Zobrazeno 1 - 10
of 859
pro vyhledávání: '"Dragomir D."'
Autor:
Dragomir D. Sângeorzan, Florin Păcurar, Albert Reif, Holger Weinacker, Evelyn Rușdea, Ioana Vaida, Ioan Rotar
Publikováno v:
Remote Sensing, Vol 16, Iss 11, p 2012 (2024)
Arnica montana L. is a medicinal plant with significant conservation importance. It is crucial to monitor this species, ensuring its sustainable harvesting and management. The aim of this study is to develop a practical system that can effectively de
Externí odkaz:
https://doaj.org/article/b3a55367df4b4412b53fbb43a4f81db3
Autor:
Dragomir D. SÂNGEORZAN, Ioan ROTAR
Publikováno v:
Bulletin of University of Agricultural Sciences and Veterinary Medicine Cluj-Napoca: Agriculture, Vol 77, Iss 2 (2020)
In the era of abundant information, wisdom has become a scarce resource. Exploration and measurement of biodiversity yield copious amounts of information fragmented into numerous categories and types, following the pattern of life itself. We aim to r
Externí odkaz:
https://doaj.org/article/b7871952c2d64dd4a01077c4e647bc09
Autor:
Orell-Miquel, J., Carleo, I., Murgas, F., Nowak, G., Palle, E., Luque, R., Masseron, T., Sanz-Forcada, J., Dragomir, D., Dalba, P. A., Tronsgaard, R., Wittrock, J., Kim, K., Stibbards, C., Collins, K. I., Plavchan, P., Howell, S. B., Furlan, E., Buchhave, L. A., Gnilka, C. L., Gupta, A. F., Henning, Th., Lester, K. V., Rodriguez, J. E., Scott, N. J., Osborn, H. P., Villanueva Jr., S., Seager, S., Winn, J. N., Jenkins, J. M., Vanderspek, R., Latham, D. W., Rowden, P., Watanabe, D., Torres, G., Burke, C. J., Daylan, T., Barclay, T., Twicken, J. D., Ricker, G. R.
The Transiting Exoplanet Survey Satellite (TESS) provides a continuous suite of new planet candidates that need confirmation and precise mass determination from ground-based observatories. This is the case for the G-type star TOI-1710, which is known
Externí odkaz:
http://arxiv.org/abs/2401.13574
Autor:
Parviainen, Hannu, Murgas, Felipe, Esparza-Borges, Emma, Peláez-Torres, A., Palle, Enric, Luque, Rafael, Zapatero-Osorio, M. R., Korth, Judith, Fukui, Akihiko, Narita, Norio, Collins, K. A., Béjar, V. J. S., Morello, Guiseppe, Monelli, M., Garcia, N. Abreu, Chen, Guo, Crouzet, N., de Leon, J. P., Isogai, K., Kagetani, T., Kawauchi, K., Klagyivik, P., Kodama, T., Kusakabe, N., Livingston, J. H., Meni, P., Mori, M., Nowak, G., Tamura, M., Terada, Y., Watanabe, N., Ciardi, D. R., Lund, M. B., Christiansen, J. L., Dressing, C. D., Giacalone, S., Savel, A. B., Hirsch, L., Parsons, S. G., Brown, P., Collins, K. I., Barkaoui, K., Timmermans, M., Ghachoui, M., Soubkiou, A., Benkhaldoun, Z., McDermott, S., Pritchard, T., Rowden, P., Striegel, S., Gan, T., Horne, K., Jensen, E. L. N., Schwarz, R. P., Shporer, A., Srdoc, G., Seager, S., Winn, J. N., Jenkins, J. M., Ricker, G., Vanderspek, R., Dragomir, D.
