Publications |
- The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue |Watson, M. G., Schroder, A. C., et al. | A&A | 493-339 | 2009 | 2009A&A...493..339W | http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W
- An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy |Levan, A. J., Tanvir, N. R., et al. | Sci | 333-199 | 2011 | 2011Sci...333..199L | http://ui.adsabs.harvard.edu/#abs/2011Sci...333..199L
- Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras |Mateos, S., Saxton, R. D., et al. | A&A | 496-879 | 2009 | 2009A&A...496..879M | http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M
- A Correlation Between Host Star Activity and Planet Mass for Close-in Extrasolar Planets? |Poppenhaeger, K., Schmitt, J. H. M. M., | ApJ | 735-59 | 2011 | 2011ApJ...735...59P | http://ui.adsabs.harvard.edu/#abs/2011ApJ...735...59P
- The XMM Cluster Survey: optical analysis methodology and the first data release |Mehrtens, Nicola, Romer, A. Kathy, et al. | MNRAS | 423-1024 | 2012 | 2012MNRAS.423.1024M | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M
- The Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-Newton Observations |Henley, David B., Shelton, Robin L., et al. | ApJ | 723-935 | 2010 | 2010ApJ...723..935H | http://ui.adsabs.harvard.edu/#abs/2010ApJ...723..935H
- Estimation of the XUV radiation onto close planets and their evaporation |Sanz-Forcada, J., Micela, G., et al. | A&A | 532-6 | 2011 | 2011A&A...532A...6S | http://ui.adsabs.harvard.edu/#abs/2011A&A...532A...6S
- A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations |Muno, M. P., Gaensler, B. M., et al. | ApJ | 680-639 | 2008 | 2008ApJ...680..639M | http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M
- Extrasolar Giant Planets and X-Ray Activity |Kashyap, Vinay L., Drake, Jeremy J., | ApJ | 687-1339 | 2008 | 2008ApJ...687.1339K | http://ui.adsabs.harvard.edu/#abs/2008ApJ...687.1339K
- A scenario of planet erosion by coronal radiation |Sanz-Forcada, J., Ribas, I., et al. | A&A | 511-8 | 2010 | 2010A&A...511L...8S | http://ui.adsabs.harvard.edu/#abs/2010A&A...511L...8S
- Coronal properties of planet-bearing stars |Poppenhaeger, K., Robrade, J., | A&A | 515-98 | 2010 | 2010A&A...515A..98P | http://ui.adsabs.harvard.edu/#abs/2010A&A...515A..98P
- Coronal properties of planet-bearing stars (Corrigendum) |Poppenhaeger, K., Robrade, J., | A&A | 529-1 | 2011 | 2011A&A...529C...1P | http://ui.adsabs.harvard.edu/#abs/2011A&A...529C...1P
- An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 |Henley, David B., Shelton, Robin L., | ApJS | 187-388 | 2010 | 2010ApJS..187..388H | http://ui.adsabs.harvard.edu/#abs/2010ApJS..187..388H
- General X-ray properties of hot, massive stars |Naze, Yael, | BSRSL | 80-109 | 2011 | 2011BSRSL..80..109N | http://ui.adsabs.harvard.edu/#abs/2011BSRSL..80..109N
- An All-Sky Atlas of Radio/X-ray Associations |Flesch, E., | PASA | 27-283 | 2010 | 2010PASA...27..283F | http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F
- The XMM Cluster Survey: X-ray analysis methodology |Lloyd-Davies, E. J., Romer, A. Kathy, et al. | MNRAS | 418-14 | 2011 | 2011MNRAS.418...14L | http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L
- An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities |Henley, David B., Shelton, Robin L., | ApJS | 202-14 | 2012 | 2012ApJS..202...14H | http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H
- The XMM-Newton serendipitous ultraviolet source survey catalogue |Page, M. J., Brindle, C., et al. | MNRAS | 426-903 | 2012 | 2012MNRAS.426..903P | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P
- Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey |Pineau, F.-X., Motch, C., et al. | A&A | 527-126 | 2011 | 2011A&A...527A.126P | http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P
- A systematic cross-search for radio/infrared counterparts of XMM- Newton sources |Combi, J. A., Albacete Colombo, J. F., et al. | Ap&SS | 331-53 | 2011 | 2011Ap&SS.331...53C | http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C
- Exploring X-ray and radio emission of type 1 AGN up to z virgul 2.3 |Ballo, L., Heras, F. J. H., et al. | A&A | 545-66 | 2012 | 2012A&A...545A..66B | http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B
- An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission |Henley, David B., Shelton, Robin L., | ApJ | 773-92 | 2013 | 2013ApJ...773...92H | http://ui.adsabs.harvard.edu/#abs/2013ApJ...773...92H
- Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift |Yershov, V. N., | Ap&SS | 354-97 | 2014 | 2014Ap&SS.354...97Y | http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y
