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2XMM J112021.0+125846 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST05:07:51 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2005ApJS..157...59L | 840 | 130 | Ultraluminous X-ray sources in nearby galaxies from ROSAT high resolution imager observations I. Data analysis. | LIU J.-F. and BREGMAN J.N. | |||||
2006ApJS..166..154P | 71 | 44 | Optical counterparts of ultraluminous X-ray sources identified from archival HST WFPC2 images. | PTAK A., COLBERT E., VAN DER MAREL R.P., et al. | |||||
2009ApJ...703..159S | 107 | 57 | Ultraluminous X-ray source correlations with star-forming regions. | SWARTZ D.A., TENNANT A.F. and SORIA R. | |||||
2011ApJ...741...49S | 15 | D | 2 | 169 | 167 | A complete sample of ultraluminous X-ray source host galaxies. | SWARTZ D.A., SORIA R., TENNANT A.F., et al. | ||
2012A&A...544A.113W | 15 | D | 1 | 7 | 3 | NGC 3627: a galaxy-dwarf collision ? | WEZGOWIEC M., SOIDA M. and BOMANS D.J. | ||
2014MNRAS.442.1054H | 212 | D | X | 6 | 102 | 27 | Near-infrared counterparts of ultraluminous X-ray sources. | HEIDA M., JONKER P.G., TORRES M.A.P., et al. | |
2016MNRAS.455L..91A | 546 | A | X C | 13 | 24 | 9 | Optical counterparts of two ULXs in NGC 5474 and NGC 3627 (M 66). | AVDAN S., VINOKUROV A., FABRIKA S., et al. | |
2018ApJ...854..176V | 83 | X | 2 | 23 | 27 | Optical counterparts of ultraluminous X-ray sources NGC 4559 X-10 and NGC 4395 ULX-1. | VINOKUROV A., FABRIKA S. and ATAPIN K. | ||
2019ApJ...878...71L | 17 | D | 2 | 165 | 5 | Uncovering red and dusty ultraluminous X-ray sources with Spitzer. | LAU R.M., HEIDA M., WALTON D.J., et al. | ||
2020MNRAS.497..917L | 17 | D | 2 | 86 | ~ | NIR counterparts to ULXs (III): completing the photometric survey and selected spectroscopic results. | LOPEZ K.M., HEIDA M., JONKER P.G., et al. | ||
2022ApJ...936..162S | 448 | S X C | 8 | 22 | 3 | NuSTAR Observations of AGNs with Low Observed X-Ray to [O III] Luminosity Ratios: Heavily Obscured AGNs or Turned-off AGNs? | SAADE M.L., BRIGHTMAN M., STERN D., et al. |