Zobrazeno 1 - 10
of 68
pro vyhledávání: '"Shuping R"'
Autor:
Gordon, M. S., Lopez-Rodriguez, E., Andersson, B. -G., Clarke, M., Coude, S., Moullet, A., Richards, S. N., Shuping, R. Y., Vacca, W., Yorke, H.
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a Boeing 747SP aircraft modified to accommodate a 2.7 meter gyro-stabilized telescope, which is mainly focused to studying the Universe at infrared wavelengths. As part of the Strategic
Externí odkaz:
http://arxiv.org/abs/1811.03100
We report the discovery of twelve faint Herbig-Haro (HH) objects in LDN 673 found using a novel color-composite imaging method that reveals faint H{\alpha} emission in complex environments. Follow-up observations in [S II] confirmed their classificat
Externí odkaz:
http://arxiv.org/abs/1712.00305
Autor:
Shuping, R. Y., Krzaczek, R., Vacca, W. D., Charcos-Llorens, M., Reach, W. T., Alles, R., Clarke, M., Melchiorri, R., Radomski, J., Shenoy, S., Sandel, D., Omelian, E. B.
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is an airborne astronomical observatory comprised of a 2.5-meter telescope mounted in the aft section of a Boeing 747SP aircraft. During routine operations, several instruments will be avai
Externí odkaz:
http://arxiv.org/abs/1412.5546
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is an airborne astronomical observatory comprised of a 2.5 meter infrared telescope mounted in the aft section of a Boeing 747SP aircraft that flies at operational altitudes between 37,000
Externí odkaz:
http://arxiv.org/abs/1309.6994
Publikováno v:
AJ 2012, 144, 116
We present high S/N, moderate resolution near-infrared spectra, as well as 10 micron imaging, for the brightest members of the central stellar cluster in the W40 HII region, obtained using the SpeX and MIRSI instruments at NASA's Infrared Telescope F
Externí odkaz:
http://arxiv.org/abs/1208.4648
Autor:
Young, E. T., Becklin, E. E., Marcum, P. M., Roellig, T. L., De Buizer, J. M., Herter, T. L., Güsten, R., Dunham, E. W., Temi, P., Andersson, B. -G., Backman, D., Burgdorf, M., Caroff, L. J., Casey, S. C., Davidson, J. A., Erickson, E. F., Gehrz, R. D., Harper, D. A., Harvey, P. M., Helton, L. A., Horner, S. D., Howard, C. D., Klein, R., Krabbe, A., McLean, I. S., Meyer, A. W., Miles, J. W., Morris, M. R., Reach, W. T., Rho, J., Richter, M. J., Roeser, H. -P., Sandell, G., Sankrit, R., Savage, M. L., Smith, E. C., Shuping, R. Y., Vacca, W. D., Vaillancourt, J. E., Wolf, J., Zinnecker, H.
Publikováno v:
The Astrophysical Journal Letters, Volume 749, Issue 2, article id. L17 (2012)
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is an airborne observatory consisting of a specially modified Boeing 747SP with a 2.7-m telescope, flying at altitudes as high as 13.7 km (45,000 ft). Designed to observe at wavelengths fro
Externí odkaz:
http://arxiv.org/abs/1205.0791
Autor:
Shuping, R. Y., Morris, Mark R., Herter, Terry L., Adams, Joseph D., Gull, G. E., Schoenwald, J., Henderson, C. P., Becklin, E. E., De Buizer, James M., Vacca, William D., Zinnecker, Hans, Megeath, S. Thomas
We present new mid-infrared images of the central region of the Orion Nebula using the newly commissioned SOFIA airborne telescope and its 5 -- 40 micron camera FORCAST. The 37.1 micron images represent the highest resolution observations (<4") ever
Externí odkaz:
http://arxiv.org/abs/1202.4479
Autor:
Salgado, F., Berne, O., Adams, J. D., Herter, T. L., Gull, G., Schoenwald, J., Keller, L. D., De Buizer, J. M., Vacca, W. D., Becklin, E. E., Shuping, R. Y., M., A. G. G., Tielens, Zinnecker, H.
The massive star forming region W3 was observed with the faint object infrared camera for the SOFIA telescope (FORCAST) as part of the Short Science program. The 6.4, 6.6, 7.7, 19.7, 24.2, 31.5 and 37.1 \um bandpasses were used to observe the emissio
Externí odkaz:
http://arxiv.org/abs/1202.3582
SOFIA presents a number of interesting challenges for the development of a data reduction environment which, at its initial phase, will have to incorporate pipelines from seven different instruments. Therefore, the SOFIA data reduction software must
Externí odkaz:
http://arxiv.org/abs/1101.2000
Publikováno v:
Astrophys.J. 644 (2006) L71-L74
We present 8--13 micron low resolution spectra (R~100) of 8 low-mass protostellar objects ("proplyds") in the Orion Nebula using the Long Wavelength Spectrometer (LWS) at the W. M. Keck Observatory. All but one of the sources in our sample show stron
Externí odkaz:
http://arxiv.org/abs/astro-ph/0605174