We validate the Transiting Exoplanet Survey Satellite (TESS) object of interest TOI-2266.01 (TIC 348911) as a small transiting planet (most likely a super-Earth) orbiting a faint M5 dwarf ($V=16.54$) on a 2.33~d orbit. The validation is based on an a
Externí odkaz:
http://arxiv.org/abs/2401.11879
Autor:
Carleo, I., Malavolta, L., Desidera, S., Nardiello, D., Wang, S., Turrini, D., Lanza, A. F., Baratella, M., Marzari, F., Benatti, S., Biazzo, K., Bieryla, A., Brahm, R., Bonavita, M., Collins, K. A., Hellier, C., Locci, D., Hobson, M. J., Maggio, A., Mantovan, G., Pinamonti, S. Messina M., Rodriguez, J. E., Sozzetti, A., Stassun, K., Wang, X. Y., Ziegler, C., Damasso, M., Giacobbe, P., Murgas, F., Parviainen, H., Andreuzzi, G., Barkaoui, K., Berlind, P., Bignamini, A., Borsa, F., Briceño, C., Brogi, M., Cabona, L., Calkins, M. L., Capuzzo-Dolcetta, R., Cecconi, M., Colon, K. D., Cosentino, R., Dragomir, D., Esquerdo, G. A., Henning, T., Ghedina, A., Goeke, R. F., Gratton, R., Horta, F. Grau, Gupta, A. F., Jenkins, J. M., Jordán, A., Knapic, C., Latham, D. W., Mireles, I., Law, N., Lorenzi, V., Lund, M. B., Maldonado, J., Mann, A. W., Molinari, E., Pallé, E., Paegert, M., Pedani, M., Quinn, S. N., Scandariato, G., Seager, S., Winn, J. N., Wohler, B., Zingales, T.
Context. Different theories have been developed to explain the origins and properties of close-in giant planets, but none of them alone can explain all of the properties of the warm Jupiters (WJs, Porb = 10 - 200 days). One of the most intriguing cha
Externí odkaz:
http://arxiv.org/abs/2311.11903
Autor:
Rescigno, F., Hébrard, G., Vanderburg, A., Mann, A. W., Mortier, A., Morrell, S., Buchhave, L. A., Collins, K. A., Mann, C. R., Hellier, C., Haywood, R. D., West, R., Stalport, M., Heidari, N., Anderson, D., Huang, C. X., López-Morales, M., Cortés-Zuleta, P., Lewis, H. M., Dumusque, X., Boisse, I., Rowden, P., Cameron, A. Collier, Deleuil, M., Vezie, M., Pepe, F. A., Delfosse, X., Charbonneau, D., Rice, K., Demangeon, O., Quinn, S. N., Udry, S., Forveille, T., Winn, J. N., Sozzetti, A., Hoyer, S., Seager, S., Wilson, T. G., Dalal, S., Martioli, E., Striegel, S., Boschin, W., Dragomir, D., Fiorenzano, A. F. Martínez, Cosentino, R., Ghedina, A., Malavolta, L., Affer, L., Lakeland, B. S., Nicholson, B. A., Foschino, S., Wünsche, A., Barkaoui, K., Srdoc, G., Randolph, J., Guillet, B., Conti, D. M., Ghachoui, M., Gillon, M., Benkhaldoun, Z., Pozuelos, F. J., Timmermans, M., Girardin, E., Matutano, S., Bosch-Cabot, P., Muñoz, J. A., Forés-Toribio, R.
We present the characterisation of an inner mini-Neptune in a 9.2292005$\pm$0.0000063 day orbit and an outer mono-transiting sub-Saturn planet in a 95.50$^{+0.36}_{-0.25}$ day orbit around the moderately active, bright (mv=8.9 mag) K5V star TOI-2134.
Externí odkaz:
http://arxiv.org/abs/2310.13623
Autor:
Ulmer-Moll, S., Lendl, M., Gill, S., Villanueva, S., Hobson, M. J., Bouchy, F., Brahm, R., Dragomir, D., Grieves, N., Mordasini, C., Anderson, D. R., Acton, J. S., Bayliss, D., Bieryla, A., Burleigh, M. R., Casewell, S. L., Chaverot, G., Eigmüller, P., Feliz, D., Gaudi, S., Gillen, E., Goad, M. R., Gupta, A. F., Günther, M. N., Henderson, B. A., Henning, T., Jenkins, J. S., Jones, M., Jordán, A., Kendall, A., Latham, D. W., Mireles, I., Moyano, M., Nadol, J., Osborn, H. P., Pepper, J., Pinto, M. T., Psaridi, A., Queloz, D., Quinn, S., Rojas, F., Sarkis, P., Schlecker, M., Tilbrook, R. H., Torres, P., Trifonov, T., Udry, S., Vines, J. I., West, R., Wheatley, P., Yao, X., Zhao, Y., Zhou, G.
