4,487 datasets found

Keywords: infrared photometry

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  • ASPIC MUSE-Wide DR1 catalogue

    Photometry, spectral features, and physical parameters of MUSE-Wide sources on GOODS-South field.
  • ASPIC VUDS-DR1 catalogue on COSMOS field

    Photometry, spectral features, and physical parameters of VUDS (DR1) sources on COSMOS field.
  • Master catalog of infrared proper motions

    The most recently formed young stellar objects (YSOs) in active star-forming regions are excellent tracers of their parent cloud motion. Their positions and dynamics provide...
  • YSOs in GRSMC 045.49+00.04 from IR obs.

    Understanding the characteristics of young stellar populations is essential for deriving insights into star formation processes within parent molecular clouds and the influence...
  • KiDS-450: Weak lensing shear measurements

    We present cosmological parameter constraints from a tomographic weak gravitational lensing analysis of ~450deg^2^ of imaging data from the Kilo Degree Survey (KiDS). For a flat...
  • VIKING catalogue data release 4

    We describe the VISTA Science Archive (VSA) and its first public release of data from five of the six VISTA public surveys. The VSA exists to support the VISTA surveys through...
  • TI-DYE. II. HIP 67522 light curves & transit data

    The youngest (<50Myr) planets are vital to understand planet formation and early evolution. The 17 Myr system HIP 67522 is already known to host a giant (~10R_{Earth}) planet...
  • TESS & KPF: TOI-2364 light & radial velocity curves

    We measure the true obliquity of TOI-2364, a K dwarf with a sub-Saturn-mass (M_p_=0.18M_J_) transiting planet on the upper edge of the hot-Neptune desert. We used new...
  • TI-DYE. III. TOI-2076 light curves & comoving stars

    Young (<500Myr) multiplanet transiting systems are valuable environments for understanding planet evolution by offering an opportunity to make direct comparisons between...
  • BASALT faint blazar candidates

    We present a sample of blazar candidates from the Very Large Array Sky Survey (VLASS) catalog, with cross-referencing to optical and infrared data from the Panoramic Survey...
  • Taurus and Upper Sco brown dwarfs phot. and masses

    Free-floating planetary mass objects -worlds that roam interstellar space untethered to a parent star-challenge conventional notions of planetary formation and migration, but...
  • S-PLUS Fornax Project (S+FP)

    Observational extragalactic catalogs over wide sky areas are essential for uncovering the large-scale structure of the Universe. They allow, among others, cosmological studies...
  • JWST/NIRCam data of CEERS galaxies at 4<z<9.5

    We analyze 347 galaxies at redshift 4
  • HECATEv2

    We present HECATEv2, the second release of the Heraklion Extragalactic Catalogue (HECATE), an all-sky, value-added galaxy catalogue comprising 204733 galaxies from the HyperLEDA...
  • MOBStIRS: Bow shocks parameters from Zooniverse

    Mass-loss influences stellar evolution, especially for massive stars with strong winds. Stellar wind bow shock nebulae driven by Galactic OB stars can be used to measure...
  • Multiwavelength photometry of SN 2022xkq

    We present optical, infrared, ultraviolet, and radio observations of SN 2022xkq, an underluminous fast-declining Type Ia supernova (SN Ia) in NGC 1784 (D~31Mpc), from <1 to...
  • Extreme emission-line galaxies at z~4-9

    We investigate the properties of extreme emission line galaxies (EELGs) at z=4-9 and their role in reionization. Compact, low-mass galaxies with intense optical emission lines...
  • NIRCAm photometric properties of ONC disks

    The Orion Nebula Cluster (ONC) provides the closest example of ongoing star and planet formation in highly irradiated environments. In particular, it is a key region to study...
  • Nuclear star cluster at 3pc from Sgr A*

    The Milky Way's nuclear star cluster (NSC) offers a unique laboratory for studying the formation and evolution of dense stellar systems around a supermassive black hole....
  • Euclid Perseus ETG photometry

    The Euclid Early Release Observations (ERO) programme targeted the Perseus galaxy cluster in its central region over 0.7deg^2^. We combined the exceptional image quality and...
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