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5 catalogs found
  
J/ApJ/871/258
  ELQS in SDSS. III. The full ELQS quasar catalog (Schindler+, 2019)
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    J/ApJ/871/258/elqs(c)The full Extremely Luminous Quasar Survey (ELQS) quasar catalog (407 rows)
    J/ApJ/871/258/table2(c)Newly discovered quasars at z≥2.8 in the ELQS-S sample (70 rows)
    J/ApJ/871/258/table10(c)Newly discovered quasars at z<2.8 in the ELQS sample (18 rows)
    J/ApJ/871/258/table11(c)Newly discovered quasars not part of the ELQS primary candidate catalog (51 rows)
  
J/ApJS/243/5
  The ELQS in the PS1 footprint (PS-ELQS) (Schindler+, 2019)
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    J/ApJS/243/5/table7(c)Full Pan-STARRS 1 Extremely Luminous Quasar Survey (PS-ELQS) quasar catalog (592 rows)
    J/ApJS/243/5/table8(c)Newly discovered quasars at z≥2.8 in the PS-ELQS sample (190 rows)
    J/ApJS/243/5/table9(c)Newly discovered quasars at z<2.8 in the PS-ELQS sample (28 rows)
    J/ApJS/243/5/table10(c)Properties of the remaining good PS-ELQS candidates (44 rows)
  
J/A+A/414/487
  Optically bright AGN in ROSAT-FSC (Veron-Cetty+, 2004)
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    J/A+A/414/487/table2(c)List of the 185 galaxy candidates (185 rows)
    J/A+A/414/487/table3(c)List of the 76 known AGN brighter than O(USNO)=16.5, located within 35" of a ROSAT-FSC source (76 rows)
    J/A+A/414/487/table4(c)List of 103 QSO candidates identified with a ROSAT-FSC source and located in zone IVa. (103 rows)
  
J/A+A/655/A109
  Chandra view of the LX-LUV relation in quasars (Bisogni+, 2021)
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    J/A+A/655/A109/table2(c)Properties of the 3430 X-ray observations (3430 rows)
  
J/AJ/133/313
  AGN from RASS and SDSS DR5 (Anderson+, 2007)
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    J/AJ/133/313/BAL(c)Observed and derived parameters of Broad-Line RASS/SDSS AGNs (tables 1 and 2 of paper) (6224 rows)
    J/AJ/133/313/AGN(c)Observed and derived parameters of RASS/SDSS AGNs having narrower permitted emission (tables 3 and 4 of paper) (515 rows)
    J/AJ/133/313/BLLac(c)Observed and derived parameters of RASS/SDSS BL Lac candidates (tables 5 and 6 of paper) (266 rows)

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       (c)  indicates tables which contain celestial coordinates 
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