Relevant bibliographies by topics / Reverberation mapping

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Reverberation mapping'

Author: Grafiati
Published: 4 June 2021
Last updated: 5 February 2022

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Journal articles on the topic "Reverberation mapping"

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Fine, S., T. Shanks, P. Green, B. C. Kelly, S. M. Croom, R. L. Webster, E. Berger, et al. "Stacked reverberation mapping." Monthly Notices of the Royal Astronomical Society: Letters 434, no. 1 (June 12, 2013): L16—L20. http://dx.doi.org/10.1093/mnrasl/slt069.

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Brewer, Brendon J., and Tom M. Elliott. "Hierarchical reverberation mapping." Monthly Notices of the Royal Astronomical Society: Letters 439, no. 1 (January 16, 2014): L31—L35. http://dx.doi.org/10.1093/mnrasl/slt174.

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Shen, Yue. "ASTROMETRIC REVERBERATION MAPPING." Astrophysical Journal 757, no. 2 (September 12, 2012): 152. http://dx.doi.org/10.1088/0004-637x/757/2/152.

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Fine, S., T. Shanks, S. M. Croom, P. Green, B. C. Kelly, E. Berger, R. Chornock, W. S. Burgett, E. A. Magnier, and P. A. Price. "Composite reverberation mapping." Monthly Notices of the Royal Astronomical Society 427, no. 4 (December 21, 2012): 2701–10. http://dx.doi.org/10.1111/j.1365-2966.2012.21248.x.

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Peterson, Bradley M. "Space Telescope and Optical Reverberation Mapping Project: A Leap Forward in Reverberation Mapping." Proceedings of the International Astronomical Union 12, S324 (September 2016): 215–18. http://dx.doi.org/10.1017/s1743921316012680.

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AbstractIn 2014, a 179-orbit allocation of Hubble Space Telescope time anchored a massive reverberation-mapping program on the well-studied Seyfert 1 galaxy NGC 5548. Supporting imaging and spectrophotometric observations were provided by Swift, Chandra, Spitzer, and a world-wide network of ground-based telescopes. Understanding the data remains a significant challenge, partly because the level of detail is far beyond what has been seen before and partly because the behavior of the AGN was not typical of its past behavior. Based on analysis to date, the following conclusions can be reached: (1) the AGN accretion disk has a temperature profile that is consistent with that predicted by the Shakura–Sunyaev model, but is about three times larger than expected; (2) at least part of the broad-line region appears to be a Keplerian disk seen at intermediate inclination, and (3) the broad-line emission response from the far side of the disk is weaker than expected.
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Peterson, Bradley M. "Reverberation mapping of active nuclei." Advances in Space Research 21, no. 1-2 (January 1998): 57–66. http://dx.doi.org/10.1016/s0273-1177(97)00614-5.

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Yu, Z., C. S. Kochanek, B. M. Peterson, Y. Zu, W. N. Brandt, E. M. Cackett, M. M. Fausnaugh, and I. M. McHardy. "On reverberation mapping lag uncertainties." Monthly Notices of the Royal Astronomical Society 491, no. 4 (December 11, 2019): 6045–64. http://dx.doi.org/10.1093/mnras/stz3464.

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ABSTRACT We broadly explore the effects of systematic errors on reverberation mapping lag uncertainty estimates from javelin and the interpolated cross-correlation function (ICCF) method. We focus on simulated light curves from random realizations of the light curves of five intensively monitored AGNs. Both methods generally work well even in the presence of systematic errors, although javelin generally provides better error estimates. Poorly estimated light-curve uncertainties have less effect on the ICCF method because, unlike javelin , it does not explicitly assume Gaussian statistics. Neither method is sensitive to changes in the stochastic process driving the continuum or the transfer function relating the line light curve to the continuum. The only systematic error we considered that causes significant problems is if the line light curve is not a smoothed and shifted version of the continuum light curve but instead contains some additional sources of variability.
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Mastroserio, Guglielmo, Adam Ingram, and Michiel van der Klis. "Multi-timescale reverberation mapping of Mrk 335." Monthly Notices of the Royal Astronomical Society 498, no. 4 (September 10, 2020): 4971–82. http://dx.doi.org/10.1093/mnras/staa2735.

