Relevant bibliographies by topics / ROSAT

Academic literature on the topic 'ROSAT'

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Published: 4 June 2021
Last updated: 21 February 2023

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Journal articles on the topic "ROSAT"

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Cowen, Ron. "Rosat Revelations." Science News 139, no. 26 (June 29, 1991): 408. http://dx.doi.org/10.2307/3975332.

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TRÜMPER, JOACHIM E. "ROSAT: Early Results." Annals of the New York Academy of Sciences 647, no. 1 Texas/ESO-Cer (December 1991): 141–50. http://dx.doi.org/10.1111/j.1749-6632.1991.tb32165.x.

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Hasinger, Günther. "ROSAT Deep Surveys." Highlights of Astronomy 9 (1992): 199–204. http://dx.doi.org/10.1017/s1539299600008923.

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AbstractA series of 20 deep pointed observations with the ROSAT PSPC is discussed. 530 X-ray sources with 0.5-2 keV fluxes down to 3·10-15erg cm-2 s-1 have been discovered in 5.9 deg2. The N(>S) relation of the sources selected in the 0.5-2 keV band shows a density in excess of 200 deg-2 at the faintest fluxes and a flattening below 2·10-14erg cm-2 s-1. The average spectrum of those sources is a power law with energy index 1.2 ±0.1. The absorption column densities are consistent with the galactic HI columns. More than 50% of the 1-2 keV background has been resolved into discrete sources in the deepest field. The total background spectrum shows an emission line feature around 0.65 keV, most probably due to OVII-OVIII from a 2·106K plasma. Above ~ 1 keV the background is dominated by a power law spectrum with a normalization of 13.4 ± 0.2 keV cm-2 s-1 sr-1 keV-1 and a slope 1.2 ± 0.1, i.e. considerably steeper than the extrapolation from higher energies.
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Trümper, J. "The ROSAT Mission." International Astronomical Union Colloquium 115 (1990): 291–94. http://dx.doi.org/10.1017/s0252921100012483.

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AbstractThe scientific payload of ROSAT consists of a 83 cm X-ray telescope (6 – 100 Å) and a 60 cm XUV-telescope (60 – 300 Å) which are looking parallel. An important objective of the mission is to perform the first all-sky survey with imaging X-ray telescopes providing an improvement in sensitivity by several orders of magnitude compared with previous surveys. A large number of new X-ray sources (~ 105) is expected to be discovered and located with an accuracy of 1 arcmin or better, depending on source strength. The sources discovered will represent almost all types of astronomical objects, ranging from nearby normal stars to distant quasars.After completion of the sky survey which will take half a year, the instruments will be used for detailed investigations of selected sources with respect to spatial structures, spectra and time variability. In this pointing mode, which will be open for guest observers, ROSAT is expected to provide substantial improvements over the imaging instruments of the Einstein observatory.
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Hasinger, G. "ROSAT deep surveys." Advances in Space Research 13, no. 12 (December 1993): 241–51. http://dx.doi.org/10.1016/0273-1177(93)90116-s.

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Gottwald, Manfred, and Günther Hasinger. "Der Röntgensatellit ROSAT." Physik in unserer Zeit 21, no. 6 (1990): 258–66. http://dx.doi.org/10.1002/piuz.19900210604.

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Trümper, J. "Der Röntgensatellit ROSAT." Physik Journal 46, no. 5 (May 1990): 137–43. http://dx.doi.org/10.1002/phbl.19900460502.

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Sietmann, Richard, and Tony Jones. "Astronomy: ROSAT rolls onward." Physics World 3, no. 9 (September 1990): 7. http://dx.doi.org/10.1088/2058-7058/3/9/5.

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Bühler, P., T. J. L. Courvoisier, R. Staubert, H. Brunner, and G. Lamer. "ROSAT Spectra of Quasars." Symposium - International Astronomical Union 159 (1994): 369. http://dx.doi.org/10.1017/s007418090017562x.

