Journal articles: 'Astrophysics and Space Science'

1

Dopita, Michael A. "Astrophysics & Space Science editorial." Astrophysics and Space Science 312, no. 1-2 (October 5, 2007): 1–2. http://dx.doi.org/10.1007/s10509-007-9652-z.

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Zheleznyakov, V. V. "New Books: Astrophysics and Space Science." Physics Essays 10, no. 3 (September 1997): 534–35. http://dx.doi.org/10.4006/1.3041626.

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Makishima, Kazuo. "Space Astrophysics in Japan." Publications of the Astronomical Society of Australia 9, no. 1 (1991): 57–59. http://dx.doi.org/10.1017/s1323358000024887.

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4

Riegler, Guenter R. "Science Operations for Future Space Astrophysics Missions." International Astronomical Union Colloquium 123 (1990): 317–21. http://dx.doi.org/10.1017/s0252921100077228.

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AbstractPlans for astrophysics science operations during the decade of the nineties are described from the point of view of a scientist who wishes to make a space-borne astronomical observation or to use archival astronomical data. In the process of preparing a proposal, making an observation, and carrying out data processing, analysis, and dissemination of results, the scientist will be able to use a variety of services and infrastructure, including the “Astrophysics Data System”. The current status and plans for these science operations services are described.

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Stankus, Tony. "Astronomy, Astrophysics, and Space Sciences." Serials Librarian 27, no. 2-3 (April 8, 1996): 59–65. http://dx.doi.org/10.1300/j123v27n02_04.

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Glanz, J. "ASTROPHYSICS: X-rays Hint at Space Pirouette." Science 278, no. 5340 (November 7, 1997): 1012b—1013. http://dx.doi.org/10.1126/science.278.5340.1012b.

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Irion, R. "ASTROPHYSICS: Stanford Gets Serious About Space Physics." Science 299, no. 5606 (January 24, 2003): 492b—492. http://dx.doi.org/10.1126/science.299.5606.492b.

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Agnello, S. Dell’, G. Delle Monache, R. Vittori, A. Boni, C. Cantone, E. Ciocci, M. Martini, et al. "Advanced Laser Retroreflectors for Astrophysics and Space Science." Journal of Applied Mathematics and Physics 03, no. 02 (2015): 218–27. http://dx.doi.org/10.4236/jamp.2015.32032.

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Lawler, A. "Astronomy and Astrophysics: Crunch Ahead for Space Science." Science 271, no. 5256 (March 22, 1996): 1660b—1661. http://dx.doi.org/10.1126/science.271.5256.1660b.

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Kestenbaum, D. "ASTROPHYSICS: X-ray Flickers Reveal a Space Warp." Science 280, no. 5364 (May 1, 1998): 674–75. http://dx.doi.org/10.1126/science.280.5364.674.

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Eichler, David. "Ongoing space physics – Astrophysics connections." Advances in Space Research 38, no. 1 (January 2006): 16–20. http://dx.doi.org/10.1016/j.asr.2004.12.079.

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Turon, Catherine. "ESA Space Science Programme, Cosmic Vision 2015-2025, for astrophysics." Proceedings of the International Astronomical Union 2, no. 14 (August 2006): 530–31. http://dx.doi.org/10.1017/s1743921307011702.

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Normile, D. "ASTROPHYSICS: Space Mission to Shine a Light on Solar Flares." Science 313, no. 5793 (September 15, 2006): 1553a. http://dx.doi.org/10.1126/science.313.5793.1553a.

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Livadiotis, G., and D. J. McComas. "Understanding Kappa Distributions: A Toolbox for Space Science and Astrophysics." Space Science Reviews 175, no. 1-4 (May 7, 2013): 183–214. http://dx.doi.org/10.1007/s11214-013-9982-9.

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Bessell, Michael S. "Beauty and Astrophysics." Publications of the Astronomical Society of Australia 17, no. 2 (2000): 179–84. http://dx.doi.org/10.1071/as00179.