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ABSTRACT Time lags due to X-ray reverberation have been detected in several Seyfert galaxies. The different traveltime between reflected and directly observed rays naturally causes this type of lag, which depends directly on the light-crossing time-scale of the system and hence scales with the mass of the central black hole. Featureless ‘hard lags’ not associated with reverberation, and often interpreted as propagating mass accretion rate fluctuations, dominate the longer time-scale variability. Here we fit our reltrans model simultaneously to the time-averaged energy spectrum and the lag-energy spectra of the Seyfert galaxy Mrk 335 over two time-scales (Fourier frequency ranges). We model the hard lags as fluctuations in the slope and strength of the illuminating spectrum, and self-consistently account for the effects that these fluctuations have on the reverberation lags. The resulting mass estimate is $1.1^{+2.0}_{-0.7} \times 10^6~\mathrm{ M}_\odot$, which is significantly lower than the mass measured with the optical reverberation mapping technique (14–26 million M⊙). When we add the correlated variability amplitudes to the time lags by fitting the full complex cross-spectra, the model is unable to describe the characteristic reverberation Fe K α line and cannot constrain the black hole mass. This may be due to the assumption that the direct radiation is emitted by a point-like source.
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Denney, Kelly D., B. M. Peterson, R. W. Pogge, M. C. Bentz, C. M. Gaskell, T. Minezaki, C. A. Onken, S. G. Sergeev, and M. Vestergaard. "Reverberation Mapping Results from MDM Observatory." Proceedings of the International Astronomical Union 5, S267 (August 2009): 201. http://dx.doi.org/10.1017/s1743921310006216.

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Reverberation mapping takes advantage of the presence of a time delay or lag, τ, between continuum and emission line flux variations observed through spectroscopic monitoring campaigns to infer the radius of the broad-line region (BLR) and, subsequently, the central black hole mass in type 1 AGNs. We present results from a multi-month reverberation mapping campaign undertaken primarily at MDM Observatory with supporting observations from around the world. We measure BLR radii and black hole masses for six objects. The primary goal of this campaign was to obtain either new or improved Hβ reverberation lag measurements for several relatively low-luminosity AGNs. Using cross correlation techniques to measure the time delay between the mean optical continuum flux density around 5100 Å and the integrated Hβ flux, we determine the Hβ lags and black hole mass measurements listed in columns 2 and 3 of Table 1, respectively. Column 4 tells if this measurement is new, an improvement meant to replace a previous, less reliable measurement, or simply an additional measurement not used to replace a previous value. The complete results from this study are currently being prepared for publication. A subsequent velocity-resolved analysis of the Hβ response shows that three of the six primary targets demonstrate kinematic signatures (column 5) of infall, outflow, and non-radial virialized motions (see Denney et al. 2009).
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Peterson, Bradley M., and Misty C. Bentz. "Black hole masses from reverberation mapping." New Astronomy Reviews 50, no. 9-10 (November 2006): 796–99. http://dx.doi.org/10.1016/j.newar.2006.06.062.

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Dissertations / Theses on the topic "Reverberation mapping"

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Starkey, D., Keith Horne, M. M. Fausnaugh, B. M. Peterson, M. C. Bentz, C. S. Kochanek, K. D. Denney, et al. "SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT.VI. REVERBERATING DISK MODELS FOR NGC 5548." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/622875.

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We conduct a multiwavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investigate the temperature structure of its accretion disk. The 19 overlapping continuum light curves (1158 angstrom to 9157 angstrom) combine simultaneous Hubble Space Telescope, Swift, and ground-based observations over a 180 day period from 2014 January to July. Light-curve variability is interpreted as the reverberation response of the accretion disk to irradiation by a central time-varying point source. Our model yields the disk inclination i = 36 degrees +/- 10 degrees, temperature T-1= (44 +/- 6) x 10(3) K at 1 light day from the black hole, and a temperature-radius slope (T proportional to r(-alpha)) of alpha = 0.99 +/- 0.03. We also infer the driving light curve and find that it correlates poorly with both the hard and soft X-ray light curves, suggesting that the X-rays alone may not drive the ultraviolet and optical variability over the observing period. We also decompose the light curves into bright, faint, and mean accretion-disk spectra. These spectra lie below that expected for a standard blackbody accretion disk accreting at L/L-Edd = 0.1.
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Comins, Megan. "Systematic errors in black hole mass measurement using reverberation mapping." Connect to resource, 2008. http://hdl.handle.net/1811/32152.

