Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Quiroga-Nunez Luis Henry"'
Autor:
Bhattacharya, Rajorshi, Medina, Brandon M., Pihlström, Ylva M., Sjouwerman, Loránt O., Lewis, Megan O., Sahai, Raghvendra, Stroh, Michael C., Quiroga-Nuñez, Luis Henry, van Langevelde, Huib Jan, Claussen, Mark J, Weller, Rachel
We present a method to estimate distances to Asymptotic Giant Branch (AGB) stars in the Galaxy, using spectral energy distributions (SEDs) in the near- and mid-infrared. By assuming that a given set of source properties (initial mass, stellar tempera
Externí odkaz:
http://arxiv.org/abs/2405.02459
Autor:
Quiroga-Nuñez, Luis Henry, van Langevelde, Huib Jan, Sjouwerman, Loránt O., Pihlström, Ylva M., Brown, Anthony G. A., Rich, R. Michael, Stroh, Michael C., Lewis, Megan O., Habing, Harm J.
Radio campaigns using maser stellar beacons have provided crucial information to characterize Galactic stellar populations. Currently, the Bulge Asymmetries and Dynamical Evolution (BAaDE) project is surveying infrared (IR) color-selected targets for
Externí odkaz:
http://arxiv.org/abs/2009.01909
We present 43 GHz VLA spectra for 51 AGB sources with the goal of verifying an infrared (IR) color cut intended to separate Carbon-rich (C) and Oxygen-rich (O) AGB sources throughout the Galaxy. The color cut is a simple line in the $[K_s]-[A]$ versu
Externí odkaz:
http://arxiv.org/abs/2008.06535
Autor:
Venturi, Tiziana, Paragi, Zsolt, Lindqvist, Michael, Bartkiewicz, Anna, Beswick, Rob, Bogdanović, Tamara, Brisken, Walter, Charlot, Patrick, Colomer, Francisco, Conway, John, Frey, Sándor, Guirado, José Carlos, Gurvits, Leonid, van Langevelde, Huib, Lobanov, Andrei, McKean, John, Morganti, Raffaella, Muxlow, Tom, Pérez-Torres, Miguel, Rygl, Kazi, Schulz, Robert, Szomoru, Arpad, de Vicente, Pablo, An, Tao, Anglada, Guillem, Argo, Megan, Azulay, Rebecca, van Bemmel, Ilse, Bocanegra, Tatiana, Boccardi, Biagina, Castangia, Paola, Chibueze, James, Cimò, Giuseppe, Climent, Juan-Bautista, Deane, Roger, Deller, Adam, Dodson, Richard, Duev, Dmitry, Etoka, Sandra, Fenech, Danielle, Gabányi, Krisztina, Gabuzda, Denise, Garrett, Michael, Gawroński, Marcin, Ghirlanda, Giancarlo, Giroletti, Marcello, Goddi, Ciriaco, Gómez, Jose Luis, Gray, Malcolm, Greaves, Jane, Hessels, Jason, van der Horst, Alexander, Hunter, Todd, Laing, Robert, Lal, Dharam Vir, Lambert, Sébastien, Loinard, Laurent, Marcote, Benito, Merloni, Andrea, Miller-Jones, James, Calvés, Guifré Molera, Moscadelli, Luca, Olofsson, Hans, Petrov, Leonid, Pizzo, Roberto, Possenti, Andrea, Quiroga-Nuñez, Luis Henry, Reynolds, Cormac, Richards, Anita, Rioja, Maria, Sanna, Alberto, Savolainen, Tuomas, Sbarrato, Tullia, Spingola, Cristiana, Surcis, Gabriele, Trigilio, Corrado, Varenius, Eskil, Vlemmings, Wouter, van Velzen, Sjoert, van der Walt, Johan
This white paper describes the science case for Very Long Baseline Interferometry (VLBI) and provides suggestions towards upgrade paths for the European VLBI Network (EVN). The EVN is a distributed long-baseline radio interferometric array, that oper