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AbstractSpectacular colour images have been made by combining CCD images in three different passbands using Adobe Photoshop. These beautiful images highlight a variety of astrophysical phenomena and should be a valuable resource for science education and public awareness of science. The wide field images were obtained at the Siding Spring Observatory (SSO) by mounting a Hasselblad or Nikkor telephoto lens in front of a 2K × 2K CCD. Options of more than 30 degrees or 6 degrees square coverage are produced in a single exposure in this way. Narrow band or broad band filters were placed between lens and CCD enabling deep, linear images in a variety of passbands to be obtained. We have mapped the LMC and SMC and are mapping the Galactic Plane for comparison with the Molonglo Radio Survey. Higher resolution images have also been made with the 40 inch telescope of galaxies and star forming regions in the Milky Way.

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Unwin, S. C., A. E. Wehrle, D. L. Meier, D. L. Jones, and B. G. Piner. "Quasar astrophysics with the Space Interferometry Mission." Proceedings of the International Astronomical Union 3, S248 (October 2007): 288–89. http://dx.doi.org/10.1017/s1743921308019352.

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AbstractOptical astrometry of quasars and active galaxies can provide key information on the spatial distribution and variability of emission in compact nuclei. The Space Interferometry Mission (SIM PlanetQuest) will have the sensitivity to measure a significant number of quasar positions at the microarcsecond level. SIM will be very sensitive to astrometric shifts for objects as faint as V=19. A variety of AGN phenomena are expected to be visible to SIM on these scales, including time and spectral dependence in position offsets between accretion disk and jet emission. These represent unique data on the spatial distribution and time dependence of quasar emission. It will also probe the use of quasar nuclei as fundamental astrometric references. Comparisons between the time-dependent optical photocenter position and VLBI radio images will provide further insight into the jet emission mechanism. Observations will be tailored to each specific target and science question. SIM will be able to distinguish spatially between jet and accretion disk emission; and it can observe the cores of galaxies potentially harboring binary supermassive black holes resulting from mergers.

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Bingham, R., D. C. Speirs, B. J. Kellett, I. Vorgul, S. L. McConville, R. A. Cairns, A. W. Cross, A. D. R. Phelps, and K. Ronald. "Laboratory astrophysics: Investigation of planetary and astrophysical maser emission." Space Science Reviews 178, no. 2-4 (March 8, 2013): 695–713. http://dx.doi.org/10.1007/s11214-013-9963-z.

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18

Minier, V., and M. Rouzé. "Exploring science and technology through the Herschel space observatory." Proceedings of the International Astronomical Union 10, H16 (August 2012): 647. http://dx.doi.org/10.1017/s174392131401268x.

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AbstractBecause modern astronomy associates the quest of our origins and high-tech instruments, communicating and teaching astronomy explore both science and technology. We report here on our work in communicating astronomy to the public through Web sites (www.herschel.fr), movies on Dailymotion (www.dailymotion.com/AstrophysiqueTV) and new ITC tools that describe interactively the technological dimension of a space mission for astrophysics.

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19

SMITH, HARLAN J. "Summary: Miniworkshops on Space-based Astrophysics." Annals of the New York Academy of Sciences 647, no. 1 Texas/ESO-Cer (December 1991): 628–34. http://dx.doi.org/10.1111/j.1749-6632.1991.tb32212.x.

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20

Crosby, Norma B. "Space weather: science and effects." Proceedings of the International Astronomical Union 4, S257 (September 2008): 47–56. http://dx.doi.org/10.1017/s174392130902907x.

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AbstractFrom the point-of-view of somebody standing outside on a cold winter night looking up at a clear cloudless sky, the space environment seems to be of a peaceful and stable nature. Instead, the opposite is found to be true. In fact the space environment is very dynamic on all spatial and temporal scales, and in some circumstances may have unexpected and hazardous effects on technology and humans both in space and on Earth. In fact the space environment seems to have a weather all of its own – its own “space weather”. Our Sun is definitely the driver of our local space weather. Space weather is an interdisciplinary subject covering a vast number of technological, scientific, economic and environmental issues. It is an application-oriented discipline which addresses the needs of “space weather product” users. It can be truly said that space weather affects everybody, either directly or indirectly. The aim of this paper is to give an overview of what space weather encompasses, emphasizing how solar-terrestrial physics is applied to space weather. Examples of “space weather product” users will be given highlighting those products that we as a civilization are most dependent on.

