with CACTI" Outreach Exercise at the AAT. From top left to bottom right they are: 1. Stellar cluster + Nebula NGC 1949, 2. Globular cluster NGC 2121, 3. SN remnant NGC 2018, 4. Stellar cluster + Nebula NGC 1850. Credit of the images: Digital Sky Survey, except for NGC 1850 (ESO, image obtained using the FORS1 instrument at the VLT.

Objects chosen for the “LMC Little Gems with CACTI” Outreach Exercise at the AAT. From top left to bottom right they are: 1. Stellar cluster + Nebula NGC 1949, 2. Globular cluster NGC 2121, 3. SN remnant NGC 2018, 4. Stellar cluster + Nebula NGC 1850. Credit of the images: Digital Sky Survey, except for the image of NGC 1850, credited to ESO (image obtained using the FORS1 instrument at the VLT).

I chose objects in the LMC because this region of the sky can be observed during all night this time of the year.

In addition, getting these data for outreach purposes will not interfere too much with the scientific observations, as we need to change the configuration of the instrument (the gratings of the AAOmega spectrograph) and, while the night assistant is doing that, I will be taking the data of the object chosen by the public for this outreach exercise.

So, what do you think? What do you want the AAT observes tonight?

Please use your Twitter account and cast your vote following this link.

Assuming the weather is good and we don’t have any technical problems, I should have a new, nice outreach image obtained with CACTI at the AAT by tomorrow, Friday 25th November. Stay tuned!

Spiral galaxy NGC 4027 with AAT: an outreach exercise

During this week I’m curator of the @astrotweep, a Twitter account that each week features an astronomer or planetary scientist taking about their research, science and life. I’m having a lot of fun with it, although I have to recognize it is extra work.

I chose to do it this week because there are some few things happening. In particular, I’m supporting observations at the Anglo-Australian Telescope (Siding Spring Observatory, NSW, Australia) using the 2dF / HERMES instruments. I thought it would be nice to be tweeting life how observations are doing. And that is precisely what I’ve doing today.

On top of that, “this morning” I had an idea. As we always have some “free time” at the AAT after completing the “2dF first night setup” (1) I decided to observe a nice bright deep sky object and get a nice image with the AAT. I was starting to search for a suitable target, but then I though, why don’t I ask the public what do they want to observe?

After consulting with my supervisors and getting the OK to do this, I initiated a poll in both @astrotweeps and @AAOastro asking the public to vote for one of the four following astro objects:

  1. The elliptical galaxy NGC 2865.
  2. The planetary nebula NGC 4361.
  3. The warped and almost edge-on spiral galaxy ESO 510-G13.
  4. The barred spiral galaxy NGC 4027.

For around 8 hours people were casting their vote, we received 153 unique votes in total combining the @AAOastro and the @astrotweets accounts.

And the winner (2) was… the barred spiral galaxy NGC 4027!

But surprises didn’t end here. In the afternoon, when I was starting to prepare the instruments for the night (I’m conducting observations remotely from Sydney), I explained to astronomers and technicians at the AAT what we were doing. Rob Paterson, our afternoon technician, then told me “Do you know we already have the new CCD camera installed in 2dF and just waiting for testing it?

Let me explain why I was so excited when I heard this. For years the 2dF instrument has had an auxiliary camera, the FPI camera, that we use for properly positioning 2dF in the requested field. Rarely it has been used for science, as it is just a 516×516 pixels camera without filters. Occasionally I have also used it for getting some images of deep sky objects. But, as it has no filters, I had to get the color of the images elsewhere, usually taking archive data taken with other telescopes. But the new CCD camera in 2dF does have filters!

Rob phoned Steve Lee, the head of the Night Assistants at the AAT, and with Bob Dean the three of them managed to prepare CACTI (that is the name of the new camera) to have it ready for us.

Although there is still a lot to be done and tests to be conducted, the very first images I got this evening are quite promising. Here is the final result:

Spiral galaxy NGC 4027 located at around 75 million light years in Corvus (The Crow). This barred spiral galaxy, also identified as Arp 22, is identified as a peculiar galaxy by the extended arm, thought to be the result of a collision with another galaxy millions of years ago. This image is the “First Light” of the new CACTI camera in 2dF @ 3.9m Anglo-Australian Telescope. Color image using B (4 x 120 s, blue) + V (6 x 60 s, green) + R (6 x 60 s, red) filters. The data were taken on 11 May 2016 as part of an “outreach exercise” via social media. Click here to get a higher resolution image. Credit: Ángel R. López-Sánchez (AAO/MQ) & Steve Lee, Robert Paterson & Robert Dean (AAO). Night assistant at the AAT: Andre Phillips (AAO).

