Gotowa bibliografia na temat „Mass photometry”
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Artykuły w czasopismach na temat "Mass photometry"
Prokhorov, M. E., A. I. Zakharov, V. G. Moshkalev, N. L. Krusanova i M. S. Tuchin. "Mass Computations of the Brightness of Stars in an Arbitrary Spectral Band". Астрономический журнал 100, nr 6 (1.06.2023): 500–511. http://dx.doi.org/10.31857/s0004629923050092.
Pełny tekst źródłaSarrouh, Ghassan T. E., Adam Muzzin, Kartheik G. Iyer, Lamiya Mowla, Sunna Withers, Nicholas S. Martis, Roberto Abraham i in. "Exposing Line Emission: The Systematic Differences of Measuring Galaxy Stellar Masses with JWST NIRCam Medium versus Wide Band Photometry". Astrophysical Journal Letters 967, nr 1 (1.05.2024): L17. http://dx.doi.org/10.3847/2041-8213/ad43e8.
Pełny tekst źródłaČAVLOVIĆ, ANKA OZANA, i IVAN BEŠLIĆ. "APPLICATION OF PHOTOMETRY IN DETERMINING THE DUST MASS CONCENTRATION OF HARDWOODS". WOOD RESEARCH 66(4) 2021 66, nr 4 (9.09.2021): 678–88. http://dx.doi.org/10.37763/wr.1336-4561/66.4.678688.
Pełny tekst źródłaCernic, Vitor. "Stellar Population Photometric Synthesis with AI of S-PLUS galaxies". Proceedings of the International Astronomical Union 16, S362 (czerwiec 2020): 148–49. http://dx.doi.org/10.1017/s1743921322001430.
Pełny tekst źródłaJerzykiewicz, M. "Two Aspects of Using Hipparcos Data for Studying Multiperiodic Stellar Pulsations". International Astronomical Union Colloquium 176 (2000): 46–49. http://dx.doi.org/10.1017/s0252921100057043.
Pełny tekst źródłaSchilbach, E., H. Meusinger i J. Souchay. "Luminosity and Mass Functions for the Pleiades from the Schmidt Survey". Symposium - International Astronomical Union 164 (1995): 379. http://dx.doi.org/10.1017/s0074180900108976.
Pełny tekst źródłaSchmehl, T., J. Gebhart, H. Schutte, A. Scharmann i W. Seeger. "On-line laser-photometric monitoring of aerosol deposition in ventilated rabbit lungs". Journal of Applied Physiology 80, nr 1 (1.01.1996): 351–56. http://dx.doi.org/10.1152/jappl.1996.80.1.351.
Pełny tekst źródłaWu, Di, i Grzegorz Piszczek. "Standard protocol for mass photometry experiments". European Biophysics Journal 50, nr 3-4 (2.03.2021): 403–9. http://dx.doi.org/10.1007/s00249-021-01513-9.
Pełny tekst źródłaLombardo, Linda, Patrick François, Piercarlo Bonifacio, Elisabetta Caffau, Aroa del Mar Matas Pinto, Corinne Charbonnel, Georges Meynet, Lorenzo Monaco, Gabriele Cescutti i Alessio Mucciarelli. "Young giants of intermediate mass". Astronomy & Astrophysics 656 (grudzień 2021): A155. http://dx.doi.org/10.1051/0004-6361/202141408.
Pełny tekst źródłaInnis, John, i Denis Coates. "NEW CMOS PHOTOMETRY AND ARCHIVAL PHOTOGRAPHIC OBSERVATIONS OF THE W UMA STAR V752 CEN: EXTENDING THE O-C RECORD OF PERIOD CHANGES". Open European Journal on Variable stars, nr 224 (2022): 1–18. http://dx.doi.org/10.5817/oejv2022-0224.
Pełny tekst źródłaRozprawy doktorskie na temat "Mass photometry"
Steele, Iain A. "Photometry and spectroscopy of low mass stars and brown dwarfs". Thesis, University of Leicester, 1994. http://hdl.handle.net/2381/35798.
