Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Trinh, Christopher"'
Autor:
Jones, Terry Jay, Kim, Jin-Ah, Dowell, C. Darren, Morris, Mark R., Pineda, Jorge L., Benford, Dominic J., Berthoud, Marc, Chuss, David T., Dale, Daniel A., Fissel, L. M., Goldsmith, Paul F., Hamilton, Ryan T., Hanany, Shaul, Harper, Doyal A., Henning, Thomas K., Lazarian, Alex, Looney, Leslie W., Michail, Joseph M., Novak, Giles, Santos, Fabio P., Sheth, Kartik, Siah, Javad, Stacey, Gordon J., Staguhn, Johannes, Stephens, Ian W., Tassis, Konstantinos, Trinh, Christopher Q., Vaillancourt, John E., Ward-Thompson, Derek, Werner, Michael, Wollack, Edward J., Zweibel, Ellen G.
SOFIA HAWC+ polarimetry at $154~\micron$ is reported for the face-on galaxy M51 and the edge-on galaxy NGC 891. For M51, the polarization vectors generally follow the spiral pattern defined by the molecular gas distribution, the far-infrared (FIR) in
Externí odkaz:
http://arxiv.org/abs/2008.07897
Autor:
Santos, Fabio P., Chuss, David T., Dowell, C. Darren, Houde, Martin, Looney, Leslie W., Rodriguez, Enrique Lopez, Novak, Giles, Ward-Thompson, Derek, Berthoud, Marc, Dale, Daniel A., Guerra, Jordan A., Hamilton, Ryan T., Hanany, Shaul, Harper, Doyal A., Henning, Thomas K., Jones, Terry Jay, Lazarian, Alex, Michail, Joseph M., Morris, Mark R., Staguhn, Johannes, Stephens, Ian W., Tassis, Konstantinos, Trinh, Christopher Q., Van Camp, Eric, Volpert, C. G., Wollack, Edward J.
We report on polarimetric maps made with HAWC+/SOFIA toward Rho Oph A, the densest portion of the Rho Ophiuchi molecular complex. We employed HAWC+ bands C (89 $\mu$m) and D (154 $\mu$m). The slope of the polarization spectrum was investigated by def
Externí odkaz:
http://arxiv.org/abs/1905.00705
Autor:
Jones, Terry Jay, Dowell, C. Darren, Rodriguez, Enrique Lopez, Zweibel, Ellen G., Berthoud, Marc, Chuss, David T., Goldsmith, Paul F., Hamilton, Ryan T., Hanany, Shaul, Harper, Doyal A., Lazarian, 7 Alex, Looney, Leslie W., Michail, Joseph M., Morris, Mark R., Novak, Giles, Santos, Fabio P., Sheth, Kartik, Stacey, Gordon J., Staguhn, Johannes, Stephens, Ian W., Tassis, Konstantinos, Trinh, Christopher Q., Volpert, C. G., Werner, Michael, Wollack, Edward J.
We present Far-Infrared polarimetry observations of M82 at 53 and $154~\mu \rm{m}$ and NGC 253 at $89~\mu \rm{m}$, which were taken with HAWC+ in polarimetry mode on the Stratospheric Observatory for Infrared Astronomy (SOFIA). The polarization of M8
Externí odkaz:
http://arxiv.org/abs/1812.06816
Autor:
Chuss, David T., Andersson, B-G, Bally, John, Dotson, Jessie L., Dowell, C. Darren, Guerra, Jordan A., Harper, Doyal A., Houde, Martin, Jones, Terry Jay, Lazarian, A., Rodriguez, Enrique Lopez, Michail, Joseph M., Morris, Mark R., Novak, Giles, Siah, Javad, Staguhn, Johannes, Vaillancourt, John E., Volpert, C. G., Werner, Michael, Wollack, Edward J., Benford, Dominic J., Berthoud, Marc, Cox, Erin G., Crutcher, Richard, Dale, Daniel A., Fissel, L. M., Goldsmith, Paul F., Hamilton, Ryan T., Hanany, Shaul, Henning, Thomas K., Looney, Leslie W., Moseley, S. Harvey, Santos, Fabio P., Stephens, Ian, Tassis, Konstantinos, Trinh, Christopher Q., Van Camp, Eric, Ward-Thompson, Derek
We report new polarimetric and photometric maps of the massive star-forming region OMC-1 using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy (SOFIA). We present continuum polarimetric and photometric measurements of thi
Externí odkaz:
http://arxiv.org/abs/1810.08233
Autor:
Content, Robert, Bland-Hawthorn, Joss, Ellis, Simon, Gers, Luke, Haynes, Roger, Horton, Anthony, Lawrence, Jon, Leon-Saval, Sergio, Lindley, Emma, Min, Seong-Sik, Shortridge, Keith, Staszak, Nick, Trinh, Christopher, Xavier, Pascal, Zhelem, Ross
PRAXIS is a second generation instrument that follows on from GNOSIS, which was the first instrument using fibre Bragg gratings for OH background suppression. The Bragg gratings reflect the NIR OH lines while being transparent to light between the li
Externí odkaz:
http://arxiv.org/abs/1407.6438
Autor:
Trinh, Christopher Q., Barton, Elizabeth J., Bullock, James S., Cooper, Michael C., Zentner, Andrew R., Wechsler, Risa H.
