Mays was recently awarded a Fulbright Grant to travel to Santiago, Chile and work with international
teams of astronomers who study Chile's northern deserts in 2010.
He leads
a team of astronomers who have been using the Large Binocular Telescope (LBT) to look for failed supernovae in other galaxies.
The team of astronomers who discovered it — led by Robert Quimby of the California Institute of Technology (Caltech) in Pasadena — tentatively have labeled the 4.7 billion light - years away ex-star a Type II - L supernova because of its brightness and because its light spectrum shows a primarily hydrogen content.
The SLUGGS survey is comprised of an international
team of astronomers who aim to understand the formation and evolution of galaxies and their globular cluster systems.
Not exact matches
This intriguing fingerprint quickly triggered additional observations by
teams of astronomers worldwide
who obtained observing time with additional space observatories including NASA's Chandra X-ray Observatory and NASA's Nuclear Spectroscopic Telescope Array (NuSTAR).
In fact, Swift X-ray and optical observations were carried out two days after FRB 131104, thanks to prompt analysis by radio
astronomers (
who were not aware
of the gamma - ray counterpart) and a nimble response from the Swift mission operations
team, headquartered at Penn State.
Further studies
of SN 2009ip and its aftermath will help tease out the physics
of these exotic supernovae, says Armin Rest, an
astronomer at the Space Telescope Science Institute in Maryland,
who was not part
of the study
team.
The key observation from the new research is that the small dip in the HAT - P - 7 b light curve when the planet passes behind its star «is roughly equivalent to the signal
of an Earth - size planet when it passes in front
of its parent star,» says Paul Kalas, an
astronomer at the University
of California, Berkeley,
who is not part
of the Kepler
team.
The
team has also found evidence to silence a minority
of sceptics
who argue that what most
astronomers take to be microlensing events are actually caused by natural variations in the intrinsic brightness
of the stars being observed.
But as Johnson explained here today at the 219th meeting
of the American Astronomical Society, that all changed thanks to British amateur
astronomer Kevin Apps,
who is working closely with the Kepler science
team.
«We saw what looked like a new star,» says
astronomer Edo Berger
of Harvard University,
who led a
team that spotted the light with the DECam on the Blanco telescope in Chile.
Among other things, the new map will help
astronomers to understand and explain the motion
of the Milky Way, which is apparently being tugged by the gravity
of neighboring groups and clusters
of galaxies, says 2MASS
team member Karen Masters
of the University
of Portsmouth in the United Kingdom,
who presented the it here at the summer meeting
of the American Astronomical Society.
Lawrence Rudnick, the
astronomer who led the
team that found the void, was studying data from the Very Large Array, a network
of 27 radio antennas in New Mexico, when he spotted a gap in the constellation Eridanus where radio signals from galaxies appear unusually faint.
Previous predictions are «exactly what was observed» by the research
team, says
astronomer Greg Laughlin
of the University
of California, Santa Cruz,
who was not affiliated with the study.
Hendrik Hildebrandt from the Argelander - Institut für Astronomie in Bonn, Germany and Massimo Viola from the Leiden Observatory in the Netherlands led a
team of astronomers [1] from institutions around the world
who processed images from the Kilo Degree Survey (KiDS), which was made with ESO's VLT Survey Telescope (VST) in Chile.
«Last Sunday, after seven years in space traveling nearly three billion miles, Stardust landed in the Great Salt Lake Desert with a treasure from when the solar system formed 4.6 billion years ago,» says
astronomer Donald Brownlee
of the University
of Washington,
who led the Stardust
team.
Gathering all this mass in under 690 million years is an enormous challenge for theories
of supermassive black hole growth, explains Eduardo Bañados, an
astronomer at the Carnegie Institution for Science
who led the international
team of scientists.
«It certainly is a very exciting discovery,» says Howard Bond, an
astronomer at the Space Telescope Science Institute in Baltimore, Md.,
who was not part
of the discovery
team.
It is exciting,» says Alain Léger, an
astronomer at the University
of Paris - South at Orsay
who is familiar with the French
team's work.
«Finally, we now have separate images where you can see, actually see, the planet,» says
astronomer Mark Marley
of the NASA Ames Research Center at Moffett Field, Calif.,
who did not participate in the research but wrote an article for Science summarizing and analyzing the
teams» results.
The discovery was announced on May 17, 2016, in a Central Bureau for Astronomical Telegrams (CBAT) electronic telegram by University
of California at Berkeley research
astronomer Mike Wong,
who led the
team that analyzed the Hubble data.
«Many
astronomers are surprised at this discovery, because they didn't expect such strong radio emission from this object,» said Shri Kulkarni, a Caltech professor
who was on the
team that first discovered a brown dwarf in 1995, and advisor to one
of the students.
«Thirty - seven
of the brightest galaxies were detected, including a quasar, but thousands
of galaxies were probably in the string, according to
astronomer Dr. Paul Francis
who heads the
team.
As Brown also surmised in Nature, «If I read this paper out
of the blue, my first reaction would be that it was crazy,» says Mike Brown, an
astronomer at the California Institute
of Technology in Pasadena,
who was part
of the research
team.
The Caltech
team reporting on this discovery consists
of Zitrin, Ellis, and Belli
who lead an international collaboration involving
astronomers at Yale and the University
of Arizona, and fellow European researchers from Leiden University in the Netherlands and the University
of Durham and the Univeristy College London in England.
The result is reported in the Dec. 10 issue
of Nature magazine by the
team of Liverpool John Moores University (LJMU)
astronomers who built and operate the telescope and its unique scientific camera, named RINGO.
The ice mountains rise up from a region
of the heart - shaped feature, which Stern and his
team have informally nicknamed Tombaugh Regio in honor
of the late
astronomer Clyde Tombaugh,
who discovered Pluto in 1930.
«With this one amazing picture, we can explore the earliest days
of black holes in the Universe and see how they change over billions
of years,» Niel Brandt
of Pennsylvania State University in University Park, Pennsylvania,
who led a
team of astronomers studying the deep image, said in a statement.