Pełny tekst źródłaScandariato, Gaetano. "The Initial Mass Function of the Orion Nebula Cluster from Near-Infrared Photometry". Doctoral thesis, Università di Catania, 2012. http://hdl.handle.net/10761/1027.
Pełny tekst źródłaVika, Marina. "Supermassive black holes : the local supermassive black hole mass function". Thesis, University of St Andrews, 2012. http://hdl.handle.net/10023/2553.
Pełny tekst źródłaKrawchuk, Curtis A. P. "The determination of metallicity and temperature of low-mass stars using broad-band photometry". Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1997. http://www.collectionscanada.ca/obj/s4/f2/dsk2/tape15/PQDD_0035/MQ27361.pdf.
Pełny tekst źródłaKing, Robert R. "Low-mass stars and brown dwarfs : optical/infrared photometry and spectroscopy of low-mass stars and brown dwarfs in the Field and Young Clusters". Thesis, University of Exeter, 2009. http://hdl.handle.net/10036/97095.
Pełny tekst źródłaPalmese, A., O. Lahav, M. Banerji, D. Gruen, S. Jouvel, P. Melchior, J. Aleksić i in. "Comparing Dark Energy Survey and HST–CLASH observations of the galaxy cluster RXC J2248.7−4431: implications for stellar mass versus dark matter". OXFORD UNIV PRESS, 2016. http://hdl.handle.net/10150/622739.
Pełny tekst źródłaGarcia, E. Victor, Thayne Currie, Olivier Guyon, Keivan G. Stassun, Nemanja Jovanovic, Julien Lozi, Tomoyuki Kudo i in. "SCExAO AND GPI Y JH BAND PHOTOMETRY AND INTEGRAL FIELD SPECTROSCOPY OF THE YOUNG BROWN DWARF COMPANION TO HD 1160". IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/623097.
Pełny tekst źródłaPagotto, Ilaria. "Mass determination of supermassive black holes in nearby galaxies". Doctoral thesis, Università degli studi di Padova, 2018. http://hdl.handle.net/11577/3427292.
Pełny tekst źródłaQuesto lavoro di tesi è dedicato alla misura della massa dei buchi neri supermassicci (SBH) che si celano al centro delle galassie quiescenti vicine. Aumentare il campione di SBH di massa nota permette di studiarne le relazioni con le altre proprietà delle galassie per poterne investigare l'evoluzione congiunta. Nuovi limiti stringenti sulla massa del SBH di 7 galassie sono stati fissati dalla misura della larghezza delle righe nebulari del gas ionizzato in spettri presi con l'Hubble Space Telescope (HST) entro aperture di dimensioni inferiori al secondo d'arco. La dispersione di velocità delle stelle è stata misurata con spettri a fenditura lunga presi da terra e il raggio efficace è stato ricavato dalla decomposizione fotometrica di immagini della Sloan Digital Sky Survey. Questi limiti di massa si dispongono parallelamente e al di sopra della relazione tra la massa del SBH e la dispersione di velocità delle stelle e non dipendono dalla morfologia o dalla distanza delle galassie. Questo suggerisce che il potenziale gravitazionale nei nuclei galattici è ben tracciato dalla larghezza delle righe di emissione se il gas si concentra verso il centro. Il numero delle galassie con un limite sulla massa del SBH ricavato dalla larghezza delle righe di emissione sale così a 114 oggetti. Queste galassie sono state ulteriormente analizzate includendo nel modello dinamico il contributo della massa stellare per ottenere limiti ancora più stringenti sulla massa del SBH. A tale scopo la brillanza superficiale misurata da immagini HST e il rapporto massa-luminosità tipico di una popolazione stellare vecchia e ricca in metalli sono stati usati per 100 galassie vicine (D<100 Mpc) e con un'ampia varietà di morfologie (E-Sc) e dispersioni di velocità (58-419 km/s). La forma dei profili delle righe di emissione e dell'andamento radiale del loro flusso sono stati studiati per escludere che le forze non gravitazionali giocassero un ruolo rilevante nella stima della massa del SBH. Il contributo stellare è maggiore per galassie con bassa dispersione di velocità, anche