Zobrazeno 1 - 10
of 1 764
pro vyhledávání: '"Debes, P. P."'
Autor:
Debes, P. P., Langer, M., Pagel, M., Menna, E., Smarsly, B., Osella, S., Gallego, J., Gatti, T.
Publikováno v:
Chem. Nano. Mat. 2024, 10, e202300471
Chemical functionalization of carbon nanodots (CNDs) offers a valuable opportunity to tailor multifunctionality in these nanocarbons, by engineering the composition of their molecular surface. Therefore, it is important to elucidate the type and amou
Externí odkaz:
http://arxiv.org/abs/2410.06677
Autor:
Limbach, Mary Anne, Vanderburg, Andrew, Venner, Alexander, Blouin, Simon, Stevenson, Kevin B., MacDonald, Ryan J., Jenkins, Sydney, Bowens-Rubin, Rachel, Soares-Furtado, Melinda, Morley, Caroline, Janson, Markus, Debes, John, Xu, Siyi, Kleisioti, Evangelia, Kenworthy, Matthew, Butler, Paul, Crane, Jeffrey D., Osip, Dave, Shectman, Stephen, Teske, Johanna
The MIRI Exoplanets Orbiting White dwarfs (MEOW) Survey is a cycle 2 JWST program to search for exoplanets around dozens of nearby white dwarfs via infrared excess and direct imaging. In this paper, we present the detection of mid-infrared excess at
Externí odkaz:
http://arxiv.org/abs/2408.16813
Autor:
M., Sai Krishanth P., Douglas, Ewan S., Anche, Ramya M., Hom, Justin, Cahoy, Kerri L., Debes, John H., Jang-Condell, Hannah, Rebollido, Isabel, Ren, Bin B., Stark, Christopher C., Thompson, Robert, Xin, Yinzi
Publikováno v:
The Astronomical Journal, 168:169 (10pp), 2024 October
Epsilon Eridani ($\epsilon$ Eri) is one of the first debris disk systems detected by the Infrared Astronomical Satellite (IRAS). However, the system has thus far eluded detection in scattered light with no components having been directly imaged. Its
Externí odkaz:
http://arxiv.org/abs/2408.06973
Autor:
Casewell, S. L., Debes, J., Dupuy, T. J., Dufour, P., Bonsor, A., Rebassa-Mansergas, A., Murillo-Ojeda, R., French, J. R., Alexander, R. D., Xu, Siyi, Martin, E., Manjavacas, E.
We present new results on PHL 5038AB, a widely separated binary system composed of a white dwarf and a brown dwarf, refining the white and brown dwarf parameters and determining the binary separation to be $66^{+12}_{-24}$~AU. New spectra of the whit
Externí odkaz:
http://arxiv.org/abs/2404.05488
Autor:
Ren, Bin B., Fogarty, Kevin, Debes, John H., Meyer, Eileen T., Mo, Youbin, Mawet, Dimitri, Perrin, Marshall D., Ogle, Patrick M., Sahlmann, Johannes
The close-in regions of bright quasars' host galaxies have been difficult to image due to the overwhelming light from the quasars. With coronagraphic observations in visible light using the Space Telescope Imaging Spectrograph (STIS) on the Hubble Sp
Externí odkaz:
http://arxiv.org/abs/2402.09505
Autor:
Hom, Justin, Patience, Jennifer, Chen, Christine H., Duchêne, Gaspard, Mazoyer, Johan, Millar-Blanchaer, Maxwell A., Esposito, Thomas M., Kalas, Paul, Crotts, Katie A., Gonzales, Eileen C., Kolokolova, Ludmilla, Lewis, Briley L., Matthews, Brenda C., Rice, Malena, Weinberger, Alycia J., Wilner, David J., Wolff, Schuyler G., Bruzzone, Sebastián, Choquet, Elodie, Debes, John, De Rosa, Robert J., Donaldson, Jessica, Draper, Zachary, Fitzgerald, Michael P., Hines, Dean C., Hinkley, Sasha, Hughes, A. Meredith, López, Ronald A., Marchis, Franck, Metchev, Stanimir, Moro-Martin, Amaya, Nesvold, Erika, Nielsen, Eric L., Oppenheimer, Rebecca, Padgett, Deborah, Perrin, Marshall D., Pueyo, Laurent, Rantakyrö, Frederik, Ren, Bin B., Schneider, Glenn, Soummer, Remí, Song, Inseok, Stark, Christopher C.
