3,985 datasets found

Keywords: photometry

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  • Machine-learned ASAS Classification Cat. (MACC)

    Here, we describe a process to produce a probabilistic classification catalog of variability with machine learning from a multi-epoch photometric survey. In addition to...
  • Counterparts to 1.4GHz sources in ECDF-S

    We study a sample of 883 sources detected in a deep Very Large Array survey at 1.4GHz in the Extended Chandra Deep Field South. This paper focuses on the identification of their...
  • Photometric Catalog of the Deep Ecliptic Survey

    A photometric catalog, developed for the calibration of the Deep Ecliptic Survey, is presented. The catalog contains 213272 unique sources that were measured in V and R filters...
  • Variable stars in Cygnus OB2

    We present a catalog of photometrically variable stars discovered within two 21.3'x21.3' fields centered on the Cygnus OB2 association (Cyg OB2). There have hitherto been no...
  • Light curves for 165 SNe

    We present BVRI light curves of 165 Type Ia supernovae (SNe Ia) from the Lick Observatory Supernova Search follow-up photometry program from 1998 through 2008. Our light curves...
  • VI photometry and spectroscopy in h+{chi} Per

    From photometric observations of ~47000 stars and spectroscopy of ~11000 stars, we describe the first extensive study of the stellar population of the famous Double Cluster, h...
  • Cepheids in 3 host galaxies

    This is the first of two papers reporting measurements from a program to determine the Hubble constant to ~5% precision from a refurbished distance ladder. We present new...
  • AEGIS-X: Chandra deep survey

    We present the EGIS-X survey, a series of deep Chandra ACIS-I observations of the Extended Groth Strip. The survey comprises pointings at eight separate positions, each with...
  • Subaru/XMM-Newton deep survey IV. (SXDS)

    We present luminosity functions (LFs) and various properties of Ly{alpha} emitters (LAEs) at z=3.1, 3.7, and 5.7, in a 1deg^2^ sky of the Subaru/XMM-Newton Deep Survey (SXDS)...
  • Subaru/XMM-Newton deep survey (SXDS). II.

    We present multi-wave band optical imaging data obtained from observations of the Subaru/XMM-Newton Deep Survey (SXDS). The survey field, centered at RA=02:18:00, DE=-05:00:00,...
  • GALEX/Spitzer photometry in NGC 7331

    We present images of NGC 7331 obtained with GALEX and Spitzer, tracing UV and IR signatures of star formation. NGC 7331's morphology at 8-850um is dominated by a central dust...
  • Infrared observations of the Pleiades

    We make use of new near- and mid-IR photometry of the Pleiades cluster in order to help identify proposed cluster members. We also use the new photometry with previously...
  • SEXSI catalog. III

    We present the catalog of 477 spectra from the Serendipitous Extragalactic X-ray Source Identification (SEXSI) program, a survey designed to probe the dominant contributors to...
  • Spectrophotometry of nearby galaxies

    We present integrated optical spectrophotometry for a sample of 417 nearby galaxies. Our observations consist of spatially integrated, S/N=10-100 spectroscopy between 3600 and...
  • SEXSI catalog. II

    The Serendipitous Extragalactic X-ray Source Identification (SEXSI) Program is designed to expand significantly the sample of identified extragalactic hard X-ray sources at...
  • Chandra Deep Field-South: Optical spectroscopy

    We present the results of our spectroscopic follow-up program of the X-ray sources detected in the 942ks exposure of the Chandra Deep Field-South (CDFS). A total of 288 possible...
  • EXtended-UV galaxies surface brightness

    Extended-UV (XUV) galaxies are galaxies presenting an extended outer ultraviolet disks. Although some Giant Low Surface Brightness (GLSB) galaxies are also XUV, their relation...
  • Candidate mpc separation massive BH binaries

    The role of mergers in the evolution of massive black holes is still unclear,and their dynamical evolution, from the formation of pairs to binaries and the final coalescence,...
  • Compiled photometry for Cham I and II members

    We present the results of a proper motion study aiming at providing further evidence on the origin of the proposed stellar members of the Chamaeleon I and II clouds and to...
  • CHEOPS and TESS photometry of KELT-7

    Early theoretical works suggested that ultrahot Jupiters have inverted temperature-pressure (T-P) profiles in the presence of optical absorbers, such as TiO and VO. Recently, an...
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