Name and surname:
|
Mgr. Adrián Galád, PhD.
|
Document type:
|
Research/art/teacher profile of a person
|
The name of the university:
|
Comenius University Bratislava
|
The seat of the university:
|
Šafárikovo námestie 6, 818 06 Bratislava
|
III.a - Occupation-position | III.b - Institution | III.c - Duration |
---|---|---|
resarch assistant | Comenius University in Bratislava, Faculty o Mathematics, Physics and Informatics | 1994-2013 |
resarcher | Comenius University in Bratislava, Faculty o Mathematics, Physics and Informatics | 2013- |
resarcher | Academy of Sciences of the Czech Republic, Astronomical Institute in Ondřejov | 2004-2017 (part time job) |
IV.a - Activity description, course name, other | IV.b - Name of the institution | IV.c - Year |
---|---|---|
Basics of Python programming language | National competence center for HPC | 2021 |
Data processing and visualization in Python | National competence center for HPC | 2022 |
V.5.a - Name of the course | V.5.b - Study programme | V.5.c - Degree | V.5.d - Field of study |
---|---|---|---|
Asteroids | Astronomy and astrophysics | II. | Physics |
Laboratory work (1) | Astronomy and astrophysics | II. | Physics |
Internship | Astronomy and astrophysics | II. | Physics |
Pravec, P., et al.: Photometric survey of binary near-Earth asteroids, Icarus 181, 63-93 (2006)
Pravec, P., et al.Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations, Icarus 221, 365-387 (2012)
Pravec, P., et al.: Formation of asteroid pairs by rotational fission, Nature 466, 1085-1088 (2010)
Lowry, S. C., et al: Direct Detection of the Asteroidal YORP Effect, Science 316, 272-274 (2007)
Pravec, P., et al.: Tumbling asteroids, Icarus 173, 108-131 (2005)
Pravec, P., et al.: Asteroid pairs: A complex picture, Icarus 333, 429-463 (2019)
Scheirich, P., et al.: A satellite orbit drift in binary near-Earth asteroids (66391) 1999 KW4 and (88710) 2001 SL9 -Indication of the BYORP effect, Icarus 360, article id. 114321 (2021)
Oszkiewicz, D., et al.: Spin rates of V-type asteroids, Astronomy & Astrophysics 643, id.A117 (2020)
Oszkiewicz, D., et al.: First survey of phase curves of V-type asteroids, Icarus 357, article id. 114158 (2021)
Ďurech, J., et al.: Secular change in the spin states of asteroids due to radiation and gravitation torques. New detections and updates of the YORP effect, Astronomy & Astrophysics 682, id. A93 (2024)
Pravec, P., et al.: Spin rate distribution of small asteroids, Icarus 197, 497-504 (2008): Mainzer, A., et al.: Preliminary Results from NEOWISE: An Enhancement to the Wide-field Infrared Survey Explorer for Solar System Science, Astrophys. J. 731, 53 (2011) (738/653 cit.)
Pravec, P., et al.: Photometric survey of binary near-Earth asteroids, Icarus 181, 63-93 (2006): Naoz, S.: The Eccentric Kozai-Lidov Effect and Its Applications, Annual Review of Astronomy and Astrophysics, vol. 54, p.441-489 (2016) (638/566 Cit)
Pravec, P., et al.: Formation of asteroid pairs by rotational fission, Nature 466, 1085-1088 (2010): Graham, M. J.et al.: The Zwicky Transient Facility: Science Objectives, Publications of the Astronomical Society of the Pacific, 131, Issue 1001, pp. 078001 (2019) (652/535 Cit.)
Pravec, P., et al.: Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations, Icarus 221, 365-387 (2012): Mainzer, A., et al.: Initial Performance of the NEOWISE Reactivation Mission, Astrophys. J. 792, id. 30, (2014) (565/480 cit.)
Ďurech, J., et al: Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes, Icarus 214, 652-670 (2011): Carry, B.: Density of asteroids, Planetary and Space Science 73, 98-118 (2012) (446/437 cit.)
VEGA 1/0911/17 (2017 - 2020) Evolution of bodies under the influence of gravitational and non-gravitational forces.
The aim is to verify the real effect of non-gravitational forces on the motion of dust particles, as the effect of the solar wind in particular is proving to be so far underestimated for certain specific particle sizes. In the observation part, there is an attempt to compare the rotational characteristics of the V types of asteroids we observed with the characteristics of other types. - a project representative
VEGA 1/0530/22 (2022 - 2025) Slope parameters, absolute magnitudes and senses of rotation of V-types of asteroids.
With our targeted long-term photometric observations of a number of asteroids of taxonomic type V, being located either in the Vesta family or outside it, at different phase angles and different geometric conditions, we determine, among other things, the values of the slope parameters and absolute magnitudes. In addition, for a part of the examined bodies we gradually obtain valuable material for determination of their approximate shape and sense of rotation..- a project leader
In Chapter VI. 1.1 only journal outputs are included (not electronic circulars, conference papers, or popularization papers)
In Chapter VI. 1.3 only the lower limit estimations are given
in 2013, the scientific qualification level of VKS IIa was achieved