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Fausnaugh, Michael Martin. "Reverberation Mapping of the Continuum Source in Active Galactic Nuclei." The Ohio State University, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=osu1494244528720735.

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Grier, C. J., J. R. Trump, Yue Shen, Keith Horne, Karen Kinemuchi, Ian D. McGreer, D. A. Starkey, et al. "The Sloan Digital Sky Survey Reverberation Mapping Project: Hα and Hβ Reverberation Measurements from First-year Spectroscopy and Photometry." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/627102.

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We present reverberation mapping results from the first year of combined spectroscopic and photometric observations of the Sloan Digital Sky Survey Reverberation Mapping Project. We successfully recover reverberation time delays between the g+i band emission and the broad H beta emission line for a total of 44 quasars, and for the broad Ha emission line in 18 quasars. Time delays are computed using the JAVELIN and CREAM software and the traditional interpolated cross-correlation function (ICCF): using well-defined criteria, we report measurements of 32 H beta and 13 Ha lags with JAVELIN, 42 H beta and 17 Ha lags with CREAM, and 16 H beta and eight Ha lags with the ICCF. Lag values are generally consistent among the three methods, though we typically measure smaller uncertainties with JAVELIN and CREAM than with the ICCF, given the more physically motivated light curve interpolation and more robust statistical modeling of the former two methods. The median redshift of our H beta-detected sample of quasars is 0.53, significantly higher than that of the previous reverberation mapping sample. We find that in most objects, the time delay of the Ha emission is consistent with or slightly longer than that of H beta. We measure black hole masses using our measured time delays and line widths for these quasars. These black hole mass measurements are mostly consistent with expectations based on the local M-BH-sigma* relationship, and are also consistent with single-epoch black hole mass measurements. This work increases the current sample size of reverberation-mapped active galaxies by about two-thirds and represents the first large sample of reverberation mapping observations beyond the local universe (z < 0.3).
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Carroll, Carla June. "A Feasibility Study of Photometric Reverberation Mapping with Meter-Class Telescopes." BYU ScholarsArchive, 2015. https://scholarsarchive.byu.edu/etd/5469.

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For the past several decades, mass estimates for supermassive black holes hosted by active galactic nuclei (AGN) have been made with the reverberation mapping (RM) technique. This methodology has produced consistent results and has been used to establish several relations that link the characteristics of the host galaxy to the mass of the central black hole. Despite this success, there are less than 50 AGN with black hole masses derived from RM. This low number is generally attributed to the difficulties in coordinating large blocks of telescope time for making simultaneous photometric and spectroscopic observations. Spectroscopic observations also generally require several months of nightly observations with moderate to large size telescopes as the signal-to-noise ratio is too low for smaller telescopes. We have made photometric observations of NGC 5548 in four filters (a custom-made Hα10 filter, the Strömgren y filter, the Johnson/Cousins V filter and the Johnson/Cousins R filter) in order to evaluate a photometric methodology for determining the lag time between the variations observed in the continuum and the Hα emission from the broad-line region (BLR) gas. This time delay represents the mean light travel time to the BLR and is therefore a measurement of the mean BLR radius. Multiple JAVELIN analyses of the three continuum light curves (y, V, and R), relative to the light curve from the Hα10 filter yields a value for τ = 3.3 ± 0.1 days. Adopting a value of f = 5.5, along with a single-epoch spectroscopic measurement from Park et of Δv = 4354±25 km/s, enables us to estimate a black hole mass of M_BH = 67.2±2.2x10^6 M_sun.
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Meng, Huan Y. A., Peter Plavchan, George H. Rieke, Ann Marie Cody, Tina Güth, John Stauffer, Kevin Covey, et al. "PHOTO-REVERBERATION MAPPING OF A PROTOPLANETARY ACCRETION DISK AROUND A T TAURI STAR." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621264.