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X–ray observations of AGN with Einstein, EXOSAT and Ginga have shown, that the spectra of quasars in the energy range 2 to 10 keV can be approximately described by a single power law model with a photon index of 1.7 to 2.0. They also suggested that a soft X-ray excess component (below ≈ 1 keV) is a common feature in many quasars. In order to investigate whether a soft excess is characteristic for a certain class of objects we analysed the data of the pointed ROSAT PSPC observations of the six radio-loud quasars PG0007+106, PKS0135-247, QSO0537-286, QSO0923+392, PG1225+317, 3C273 and the radio-quiet quasar PG0804+761. In a first step the observed spectra were fitted with an absorbed single power law model. The hydrogen column density was fixed to its galactic value and the normalisation at 1 keV and the spectral index α were the free fit parameters. In order to decide whether a soft component is present in a source, the resulting power law index was compared with the hard X-ray power law index (2–10 keV) determined in the past with other instruments. A steep ROSAT PSPC spectrum indicates the presence of an additional soft X–ray component. In four cases (PKS0135-247, PG0804+761, QSO0923+392, 3C273) we find that the spectra in the PSPC band are considerably steeper than the spectra above 2 keV and therefore suggest the presence of a soft excess. In order to quantify the contribution of the soft excess these spectra were successively fitted with a model containing a hard power law component and an additional soft component described either by a power law, thermal bremsstrahlung or black body model. For the other three members of our sample (0007+106, 0537-286, 1225+317) the fitted power law index is not enhanced. This means that no soft component has been detected, but not necessarily that it does not exist. There are two effects which render more difficult the detection of a soft component in ROSAT spectra, the absorption of photons by interstellar material and the shift of the spectra towards lower energies due to the redshift. Both processes have first an effect on the soft part of the observed spectrum and it is therefore evident, that this leads to a decrease of the sensitivity for soft X–rays of the emitted spectrum. For the three quasars in our sample, where no soft excess has been detected, either the column density (0007+106) or the redshift (0537-286, 1225+317) is especially large and therefore an eventually present soft component could have remained undetected. In these cases we calculated upper limits for the strength of such a soft component (P. Bühler et al., to be published in A&A.)
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Lehmann, I., G. Hasinger, M. Schmidt, R. Giacconi, J. Trümper, G. Zamorani, J. E. Gunn, et al. "The ROSAT Deep Survey." Astronomy & Astrophysics 371, no. 3 (June 2001): 833–57. http://dx.doi.org/10.1051/0004-6361:20010419.

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Dissertations / Theses on the topic "ROSAT"

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Siddiqui, Hassan. "ROSAT observations of clusters of galaxies." Thesis, University of Leicester, 1995. http://hdl.handle.net/2381/35783.

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Observations of four rich clusters of galaxies made using the Position Sensitive Proportional Counter (PSPC) instrument onboard the German Rontgensatellit (ROSAT) observatory were analysed. These data were complemented by ROSAT Wide Field Camera (WFC), Ginga and optical Automated Plate Measuring Machine (APM) information. Cluster properties, including the temperature profile, gas mass and total gravitational mass were investigated. Estimates for the mass deposition rates of central cooling flows, where appropriate, were made. Substructure was investigated using isophotal analysis and the employment of hardness ratios. The presence of central, intrinsic absorption, discovered previously in some similar clusters was confirmed. This is probably due to cold gas clouds. In the case of A2199, the WFC/PSPC data provided useful constraints to the partial covering fraction of these putative gas clouds. Abell 2142, which is classified in the optical as a binary cluster was shown to have a complex substructure. It is highly elliptical out to ~ 2 Mpc which can be explained in terms of a merger between two subclusters of differing sizes. The temperature and luminosities measured for A2218 and A1061, both of which have high velocity dispersions, indicate that these dispersion measurements are overestimated. Substructure is the most plausible explanation; spatial analysis supports this view. The galaxy density profiles obtained from the APM data were found to be consistent with the King approximation, and their luminosity functions were in reasonable agreement with the 'universal' Schechter model with a characteristic absolute magnitude of Bj = -21.6. Finally, the x-ray data showed that the gas mass fraction continues to rise with radius at the limit of detectability of ~ 2 Mpc. Including the optical data, the baryonic fraction at this radius is = 0.3. This result is difficult to reconcile with the universal fraction determined from standard cosmological nucleosynthesis models.
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Daniels, Julian. "The ROSAT wide field camera scientific simulator." Thesis, University of Leicester, 1990. http://hdl.handle.net/2381/35862.

