TEMPO Air Pollution Sensor Treks Toward Satellite Integration
NASA Media Call on Upcoming Air Quality Satellite Launch
Media Advisory: New Space Instrument To Deliver Near Real-Time Air Pollution Data
Air Pollution Sensor Integrated and Tested with Commercial Satellite Host
First Rocky Exoplanet Confirmed with NASA's JWST
A Leading Light in Atmospheric Science
New from JWST: An Exoplanet Atmosphere as Never Seen Before
Astronomers Warn of Risk of Misinterpreting JWST Planetary Signals
New Grant Supports Teen Air Quality Studies
Astronomers Detect Carbon Dioxide on Planet for the First Time with JWST
TEMPO Air Pollution Instrument Completes Satellite Integration
GMACS - Moderate Dispersion Optical Spectrograph for the Giant Magellan Telescope is a powerful optical spectrograph that will unlock the power of the Giant Magellan Telescope for research ranging from the formation of stars and planets to cosmology.
HITRAN and HITEMP Database
With techniques developed in quantum mechanics, molecular spectra can be modeled by a set of discrete fundamental parameters. The knowledge of these reference molecular spectroscopic parameters is essential to correctly characterize constituents of their environments, model their spectra and atmospheric conditions. Physicists at the Center for Astrophysics | Harvard & Smithsonian maintain the HIgh-resolution TRANsmission (HITRAN) and HIgh TEMPerature (HITEMP) databases of molecular spectral parameters, along with the HITRAN Application Programming Interface (HAPI) which also enables one to access the database archive and process the data.
Sensing the Dynamic Universe
The Sensing the Dynamic Universe (SDU) project creates sonified videos exploring the multitude of celestial variables such as stars, supernovae, quasars, gamma ray bursts and more. We sonify lightcurves and spectra, making the astrophysics of variables and transients accessible to the general public, with particular attention to accessibility for those with visual and/or neurological differences.
In extreme environments, where pressure, temperature, and density are high, atoms change the way they emit and absorb light. Electrons are stripped from nuclei, forming a plasma, and the ions emit X-rays when struck by free electrons. To assist astronomers in identifying atoms under these harsh conditions, the Center for Astrophysics | Harvard & Smithsonian maintains the AtomDB database of X-ray spectra. This catalog provides essential information for studying conditions in many astrophysical environments, including those near black holes, stars, and neutron stars.
PINTofALE (Package for Interactive Analysis of Line Emission)
Astrophysical environments are often strikingly different from those on Earth, but there’s no direct way for astronomers to measure conditions in space. Instead, they must infer environmental properties from the behavior of atoms, particularly the way they absorb and emit light. For this to work, researchers need to use databases of atomic spectra, which requires writing or using computer code. PINTofALE (Package for Interactive Analysis of Line Emission) is a software toolkit designed to streamline this process, giving astronomers a powerful way to use X-ray and ultraviolet atomic data without having to write their own code every time. The package was developed by researchers at the Center for Astrophysics | Harvard & Smithsonian, and is provided for free as a service to astronomers.