per la presenza di un ammasso/disco stellare nucleare, e trascurabile per le ellittiche. Esso dipende dalle dimensioni dell'apertura ma non dalla distanza della galassia. I nuovi limiti di massa si dispongono parallelamente alla relazione tra la massa del SBH e la dispersione di velocità ed eccedono il valore predetto dalla medesima solo di un fattore 1.7. Questo è un risultato notevole visto che il modello dinamico si basa su una distribuzione e cinematica del gas non spazialmente risolte. Infine, sono state ottenute nuove misure di dispersione di velocità stellare nel nucleo di 28 galassie. Gli spettri HST ottenuti con il reticolo G750M sono stati interpolati con modelli di popolazioni stellari e varie righe di emissione gaussiane, vincolando la popolazione stellare nel nucleo delle galassie grazie a spettri presi con il reticolo G430L. Queste misure permettono di porre dei forti vincoli sulla massa del SBH come mostrano i casi di NGC 4435 e NGC 4459. Si tratta di due galassie lenticolari caratterizzate da valori simili di dispersione di velocità stellare ma con masse di SBH molto diverse. In particolare, quella di NGC 4435 è molto più bassa rispetto a quanto predetto dalla relazione tra la massa del SBH e la dispersione di velocità stellare. Grazie a modelli dinamici stellari assisimmetrici è stata riprodotta la cinematica ottenuta da spettroscopia a campo integrale usando immagini HST e adottando come massa del SBH quella predetta dalla relazione con la dispersione di velocità. Questi modelli permettono di predire il valore centrale di dispersione di velocità e di confrontarlo con il valore osservato. Mentre per NGC 4459 il valore teorico e quello osservato sono in accordo, il valore misurato per NGC 4435 è molto più basso rispetto che a quello del modello dinamico indicando che la galassia ospita un SBH meno massiccio del normale.
Randriamampandry, Solohery Mampionona. "Stellar masses of star forming galaxies in clusters". University of the Western Cape, 2010. http://hdl.handle.net/11394/3028.
Pełny tekst źródłaWe determine the stellar mass of star forming galaxies in the X-ray luminous cluster MS 0451.6-0305 at z ∼ 0.54. The stellar masses are estimated from fitting model spectral energy distributions (SEDs) to deep, optical UBRIz observations obtained from WIYN 3.5m telescope and public NIR K-band image from Palomar Observatory telescope. The model SEDs are based on the stellar population synthesis (SPS) model of Bruzual & Charlot (2003) and Conroy et al. (2009) that span a wide range of age, star formation history, Initial Mass Function (IMF), metallicity and dust content. We measure stellar masses for galaxies down to M∗∼2×10⁸M(.) We find a tight correlation between stellar masses derived from the two SPSs. We compare the derived stellar masses to the dynamical masses for a set of 25 star forming galaxies. The dynamical masses are derived from high resolution, spectroscopic observations of emission lines from the DEIMOS spectrograph on the Keck telescope. A strong correlation is seen between the dynamical and stellar mass for the galaxies; and the star forming galaxies show fairly constant ratio between stellar and dynamical mass. When comparing to the field sample of Guzm ́an et al. (2003) of luminous compact blue galaxies, we see an excess of low mass galaxies in the cluster.
South Africa
Czanik, Robert Johann. "An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik". Thesis, North-West University, 2013. http://hdl.handle.net/10394/9102.
Pełny tekst źródłaThesis (MSc (Space Physics))--North-West University, Potchefstroom Campus, 2013
Książki na temat "Mass photometry"
Photodetector development for the wheel abrasion experiment on the sojourner microrover of the Mars Pathfinder mission. [Washington, D.C: National Aeronautics and Space Administration, 1997.