Externí odkaz:
http://arxiv.org/abs/2007.02347
Autor:
Kennedy, Grant M., Ginski, Christian, Kenworthy, Matthew A., Benisty, Myriam, Henning, Thomas, van Holstein, Rob G., Kral, Quentin, Ménard, François, Milli, Julien, Quiroga-Nuñez, Luis Henry, Rab, Christian, Stolker, Tomas, Sturm, Ardjan
RZ Psc is a young Sun-like star with a bright and warm infrared excess that is occasionally dimmed significantly by circumstellar dust structures. Optical depth arguments suggest that the dimming events do not probe a typical sight line through the c
Externí odkaz:
http://arxiv.org/abs/2005.14203
Autor:
van Langevelde, Huib, Quiroga-Nuñez, Luis Henry, Vlemmings, Wouter, Loinard, Laurent, Honma, Mareki, Nakagawa, Akiharu, Immer, Katharina, Burns, Ross, Pihlström, Ylva, Sjouwerman, Lorant, Rich, R. Michael, Natarajan, Iniyan, Deane, Roger
With the publication of Gaia DR2, 1.3 billion stars now have public parallax and proper motion measurements. In this contribution, we compare the results for sources that have both optical and radio measurements, focusing on circumstellar masers. For
Externí odkaz:
http://arxiv.org/abs/1901.07804
Autor:
Pihlström, Ylva M., Sjouwerman, Loránt O., Claussen, Mark J, Morris, Mark R., Rich, R. Michael, van Langevelde, Huib Jan, Quiroga-Nuñez, Luis Henry
Observations of dust-enshrouded evolved stars selected from infrared catalogs requiring high positional accuracy, like infrared spectroscopy or long baseline radio interferometric observations, often require preparational observational steps determin
Externí odkaz:
http://arxiv.org/abs/1811.04511
Autor:
Kraus, Stefan, Monnier, John D., Ireland, Michael J., Duchene, Gaspard, Espaillat, Catherine, Hoenig, Sebastian, Juhasz, Attila, Mordasini, Chris, Olofsson, Johan, Paladini, Claudia, Stassun, Keivan, Turner, Neal, Vasisht, Gautam, Harries, Tim J., Bate, Matthew R., Gonzalez, Jean-Francois, Matter, Alexis, Zhu, Zhaohuan, Panic, Olja, Regaly, Zsolt, Morbidelli, Alessandro, Meru, Farzana, Wolf, Sebastian, Ilee, John, Berger, Jean-Philippe, Zhao, Ming, Kral, Quentin, Morlok, Andreas, Bonsor, Amy, Ciardi, David, Kane, Stephen R., Kratter, Kaitlin, Laughlin, Greg, Pepper, Joshua, Raymond, Sean, Labadie, Lucas, Nelson, Richard P., Weigelt, Gerd, Brummelaar, Theo ten, Pierens, Arnaud, Oudmaijer, Rene, Kley, Wilhelm, Pope, Benjamin, Jensen, Eric L. N., Bayo, Amelia, Smith, Michael, Boyajian, Tabetha, Quiroga-Nunez, Luis Henry, Millan-Gabet, Rafael, Chiavassa, Andrea, Gallenne, Alexandre, Reynold, Mark, de Wit, Willem-Jan, Wittkowski, Markus, Millour, Florentin, Gandhi, Poshak, Almeida, Cristina Ramos, Herrero, Almudena Alonso, Packham, Chris, Kishimoto, Makoto, Tristram, Konrad R. W., Pott, Joerg-Uwe, Surdej, Jean, Buscher, David, Haniff, Chris, Lacour, Sylvestre, Petrov, Romain, Ridgway, Steve, Tuthill, Peter, van Belle, Gerard, Armitage, Phil, Baruteau, Clement, Benisty, Myriam, Bitsch, Bertram, Paardekooper, Sijme-Jan, Pinte, Christophe, Masset, Frederic, Rosotti, Giovanni P.
