Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Máté Ádámkovics"'
Publikováno v:
Remote Sensing, Vol 14, Iss 18, p 4567 (2022)
We obtained high-resolution spectra of Jupiter between 4.6 and 5.4 µm using NIRSPEC on the Keck 2 telescope in February 2017. We measured the spatial variation of NH3, H2O, and the pressure level of deep (p > 3 bar) clouds using two geometries. We a
Externí odkaz:
https://doaj.org/article/ce59aea25e9d4006ac39da127c7867c8
Publikováno v:
Planetary Science Journal, 1(2)
We present observations obtained with the 10-m Keck telescopes of the forbidden SO rovibronic transition at 1.707 micron on Io while in eclipse. We show its spatial distribution at a resolution of ~0.12" and a spectral resolution of R ~2500, as well
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b6bb57c5d1205fda660442c95ca6af98
http://arxiv.org/abs/2101.01789
http://arxiv.org/abs/2101.01789
Autor:
Alexander G. Hayes, Michael Malaska, James J. Wray, Sarah M. Hörst, Jason D. Hofgartner, Lucas Liuzzo, Ralph D. Lorenz, Elizabeth P. Turtle, George D. McDonald, Morgan L. Cable, Máté Ádámkovics, Paul Corlies, Jacob Buffo
From orbit, the visibility of Titan's surface is limited to a handful of narrow spectral windows in the near-infrared (near-IR), primarily from the absorption of methane gas. This has limited the ability to identify specific compounds on the surface
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c7586fd136255c54b6d4be37561e315
Autor:
Juan M. Lora, Fiona Nichols-Fleming, Alexander G. Hayes, Jason M. Soderblom, Patricio Rojo, Paul Corlies, Sebastien Rodriguez, Máté Ádámkovics, Elizabeth P. Turtle
Publikováno v:
The Planetary Science Journal. 2:180
While it has long been known that Titan’s haze and atmosphere are dynamic on seasonal timescales, recent results have revealed that they also exhibit significant subseasonal variations. Here, we report on observations of Titan acquired over an eigh
Publikováno v:
Icarus. 297:265-281
We present observations of Io's Loki Patera taken with the 10-m Keck telescopes between 1998 and 2016. Adding these data to those published by Rathbun and Spencer (2006) and the Gemini data of de Kleer and de Pater (2016a, 2017) results in a database
Autor:
Imke de Pater, Máté Ádámkovics
Publikováno v:
Icarus. 290:134-149
We observed Titan with the OH Suppressing InfraRed Imaging Spectrograph (OSIRIS) at the W. M. Keck observatory from 2006 through 2015 using adaptive optics. The sunlight scattered by atmospheric haze was spatially resolved in the 2.0 µm (K) band win
Autor:
Juan M. Lora, Máté Ádámkovics
Publikováno v:
Icarus. 286:270-279
We retrieve vertical and meridional variations of methane mole fraction in Titan's lower troposphere by re-analyzing near-infrared ground-based observations from 17 July 2014 UT (Adamkovics et al., 2016). We generate synthetic spectra using atmospher
Autor:
Ellen S. Howell, Laird M. Close, Michael C. Nolan, Vishnu Reddy, Patrick A. Taylor, B. Timerson, Alan W. Harris, Brian D. Warner, Linda A. Rodriguez-Ford, Máté Ádámkovics, Jon D. Giorgini, Mikko Kaasalainen, Matti Viikinkoski, Lance A. M. Benner, Katherine de Kleer, Christopher Magri, Katie M. Morzinski, James E. Richardson, Imke de Pater, Al Conrad, Michael K. Shepard, Jared R. Males
Publikováno v:
Icarus. 281:388-403
Using the S-band radar at Arecibo Observatory, we observed 16 Psyche, the largest M-class asteroid in the main belt. We obtained 18 radar imaging and 6 continuous wave runs in November and December 2015, and combined these with 16 continuous wave run
Autor:
Arielle Moullet, Yasumasa Kasaba, Gordon L. Bjoraker, Leigh N. Fletcher, John H. Rogers, Imke de Pater, E. Villard, Richard Cosentino, David DeBoer, Padraig T. Donnelly, Máté Ádámkovics, Charles Goullaud, Bryan J. Butler, Michael H. Wong, Robert J. Sault, Chris Moeckel, Glenn S. Orton, James Sinclair
Publikováno v:
The Astronomical Journal
Astronomical Journal, 158(4)
Astronomical Journal, 158(4)
We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 3-5 January 2017, just days after an energetic eruption at 16.5S jovigraphic latitude had been reported by the amateur communit
We report the detection of hot H$_{2}$O and OH emission from the Herbig Ae/Be star HD$~101412$ using the Cryogenic Infrared Echelle Spectrograph on the $\textit{Very Large Telescope}$. Previous studies of Herbig Ae/Be stars have shown the presence of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::993b7a72b0b2620182db1f5f9f82fcc5
http://arxiv.org/abs/1812.07094
http://arxiv.org/abs/1812.07094