Znajdź pełny tekst źródłaCzęści książek na temat "Mass photometry"
Bacon, R. "Mass-to-light ratio of elliptical galaxies". W New Aspects of Galaxy Photometry, 315–18. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/bfb0030967.
Pełny tekst źródłaDuval, M. F., i G. Monnet. "Mass to luminosity ratio of bars in spiral galaxies". W New Aspects of Galaxy Photometry, 323–24. Berlin, Heidelberg: Springer Berlin Heidelberg, 1985. http://dx.doi.org/10.1007/bfb0030970.
Pełny tekst źródłaHéraudeau, Ph, F. Simien i G. A. Mamon. "Mass Models from Near-Infrared Surface Photometry". W Spiral Galaxies in the Near-IR, 235–39. Berlin, Heidelberg: Springer Berlin Heidelberg, 1996. http://dx.doi.org/10.1007/978-3-540-49739-4_35.
Pełny tekst źródłaKent, S. "Photometry and Mass Modeling of Spiral Galaxies". W Nearly Normal Galaxies, 81–89. New York, NY: Springer New York, 1987. http://dx.doi.org/10.1007/978-1-4612-4762-3_11.
Pełny tekst źródłavon Hippel, T., G. Gilmore i D. H. P. Jones. "HST Photometry of Low-Mass Stars in Open Clusters". W The Bottom of the Main Sequence — And Beyond, 201–4. Berlin, Heidelberg: Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-540-49217-7_30.
Pełny tekst źródłaMalkov, Oleg. "Unresolved Binaries and the Initial Mass Function". W Census of the Galaxy: Challenges for Photometry and Spectrometry with GAIA, 129–32. Dordrecht: Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-010-0361-2_20.
Pełny tekst źródłaSmith, Myron A., i Lin Huang. "NRP Mode Typing for 53 Persei: Results From Voyager Photometry". W Pulsation, Rotation and Mass Loss in Early-Type Stars, 37–38. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1030-3_12.
Pełny tekst źródłaÁbrahám, P., Ch Leinert, D. Lemke, A. Burkert i Th Henning. "Far-Infrared Photometry of Circumstellar Matter Around Intermediate Mass Stars". W Astrophysics and Space Science, 45–51. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5076-7_6.
Pełny tekst źródłaJiménez-Esteban, F., D. Engels, P. García-Lario i L. Agudo-Mérida. "Identification and NIR Photometry of the Arecibo Sample of OH/IR Stars". W Mass-Losing Pulsating Stars and their Circumstellar Matter, 223–24. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_45.
Pełny tekst źródłaFabregat, J., J. M. Torrejón, P. Reig i G. Bernabeu. "Simultaneous uvbyβ Photometry and Hα Spectroscopy of Be Stars in Open Clusters". W Pulsation, Rotation and Mass Loss in Early-Type Stars, 309–10. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1030-3_84.
Pełny tekst źródłaStreszczenia konferencji na temat "Mass photometry"
Seleznev, A. F., i A. A. Malofeeva. "A search of unresolved binaries in open clusters by the photometry data in visible and infrared". W ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.194.
Pełny tekst źródłaDemianenko, M., K. Grishin, V. Toptun, I. Chilingarian, I. Katkov, V. Goradzhanov i I. Kuzmin. "Optical light curves of light-weight supermassive black holes produced by the Zwicky Transient Facility Forced Photometry Service". W ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.144.
Pełny tekst źródłaNorthrop, William F., Darrick Zarling i Xuesong Li. "Considerations in Using Photometer Instruments for Measuring Total Particulate Matter Mass Concentration in Diesel Engine Exhaust". W ASME 2017 Internal Combustion Engine Division Fall Technical Conference. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/icef2017-3640.