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The ROSAT spacecraft is due for launch in June 1990. On board will be an X-Ray Telescope (XRT) and an XUV Wide Field Camera (WFC). The XRT will perform the first ever imaging all sky survey in the 0.1 keV- 2.0 keV wave-band. This will be complemented by the first all sky survey in the 0.062 keV - 0.21 keV wave-band using the WFC. A scientific simulator has been developed to assist the WFC mission in the following areas: 1. Production of representative telemetry to develop and test the ROSAT WFC ground system software. 2. Determination of optimum parameters for several WFC firmware and hardware features. 3. Evaluation of background radiation effects on operational and astrophysical aspects of the WFC mission. The modelling and simulation of the performance aspects of the WFC telescope and its interaction with the predicted environment is described here. The complete model has been implemented as a user orientated software package and can be run to produce scientific telemetry and other simulated output that interface with the ROSAT WFC ground system software. The results of the simulator provide essential foresight into the following: The efficacy of image analysis software. The efficiency of in-orbit WFC low energy (50 keV) electron rejection. Prediction of all sky exposure coverage, the background environment, and minimum source sensitivity.
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Piters, Anna Johanna Maria. "ROSAT all-sky survey observations of normal stars." Amsterdam : Amsterdam : Sterrenkundig Instituut 'Anton Pannekoek' ; Universiteit van Amsterdam [Host], 1995. http://dare.uva.nl/document/92469.

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Clayton, Kathryn L. "ROSAT and HST observations of magnetic cataclysmic variables." Thesis, University of Leicester, 1995. http://hdl.handle.net/2381/35858.

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This thesis describes principally ROSAT and HST observations of magnetic (or proposed magnetic) cataclysmic variables. Chapter 2 details a ROSAT observation of the polar EK UMa. The orbital light curve reveals a single bright phase. During this bright phase deep dips in the flux are seen, consistent with accretion stream occultation. The soft X-ray spectrum has an unusually high temperature of 50 KTBB 62 eV. No hard X-ray flux is detected. Chapter 3 details ROSAT observations of proposed intermediate polars SW UMa and 1H0709-360. The previously reported X-ray/optical periodicities in SW UMa were not detected. Spectral analysis indicates a two-temperature model is appropriate. The weak signal from 1H0709-360 precludes a detailed spectral analysis. 1H0709-360 has dropped in flux by ~ 2 orders of magnitude since its detection. The intermediate polar classification of these two systems remains unconfirmed. Chapter 4 describes ROSAT and contemporaneous optical and HST observations of the intermediate polar AE Aqr. During this observation X-ray flares were detected for the first time. The white dwarf spin modulated count rate increased only slightly with increased intensity. AE Aqr has an unusually soft spectrum which is only fit by a two temperature optically thin plasma emission model. Chapters 5 and 6 detail ROSAT, HST, EUVE and complementary optical observations of the polar QS Tel. The soft X-ray/EUV data showed a bright-faint morphology. The EUVE observations, ~ 1 year later, revealed a change in morphology, indicating that both poles were active. A deep narrow dip is observed in both the ROSAT and EUVE observations. The HST (FOS) observation had a mean spectrum of an underlying continuum with strong emission lines superposed. Orbital modulation was present in both. A narrow dip is observed in the continuum fold which is consistent with the dip observed by ROSAT and EUVE.
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Spurgeon, Louise Elizabeth. "XMM and ROSAT observations of clusters of galaxies." Thesis, University of Leicester, 2003. http://hdl.handle.net/2381/30665.

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I present an investigation into the X-ray properties of galaxy clusters, consisting of a principal component analysis of ROSAT data and studies of three clusters observed with the XMM-Newton satellite. The principal component analysis provides an investigation into similarities between cluster surface brightness profiles. Initial results for 42 clusters are presented and compared to existing models. The cluster profiles are reproduced to good accuracy using three principal components. Correlation of the principal components to physical properties is investigated but the results are inconclusive. Observations of Abell 1413, Abell 665 and Abell 2163 made with XMM-Newton were investigated spectrally and spatially to determine cluster properties. Global temperatures were found to be 7.08 +/- 0.140.13 keV for Abell 665 and 11.98 +/- 1.2 keV for Abell 2163. The temperature and abundance profiles of the clusters are very different, with some differences attributed to the recent merging of subclusters in Abell 665 and Abell 2163. Spatial analysis of the cluster surface brightness profiles is undertaken with beta and NFW models. The profiles produced for the three clusters are used to estimate the variation of gas, gravitational and iron mass with radius. These are used to draw general conclusions, such supernovae numbers (NSNII 109--11). The cosmological density and matter density parameters are found; &OHgr;0 = 0.22 -- 0.33 +/- 0.1 and &OHgr; m ? 0.12+/-0.060.04. This suggests a low density universe, but is subject to uncertainty due to extrapolation to larger radii.
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Pislar, Vincent. "Etude d'Amas de Galaxies observés avec le satellite ROSAT." Phd thesis, Université Pierre et Marie Curie - Paris VI, 1998. http://tel.archives-ouvertes.fr/tel-00068737.

