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  1. Home
  2. Browse by Author

Browsing by Author "Bauer, Franz Erik"

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    A 'high-hard' outburst of the black hole X-ray binary GS 1354-64
    (2016) Koljonen, KII; Russell, D. M.; Corral Santana, J. M.; Padilla, Armas M.; Muñoz Darias, T.; Lewis, F.; Coriat, M.; Bauer, Franz Erik
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    A Catalog of X-ray Point Sources from Two Megaseconds of Chandra Observations of the Galactic Center
    (2009) Muno, M P.; Bauer, Franz Erik
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    A Chandra Catalog of X-Ray Sources in the Central 150 pc of the Galaxy
    (2006) Muno, M P.; Bauer, Franz Erik
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    A Chandra observation of the z= 2.285 galaxy FSC 10214+4724: evidence for a Compton-thick quasar?
    (2005) Bauer, Franz Erik
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    A Chandra Perspective on Galaxy-Wide X-ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxies
    (2010) Lehmer, B. D.; Bauer, Franz Erik
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    A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy
    (2018) Hailey, Charles J.; Mori, Kaya; Bauer, Franz Erik; Berkowitz, Michael E.; Hong, Jaesub; Hord, Benjamin J.
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    A first look at the X-Ray population of the young massive cluster VVV CL077
    (2015) Bodaghee, A.; Tomsick, J.; Fornasini F.; Rahoui, F.; Bauer, Franz Erik
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    A GEOMETRICALLY SUPPORTED z similar to 10 CANDIDATE MULTIPLY IMAGED BY THE HUBBLE FRONTIER FIELDS CLUSTER A2744
    (2014) Zitrin, A.; Zheng, W.; Broadhurst, T.; Moustakas, J.; Lam, D.; Shu, X.; Huang, X.; Diego J. M.; Bauer, Franz Erik; Infante Lira, Leopoldo
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    A Hard X-Ray Test of HCN Enhancements As a Tracer of Embedded Black Hole Growth
    (2020) Privon, George C.; Ricci, Claudio; Aalto, S.; Viti, Serena; Armus, Lee; Diaz-Santos, Tanio; González-Alfonso, E.; Treister, Ezequiel; Bauer, Franz Erik; Garg, P.
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    A kilonova as the electromagnetic counterpart to a gravitational-wave source
    (2017) Smartt, S; Chen, T; Jerkstrand, A; Coughlin, M; Kankare, E; Sim, S; Fraser, M; Inserra, C; Maguire, K; Bauer, Franz Erik; Chambers, K; Huber, M; Kruhler, T; Leloudas, G; Magee, M; Shingles, L
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    A magnetar-powered X-ray transient as the aftermath of a binary neutron-star merger
    (2019) Xue, Yongquan; Zheng, X. C.; Li, Y.; Brandt, W. N.; Zhang, Bryna; Luo, Bruce; Zhang, Boce; Bauer, Franz Erik; Sun, H.; Lehmer, B. D.; Wu, Xuefeng; Yang, Guang; Kong, Xu; Li, J. Y.; Sun, M. Y.; Wang, Junxian; Vito, Fabio
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    A New Compton-thick AGN in Our Cosmic Backyard: Unveiling the Buried Nucleus in NGC 1448 with NuSTAR
    (2017) Annuar, A.; Alexander, D.; Gandhi, P.; Lansbury, G.; Asmus, D.; Ballantyne, D.; Bauer, Franz Erik; Boggs, S.; Boorman, P.; Brandt W.; Brightman, M.|Christensen, F.; Craig, W.; Farrah, D.; Goulding, A.; Hailey, C.; Harrison, F.; Koss, M.; Lamassa, S.; Murray, S.; Ricci, Claudio; Rosario, D.; Stanley, F.; Stern, D.; Zhang, W.
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    A new population of compton-thick AGNs identified using the spectral curvature above 10 keV.
    (2016) Koss, M.; Bauer, Franz Erik; Ricci, Claudio; Treister, Ezequiel; Assef T., Roberto; Balokovic, M.; Stern, Daniel.; Gandhi, P.; Lamperti, I.; Alexander, D. M.
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    A new, faint population of X-ray transients.
    (2017) Bauer, Franz Erik; Treister, Ezequiel; Schulze, Steve.; Schawinski, Kevin; Luo, B.; Alexander, D. M.; Brandt, W N.; Comastri, A.; Forster, Francisco; Gilli, Roberto
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    A NuStar survey of nearby ultraluminous infrared galaxies
    (2015) Teng, Stacy H.; Rigby, Jane R.; Stern, Daniel; Ptak, Andrew; Alexander, D. M.; Bauer, Franz Erik; Boggs, Stephen E.; Brandt, W. Niel; Christensen, Finn E.; Comastri, Andrea
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    A NuSTAR survey of nearby ultraluminous infrared galaxies.
    (2015) Teng, Stacy H.; Bauer, Franz Erik; Treister, Ezequiel; Rigby, Jane R.; Stern, Daniel.; Ptak, Andrew.; Alexander, D. M.; Boggs, Stephen E.; Brandt, W N.; Christensen, Finn E.
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    A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). III. A Large Sample of ALMA Sources in the GOODS-S
    (2018) Cowie, L. L.; Gonzalez-Lopez, J.; Barger, A. J.; Bauer, Franz Erik; Hsu, L. -Y.; Wang, W. -H.
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    A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). IV. The Submillimeter Properties of X-Ray Sources in the CDF-S
    (2019) Barger, A.J.; Cowie, L.L.; Bauer, Franz Erik; González López, Jorge
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    A Unified Binary Neutron Star Merger Magnetar Model for the Chandra X-Ray Transients CDF-S XT1 and XT2
    (2019) Sun, H.; Li, Y.; Zhang, B.B.; Zhang, B.; Bauer, Franz Erik; Xue, Y.Q.; Yuan, W.M.
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    AGN Feedback and Star Formation of Quasar Host Galaxies: Insights from the Molecular Gas
    (2020) Shangguan, Jinyi ; Ho, Luis C. ; Bauer, Franz Erik; Wang, Ran ; Treister, Ezequiel
    Molecular gas serves as a key probe of the complex interplay between black hole accretion and star formation in the host galaxies of active galactic nuclei (AGNs). We use CO(2-1) observations from a new Atacama Large Millimeter/submillimeter Array survey, in conjunction with literature measurements, to investigate the molecular gas properties of a representative sample of 40z < 0.3 Palomar-Green quasars, the largest and most sensitive study of molecular gas emission to date for nearby quasars. We find that the AGN luminosity correlates with both the CO luminosity and black hole mass, suggesting that AGN activity is loosely coupled to the cold gas reservoir of the host. The observed strong correlation between host galaxy total infrared luminosity and AGN luminosity arises from their common dependence on the molecular gas. We argue that the total infrared luminosity, at least for low-redshift quasars, can be used to derive reliable star formation rates for the host galaxy. The host galaxies of low-redshift quasars have a molecular gas content similar to that of star-forming galaxies of comparable stellar mass. Moreover, they share similar gas kinematics, as evidenced by their CO Tully-Fisher relation and the absence of detectable molecular outflows down to sensitive limits. There is no sign that AGN feedback quenches star formation for the quasars in our sample. On the contrary, the abundant gas supply forms stars prodigiously, at a rate that places most of them above the star-forming main sequence and with an efficiency that rivals that of starburst systems.
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