Note that this image, that actually is the “first light” of the CACTI camera, only combines 6 minutes in V and R and 8 minutes in B, that is, it is not deep at all. Furthermore not extra calibrations were taken (some flatfield images would have been nice). The deep image obtained by the 3.6m NTT telescope (ESO La Silla Observatory, Chile) provides many more details and resolution… but of course they were using the EFOSC instrument, which was specifically designed for deep imaging in optical filters. And the  image of NGC 4027 obtained by David Malin (AAO) using photographic plates at the AAT in 1982 is much more colorful.

But I still think it is a pretty result, particularly as this new image of NGC 4027 was obtained as a completely improvised “outreach exercise” using social media, in which 153 people voted for their favorite object to be observed at the 3.9m Anglo-Australian Telescope.

I really hope to repeat this exercise soon.

(1) A 2dF Plate must be configured with a scientific field, that is, allocating ~350 optical fibres to different objects in the sky. This takes ~ 20-30 minutes.

(2) Just to provide the details of the votes, see table below:

OBJECT    @Astrotweeps   @AAOastro       COMBINED

NGC 2865               5                  4                    9    ( 6% )

NGC 4361            36                   9                   45   (29%)

ESO 510-G13      36                  7                     43   (28%)

NGC 4027           36                20                    56   (37%)

TOTAL              113                 40                   153

Starburst spiral galaxy NGC 3310 with Gemini North

Last Tuesday 1st of March the famous NASA webpage Astronomy Picture of the Day (APOD) released a very nice image of the galaxy NGC 3310 obtained with the 8.2m Gemini North Telescope in Hawaii (U.S.A.).

Nice image of the starburst spiral galaxy NGC 3310 in the Ursa Major obtained with the 8.2m Gemini North Telescope in Hawaii (U.S.A.). This image was obtained for the “Cosmic Poll” contest organized by the International Telescopes Support Office at the Australian Astronomical Observatory (AAO) and appeared as APOD on 1st March 2016. Colours codify the light received in blue (B, blue) and red (R, green) filters, plus the emission of the ionized gas (Hα filter) coded in red.AAO ITSO Office, Gemini Obs./AURA & T. A. Rector (U. Alaska Anchorage).

NGC 3310 lies at a distance of around 50 million years from us, within stars of the Northern constellation of the Ursa Mayor (meaning we cannot see it here from Australia, well, it has a maximum elevation of ~5 degrees from Siding Spring Observatory). The spiral structure in NGC 3310 looks like what we expect for our own Milky Way galaxy, with plenty of star-forming regions (in red-pink colours tracing the Hα emission). However in the case of NGC 3310, the star-formation activity seems to be more extreme.

It seems that NGC 3310 started experiencing an interaction with a dwarf galaxy around 100 million years ago. This interaction has triggered a very strong star-formation event (that is why NGC 3310 is defined as a starburst galaxy), and has “broken” the external areas of the galaxy as consequence of the intense tidal forces. In the image, all regions showing red-pink colours (tracing Hα emission) are nebulae. These regions are found almost everywhere within NGC 3310, sometimes even forming some peculiar alignments of red-pink-ish regions as that “ray” that goes from the centre of the galaxy till the upper left corner. It is interesting to note that, although the interaction with the dwarf galaxy happened ~100 million years ago, the fact of finding this large amount of Hα emission informs that the star-formation activity is still important today. The colliding dwarf galaxy was probably engulfed by NGC 3310, its remaining debris could be that diffuse arc-like structure we observed in the outskirts of the galaxy in the upper part of the image.

These are the kind of objects (starburst galaxies) and the kind of features (enhanced Hα activity, tidal distortions of the stellar component of the galaxy, tails, rays…) I studied in a sample of dwarf galaxies for my PhD Thesis (I still have to tell all of that here…).

Beside tracing the nebular (Hα) emission, the image also allows to distinguish that the majority of the stars in NGC 3310 have blue colours, even in its external areas. Again, this fact informs that the dominant stellar populations in this galaxy are relatively young, as only young stars emit a lot of light in blue and ultraviolet colours.

Although it was not said in the APOD I would like to remark that the idea of observing this galaxy in the 8.2m Gemini North Telescope came from the International Telescopes Support Office at the Australian Astronomical Observatory (AAO). In particular, mi colleagues Elaina Hyde, Richard McDermid, Caroline Foster-Guanzon and Stuart Ryder (AAO) organized a very interesting outreach initiative, the Cosmic Poll, asking the people to emit a vote for which kind of object would they like to be observed at the 8.2m Gemini Telescope. The winning entry was “an individual galaxy”, and later they decided to observe NGC 3310. Furthermore they organised an on-line event,a live-stream with the Gemini North Telescope (is available on YouTube) explaining how the telescope works and giving details of the observatory. The Gemini Observatory website also included this in its blog. After processing and cleaning the images, the final result is that you see in APOD.