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21

Collier, Michael R., David G. Siebeck, Thomas E. Cravens, Ina P. Robertson, and Nick Omidi. "Astrophysics Noise: A Space Weather Signal." Eos, Transactions American Geophysical Union 91, no. 24 (June 15, 2010): 213–14. http://dx.doi.org/10.1029/2010eo240001.

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22

Rycroft, Michael J. "J.Lilensten (ed.), Space weather: research towards applications in Europe, Astrophysics and space science library, volume 344." Surveys in Geophysics 28, no. 1 (June 1, 2007): 115–16. http://dx.doi.org/10.1007/s10712-007-9015-x.

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23

B., A. J. "Galactic and Extragalactic Infrared Spectroscopy (Astrophysics and Space Science Library Vol. 108)." Journal of Molecular Structure 131, no. 1-2 (October 1985): 183. http://dx.doi.org/10.1016/0022-2860(85)85113-9.

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24

Dopita, Michael. "Astrophysics & Space Science subscribes to the Singapore Statement on Research Integrity." Astrophysics and Space Science 337, no. 1 (January 2012): 1. http://dx.doi.org/10.1007/s10509-011-0959-4.

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25

Livadiotis, G., and D. J. McComas. "Erratum to: Understanding Kappa Distributions: A Toolbox for Space Science and Astrophysics." Space Science Reviews 175, no. 1-4 (June 2013): 215. http://dx.doi.org/10.1007/s11214-013-9996-3.

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26

Onuora, Lesley I. "Astronomy in Nigeria." Highlights of Astronomy 10 (1995): 666–67. http://dx.doi.org/10.1017/s1539299600012491.

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One major problem in Africa in general is to convince governments and agencies that astronomy is relevant to Africa. Attention has been focussed on technology transfer, neglecting science and research. This attitude encourages the continued dependence on industrialized countries.In Nigeria there has been some success in projecting the idea that Space Science does not just mean remote sensing, but that basic space science, i.e. astronomy and astrophysics, cosmology, planetary science etc. is important and necessary. Evidence of this is that Nigeria’s expert committee on space policy recommended that one of three proposed National Centres should be for basic space science, laying emphasis on fundamental physics, astronomy and astrophysics, solarterrestrial interactions and their influence on climate, planetary and atmospheric studies. In addition, the Government of Nigeria hosted the Third UN/ESA Workshop on Basic Space Science in October, 1993.

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27

Kitamura, Masatoshi, Don Wentzel, Arne Henden, Jeffrey Bennett, H. M. K. Al-Naimiy, A. M. Mathai, Nat Gopalswamy, et al. "The United Nations Basic Space Science Initiative: the TRIPOD concept." Proceedings of the International Astronomical Union 2, SPS5 (August 2006): 277–84. http://dx.doi.org/10.1017/s1743921307007156.

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AbstractSince 1990, the United Nations has held an annual workshop on basic space science for the benefit of the worldwide development of astronomy. Additional to the scientific benefits of the workshops and the strengthening of international cooperation, the workshops lead to the establishment of astronomical telescope facilities through the Official Development Assistance (ODA) of Japan. Teaching material, hands-on astrophysics material, and variable star observing programmes had been developed for the operation of such astronomical telescope facilities in the university environment. This approach to astronomical telescope facility, observing programme, and teaching astronomy has become known as the basic space science TRIPOD concept. Currently, a similar TRIPOD concept is being developed for the International Heliophysical Year 2007, consisting of an instrument array, data taking and analysis, and teaching space science.

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28

Battiston, R. "Particle astrophysics." Advances in Space Research 37, no. 10 (January 2006): 1833. http://dx.doi.org/10.1016/j.asr.2006.03.014.

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29

Clampin, Mark, David Lumb, Marco Sirianni, and Edward Smith. "Detectors For Space Science." Experimental Astronomy 19, no. 1-3 (June 29, 2006): 45–67. http://dx.doi.org/10.1007/s10686-005-9010-5.

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30

Barclay, T. "The Space-Based Photometry Revolution." Proceedings of the International Astronomical Union 14, S339 (November 2017): 21. http://dx.doi.org/10.1017/s1743921318002120.

