1,026 datasets found

Keywords: astrophysical processes

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  • LCO i'band LC of SAX J1808.4-3658

    We report on an optical photometric and polarimetric campaign on the accreting millisecond X-ray pulsar (AMXP) SAX J1808.4-3658 during its 2019 outburst. The emergence of a...
  • g- and r- band LCs of Q0957+561 & SBS0909+532

    We present a microlensing analysis of updated light curves in three filters, the g-band, r-band, and H-band, for the gravitationally lensed quasars Q0957+561 and SBS0909+532....
  • ZTF candidate counterparts to 13 GW follow-up

    We present a systematic search for optical counterparts to 13 gravitational wave (GW) triggers involving at least one neutron star during LIGO/Virgo's third observing run (O3)....
  • NICER SGR 1935+2154 burst and persistent emission

    We report on NICER observations of the magnetar SGR1935+2154, covering its 2020 burst storm and long-term persistent emission evolution up to ~90days postoutburst. During the...
  • 4FGLJ0407.7-5702 optical spectroscopy & light curve

    We report the discovery of a variable optical and X-ray source within the error ellipse of the previously unassociated Fermi Large Area Telescope {gamma}-ray source...
  • UV-NIR obs. compilation of GW170817 counterpart

    We present the first effort to aggregate, homogenize, and uniformly model the combined ultraviolet, optical, and near-infrared data set for the electromagnetic counterpart of...
  • Statistical studies of solar white-light flares

    Recently, many superflares on solar-type stars have been discovered as white- light flares (WLFs). The statistical study found a correlation between their energies (E) and...
  • SLACS. XIII. Galaxy-scale strong lens candidates

    We present the full sample of 118 galaxy-scale strong-lens candidates in the Sloan Lens ACS (SLACS) Survey for the Masses (S4TM) Survey, which are spectroscopically selected...
  • Spectroscopy of the fields of gravitational lenses

    Strong gravitational lensing provides an independent measurement of the Hubble parameter (H_0_). One remaining systematic is a bias from the additional mass due to a galaxy...
  • Opt. follow-up of GW events with LCO

    We present an implementation of the Gehrels+ (2016ApJ...820..136G) galaxy-targeted strategy for gravitational-wave (GW) follow-up using the Las Cumbres Observatory global...
  • Opt. follow-up of GW170817 counterpart

    We present the results of prompt optical follow-up of the electromagnetic counterpart of the gravitational-wave event GW170817 by the Transient Optical Robotic Observatory of...
  • Counterpart of GW170817. I. DECam obs.

    We present the Dark Energy Camera (DECam) discovery of the optical counterpart of the first binary neutron star merger detected through gravitational-wave emission, GW170817....
  • Polar network index for the solar cycle studies

    The Sun has a polar magnetic field which oscillates with the 11 yr sunspot cycle. This polar magnetic field is an important component of the dynamo process which operates in the...
  • Spitzer/IRAC Sgr A* light curve data

    We present the first detection from the Spitzer Space Telescope of 4.5 {mu}m variability from Sgr A, the emitting source associated with the Milky Way's central black hole. The...
  • SEAMBHs. II. Continuum and Hbeta LCs

    This is the second in a series of papers reporting on a large reverberation mapping (RM) campaign to measure black hole (BH) mass in high accretion rate active galactic nuclei...
  • Lensed z~6-8 galaxies behind CLASH clusters

    We utilize 16 band Hubble Space Telescope (HST) observations of 18 lensing clusters obtained as part of the Cluster Lensing And Supernova survey with Hubble (CLASH) Multi-Cycle...
  • Light curves of the quasar He 0435-1223

    Microlensing has proved an effective probe of the structure of the innermost regions of quasars and an important test of accretion disk models. We present light curves of the...
  • Strong and weak lensing analysis of A2261

    We precisely constrain the inner mass profile of A2261 (z=0.225) for the first time and determine that this cluster is not "overconcentrated" as found previously, implying a...
  • Conversion from magnetoacoustic to Alfven waves

    Alfven waves may be generated via mode conversion from fast magnetoacoustic waves near their reflection level in the solar atmosphere, with implications both for coronal...
  • Pulsed Alfven waves in the solar wind

    Using 3s plasma and magnetic field data from the Wind spacecraft located in the solar wind well upstream from Earth, we report observations of isolated, pulse-like Alfvenic...
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