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Ce travail est composé de deux parties.

La première partie concerne l' étude de l'amas de galaxies Abell 85 en utilisant les données en rayons X du satellite ROSAT ainsi que des données optiques et radio. Plusieurs méthodes d'analyse ont été appliquées aux données. Nous avons ainsi pu étudier des régions particulières de l'amas comme la partie centrale, siège des courants de refroidissement ou la région de la radiosource 0038-096 où la mesure des flux X et radio a permis d'obtenir la valeur du champ magnétique.

Une seconde partie du travail a consisté à étudier les
caractéristiques des courants de refroidissement ainsi que la masse de gaz et de matière noire dans 11 amas de galaxies, grâce à un programme conçu pour ajuster les données de ROSAT. Nous avons également obtenu la fraction de baryons de ces amas et discuté les conséquences cosmologiques des valeurs obtenues.
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Canosa, Celestino Miguel. "FRI-BL Lac unification using ROSAT X-ray observations." Thesis, University of Bristol, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.340153.

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Pislar, Vincent. "Étude d'amas de galaxies observés avec le satellite ROSAT." Paris 6, 1998. http://www.theses.fr/1998PA066594.

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Ce travail est composé de deux parties. La première partie concerne l'étude de l'amas de galaxies Abell 85 en utilisant les données en rayons x du satellite Rosat ainsi que des données optiques et radio. Plusieurs méthodes d'analyse ont été appliquées aux données. Nous avons ainsi pu étudier des régions particulières de l'amas comme la partie centrale, siège des courants de refroidissement ou la région de la radiosource 0038-096 ou la mesure des flux x et radio a permis d'obtenir la valeur du champ magnétique. Une seconde partie du travail a consisté à étudier les caractéristiques des courants de refroidissement ainsi que la masse de gaz et de matière noire dans 11 amas de galaxies, grâce à un programme conçu pour ajuster les données de Rosat. Nous avons également obtenu la fraction de baryons de ces amas et discuté les conséquences cosmologiques des valeurs obtenues.
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Egger, Roland. "Der Supernova-Überrest North Polar Spur in der ROSAT- Himmelsdurchmusterung." Garching bei München : Max-Planck-Institut für extraterrestrische Physik, 1993. http://catalog.hathitrust.org/api/volumes/oclc/29509967.html.

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Morley, John E. "Cool stars in the galaxy : a ROSAT and ASCA view." Thesis, University of Leicester, 1999. http://hdl.handle.net/2381/30624.

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This thesis describes work undertaken using data from the ROSAT and ASCA missions, in order to study the coronal x-ray emission of cool, late type stars. Chapters 1 and 2 summarise the emission processes involved and the methods by which the x-rays are detected and analysed, including a discussion of the ROSAT and ASCA missions. Chapter 3 details a deep soft x-ray survey of the Galactic Plane using the ROSAT Position Sensitive Proportional Counter. The data consist of 9 fields, each of 10ks exposure, pointed at positions on or very close to the plane. Presented are the source list, number-flux relation and the x-ray to optical flux ratios. I present the results of source count modelling which suggest 50% stellar and 8% extra-galactic contributions. The nature of the unidentified population is discussed. Chapter 1 discusses the temporal variability of the x-ray emission of stars in the Hyades cluster. The data consist of 13 PSPC fields, each of 20ks exposure, targeted in the central regions of the cluster. Little evidence is present to suggest long term variability, though 14 do exhibit short term variability. Time resolved spectra of detected flares are presented. Flare modelling results suggest flare loop heights of 1-2 solar radii. Chapters 5 details observations, obtained using the ASCA satellite, of 3 sources, VW Cep. SW Lac and 44i Boo. These observations form part of an ongoing survey of W UMa systems. Spectral and temporal results are compared to a previous ROSAT survey. I show that the observed systems have a high temperature component comparable with that seen in RS CVN and BY Dra systems. I also provide evidence for non-solar metal abundances in these systems.
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Books on the topic "ROSAT"

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Duck, Simon Robert. ROSAT observations of cataclysmic variables. Birmingham: University of Birmingham, 1993.

