Rafael T Eufrasio, Ph.D. - Publications

Affiliations: 
Physics Department The Catholic University of America, Washington, DC 
Area:
Astrophysics and Cosmology

12 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2020 Lehmer BD, Ferrell AP, Doore K, Eufrasio RT, Monson EB, Alexander DM, Basu-Zych A, Brandt WN, Sivakoff GR, Tzanavaris P, Yukita M, Fragos T, Ptak A. X-ray Binary Luminosity Function Scaling Relations in Elliptical Galaxies: Evidence for Globular Cluster Seeding of Low-Mass X-ray Binaries in Galactic Fields Astrophysical Journal Supplement Series. 248: 31. DOI: 10.3847/1538-4365/Ab9175  0.412
2020 Santana-Silva L, Goncalves TS, Basu-Zych A, Soares-Santos M, Menendez-Delmestre K, Drlica-Wagner A, Riguccini L, Kuropatkin NP, Yanny B, Eufrasio RT. The Environment of Lyman Break Analogues (ELBA) survey: Star-forming galaxies in small groups Monthly Notices of the Royal Astronomical Society. DOI: 10.1093/Mnras/Staa2757  0.612
2019 Lehmer BD, Eufrasio RT, Tzanavaris P, Basu-Zych A, Fragos T, Prestwich A, Yukita M, Zezas A, Hornschemeier AE, Ptak A. X-Ray Binary Luminosity Function Scaling Relations for Local Galaxies Based on Subgalactic Modeling Astrophysical Journal Supplement Series. 243: 3. DOI: 10.3847/1538-4365/Ab22A8  0.389
2019 Miller R, Kennefick D, Kennefick J, Abdeen MS, Monson E, Eufrasio RT, Shields DW, Davis BL. Investigating the Origins of Spiral Structure in Disk Galaxies through a Multiwavelength Study The Astrophysical Journal. 874: 177. DOI: 10.3847/1538-4357/Ab0D26  0.539
2017 Lehmer BD, Eufrasio RT, Markwardt L, Zezas A, Basu-Zych A, Fragos T, Hornschemeier AE, Ptak A, Tzanavaris P, Yukita M. On the Spatially Resolved Star Formation History in M51. II. X-Ray Binary Population Evolution The Astrophysical Journal. 851: 11. DOI: 10.3847/1538-4357/Aa9578  0.577
2017 Eufrasio RT, Lehmer BD, Zezas A, Dwek E, Arendt RG, Basu-Zych A, Wiklind T, Yukita M, Fragos T, Hornschemeier AE, Markwardt L, Ptak A, Tzanavaris P. On the Spatially Resolved Star Formation History in M51. I. Hybrid UV+IR Star Formation Laws and IR Emission from Dust Heated by Old Stars The Astrophysical Journal. 851: 10. DOI: 10.3847/1538-4357/Aa9569  0.598
2017 Peacock MB, Zepf SE, Kundu A, Maccarone TJ, Lehmer BD, Maraston C, Gonzalez AH, Eufrasio RT, Coulter DA. Further Constraints on Variations in the Initial Mass Function from Low-mass X-ray Binary Populations The Astrophysical Journal. 841: 28. DOI: 10.3847/1538-4357/Aa70Eb  0.597
2017 Coulter DA, Lehmer BD, Eufrasio RT, Kundu A, Maccarone T, Peacock M, Hornschemeier AE, Basu-Zych A, Gonzalez AH, Maraston C, Zepf SE. Testing the Universality of the Stellar IMF withChandraandHST The Astrophysical Journal. 835: 183. DOI: 10.3847/1538-4357/835/2/183  0.534
2016 Lehmer B, Basu-Zych A, Mineo S, Brandt WN, Eufrasio RT, Fragos T, Hornschemeier AE, Luo B, Xue Y, Bauer FE, Gilfanov M, Ranalli P, Schneider DP, Shemmer O, Tozzi P, et al. The Evolution of Normal Galaxy X-Ray Emission Through Cosmic History: Constraints from the 6 MS Chandra Deep Field-South The Astrophysical Journal. 825: 7. DOI: 10.3847/0004-637X/825/1/7  0.548
2015 Straughn AN, Voyer EN, Eufrasio RT, Mello DD, Petty S, Kassin S, Gardner JP, Ravindranath S, Soto E. A MULTIWAVELENGTH STUDY of TADPOLE GALAXIES in the HUBBLE ULTRA DEEP FIELD Astrophysical Journal. 814. DOI: 10.1088/0004-637X/814/2/97  0.632
2014 Eufrasio RT, Dwek E, Arendt RG, De Mello DF, Gadotti DA, Urrutia-Viscarra F, De Oliveira CM, Benford DJ. Star formation histories across the interacting galaxy NGC 6872, the largest-known spiral Astrophysical Journal. 795. DOI: 10.1088/0004-637X/795/1/89  0.618
2012 Eufrasio RT, De Mello DF, Urrutia-Viscarra F, De Oliveira CM, Dwek E. When the largest spiral is formed Proceedings of the International Astronomical Union. 8: 328. DOI: 10.1017/S1743921313001543  0.473
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