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Mars atmospheric profiles - From NOMAD/TGO
Profiles of pressure, temperature and species of the Martian atmosphere derived from measurements of the NOMAD instrument on board ESA's Trace Gas Orbiter. See paper... -
SOIR
Profiles of species in Venus atmosphere terminator. Data retrieved from calibrated spectra obtained with the SPICAV-SOIR instrument on board the Venus Express spacecraft. These... -
Cluster Lensing And Supernova survey with Hubble (CLASH)
By observing 25 massive galaxy clusters with HST's new panchromatic imaging capabilities (Wide-field Camera 3, WFC3, and the Advanced Camera for Surveys, ACS), CLASH will... -
Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES)
Hubble Infrared Pure Parallel Imaging Extragalactic Survey (HIPPIES) utilizes long-duration pure parallel visits (~> 3 orbits) of HST at high Galactic latitude... -
Merging galaxies in isolated env.
Extragalactic surveys provide significant statistical data for the conditions. These quantities are derived using manual or automatic methods for disturbances, star-forming... -
MUSE datacubes of T Pyx
T Pyx is one of the most enigmatic recurrent novae, and it has been proposed as a potential Galactic type-Ia supernova progenitor. Using spatially resolved data obtained with... -
APOGEE DR17 standard stars radial velocities
We present an updated catalog of 46753 radial velocity (RV) standard stars selected from the APOGEE DR17. These stars cover the Northern and Southern Hemispheres almost evenly,... -
Gaia Ultra-Cool Dwarf candidates IR spectra
The local census of very low-mass stars and brown dwarfs is crucial to improving our understanding of the stellar-substellar transition and their formation history. These... -
S CrA full L- and M-band spectra
The Cryogenic IR echelle Spectrometer (CRIRES) instrument at the Very Large Telescope (VLT) was in operation from 2006 to 2014. Great strides in characterizing the inner regions... -
Zero-polarization candidate regions
The calibration of optical polarimeters relies on the use of stars with negligible polarization (i.e., unpolarized standard stars) for determining the instrumental polarization... -
NGC 628, NGC 1365 and NGC 7496 UVIT FUV images
Polycyclic Aromatic Hydrocarbons (PAHs) are ubiquitous complex molecules in the interstellar medium and are used as an indirect indicator of star-formation. On the other hand... -
Hubble Ultra Deep Field 2009 (HUDF09)
The Hubble Ultra Deep Field 2009 (HUDF09) program observations were obtained as HST program 11563 (PI: Garth Illingworth) from August 2009 to February 2011 (Cycle 17). The...