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Truemper, J. Was der Röntgensatellit ROSAT entdeckte. Opladen: Westdeutscher Verlag, 1994.

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Diamond, Christopher James. ROSAT observations of DA white dwarfs. Birmingham: University of Birmingham, 1994.

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Manning, Rodger Alan. ROSAT observations of isolated neutron stars. Birmingham: University of Birmingham, 1994.

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Musielak, Z. E. ROSAT pointed observations of cool magnetic white dwarfs. [Washington, DC: National Aeronautics and Space Administration, 1995.

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The invisible sky: ROSAT and the age of X-ray astronomy. New York: Copernicus, 1998.

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Ebeling, Harald. Abell and ACO clusters of galaxies in the ROSAT all-sky X-ray survey: A statistical study. Garching bei München, Germany: Max-Planck-Institut für Extraterrestrische Physik, 1993.

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1954-, Schlegel Eric M., Petre Robert, and ROSAT Science Symposium (1993 : College Park, Md.), eds. The soft X-ray cosmos: ROSAT Science Symposium, College Park, MD, November 1993. New York: American Institute of Physics, 1994.

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Bouveresse, Jacques. Le philosophe et le réel: Entretiens avec Jean-Jacques Rosat. Paris: Hachette Littératures, 1998.

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Workshop on Traces of the Primordial Structure in the Universe (1990 Schloss Ringberg, Germany). Traces of the primordial structure in the universe: Proceedings of the Workshop on Traces of the Primordial Structure in the Universe held at Schloss Ringberg, Tegernsee, October 1-5, 1990. Garching bei München: Max-Planck-Institut für Extraterrestrische Physik, 1991.

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Book chapters on the topic "ROSAT"

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TrÜmper, J. "Highlights of Rosat." In Astrophysics and Space Science Library, 47–51. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0794-5_5.

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Zimmermann, H. U. "The ROSAT Mission." In Data Analysis in Astronomy IV, 115–19. Boston, MA: Springer US, 1992. http://dx.doi.org/10.1007/978-1-4615-3388-7_13.

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Trümper, J. "The Rosat Mission." In Hot Thin Plasmas in Astrophysics, 355–58. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3065-0_25.

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Trümper, Joachim E. "ROSAT — Early Results." In X-Ray Binaries and Recycled Pulsars, 19–26. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2704-2_2.

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Aschenbach, Bernd, Hermann-Michael Hahn, and Joachim Trümper. "ROSAT-Creating a Satellite." In The Invisible Sky, 37–65. New York, NY: Springer New York, 1998. http://dx.doi.org/10.1007/978-1-4612-1628-5_3.

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Bühler, P., T. J. L. Courvoisier, R. Staubert, H. Brunner, and G. Lamer. "ROSAT Spectra of Quasars." In Multi-Wavelength Continuum Emission of AGN, 369. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-010-9537-2_87.

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Snowden, S. L., and J. H. M. M. Schmitt. "Mission Planning with ROSAT." In Data Analysis in Astronomy IV, 121–29. Boston, MA: Springer US, 1992. http://dx.doi.org/10.1007/978-1-4615-3388-7_14.

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Mullis, C. R., I. M. Gioia, and J. P. Henry. "The Nep Rosat Survey." In The Hot Universe, 473–74. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4970-9_178.

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Pye, J. P., S. T. Hodgkin, R. A. Stern, J. H. M. M. Schmitt, and C. Rosso. "ROSAT Observations of the Hyades." In Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium, 345–51. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1964-1_43.

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Bickert, K. F., R. E. Stencel, and R. Luthardt. "Rosat Observations of Symbiotic Stars." In Planetary Nebulae, 405. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-2088-3_204.

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Conference papers on the topic "ROSAT"

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GUCKENBIEHL, F. "Rosat Mission Operations System." In 30th Aerospace Sciences Meeting and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1992. http://dx.doi.org/10.2514/6.1992-597.

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Lange, Gunter, Bernhard MoBbacher, and David Purll. "The ROSAT Star Tracker." In 1986 Astronomy Conferences, edited by David L. Crawford. SPIE, 1986. http://dx.doi.org/10.1117/12.968097.

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Fremont, Matthew, J. H. Beall, B. N. Dorland, and W. A. Snyder. "ROSAT observations of 3C390.3." In The soft x-ray cosmos: ROSAT science symposium and data analysis workshop. AIP, 1994. http://dx.doi.org/10.1063/1.46663.

