Correction: After this paper (Treister et al. 2011) was published and publicized a problem was discovered with the background subtraction used. Analysis by several groups, including the Treister et al. team, plus Willott (2011) and Cowie et al. (2012), shows that a significant detection of AGN (growing black holes) in the early universe can no longer be claimed.

Editor's Note: Honest errors such as this are part of the scientific process, especially on the frontiers of discovery. To quote Nobel laureate Frank Wilczek, "If you don't make mistakes, you're not working on hard enough problems. And that's a big mistake."

References:

Cowie, L. et al. 2012, ApJ, in press
https://arxiv.org/abs/1110.3326

Treister, E. et al. 2011, Nature, 474, 356
https://arxiv.org/abs/1106.3079

Willott, C. 2011, ApJ, 742, L8
https://arxiv.org/abs/1110.4118

This composite image from NASA's Chandra X-ray Observatory and Hubble Space Telescope (HST) combines the deepest X-ray, optical and infrared views of the sky. Using these images, astronomers have obtained the first direct evidence that black holes are common in the early Universe and shown that very young black holes grew more aggressively than previously thought.

If you’re one who follows astro-news regularly, you’ve probably heard by now that there will be a Chandra press conference. While we can't give out too much information in advance, we can say that this press conference covers black holes in the early Universe. This event will be televised on NASA TV and anyone can watch it live, beginning at 1pm Eastern, and follow #babyblackholes on Twitter
 

This week, the American Astronomical Society held its bi-annual meeting in the fair city of Boston. Since those of us involved with Chandra spend most of our time on the other side of the river (meaning Cambridge), this is a chance to expand our horizons ever so slightly.

Of course, the big bonus of the AAS meeting is the ability to hear talks and mingle with people who don’t work at our institution. It’s a chance to catch up with old colleagues and meet new ones. In a world increasingly dominating by electronic communication, there’s something irreplaceable about actually sitting across from someone in person.

This large Chandra image shows the Carina Nebula, a star-forming region in the Sagittarius-Carina arm of the Milky Way a mere 7,500 light years from Earth. Chandra's sharp X-ray vision has detected over 14,000 stars in this region, revealed a diffuse X-ray glow, and provided strong evidence that massive stars have already self-destructed in this nearby supernova factory.

A promise made is a debt unpaid. Robert Service
Chance favors the prepared mind. Louis Pasteur

Not long ago a request came down from above for a list of Chandra’s achievements that have “completely transformed the way we have viewed our world, solar system, sun, or universe."

In other words, how many discoveries of the century have you made this year?

A new movie from NASA's Chandra X-ray Observatory shows a sequence of Chandra images of the Crab Nebula, taken over an interval of seven months. Dramatic variations are seen, including the expansion of a ring of X-ray emission around the pulsar (white dot near center) and changes in the knots within this ring.

As part of our efforts to work with the formal education community (that is, generally K-12 schools), the Chandra EPO team works with the National Science Olympiad. The Olympiad is an excellent science competition that involves middle and high school teams from all 50 states, often getting kids involved at an even earlier age.

Jeffrey Silverman was part of the very successful Science Olympiad team from Troy High School (Fullerton, CA) team in 2001. He is now finishing his Ph.D. in astrophysics from the University of California at Berkeley, where he works mainly on exploding stars known as supernovas including 2006gy and this recent news-grabbing event. We asked Jeffrey to share with us some of his experiences during the Science Olympiad and how they helped shape his choices once he got to college and now into graduate school and beyond.

This Chandra image of the Tycho supernova remnant contains new evidence for what triggered the original supernova explosion. Tycho was formed by a Type Ia supernova, a category of stellar explosion used in measuring astronomical distances because of their reliable brightness. In the lower left region of Tycho is a blue arc of X-ray emission. Several lines of evidence support the conclusion that this arc is due to a shock wave created when a white dwarf exploded and blew material off the surface of a nearby companion star.

We are very excited to announce the launch of a new – and yet somewhat familiar -- project. Today, “From Earth to the Solar System” officially opens. As the name implies, FETTSS (our new favorite acronym) is a direct descendent of the “From Earth to the Universe” project.