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astronomnomy

An astronomy research blog run by an astronomy doctoral researcher! Explaining new astro results and documenting her thesis progress :)
Jun 12 '13

“We selected this field to test the algorithm because quite frankly I just like the name of it???”

I have arbitrary feelings about some of our fields (patches of sky the collaboration’s observed) based purely on the name. Completely independent of the importance of these patches of sky to the astronomical community. 

I really like Lockman-SWIRE but think UDS sucks. Idk why?

I like ELAIS-N1 as I did an undergrad project on that field, but felt aggrieved when I was doing something with ELAIS-S1 the other month because it felt like I was cheating.

I have a love-hate relationship with FLS because of the cirrus, it’s interesting because of the cirrus but I hate it because of the cirrus… at least that one has a reason I suppose.  

COSMOS is okay…

They’re all here, in case you want to know where they are on the sky.

1 note Tags: astronomy phd

Jun 8 '13

335 notes (via tachypomp & ebonyandunicorn)

May 31 '13

Just submitted an abstract to give a poster talk at a conference in October  :wiggles:. I could have asked for a talk but it lends itself better to small chats.

Also after the big discussion on the astronomers fb group about plagiarism (yup, there’s a fb group for professional astronomers), where people were recounting stories of having their ideas nicked by other ruthless astronomers, I’m really paranoid, so I’m not going to post the abstract up. Not that I’m big-headed enough to think it’s that good someone will steal it, but I need the publication, so.

3 notes Tags: phd personal

May 30 '13

2 notes Tags: astronomy astrophysics cosmology space science memes image macros

May 30 '13
Binary Words: Halo
We have halos in astronomy, though they’re not golden disks hovering above the righteous! Instead of light, they’re made of dark matter, which cannot be directly seen. In addition they’re not very ringed-shaped, more large, blobby masses surrounding galaxies. It is supposed that when the dark matter formed in at the beginning of the Universe, the self-gravitation of the dark matter caused it to start to clump together. These clumps and filaments of dark matter, like in the image, became the backbone of the Universe that all gas and dust fell onto, which then went on to form stars and galaxies.
A dark matter halo is far bigger than the galaxy it may host, and much rounder. Why so? Well, gas and dust particles can collide and so slow down. They can fall into a gravitational well to create a small, compact galaxy. Dark matter is thought to only interact gravitationally so it cannot collide with other dark matter particles, cannot slow down and fall in the way normal matter does so the halos stay larger for much longer.
Halos are used to explain why we see stars on the edge of galaxies moving so quickly they should be flung off into deep space, yet remain gravitationally tethered to the galaxy. If the galaxy has a lot more invisible matter inside and surrounding it, contributing to the gravitational pull of the galaxy, it could hold on to the stars. Dark matter halos fit the bill. 
All this means that there is more to a galaxy than meets the eye, quite literally!
(image credit: Virgo Consortium, the Millennium Run is one of the most well-used simulations of dark matter. Fly through here to see halos!)

Binary Words: Halo

We have halos in astronomy, though they’re not golden disks hovering above the righteous! Instead of light, they’re made of dark matter, which cannot be directly seen. In addition they’re not very ringed-shaped, more large, blobby masses surrounding galaxies. It is supposed that when the dark matter formed in at the beginning of the Universe, the self-gravitation of the dark matter caused it to start to clump together. These clumps and filaments of dark matter, like in the image, became the backbone of the Universe that all gas and dust fell onto, which then went on to form stars and galaxies.

A dark matter halo is far bigger than the galaxy it may host, and much rounder. Why so? Well, gas and dust particles can collide and so slow down. They can fall into a gravitational well to create a small, compact galaxy. Dark matter is thought to only interact gravitationally so it cannot collide with other dark matter particles, cannot slow down and fall in the way normal matter does so the halos stay larger for much longer.

Halos are used to explain why we see stars on the edge of galaxies moving so quickly they should be flung off into deep space, yet remain gravitationally tethered to the galaxy. If the galaxy has a lot more invisible matter inside and surrounding it, contributing to the gravitational pull of the galaxy, it could hold on to the stars. Dark matter halos fit the bill. 

All this means that there is more to a galaxy than meets the eye, quite literally!

(image credit: Virgo Consortium, the Millennium Run is one of the most well-used simulations of dark matter. Fly through here to see halos!)

14 notes Tags: astronomy dark matter binary words astrophysics space galaxies science cosmology universe

May 23 '13
astronemma:

ESO’s Very Large Telescope Celebrates 15 Years of Success

With this new view of a spectacular stellar nursery ESO is celebrating 15 years of the Very Large Telescope — the world’s most advanced optical instrument. This picture reveals thick clumps of dust silhouetted against the pink glowing gas cloud known to astronomers as IC 2944. These opaque blobs resemble drops of ink floating in a strawberry cocktail, their whimsical shapes sculpted by powerful radiation coming from the nearby brilliant young stars.

Read more: [x]

astronemma:

ESO’s Very Large Telescope Celebrates 15 Years of Success

With this new view of a spectacular stellar nursery ESO is celebrating 15 years of the Very Large Telescope — the world’s most advanced optical instrument. This picture reveals thick clumps of dust silhouetted against the pink glowing gas cloud known to astronomers as IC 2944. These opaque blobs resemble drops of ink floating in a strawberry cocktail, their whimsical shapes sculpted by powerful radiation coming from the nearby brilliant young stars.

Read more: [x]

20 notes (via astronemma)

May 22 '13

10 notes Tags: astronomy astrophysics space science awesome cosmology nasa esa hubble xdf galaxies

May 21 '13

Best laid schemes of mice and men…

My perfectly scheduled day today as planned:

11:30 - 12:15 : supervision about thesis plan

12:15 - 13:00 : type plan up ready for annual review later this week

13:00 - 14:00 : group lunch

14:00 - 14:30 : CRB check for public engagement

14:30 - 15:30 : chat about making science communication videos

After unfortunate cancellations what’s actually happening:

11:30 - 14:00 :  ??? work ??? food?????? on our own?????? sad???

14:00 - 14:45 : rescheduled supervision that might be late due to meeting

Thursday afternoon: chat about videos

CRB check : ??????? more sad???

:(

1 note Tags: phd personal

May 20 '13
I have no need of your sass right now Google you impudent little shite. 

I have no need of your sass right now Google you impudent little shite. 

14 notes Tags: astronomy sun personal answer is 695 500 000 metres if you're wondering

May 20 '13
distant-traveller:

NYC as seen from different planets

Take a trip around the solar system and bring the entire city of New York with you in these captivating drawings showing how the atmospheres of other planets would interact with the iconic metropolitan skyline.
The images were created by artist Nickolay Lamm of StorageFront.com, who employed the help of astrobiologist Marilyn Browning Vogel to get the details right. Lamm said the idea came to him while looking at pictures that NASA’s Curiosity rover took of Mount Sharp.

Image credit: Nickolay Lamm

distant-traveller:

NYC as seen from different planets

Take a trip around the solar system and bring the entire city of New York with you in these captivating drawings showing how the atmospheres of other planets would interact with the iconic metropolitan skyline.

The images were created by artist Nickolay Lamm of StorageFront.com, who employed the help of astrobiologist Marilyn Browning Vogel to get the details right. Lamm said the idea came to him while looking at pictures that NASA’s Curiosity rover took of Mount Sharp.

Image credit: Nickolay Lamm

493 notes (via classicallyforbiddenregions & distant-traveller)