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AbstractThe Transiting Exoplanet Survey Satellite (TESS) is a NASA Astrophysics Explorer-class mission that will perform an all-sky survey to search for planets transiting nearby bright stars. The primary goal is to search for planets smaller than Neptune that are amenable to follow-up spectroscopic observations that will yield planet masses, thereby providing prime targets for future atmospheric characterization studies. In its two-year prime mission, TESS will monitor more than 200,000 stars with four wide-field optical CCD cameras that will tile more than 90% of the sky. TESS will also obtain full-frame images (FFIs) of the entire field of view with a cadence of 30 minutes to facilitate additional science. These FFIs will provide photometry for more than 30 million objects brighter than magnitude I =16 during the two-year prime mission. The TESS legacy will be a catalogue of the nearest and brightest main-sequence stars hosting transiting exoplanets. The TESS Mission will also have a robust Guest Investigator (GI) Programme that will be managed by the TESS Science Support Center at NASA Goddard Space Flight Center. Under the GI programme, the astrophysics community may propose new 2-minute cadence targets and investigations using the 30-minute cadence FFI data. TESS GI calls for proposals will occur once per year, and about 20,000 targets will be available for each GI programme cycle.TESS was launched in April 2018, and will observe from a unique elliptical high-Earth orbit that will provide an unobstructed view of its field to obtain continuous light-curves.

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31

Lovell, Bernard. "Book Review: British Space Science: History of British Space Science." Journal for the History of Astronomy 18, no. 2 (May 1987): 144–46. http://dx.doi.org/10.1177/002182868701800218.

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32

Nakagawa, Takao. "SPICA: space infrared telescope for cosmology and astrophysics." Advances in Space Research 34, no. 3 (January 2004): 645–50. http://dx.doi.org/10.1016/j.asr.2003.04.044.

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Schawinski, Kevin, M. Dennis Turp, and Ce Zhang. "Exploring galaxy evolution with generative models." Astronomy & Astrophysics 616 (August 2018): L16. http://dx.doi.org/10.1051/0004-6361/201833800.

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Context. Generative models open up the possibility to interrogate scientific data in a more data-driven way. Aims. We propose a method that uses generative models to explore hypotheses in astrophysics and other areas. We use a neural network to show how we can independently manipulate physical attributes by encoding objects in latent space. Methods. By learning a latent space representation of the data, we can use this network to forward model and explore hypotheses in a data-driven way. We train a neural network to generate artificial data to test hypotheses for the underlying physical processes. Results. We demonstrate this process using a well-studied process in astrophysics, the quenching of star formation in galaxies as they move from low-to high-density environments. This approach can help explore astrophysical and other phenomena in a way that is different from current methods based on simulations and observations.

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BOYD, RICHARD N. "NATIONAL SCIENCE FOUNDATION VISION IN PARTICLE AND NUCLEAR ASTROPHYSICS." International Journal of Modern Physics D 16, no. 12a (December 2007): 1981–88. http://dx.doi.org/10.1142/s0218271807011243.

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The NSF has made investments in searches for dark matter, in ultrahigh energy cosmic rays and gamma rays, in neutrino physics and astrophysics, and in nuclear astrophysics. We expect the future to witness the expansion of these efforts, along with efforts to refine the measurements of the cosmic microwave background. In some of these efforts the Deep Underground Science and Engineering Laboratory is expected to play a major role.

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Ehrenfreund, P. "ASTROPHYSICAL CHEMISTRY:Molecules on a Space Odyssey." Science 283, no. 5405 (February 19, 1999): 1123–24. http://dx.doi.org/10.1126/science.283.5405.1123.

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Pittori, C., M. Tavani, and the AGILE Team. "Gamma-ray Astrophysics with the Space Detector AGILE." Chinese Journal of Astronomy and Astrophysics 6, S1 (December 31, 2006): 373–76. http://dx.doi.org/10.1088/1009-9271/6/s1/50.

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37

Kaplan, Mike. "NASA's future plans for space astronomy and astrophysics." Space Science Reviews 61, no. 1-2 (July 1992): 103–12. http://dx.doi.org/10.1007/bf00212479.

