A star called KIC 8462852 has been in the news recently for unexplained and bizarre behavior. New clues emerge in the mystery of a star with odd light patterns.
ESO’s VISTA survey telescope has spied a horde of previously hidden massive galaxies that existed when the Universe was in its infancy. By discovering and studying more of these galaxies than ever before, astronomers have, for the first time, found out exactly when such monster galaxies first appeared.
The Wide Field Infrared Survey Telescope (WFIRST) is a NASA mission currently under study for the next decade whose primary objectives are to study the nature of dark energy, via gravitational lensing, supernovae and baryon acoustic oscillations, and search for and characterize exoplanets, via microlensing and coronagraphy. This international meeting, "Community Astrophysics with WFIRST: Guest Observer and Archival Science", to be held in Pasadena from 29 Feb. through 2 March 2016, will focus on the GO and GI components of the WFIRST mission, bringing together experts in the community to discuss groundbreaking science that can be done with the GO and archival opportunities of WFIRST. Due to the synergy between WFIRST and Euclid, this meeting is of great interest to the Euclid community.
Astronomers have discovered a giant gathering of galaxies in a very remote part of the universe, thanks to NASA's Spitzer Space Telescope and Wide-field Infrared Survey Explorer (WISE). The galaxy cluster, located 8.5 billion light-years away, is the most massive structure yet found at such great distances.
NEOCam is one of 5 mission proposals picked by NASA for further study. NEOCam is an infrared asteroid-hunting telescope, which would discover 2/3 of near-Earth objects larger than 140m.
The central supermassive black hole of a recently discovered galaxy is far larger than should be possible, according to current theories of galactic evolution.
Version 4.0 of the Montage Image Mosaic Toolkit has been released with a BSD 3-clause license. This is major new release that contains new modules to support processing of data cubes, and a command-line visualization tool.
The Infrared Processing and Analysis Center (IPAC) and the Space Telescope Science Institute (STScI), in coordination with the WFIRST Study Office at GSFC and JPL, are pleased to announce that registration is now open for "Community Astrophysics with WFIRST: Guest Observer and Archival Science" - an international meeting to be held in Pasadena from 29 February through 2 March 2016.
The development of Infrared astronomy over the past fifty years has transformed our view of the Universe. This year we celebrate five decades of IR astronomy at Caltech. In particular, we honor the contributions of Gerry Neugebauer, Keith Matthews, and Tom Soifer to the past, present and future of IR astronomy at Caltech.
The Infrared Processing and Analysis Center at Caltech announces the availability of six-month graduate student fellowships beginning in the Spring of 2016. The program is designed to allow students from other institutions to visit IPAC-Caltech and perform astronomical research in close association with an IPAC staff member during Spring 2016.
NASA is seeking input from the science community that will culminate in a decision to support studies of three or four large missions to prepare for the next Decadal Survey in Astrophysics. A white paper released by NASA's Astrophysics Division lists four candidate missions, including a Far-Infrared Surveyor mission.
The fifteenth annual Greater IPAC Science Symposium will be held on Thursday and Friday, April 23 and 24, 2015. The Science Symposium is a forum for all staff members of IPAC, the Spitzer Science Center (SSC), the NASA Herschel Science Center (NHSC) and the NASA Exoplanet Science Institute (NExScI) to present, discuss and learn about the diverse research that is being carried out at the Greater IPAC.