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Theoretical models and spectroscopic observations of newborn stars suggest that protoplantary disks have an inner "wall" at a distance set by the disk interaction with the star. Around T Tauri stars, the size of this disk hole is expected to be on a 0.1 au scale that is unresolved by current adaptive optics imaging, though some model-dependent constraints have been obtained by near-infrared interferometry. Here we report the first measurement of the inner disk wall around a solar-mass young stellar object, YLW 16B in the rho Ophiuchi star-forming region, by detecting the light-travel time of the variable radiation from the stellar surface to the disk. Consistent time lags were detected on two nights, when the time series in H (1.6 mu m) and K (2.2 mu m) bands were synchronized while the 4.5 mu m emission lagged by 74.5 +/- 3.2 s. Considering the nearly edge-on geometry of the disk, the inner rim should be 0.084 au from the protostar on average, with an error of order 0.01 au. This size is likely larger than the range of magnetospheric truncations and consistent with an optically and geometrically thick disk front at the dust sublimation radius at similar to 1500 K. The widths of the cross-correlation functions between the data in different wavebands place possible new constraints on the geometry of the disk.
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Bentz, Misty C. "Black hole scaling relationships new results from reverberation mapping and Hubble Space Telescope imaging /." Columbus, Ohio : Ohio State University, 2007. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=osu1180453426.

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Goad, M. R., K. T. Korista, G. De Rosa, G. A. Kriss, R. Edelson, A. J. Barth, G. J. Ferland, et al. "SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. IV. ANOMALOUS BEHAVIOR OF THE BROAD ULTRAVIOLET EMISSION LINES IN NGC 5548." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/621259.

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During an intensive Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) UV monitoring campaign of the Seyfert 1 galaxy NGC 5548 performed from 2014 February to July, the normally highly correlated far UV continuum and broad emission line variations decorrelated for similar to 60-70 days, starting similar to 75 days after the first HST/COS observation. Following this anomalous state, the flux and variability of the broad emission lines returned to a more normal state. This transient behavior, characterized by significant deficits in flux and equivalent width of the strong broad UV emission lines, is the first of its kind to be unambiguously identified in an active galactic nucleus reverberation mapping campaign. The largest corresponding emission line flux deficits occurred for the high ionization, collisionally excited lines C IV and Si IV(+O IV]), and also He II(+O III]), while the anomaly in Ly alpha was substantially smaller. This pattern of behavior indicates a depletion in the flux of photons with E-ph > 54 eV relative to those near 13.6 eV. We suggest two plausible mechanisms for the observed behavior: (i) temporary obscuration of the ionizing continuum incident upon broad line region (BLR) clouds by a moving veil of material lying between the inner accretion disk and inner (BLR), perhaps resulting from an episodic ejection of material from the disk, or (ii) a temporary change in the intrinsic ionizing continuum spectral energy distribution resulting in a deficit of ionizing photons with energies > 54 eV, possibly due to a transient restructuring of the Comptonizing atmosphere above the disk. Current evidence appears to favor the latter explanation.
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Grier, Catherine J. "Active Galactic Nuclei: Masses and Dynamics." The Ohio State University, 2013. http://rave.ohiolink.edu/etdc/view?acc_num=osu1372681067.

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Mudd, Dale Montaine. "Understanding Supermassive Black Holes Using the Dark Energy Survey and OzDES." The Ohio State University, 2017. http://rave.ohiolink.edu/etdc/view?acc_num=osu1500305577021114.

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Books on the topic "Reverberation mapping"

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M, Gondhalekar P., Horne K, Peterson B. M, and Rutherford Appleton Laboratory. Workshop on Astronomy and Astrophysics, eds. Reverberation mapping of the broad-line region in active galactic nuclei. San Francisco: Astronomical Society of the Pacific, 1994.

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Book chapters on the topic "Reverberation mapping"

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Bentz, Misty C. "AGN Reverberation Mapping." In Astronomy at High Angular Resolution, 249–66. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-39739-9_13.

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Brewer, Brendon J. "Bayesian Analysis of Reverberation Mapping Data." In Lecture Notes in Statistics, 189–95. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-3520-4_17.

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Kaspi, S. "Reverberation Mapping of High Luminosity AGN." In Astronomical Time Series, 243–46. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-015-8941-3_34.

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Netzer, Hagai, and Bradley M. Peterson. "Reverberation Mapping and the Physics of Active Galactic Nuclei." In Astronomical Time Series, 85–108. Dordrecht: Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-015-8941-3_8.

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Xue, S. J., and F. Z. Cheng. "Reverberation Mapping Analysis of the Broad- Line Region in Seyfert Galaxy NGC 4151." In The Hot Universe, 424–25. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4970-9_155.

