22,406 datasets found

Keywords: observational astronomy

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  • LBQS0302-0019 NIRSpec spectrum

    LBQS 0302-0019 is a blue quasar (QSO) at z~3.3 that hosts powerful outflows and resides in a complex environment consisting of an obscured active galactic nucleus (AGN)...
  • NIR lines for AGN up to z~3

    Optical rest-frame spectroscopic diagnostics are usually employed to distinguish between star formation and active galactic nucleus (AGN) powered emission. However, this method...
  • TOI-858 A and TOI-858 B RV data

    We report the discovery of a hot Jupiter on a 3.28-day orbit around a 1.08M_{sun} G0 star that is the secondary component in a loose binary system. Based on follow-up radial...
  • WISE YSO candidates near {sigma} and {lambda} Ori

    We have conducted a sensitive search down to the hydrogen burning limit for unextincted stars over ~200 square degrees around Lambda Orionis and 20 square degrees around Sigma...
  • WOCS. LXVI. Radial velocity survey in M35

    The young (150Myr) open cluster M35 (NGC 2168) has been one of the core clusters of the WIYN Open Cluster Study since 1997. Over these 17years we have obtained approximately...
  • Eclipse timings of 27 eclipsing binaries in the SMC

    We present the periods of apsidal motion for 27 early-type eclipsing binaries with high eccentricity located in the Small Magellanic Cloud. New times of minima were derived from...
  • VVV globulars. I. 2MASS-GC 02, Terzan 10

    The VISTA Variables in the Via Lactea (VVV) ESO Public Survey is opening a new window to study inner Galactic globular clusters (GCs) using their variable stars. These GCs have...
  • Photometry of nova LMC 2012

    We present the results of an intensive multiwavelength campaign on nova LMC 2012. This nova evolved very rapidly in all observed wavelengths. The time to fall two magnitudes in...
  • UBVRI light curves of GSC 3208-1986

    GSC 3208 1986 is an NSVS and TYCHO binary, first observed from 1999 to 2000. It is a W UMa binary with a period of 0.405days. The present observations were taken in 2012...
  • Radial velocity curves of HD 207651

    From numerous radial velocities obtained at KPNO and Fairborn Observatory, we have determined the orbital elements of the composite spectrum triple system HD 207651. This system...
  • Radial velocity of southern visual multiple stars

    High-resolution spectra of visual multiple stars were taken in 2008-2009 to detect or confirm spectroscopic subsystems and to determine their orbits. Radial velocities of 93...
  • Spectroscopy of 299 galaxies from NewHa survey

    Using a sample of 299 H{alpha}-selected galaxies at z~~0.8, we study the relationship between galaxy stellar mass, gas-phase metallicity, and star formation rate (SFR), and...
  • Candidate IR variables from SAGE-SMC survey

    We present our study on the infrared variability of point sources in the Small Magellanic Cloud (SMC). We use the data from the Spitzer Space Telescope Legacy Program "Surveying...
  • SDSS-III/APOGEE. I. Be stars

    The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has amassed the largest ever collection of multi-epoch, high-resolution (R~22500), H-band spectra for B-type...
  • A-F type variable stars from Kepler

    The light curves of 2768 stars with effective temperatures and surface gravities placing them near the gamma Doradus ({gamma} Dor)/delta Scuti ({delta} Sct) instability region...
  • VI photometry of 8 Cepheid candidates in M31

    The ultra-long-period Cepheids (ULPCs) are classical Cepheids with pulsation periods exceeding ~80days. The intrinsic brightness of ULPCs are ~1 to ~3mag brighter than their...
  • MIPSGAL 24{mu}m point source catalog

    In this contribution, we describe the applied methods to construct a 24{mu}m based point source catalog derived from the image data of the MIPSGAL 24{mu}m Galactic Plane Survey...
  • Radial velocities of HD 54371, HR 2692, and 16 UMa

    With extensive sets of new radial velocities we have determined orbital elements for three previously known spectroscopic binaries, HD 54371, HR 2692, and 16 UMa. All three...
  • BVR light curves of V508 Oph

    In this paper, new CCD photometric observations of V508 Oph obtained in 2009 and 2010 at the Xinglong Observatory are presented. From the new observations, six new times of...
  • Modeling Faraday structures. I. 1100-1400 MHz

    Faraday rotation measures (RMs) and more general Faraday structures are key parameters for studying cosmic magnetism and are also sensitive probes of faint ionized thermal gas....
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