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Reichert, Gail A., Richard F. Mushotzky, and Alexei V. Filippenko. "ROSAT observations of LINERs." In The soft x-ray cosmos: ROSAT science symposium and data analysis workshop. AIP, 1994. http://dx.doi.org/10.1063/1.46669.

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Schlegel, Eric M. "ROSAT Observations of supernovae." In The soft x-ray cosmos: ROSAT science symposium and data analysis workshop. AIP, 1994. http://dx.doi.org/10.1063/1.46710.

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Barstow, Martin A., and Anne E. Sansom. "ROSAT WFC imaging detectors." In San Dieg - DL Tentative, edited by Oswald H. W. Siegmund and Hugh S. Hudson. SPIE, 1990. http://dx.doi.org/10.1117/12.23253.

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Supper, Rodrigo. "ROSAT PSPC observation of M31." In The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45950.

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Johnston, Helen M., Frank Verbunt, and Günther Hasinger. "ROSAT observations of globular clusters." In The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.45952.

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van Teeseling, André, and Frank Verbunt. "Rosat observations of cataclysmic variables." In The evolution of X-ray binaries. AIP, 1994. http://dx.doi.org/10.1063/1.46005.

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Willingale, R. "ROSAT Wide Field Camera Mirrors." In 31st Annual Technical Symposium, edited by C. Stuart Bowyer. SPIE, 1988. http://dx.doi.org/10.1117/12.942156.

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Reports on the topic "ROSAT"

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Hernandez, C. L., F. M. Hosking, J. Reed, D. M. Tench, and J. White. Reduced oxide soldering activation (ROSA) PWB solderability testing. Office of Scientific and Technical Information (OSTI), February 1996. http://dx.doi.org/10.2172/206566.

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Brauner, Edwin Jr, and Daniel C. Carlson. Santa Rosa Geysers Recharge Project: GEO-98-001. Final Report. Office of Scientific and Technical Information (OSTI), October 2002. http://dx.doi.org/10.2172/897791.

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Denight, Michael L., Patrick J. Guertin, Dick L. Gebhart, and Linda Nelson. Invasive Species Biology, Control, and Research. Part 2. Multiflora Rose (Rosa multiflora). Fort Belvoir, VA: Defense Technical Information Center, November 2008. http://dx.doi.org/10.21236/ada492988.

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Rhee, G. S., Yutaka Kukita, and R. R. Schultz. NRC confirmatory AP600 safety system phase I testing in the ROSA/AP600 test facility. Office of Scientific and Technical Information (OSTI), March 1996. http://dx.doi.org/10.2172/269716.

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Correa Pabon, Rosa Elvira, Thiago Euzébio, and Gustavo Pessin. Estudo preliminar: sistema de monitoramento para prevenção de avalanche em usina. Rosa Elvira Correa Pabón. ITV, 2021. http://dx.doi.org/10.29223/prod.tec.itv.mi.2021.18.pabon.

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SGC, Servicio Geológico Colombiano. Mapa geológico de la plancha 131 Santa Rosa de Osos. Escala 1:100.000. Producto. Versión 2011. Bogotá: Servicio Geológico Colombiano, January 2010. http://dx.doi.org/10.32685/10.143.2010.307.

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Pérez, Carlos. El periodismo rosa como telenovela de no-ficción en el marco de la libertad de expresión. Revista Latina de Comunicación Social, 2007. http://dx.doi.org/10.4185/rlcs-62-2007-738-151-159.

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Liu, Chao-Han. Study of Equatorial Ionospheric Irregularities with ROCSAT- 1/IPEI Data for Assessment of Impacts on Communication/Navigation System (V). Fort Belvoir, VA: Defense Technical Information Center, November 2009. http://dx.doi.org/10.21236/ada512634.

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SGC, Servicio Geológico Colombiano. Mapa Geomorfológico aplicado a movimientos en masa escala 1:100.000. Plancha 131 Santa Rosa de Osos. Producto. Bogotá: Servicio Geológico Colombiano, August 2014. http://dx.doi.org/10.32685/4.7.2014.430.

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Jessen, Paul F., John G. Locke, Thomas A. Rago, Curtis A. Collins, and Newell Garfield. Hydrographic Data from California Waters between the Santa Rosa/Cortes Ridge and the Farallones, May through October 1990. Fort Belvoir, VA: Defense Technical Information Center, August 1993. http://dx.doi.org/10.21236/ada269964.

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