- The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models. X-Ray Emission |Henley, David B., Shelton, Robin L., et al. | ApJ | 800-102 | 2015 | 2015ApJ...800..102H | http://ui.adsabs.harvard.edu/#abs/2015ApJ...800..102H
- Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters |Xiao, Weike, Chen, Chen, et al. | MNRAS | 432-41 | 2013 | 2013MNRAS.432L..41X | http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X
- XMM-Newton publication statistics |Ness, J.-U., Parmar, A. N., et al. | AN | 335-210 | 2014 | 2014AN....335..210N | http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N
- The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars |Lusso, E., Risaliti, G., | ApJ | 819-154 | 2016 | 2016ApJ...819..154L | http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L
- The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo |Miller, Matthew J., Bregman, Joel N., | ApJ | 829-9 | 2016 | 2016ApJ...829....9M | http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M
- The Million Optical - Radio/X-ray Associations (MORX) Catalogue |Flesch, Eric W., | PASA | 33-52 | 2016 | 2016PASA...33...52F | http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F
- A scenario of planet erosion by coronal radiation (Corrigendum) |Sanz-Forcada, J., Ribas, I., et al. | A&A | 520-1 | 2010 | 2010A&A...520C...1S | http://ui.adsabs.harvard.edu/#abs/2010A&A...520C...1S
- Anisotropy of the galaxy cluster X-ray luminosity-temperature relation |Migkas, Konstantinos, Reiprich, Thomas H., | A&A | 611-50 | 2018 | 2018A&A...611A..50M | http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M
- Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals |Sibeck, David G., Allen, R., et al. | SSRv | 214-79 | 2018 | 2018SSRv..214...79S | http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S
- The XMM Cluster Survey: Present status and latest results |Viana, P. T. P., Mehrtens, N., et al. | AN | 334-462 | 2013 | 2013AN....334..462V | http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V
- Testing emergent gravity on galaxy cluster scales |Tamosiunas, Andrius, Bacon, David, et al. | JCAP | 5-53 | 2019 | 2019JCAP...05..053T | http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T
- Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline |Hollowood, Devon L., Jeltema, Tesla, et al. | ApJS | 244-22 | 2019 | 2019ApJS..244...22H | http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H
- Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters |Palmese, A., Annis, J., et al. | MNRAS | 493-4591 | 2020 | 2020MNRAS.493.4591P | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P
- Constraining the Milky Way Mass with Its Hot Gaseous Halo |Guo, Fulai, Zhang, Ruiyu, | ApJ | 904-14 | 2020 | 2020ApJ...904L..14G | http://ui.adsabs.harvard.edu/#abs/2020ApJ...904L..14G
- An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge |Qu, Zhijie, Huang, Rui, et al. | ApJ | 907-14 | 2021 | 2021ApJ...907...14Q | http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q
- A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event |Brightman, Murray, Ward, Charlotte, et al. | ApJ | 909-102 | 2021 | 2021ApJ...909..102B | http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B
- Classification of 4XMM-DR9 sources by machine learning |Zhang, Yanxia, Zhao, Yongheng, | MNRAS | 503-5263 | 2021 | 2021MNRAS.503.5263Z | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z
- The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines |Qu, Zhijie, Koutroumpa, Dimitra, et al. | ApJ | 930-21 | 2022 | 2022ApJ...930...21Q | http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q
- Tidal star-planet interaction and its observed impact on stellar activity in planet-hosting wide binary systems |Ilic, N., Poppenhaeger, K., | MNRAS | 513-4380 | 2022 | 2022MNRAS.513.4380I | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.4380I
- X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 |Wolf, J., Nandra, K., et al. | A&A | 669-127 | 2023 | 2023A&A...669A.127W | http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W
- The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
- From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources |Rodriguez, Antonio C., | PASP | 136-054201 | 2024 | 2024PASP..136e4201R | http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
- Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
- Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
- Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
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