We have devised a method to select galaxies that are isolated in their dark matter halo (N=1 systems) and galaxies that reside in a group of exactly two (N=2 systems). Our N=2 systems are widely-separated (up to $\sim$\,200\,$h^{-1}$\,kpc), where clo
Externí odkaz:
http://arxiv.org/abs/1301.5870
Autor:
Trinh, Christopher Q., Ellis, Simon C., Bland-Hawthorn, Joss, Horton, Anthony J., Lawrence, Jon S., Leon-Saval, Sergio G.
We analyse the near-infrared interline sky background, OH and O2 emission in 19 hours of H band observations with the GNOSIS OH suppression unit and the IRIS2 spectrograph at the 3.9-m AAT. We find that the temporal behaviour of OH emission is best d
Externí odkaz:
http://arxiv.org/abs/1301.0326
Autor:
Trinh, Christopher Q., Ellis, Simon C., Bland-Hawthorn, Joss, Lawrence, Jon S., Horton, Anthony J., Leon-Saval, Sergio G., Shortridge, Keith, Bryant, Julia, Case, Scott, Colless, Matthew, Couch, Warick, Freeman, Kenneth, Loehmannsroeben, Hans-Gerd, Gers, Luke, Glazebrook, Karl, Haynes, Roger, Lee, Steve, O'Byrne, John, Miziarski, Stan, Roth, Martin M., Schmidt, Brian, Tinney, Christopher G., Zheng, Jessica
GNOSIS is a prototype astrophotonic instrument that utilizes OH suppression fibres consisting of fibre Bragg gratings and photonic lanterns to suppress the 103 brightest atmospheric emission doublets between 1.47-1.7 microns. GNOSIS was commissioned
Externí odkaz:
http://arxiv.org/abs/1212.1201
Autor:
Fogarty, Lisa M. R., Bland-Hawthorn, Joss, Croom, Scott M., Green, Andrew W., Bryant, Julia J., Lawrence, Jon S., Richards, Samuel, Allen, James T., Bauer, Amanda E., Birchall, Michael N., Brough, Sarah, Colless, Matthew, Ellis, Simon C., Farrell, Tony, Goodwin, Michael, Heald, Ron, Hopkins, Andrew M., Horton, Anthony, Jones, D. Heath, Lee, Steve, Lewis, Geraint, López-Sánchez, Ángel R., Miziarski, Stan, Trowland, Holly, Leon-Saval, Sergio G., Min, Seong-Sik, Trinh, Christopher, Cecil, Gerald, Veilleux, Sylvain, Kreimeyer, Kory
We present the first scientific results from the Sydney-AAO Multi-Object IFS (SAMI) at the Anglo-Australian Telescope. This unique instrument deploys 13 fused fibre bundles (hexabundles) across a one-degree field of view allowing simultaneous spatial
Externí odkaz:
http://arxiv.org/abs/1211.0352
Autor:
Croom, Scott M., Lawrence, Jon S., Bland-Hawthorn, Joss, Bryant, Julia J., Fogarty, Lisa, Richards, Samuel, Goodwin, Michael, Farrell, Tony, Miziarski, Stan, Heald, Ron, Jones, D. Heath, Lee, Steve, Colless, Matthew, Brough, Sarah, Hopkins, Andrew M., Bauer, Amanda E., Birchall, Michael N., Ellis, Simon, Horton, Anthony, Leon-Saval, Sergio, Lewis, Geraint, Lopez-Sanchez, A. R., Min, Seong-Sik, Trinh, Christopher, Trowland, Holly
We demonstrate a novel technology that combines the power of the multi-object spectrograph with the spatial multiplex advantage of an integral field spectrograph (IFS). The Sydney-AAO Multi-object IFS (SAMI) is a prototype wide-field system at the An
Externí odkaz:
http://arxiv.org/abs/1112.3367