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Castelli, C. "Innovation in the teaching of astrophysics and space science spacecraft design group study." European Journal of Physics 24, no. 2 (January 9, 2003): S9—S16. http://dx.doi.org/10.1088/0143-0807/24/2/302.

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39

Marov, MYA, AV Kolesnichenko, and AC Buckingham. "Mechanics of Turbulence of Multicomponent Gases. Astrophysics and Space Science Library, Vol 269." Applied Mechanics Reviews 56, no. 1 (2003): B11. http://dx.doi.org/10.1115/1.1523366.

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40

Klingenberg, Christian. "Numerical Astrophysics." Astronomische Nachrichten 328, no. 7 (September 2007): 661–64. http://dx.doi.org/10.1002/asna.200740005.

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41

Longair, M. S. "The Astrophysics of the Future." International Astronomical Union Colloquium 123 (1990): 421–26. http://dx.doi.org/10.1017/s0252921100077381.

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It is with some trepidation that I set down these thoughts. The history of physics and astronomy is littered with pontifications about the future, most of which simply end up embarrassing their authors. There are many projects which can be regarded as very safe bets but these might not be the ones which totally transform the nature of the discipline. The situation is analogous to that in the early 1950s when extragalactic astronomy simply meant optical astronomy since there was no other way of carrying out such studies – few would regard that as an adequate position nowadays. Similarly, it is difficult nowadays to imagine cosmology without the Microwave Background Radiation. Thus, the problem for the prognosticator is to tread the narrow line between science fiction and a simple extrapolation of what we do now with our facilities. It is in the spirit of this meeting to concentrate upon space observatories but I believe that it is instructive to look at the whole of astronomy, both from space and from the ground.

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42

ZAKHAROV, ALEXANDER F. "ASTROMETRY AND ASTROPHYSICS WITH THE SPACE TELESCOPE RADIOASTRON." International Journal of Modern Physics D 17, no. 07 (July 2008): 1055–70. http://dx.doi.org/10.1142/s0218271808012693.

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It is well-known that gravitational lensing is a powerful tool in the investigation of the distribution of matter, including that of dark matter (DM). Typical angular distances between images and typical time scales depend on the gravitational lens masses. For the case of microlensing, angular distances between images or typical astrometric shifts are about 10-5 - 10-6 arcsec. Such an angular resolution will be reached with the space–ground VLBI interferometer, Radioastron. The basic targets for microlensing searches should be bright point-like radio sources at cosmological distances. In this case, an analysis of their variability and a solid determination of microlensing could lead to an estimation of their cosmological mass density. Moreover, one could not exclude the possibility that non-baryonic dark matter could also form microlenses if the corresponding optical depth were high enough. It is known that in gravitationally lensed systems the probability (the optical depth) of observing microlensing is relatively high. Therefore, for example, gravitationally lensed objects, like the CLASS gravitational lens B1600+434, appear to be most suitable to detect astrometric microlensing, since features of photometric microlensing have been detected in these objects. However, to directly resolve these images and to directly detect the apparent motion of the knots, the Radioastron sensitivity would have to be improved, since the estimated flux density is below the sensitivity threshold. Alternatively, they may be observed by increasing an integration time, assuming that a radio source has a typical core–jet structure and microlensing phenomena are caused by the superluminal apparent motions of knots. In the case of a confirmation (or a negation) of claims about microlensing in gravitational lens systems, one can speculate about the microlens contribution to the gravitational lens mass. Astrometric microlensing due Galactic MACHOs is not very important because of low optical depths and long typical time scales. Therefore, the launch of the space interferometer Radioastron will enable the investigation of microlensing in the radio band, giving rise to the possibility of not only resolving microimages but also of observing astrometric microlensing.

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TURYSHEV, SLAVA G., ULF E. ISRAELSSON, MICHAEL SHAO, NAN YU, ALEXANDER KUSENKO, EDWARD L. WRIGHT, C. W. FRANCIS EVERITT, et al. "SPACE-BASED RESEARCH IN FUNDAMENTAL PHYSICS AND QUANTUM TECHNOLOGIES." International Journal of Modern Physics D 16, no. 12a (December 2007): 1879–925. http://dx.doi.org/10.1142/s0218271807011760.