Spatially-resolved images of debris disks are necessary to determine disk morphological properties and the scattering phase function (SPF) which quantifies the brightness of scattered light as a function of phase angle. Current high-contrast imaging
Externí odkaz:
http://arxiv.org/abs/2402.00214
Autor:
Mullally, Susan E., Debes, John, Cracraft, Misty, Mullally, Fergal, Poulsen, Sabrina, Albert, Loic, Thibault, Katherine, Reach, William T., Hermes, J. J., Barclay, Thomas, Kilic, Mukremin, Quintana, Elisa V.
We report the discovery of two directly imaged, giant planet candidates orbiting the metal-rich DAZ white dwarfs WD 1202-232 and WD 2105-82. JWST's Mid-Infrared Instrument (MIRI) data on these two stars show a nearby resolved source at a projected se
Externí odkaz:
http://arxiv.org/abs/2401.13153
Autor:
Crotts, Katie A., Matthews, Brenda C., Duchêne, Gaspard, Esposito, Thomas M., Dong, Ruobing, Hom, Justin, Oppenheimer, Rebecca, Rice, Malena, Wolff, Schuyler G., Chen, Christine H., Ó, Clarissa R. Do, Kalas, Paul, Lewis, Briley L., Weinberger, Alycia J., Wilner, David J., Ammons, Mark, Arriaga, Pauline, De Rosa, Robert J., Debes, John H., Fitzgerald, Michael P., Gonzales, Eileen C., Hines, Dean C., Hinkley, Sasha, Hughes, A. Meredith, Kolokolova, Ludmilla, Lee, Eve J., López, Ronald A., Macintosh, Bruce, Mazoyer, Johan, Metchev, Stanimir, Millar-Blanchaer, Maxwell A., Nielsen, Eric L., Patience, Jenny, Perrin, Marshall D., Pueyo, Laurent, Rantakyrö, Fredrik T., Ren, Bin B., Schneider, Glenn, Soummer, Remi, Stark, Christopher C.
The Gemini Planet Imager (GPI) has excelled in imaging debris disks in the near-infrared. The GPI Exoplanet Survey (GPIES) imaged twenty-four debris disks in polarized $H$-band light, while other programs observed half of these disks in polarized $J$
Externí odkaz:
http://arxiv.org/abs/2311.14599
Autor:
Poulsen, Sabrina, Debes, John, Cracraft, Misty, Mullally, Susan E., Reach, William T., Kilic, Mukremin, Mullally, Fergal, Albert, Loic, Thibault, Katherine, Hermes, J. J., Barclay, Thomas, Quintana, Elisa V.
The launch of JWST has ushered in a new era of high precision infrared astronomy, allowing us to probe nearby white dwarfs for cold dust, exoplanets, and tidally heated exomoons. While previous searches for these exoplanets have successfully ruled ou
Externí odkaz:
http://arxiv.org/abs/2311.14165
Autor:
Anche, Ramya M, Douglas, Ewan, Milani, Kian, Ashcraft, Jaren, Millar-Blanchaer, Maxwell A., Debes, John H, Milli, Julien, Hom, Justin
The Nancy Grace Roman Space Telescope Coronagraph Instrument will enable the polarimetric imaging of debris disks and inner dust belts in the optical and near-infrared wavelengths, in addition to the high-contrast polarimetric imaging and spectroscop
Externí odkaz:
http://arxiv.org/abs/2311.05422