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SHINE IV.
Over the past decade, large surveys with state-of-the-art planet-finder instruments such as Spectro-Polarimetric High-contrast Exoplanet REsearch on board Very Large Telescope... -
Carbon star identification in Gaia DR3
A large fraction of Asymptotic Giant Branch (AGB) stars develop carbon-rich atmospheres during their evolution. Based on their color and luminosity, these carbon stars can be... -
Fast rotators and new FGK stars
The next mission dedicated to the study of planetary atmospheres is the Ariel space mission, planned for launch in 2029, which will observe a variety of planetary systems... -
GJ 3998 RVs, SMW and Halpha indexes
The low masses of M dwarfs create attractive opportunities for exoplanet radial-velocity (RV) detections. These stars, however, exhibit strong stellar activity that may... -
ACT-PLANCK DR4DR6 f090 survey collection
This is the first field (f090) of an unpolarized map with three components corresponding to f090, f150 and f220 bands which are broad bands with center frequency roughly at 95... -
JWST F444W (beta) survey collection
The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in. Original acknowledgement... -
ACT-PLANCK DR4DR6 f220 survey collection
This is the third field (f220) of an unpolarized map with three components corresponding to f090, f150 and f220 bands which are broad bands with center frequency roughly at 95... -
VPHAS+ DR4 u filter survey collection
The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+) is surveying the southern Milky Way in u, g, r, i and Halpha at ?1 arcsec angular resolution.... -
ACT-PLANCK DR4DR6 map healpix Q survey collection
This is the Q component of a low-resolution map representing a weighted average of the f090 and f150 linear polarization. For a slightly depper map, we combine the DR4 based on... -
VISIONS DR2 color (from bands Ks, H, J) survey collection
VISIONS - VISTA Star Formation Atlas is a near-infrared (NIR) VISTA public survey covering all major nearby star-forming regions accessible from the southern hemisphere. The... -
Simbad heatmap - 2022 survey collection
This dataset has no description
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ACT-PLANCK DR4DR6 map healpix E survey collection
This is the B component of a low-resolution map representing a weighted average of the f090 and f150 linear polarization. For a slightly deeper map, we combin the DR4 based on... -
ACT-PLANCK DR4DR6 point-source filtered f090 survey collection
This is the first field (f090) of an unpolarized map with three components corresponding t f090, f150 and f220 bands which are broad bands with center frequency roughly at 95... -
JWST F210M (beta) survey collection
The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in. Original acknowledgement... -
Euclid Q1 color (NISP.H, NISP.Y, VIS) survey collection
The Euclid Q1 data release encompasses ?65 deg2 and contains the VIS and NIR data of one pass on each of the three Euclid deep fields (EDF-North, EDF-South, and EDF-Fornax), as... -
JWST F150W (beta) survey collection
The JWST Hierarchical Progressive Survey (HiPS) has been built by Daniel Durand and distributed by CDS. It sets together all JWST observations done in. Original acknowledgement... -
Euclid Q1 NISP.H survey collection
The Euclid Q1 data release encompasses ?65 deg2 and contains the VIS and NIR data of one pass on each of the three Euclid deep fields (EDF-North, EDF-South, and EDF-Fornax), as... -
Simbad heatmap - 2021 survey collection
This dataset has no description
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ACT-PLANCK DR4DR6 Color MW survey collection
This is an unpolarized map with three components corresponding to our f090, f150 and f220 bands which are broad bands with center frequency roughly at 95 GHz, 150 GHz and 220... -
VPHAS+ DR4 color (from bands Halpha, u, g, r, i) survey collection
The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+) is surveying the southern Milky Way in u, g, r, i and Halpha at ?1 arcsec angular resolution....