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Space offers unique experimental conditions and a wide range of opportunities to explore the foundations of modern physics with an accuracy far beyond that of ground-based experiments. Space-based experiments today can uniquely address important questions related to the fundamental laws of Nature. In particular, high-accuracy physics experiments in space can test relativistic gravity and probe the physics beyond the Standard Model; they can perform direct detection of gravitational waves and are naturally suited for investigations in precision cosmology and astroparticle physics. In addition, atomic physics has recently shown substantial progress in the development of optical clocks and atom interferometers. If placed in space, these instruments could turn into powerful high-resolution quantum sensors greatly benefiting fundamental physics. We discuss the current status of space-based research in fundamental physics, its discovery potential, and its importance for modern science. We offer a set of recommendations to be considered by the upcoming National Academy of Sciences' Decadal Survey in Astronomy and Astrophysics. In our opinion, the Decadal Survey should include space-based research in fundamental physics as one of its focus areas. We recommend establishing an Astronomy and Astrophysics Advisory Committee's interagency "Fundamental Physics Task Force" to assess the status of both ground- and space-based efforts in the field, to identify the most important objectives, and to suggest the best ways to organize the work of several federal agencies involved. We also recommend establishing a new NASA-led interagency program in fundamental physics that will consolidate new technologies, prepare key instruments for future space missions, and build a strong scientific and engineering community. Our goal is to expand NASA's science objectives in space by including "laboratory research in fundamental physics" as an element in the agency's ongoing space research efforts.

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Gardner, Jonathan P. "Science with the James Webb Space Telescope." Proceedings of the International Astronomical Union 1, S232 (November 2005): 87–98. http://dx.doi.org/10.1017/s1743921306000317.

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Kaaret, P. "Relativistic astrophysics explorer." Advances in Space Research 34, no. 12 (January 2004): 2662–66. http://dx.doi.org/10.1016/j.asr.2003.03.061.

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Bignami, Giovanni F. "A vision for space science." Experimental Astronomy 23, no. 1 (January 16, 2009): 1–3. http://dx.doi.org/10.1007/s10686-009-9137-x.

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Green, Lucie, Colin Forsyth, and Jim Wild. "Looking ahead for space science." Astronomy & Geophysics 51, no. 3 (June 2010): 3.23–3.24. http://dx.doi.org/10.1111/j.1468-4004.2010.51323.x.

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Whyndham, Matthew. "Space science meets smart optics." Astronomy and Geophysics 44, no. 3 (June 2003): 3.31–3.32. http://dx.doi.org/10.1046/j.1468-4004.2003.44331.x.

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Indermuehle, Balthasar T., Michael G. Burton, and Sarah T. Maddison. "The History of Astrophysics in Antarctica." Publications of the Astronomical Society of Australia 22, no. 2 (2005): 73–90. http://dx.doi.org/10.1071/as04037.

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AbstractWe examine the historical development of astrophysical science in Antarctica from the early 20th century until today. We find three temporally overlapping eras, each having a rather distinct beginning. These are the astrogeological era of meteorite discovery, the high energy era of particle detectors, and the photon astronomy era of microwave, submillimetre, and infrared telescopes, sidelined by a few niche experiments at optical wavelengths. The favourable atmospheric and geophysical conditions are briefly examined, followed by an account of the major experiments and a summary of their results.

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Longair, Malcolm. "Radio astronomy and the rise of high-energy astrophysics two anniversaries." International Journal of Modern Physics D 28, no. 02 (January 2019): 1930004. http://dx.doi.org/10.1142/s0218271819300040.

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This paper celebrates the 100th anniversary of the birth of Martin Ryle and the 50th anniversary of the discovery of pulsars by Jocelyn Bell and Antony Hewish. Ryle and Hewish received the 1974 Nobel Prize in Physics, the first in the area of astrophysics. Their interests strongly overlapped, one of the key papers on the practical implementation of the technique of aperture synthesis being co-authored by Ryle and Hewish. The discovery of pulsars and the roles played by Hewish and Bell are described. These key advances were at the heart of the dramatic rise of high-energy astrophysics in the 1960s and led to the realization that general relativity is central to the understanding of high-energy astrophysical phenomena.

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Journal articles on the topic 'Astrophysics and Space Science'

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