Publikováno v:
A&A 666, A46 (2022)
Long-period transiting planets provide the opportunity to better understand the formation and evolution of planetary systems. Their atmospheric properties remain largely unaltered by tidal or radiative effects of the host star, and their orbital arra
Externí odkaz:
http://arxiv.org/abs/2207.03911
Autor:
Naponiello, L., Mancini, L., Damasso, M., Bonomo, A. S., Sozzetti, A., Nardiello, D., Biazzo, K., Stognone, R. G., Lillo-Box, J., Lanza, A. F., Poretti, E., Lissauer, J. J., Zeng, L., Bieryla, A., Hébrard, G., Basilicata, M., Benatti, S., Bignamini, A., Borsa, F., Claudi, R., Cosentino, R., Covino, E., de Gurtubai, A., Delfosse, X., Desidera, S., Dragomir, D., Eastman, J. D., Essack, Z., Fiorenzano, A. F. M., Giacobbe, P., Harutyunyan, A., Heidari, N., Hellier, C., Jenkins, J. M., Knapic, C., König, P. -C., Latham, D. W., Magazzù, A., Maggio, A., Maldonado, J., Micela, G., Molinari, E., Molinaro, M., Morgan, E. H., Moutou, C., Nascimben, V., Pace, E., Pagano, I., Pedani, M., Piotto, G., Pinamonti, M., Quintana, E. V., Rainer, M., Ricker, G. R., Seager, S., Twicken, J. D., Vanderspek, R., Winn, J. N.
Publikováno v:
A&A 667, A8 (2022)
We investigate the exoplanet candidate TOI-1422b, which was discovered by the TESS space telescope around the high proper-motion G2V star TOI-1422 ($V=10.6$ mag), 155pc away, with the primary goal of confirming its planetary nature and characterising
Externí odkaz:
http://arxiv.org/abs/2207.03293
Autor:
Sângeorzan, Dragomir D.1 (AUTHOR) dragomir.sangeorzan@usamvcluj.ro, Păcurar, Florin1 (AUTHOR) florin.pacurar@usamvcluj.ro, Reif, Albert2 (AUTHOR) albert.reif@waldbau.uni-freiburg.de, Weinacker, Holger3 (AUTHOR) holger.weinacker@felis.uni-freiburg.de, Rușdea, Evelyn4 (AUTHOR) evelyn.rusdea@informatik.uni-freiburg.de, Vaida, Ioana1 (AUTHOR) ioan.rotar@usamvcluj.ro, Rotar, Ioan1 (AUTHOR)
Publikováno v:
Remote Sensing. Jun2024, Vol. 16 Issue 11, p2012. 25p.
Autor:
Schanche, N., Pozuelos, F. J., Günther, M. N., Wells, R. D., Burgasser, A. J., Chinchilla, P., Delrez, L., Ducrot, E., Garcia, L. J., Chew, Y. Gómez Maqueo, Jofré, E., Rackham, B. V., Sebastian, D., Stassun, K. G., Stern, D., Timmermans, M., Barkaoui, K., Belinski, A., Benkhaldoun, Z., Benz, W., Charbonneau, D., Christiansen, Jessie L., Collins, Karen A., Demory, B. -O., Dévora-Pajares, M., de Wit, J., Dragomir, D., Dransfield, G., Furlan, E., Ghachou, M., Gillon, M., Gnilka, C., Gómez-Muñoz, M. A., Guerrero, N., Harris, M., Heng, K., Henze, C. E., Hesse, K., Howell, S. B., Jehin, E., Jenkins, J., Jensen, Eric L. N., Kunimoto, M., Latham, D. W., Lester, K., McLeod, Kim K., Mireles, I., Murray, C. A., Niraula, P., Pedersen, P. P., Queloz, D., Quintana, E. V., Ricker, G., Rudat, A., Sabin, L., Safonov, B., Schroffenegger, U., Scott, N., Seager, S., Strakhov, I., Triaud, A. H. M. J., Vanderspek, R., Vezie, M., Winn, J.
Publikováno v:
A&A 657, A45 (2022)
Thanks to the relative ease of finding and characterizing small planets around M dwarf stars, these objects have become cornerstones in the field of exoplanet studies. The current paucity of planets in long-period orbits around M dwarfs make such obj
Externí odkaz:
http://arxiv.org/abs/2111.01749