Pełny tekst źródłaGontcharov, G., A. Mosenkov, M. Khovritchev, V. Il’in, A. Marchuk, S. Savchenko, A. Smirnov i P. Usachev. "The properties of Galactic globular clusters from Gaia EDR3 and other data compared with theoretical isochrones". W ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.182.
Pełny tekst źródłaBruce, Sally. "The NIST Quality System for Measurement Services: A look at its Past Decade and a Gaze towards its Future". W NCSL International Workshop & Symposium. NCSL International, 2013. http://dx.doi.org/10.51843/wsproceedings.2013.38.
Pełny tekst źródłavan Rijswick, Mathieu H. "Photometry maps to characterize incandescent and halogen lamps". W International Symposium on Optical Science and Technology, redaktor C. Benjamin Wooley. SPIE, 2002. http://dx.doi.org/10.1117/12.479657.
Pełny tekst źródłaAbahamid, A., M. Sarazin i G. Lombardi. "Photometric study of the Paranal observatory using MASS database". W SPIE Astronomical Telescopes + Instrumentation, redaktorzy Suzanne K. Ramsay, Ian S. McLean i Hideki Takami. SPIE, 2014. http://dx.doi.org/10.1117/12.2066652.
Pełny tekst źródłaIkehata, Satoshi. "Scalable, Detailed and Mask-Free Universal Photometric Stereo". W 2023 IEEE/CVF Conference on Computer Vision and Pattern Recognition (CVPR). IEEE, 2023. http://dx.doi.org/10.1109/cvpr52729.2023.01268.
Pełny tekst źródłaChatterjee, Avishek, i Venu Madhav Govindu. "Photometric refinement of depth maps for multi-albedo objects". W 2015 IEEE Conference on Computer Vision and Pattern Recognition (CVPR). IEEE, 2015. http://dx.doi.org/10.1109/cvpr.2015.7298695.
Pełny tekst źródłaQi, Haiyang, Sumei Liu, Sunqiang Pan, Pengbing Hu i Chonghui Chen. "Study on calibration of mask protective effect detector of mask based on precise photometer". W Optics in Health Care and Biomedical Optics XI, redaktorzy Qingming Luo, Xingde Li, Ying Gu i Dan Zhu. SPIE, 2021. http://dx.doi.org/10.1117/12.2600681.
Pełny tekst źródłaRaporty organizacyjne na temat "Mass photometry"
Sedlacek, Arthur, i Robert Jackson. Single-Particle Soot Photometer (SP2) Black Carbon Number and Mass Concentrations. Office of Scientific and Technical Information (OSTI), kwiecień 2024. http://dx.doi.org/10.2172/2341496.
Pełny tekst źródłaOrtiz, M. Growing Self-Organizing Maps as Predictors for Photometric Redshift. Office of Scientific and Technical Information (OSTI), sierpień 2019. http://dx.doi.org/10.2172/1557954.
Pełny tekst źródłaMayer, B. P., A. M. Williams, R. N. Leif i A. K. Vu. Extraction of Phosphonic Acids from Urine Samples and Analysis by Gas Chromatography with Detection by Mass Spectrometryand Flame Photometric Detection. Office of Scientific and Technical Information (OSTI), grudzień 2013. http://dx.doi.org/10.2172/1116967.
Pełny tekst źródłaLongworth, Terri L., John M. Baranoski i Kwok Y. Ong. Domestic Preparedness Program: Evaluation of the Agilent Gas Chromatograph - Flame Photometric Detector/Mass Selective Detector (GC-FPD/MSD) System Against Chemical Warfare Agents Summary Report. Fort Belvoir, VA: Defense Technical Information Center, maj 2003. http://dx.doi.org/10.21236/ada416884.
Pełny tekst źródłaAmirav, Aviv, i Steven Lehotay. Fast Analysis of Pesticide Residues in Agricultural Products. United States Department of Agriculture, listopad 2002. http://dx.doi.org/10.32747/2002.7695851.bard.
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