I couldn’t help myself, though, and decided to play a bit with the colours, levels, contrast and lights of the image to try to get an enhanced image of this very nice object. In my opinion, the central part of the galaxy is a bit too bright (it should be, of course, the real difference in brightness between the central part of NGC 3310 and the diffuse stellar streams in its outskirts is several orders of magnitude, but for illustration purposes I have found that it is a good idea to minimize that) and the outskirts of the galaxy are not that easy to see. So here it goes my enhanced image of NGC 3310 with Gemini North:

Comparison between the image of the starburst spiral galaxy NGC 3310 obtained by the 8.2m Gemini North Telescope and published in APOD on 1st March 2016 (left) and the same image enhanced by myself (right). Credit: AAO ITSO Office, Gemini Obs./AURA & T. A. Rector (U. Alaska Anchorage), Enhancement: Ángel R. López-Sánchez (AAO/MQ)

What do you think? What image do you like more?

Video: Space is just totally big and amazing

Last November some friends of the new Sydney on-line magazine A-star, Ryan Wittingslow and Harry Simpson, visited Siding Spring Observatory (Coonabarabran, NSW) to prepare a documentary about Astronomy and the telescopes at site. This is the nice video they have released, entitled Space is just totally big and amazing:

Documentary Space is just totally big and amazing prepared by A-star after their visit to the telescopes at Siding Spring Observatory. Credit: A-star.

As it happened while I was supporting astronomical observations at the Anglo-Australian Telescope (AAT), I was interviewed as part of the video. Although I talked about some few things (my research, my job at the AAO and my times as a young amateur astronomer in Spain), they only used my comments about astrophotography. Indeed, they asked me to include some scenes of my astronomical time-lapses on the documentary, and I think the result is great. I really love to see my astro photos and videos so well used. Thanks Ryan and Harry for this report!

The oldest stars of the Galaxy

DP ENGLISH: This story belongs to the series “Double Post” which indicates posts that have been written both in English in The Lined Wolf and in Spanish in El Lobo Rayado.

DP ESPAÑOL: Esta historia entra en la categoría “Doble Post” donde indico artículos que han sido escritos tanto en español en El Lobo Rayado como en inglés en The Lined Wolf.

Last month the prestigious journal Nature published a letter led by PhD student (and friend) Louise Howes (@Lousie, ANU/RSAA, Australia). This scientific paper, with title Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way, uses data from the 1.2m Skymapper Telescope, the 3.9m Anglo-Australian Telescope (both at Siding Spring Observatory, NSW, Australia) and the 6.5m Magellan Clay telescope (Las Campanas Observatory, Chile) to study very old stars in the Milky Way bulge.

Image of the Galactic centre obtained using Skymapper data. Credit: Chris Owen (ANU/RSAA).

Image of the Galactic centre obtained using Skymapper data. Credit: Chris Owen (ANU/RSAA).

The aim of the research was to look for signatures of really old stars: stars that old that perhaps the Milky Was was not even born when they were created! How do astronomers know that? Just studying the chemical composition of the stars via deep spectral analysis. Only hydrogen and helium (and just a bit of litium) were formed in the Big Bang: the rest of elements have been created or inside the stars (oxygen, carbon, nitrogen, iron) or because of processes happening to the stars (e.g., supernova explosions, that create heavy elements such as gold, silver, copper or uranium). As time goes by and new generations of stars are born, the amount of metals (for astronomers, metals are all elements which are not hydrogen and helium) increases. Therefore if we discover a star with very few amount of metals, we will quite sure we are observing a very old object.

Loiuse has been using the 2dF instrument at the Anglo-Australian Telescope and the MIKE spectrograph at the Magellan Clay Telescope (Chile) to get deep, high-resolution spectra of candidate old stars in the Galactic bulge. The candidate stars were identified using optical images provided by the 1.2m Skymapper Telescope. With these observations, Louise Howes and collaborators have detected 23 stars that are extremely metal-poor. These stars have surprisingly low levels of carbon, iron and other heavy elements. Indeed, they report the discovery of a star that has an abundance of iron which is 10,000 times lower than that found in the Sun! These stars were formed at redshift greater than 15, that is, we are observing in our own Milky Way stars that were formed just ~300 million years after the Big Bang!

On top of that, the study suggests that these first stars didn’t explode as normal supernova but as hypernova: poorly understood explosions of probably rapidly rotating stars producing 10 times as much energy as normal supernovae. The high-resolution spectroscopic data have been also used to study the kinematics of these very old stars, that are found on tight orbits around the Galactic centre rather that being halo stars passing through the bulge. This is also characteristic of stars that were formed at redshifts greater than 15.

Short 3 minutes video discussing the results found in this study. Credit: ANU.

I’m happy to say here that I’ve been the support astronomer for many of her nights at the AAT the last couple of years. And I’m extremely happy to see that, even because of the bad weather we have had sometimes, they managed to get these observations published in Nature! Well done, Louise!

More details:

Scientific paper in Nature: Howes et al. 2015, Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way, 11 November 2015.

Scientific paper in arXiv

ANU Press Release