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Craig, Cheryl J., and Janice Huber. "Relational Reverberations: Shaping and Reshaping Narrative Inquiries in the Midst of Storied Lives and Contexts." In Handbook of Narrative Inquiry: Mapping a Methodology, 251–79. 2455 Teller Road, Thousand Oaks California 91320 United States: SAGE Publications, Inc., 2007. http://dx.doi.org/10.4135/9781452226552.n10.

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"Ultrasound." In Echocardiography, edited by Paul Leeson, Christiana Monteiro, Daniel Augustine, Harald Becher, Paul Leeson, Christiana Monteiro, Daniel Augustine, and Harald Becher, 3–70. Oxford University Press, 2020. http://dx.doi.org/10.1093/med/9780198804161.003.0001.

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After a brief introduction to echocardiography, sound waves, and ultrasound, this chapter covers the following topics: the behaviour of ultrasound in tissue; reflection, attenuation, and depth compensation; reverberation artefacts; transthoracic, transoesophageal, and other transducers; echocardiography modes; transmit power; gain; grey scale and compression; image resolution; fundamental and second harmonic imaging; Doppler echocardiography; spectral trace analysis; continuous wave and pulsed wave Doppler; colour flow mapping; tissue Doppler imaging; second harmonic Doppler for contrast imaging; power Doppler (amplitude) imaging; 3D echocardiography, artefacts, image display, and image rendering; speckle tracking echocardiography; basic fluid dynamics; and the bioeffects of ultrasound.
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Fiore, Teresa. "All at One Point: The Unlikely Connections between Italy’s Emigration, Immigration, and (Post)Colonialism." In Pre-Occupied Spaces. Fordham University Press, 2017. http://dx.doi.org/10.5422/fordham/9780823274321.003.0001.

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The introduction opens with a reading of Italo Calvino’s poignant short story “All at One Point.” It relies on statistical data, sociological studies, and historical facts to address the connections between emigration from Italy and immigration to Italy, as well as Italian colonialism in Africa and the Mediterranean, and its postcolonial legacy. This intersection prompts a re-mapping of the Italian nation and poses Italy as a unique laboratory to rethink national belonging at large in our era of massive demographic mobility. The introduction explains the application of theories of space by de Certeau, Lefebvre, and Soja to the trans-national dimension of the Italian nation and highlights the main goals of the book. The introduction offers a fairly comprehensive survey of the fields that the book is in dialogue with by positioning itself vis-à-vis previous publications and also functions as an overview. It highlights the double approach of the book which is, on one hand to focus on texts that address both emigration and immigration or colonialism in conjunction; and, on the other, to connect texts that can be fruitfully read in tandem in order to create historical and cultural reverberations.
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Conference papers on the topic "Reverberation mapping"

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Grier, Catherine, Bradley Peterson, Kelly Denney, Misty Bentz, and Richard W. Pogge. "New results in reverberation mapping." In Narrow-Line Seyfert 1 Galaxies and their place in the Universe. Trieste, Italy: Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.126.0052.

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Pozo, Francisco, Michael Ramolla, Christian Westhues, Christoph Bruckmann, Martin Haas, Rolf Chini, Katrien Steenbrugge, and Miguel Murphy. "Photometric reverberation mapping of 3C120." In Nuclei of Seyfert galaxies and QSOs - Central engine & conditions of star formation. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.169.0035.

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Denney, Kelly. "Reverberation Mapping: Masses and Distance and Size, Oh My!" In Frank N. Bash Symposium 2013: New Horizons in Astronomy. Trieste, Italy: Sissa Medialab, 2014. http://dx.doi.org/10.22323/1.206.0010.

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Peterson, Bradley, and Elena Dalla Bontà. "Reverberation Mapping and Implications for Narrow-Line Seyfert 1 Galaxies." In Revisiting narrow-line Seyfert 1 galaxies and their place in the Universe. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.328.0008.

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Pozo Nunez, Francisco, Doron Chelouche, and Shai Kaspi. "Accretion disk reverberation mapping of Active Galactic Nuclei at Wise Observatory." In Revisiting narrow-line Seyfert 1 galaxies and their place in the Universe. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.328.0056.

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Rakshit, Suvendu, and Romain G. Petrov. "AGN BLR structure, luminosity and mass from combined reverberation mapping and optical interferometry observations." In SPIE Astronomical Telescopes + Instrumentation, edited by Jayadev K. Rajagopal, Michelle J. Creech-Eakman, and Fabien Malbet. SPIE, 2014. http://dx.doi.org/10.1117/12.2056436.

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