Poster Presentations

2017 ◽  
Vol 14 (S339) ◽  
pp. 281-282

49 posters were displayed at IAU S339. The display space was adequate to allow all to be on show throughout the conference.Poster presenters were given the option of condensing the message(s) of their posters into written summaries and/or depositing a pdf of the original poster for inclusion in the on-line version of the Proceedings. Half of the poster authors responded; 12 chose to send written summaries, 9 submitted just their original pdfs, and 4 elected to send both. Workshop 1 also converted some catalogue material into an on-line poster. This Section contains the contributions that were submitted as written summaries, arranged in alphabetical order of lead author.Near-Infrared Observations of OGLE Classical and Type II Cepheid Variables in the LMC ………. 283A. Bhardwaj, L. M. Macri, S. M. Kanbur, C-C. Ngeow and H. P. SinghMultiwavelength Light-Curve Analysis of Cepheid Variables ………. 287A. