6,632 datasets found

Keywords: interdisciplinary astronomy

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  • EXOSAT TGS Spectra and Lightcurves

    Spectra obtained using the EXOSAT transmission grating spectrometer, TGS. There are two databases TGS and TGS2 as follows: <pre> * TGS - the grating spectra averaged over...
  • EXOSAT TGS L and R Orders

    Spectra obtained using the EXOSAT transmission grating spectrometer, TGS. There are two databases TGS and TGS2 as follows: <pre> * TGS - the grating spectra averaged over...
  • Properties of IC 4665 members

    IC 4665 is one of only a dozen young open clusters with a 'lithium depletion boundary' (LDB) age. Using an astrometrically and spectroscopically filtered sample of cluster...
  • SNR and HII regions in M83 observed with MUSE

    Here we describe a new study of the supernova remnants (SNRs) and SNR candidates in nearby face-on spiral galaxy M83, based primarily on MUSE integral field spectroscopy. Our...
  • Age estimations of low-mass TESS CVZ stars

    The number of potentially habitable planets continues to increase, but we lack the time and resources to characterize all of them. With ~30 known potentially habitable planets...
  • Ages, masses & kinematics of GALAH MS turnoff stars

    Main-sequence turnoff (MSTO) stars are good tracers of Galactic populations since their ages can be reliably estimated from atmospheric parameters. Based on the GALAH survey, we...
  • Galaxies bulge & disk data from SHARDS & HST

    We investigate the assembly history of massive disk galaxies and describe how they shape their morphology through cosmic time. Using SHARDS and HST data, we modeled the surface...
  • MALS SALT-NOT survey of MIR-selected AGN at z<3.5

    We present results of an optical spectroscopic survey using SALT and the Nordic Optical Telescope to build a Wide-field Infrared Survey Explorer mid-infrared color-based,...
  • Radial velocities in W5 YSO groups

    The star-forming region W5 is a major part of the Cassiopeia OB6 association. Its internal structure and kinematics may provide hints of the star formation process in this...
  • Light curves and radial velocities for TOI-1899

    TOI-1899b is a rare exoplanet, a temperate warm Jupiter orbiting an M-dwarf, first discovered by Canas et al. (2020) from a TESS single-transit event. Using new radial...
  • K-band spectroscopy of HD 284149b

    The carbon-to-oxygen (C/O) ratio in an exoplanet atmosphere has been suggested as a potential diagnostic of planet formation. Now that a number of exoplanets have measured C/O...
  • EXPRES radial volocity for {tau} Ceti

    To accurately characterize the planets a star may be hosting, stellar parameters must first be well determined. {tau}Ceti is a nearby solar analog and often a target for...
  • SFACT. III. SFF01 -10 and -15 spectral data

    The Star Formation Across Cosmic Time (SFACT) survey is a new narrowband survey designed to detect emission-line galaxies (ELGs) and quasi-stellar objects (QSOs) over a wide...
  • GEOPS/IPSL DaCHS Server Registry

    The publishing registry for the GEOPS/IPSL DaCHS Server.
  • GEOPS/IPSL DaCHS Server TAP service

    The GEOPS/IPSL DaCHS Server's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own...
  • HEAO 1 A4 Spectra

    The UCSD/MIT Hard X-Ray and Low-Energy Gamma-Ray Instrument, A4, was flown on the HEAO 1 satellite, between August 1977 until January 1979. The experiment consisted of a...
  • HEAO 1 A2 Spectra

    The A2 experiment was flown on the HEAO-1 satellite, between August, 1977 until January 1979. The experiment consisted of six multi-layer multi-anode collimated gas proportional...
  • HEAO 1 A2 Spectra Background

    The A2 experiment was flown on the HEAO-1 satellite, between August, 1977 until January 1979. The experiment consisted of six multi-layer multi-anode collimated gas proportional...
  • DaCHS Server for LMD Registry

    The publishing registry for the DaCHS Server for LMD.
  • Data Central SSA

    Spectra from surveys hosted by Data Central. Most spectra were taken with the multi-object spectroscopy facilities 2dF (Anglo-Australian Telescope) and 6dF (UK Schmidt Telescope).
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