The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging c
Externí odkaz:
http://arxiv.org/abs/1608.00578
Akademický článek
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Autor:
Ridgway Steve, Regaly Zsolt, Kral Quentin, Gandhi Poshak, Packham Chris, Tristram Konrad R. W., Baruteau Clement, Tuthill Peter, Mordasini Chris, Matter Alexis, A. Pierens, Duchene Gaspard, Olofsson Johan, Ilee John, Bitsch Bertram, Wittkowski Markus, Pinte Christophe, Meru Farzana, Armitage Phil, Chiavassa Andrea, Berger Jean-Philippe, Millour Florentin, Buscher David, Rosotti Giovanni P., Zhao Ming, Pott Joerg-Uwe, Wolf Sebastian, ten Brummelaar Theo, Bayo Amelia, Labadie Lucas, Morlok Andreas, Millan-Gabet Rafael, Kishimoto Makoto, Gallenne Alexandre, Ciardi David, Turner Neal, Gonzalez Jean-Francois, Vasisht Gautam, Monnier John D., Zhu Zhaohuan, Weigelt Gerd, Quiroga-Nunez Luis Henry, Kratter Kaitlin, Ramos Almeida Cristina, Juhasz Attila, Kley Wilhelm, Smith Michael, Espaillat Catherine, Alonso Herrero Almudena, Paladini Claudia, Pope Benjamin, Bate Matthew R., de Wit Willem-Jan, Harries Tim J., Lacour Sylvestre, Boyajian Tabetha, Petrov Romain, Paardekooper Sijme-Jan, Laughlin Greg, Nelson Richard P., Hoenig Sebastian, Pepper Joshua, Stassun Keivan, Jensen Eric L. N., Bonsor Amy, Kraus Stefan, Haniff Chris, Reynold Mark, Panic Olja, Sean N. Raymond, Masset Frederic, van Belle Gerard, Morbidelli Alessandro, Kane Stephen R., Ireland Michael J., Surdej Jean, Oudmaijer Rene, Benisty Myriam
Publikováno v:
2016arXiv160800578K-Proceedings of SPIE 2016; doi:10.1117/12.2231067 2016-a From Conference Volume 9907 Optical and Infrared Interferometry and Imaging V Fabien Malbet; Michelle J. Creech-Eakman; Peter G. Tuthill Edinburgh, United Kingdom | June 26, 2016
2016arXiv160800578K-Proceedings of SPIE 2016; doi:10.1117/12.2231067 2016-a From Conference Volume 9907 Optical and Infrared Interferometry and Imaging V Fabien Malbet; Michelle J. Creech-Eakman; Peter G. Tuthill Edinburgh, United Kingdom | June 26, 2016, Aug 2016, Edinburgh, United Kingdom. pp.arXiv:1608.00578
OPTICAL AND INFRARED INTERFEROMETRY AND IMAGING V, 9907
NASA Astrophysics Data System
Proceedings of the SPIE
Optical and Infrared Interferometry and Imaging V
Optical and Infrared Interferometry and Imaging V, Jun 2016, Edinburgh, United Kingdom. pp.99071K, ⟨10.1117/12.2231067⟩
HAL
2016arXiv160800578K-Proceedings of SPIE 2016; doi:10.1117/12.2231067 2016-a From Conference Volume 9907 Optical and Infrared Interferometry and Imaging V Fabien Malbet; Michelle J. Creech-Eakman; Peter G. Tuthill Edinburgh, United Kingdom | June 26, 2016, Aug 2016, Edinburgh, United Kingdom. pp.arXiv:1608.00578
OPTICAL AND INFRARED INTERFEROMETRY AND IMAGING V, 9907
NASA Astrophysics Data System
Proceedings of the SPIE
Optical and Infrared Interferometry and Imaging V
Optical and Infrared Interferometry and Imaging V, Jun 2016, Edinburgh, United Kingdom. pp.99071K, ⟨10.1117/12.2231067⟩
HAL
The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes. We make the case that a breakthrough in angular resolution imaging c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::42d653121741ea2723b52b5dba82c850
https://hal.archives-ouvertes.fr/hal-01357767
https://hal.archives-ouvertes.fr/hal-01357767