RX J1230.5+4141 , the SIMBAD biblio

RX J1230.5+4141 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST18:48:57


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Title First 3 Authors
1999ApJ...519...89C 3 52 588 The nature of accreting black holes in nearby galaxy nuclei. COLBERT E.J.M. and MUSHOTZKY R.F.
2000MNRAS.315...98R 272 206 A ROSAT High Resolution Imager survey of bright nearby galaxies. ROBERTS T.P. and WARWICK R.S.
2002ApJS..143...25C viz 155 187 A catalog of candidate intermediate-luminosity X-ray objects. COLBERT E.J.M. and PTAK A.F.
2002MNRAS.337..677R 55 66 A Chandra observation of the interacting pair of galaxies NGC 4485/4490. ROBERTS T.P., WARWICK R.S., WARD M.J., et al.
2004ApJS..154..519S viz 246 305 The ultraluminous X-ray source population from the Chandra archive of galaxies. SWARTZ D.A., GHOSH K.K., TENNANT A.F., et al.
2005A&A...429.1125L viz 339 66 A catalogue of ultraluminous X-ray sources in external galaxies. LIU Q.Z. and MIRABEL I.F.
2005ApJ...633.1052F 54 65 XMM-Newton observations of ultraluminous X-ray sources in nearby galaxies. FENG H. and KAARET P.
2005ApJS..157...59L viz 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.
2006A&A...454...77L 158 15 Toward a clean sample of ultra-luminous X-ray sources. LOPEZ-CORREDOIRA M. and GUTIERREZ C.M.
2006ApJ...649..730W viz 15       D               147 115 XMM-Newton archival study of the ultraluminous X-ray population in nearby galaxies. WINTER L.M., MUSHOTZKY R.F. and REYNOLDS C.S.
2007ApJ...658L..21V 10 6 Constraints on accretion in ultraluminous X-ray sources from Spitzer IRS observations of NGC 4485/4490: infrared diagnostic diagrams. VAZQUEZ G.A., HORNSCHEMEIER A.E., COLBERT E., et al.
2008MNRAS.387...73R 167       D     X   F     4 14 30 New Hubble Space Telescope imaging of the counterparts to six ultraluminous X-ray sources. ROBERTS T.P., LEVAN A.J. and GOAD M.R.
2008ApJ...687..471B viz 15       D               2 117 49 Testing the paradigm that ultraluminous X-ray sources as a class represent accreting intermediate-mass black holes. BERGHEA C.T., WEAVER K.A., COLBERT E.J.M., et al.
2009MNRAS.397..124G 432       D     X C F     10 22 21 The ultraluminous X-ray source population of NGC 4485/4490. GLADSTONE J.C. and ROBERTS T.P.
2010ApJ...722..760Y 92       D     X         3 35 15 Long-term spectral variations of ultraluminous X-ray sources in the interacting galaxy systems M 51 and NGC 4490/85. YOSHIDA T., EBISAWA K., MATSUSHITA K., et al.
2010ApJ...723.1375R 15       D               1 70 7 The hot interstellar medium of the interacting galaxy NGC 4490. RICHINGS A.J., FABBIANO G., WANG J., et al.
2011ApJ...741...49S viz 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.
2012ApJ...756...27L viz 15       D               1 4348 64 Classification of X-ray sources in the XMM-Newton serendipitous source catalog. LIN D., WEBB N.A. and BARRET D.
2013ApJ...776..100B 62 11 The local environment of ultraluminous X-ray sources viewed by XMM-newton's optical monitor. BERGHEA C.T., DUDIK R.P., TINCHER J., et al.
2017MNRAS.469..671L 219       D S   X         5 97 7 A systematic search for near-infrared counterparts of nearby ultraluminous X-ray sources (II). LOPEZ K.M., HEIDA M., JONKER P.G., et al.
2018MNRAS.473..136J 41           X         1 56 5 Measuring the black hole mass in ultraluminous X-ray sources with the X-ray scaling method. JANG I., GLIOZZI M., SATYAPAL S., et al.
2019ApJ...875...68A 1505     A D     X C       36 18 ~ Optical counterparts of ULXs and their host environments in NGC 4490/4485. AVDAN S., AKYUZ A., VINOKUROV A., et al.
2019ApJ...878...71L viz 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.

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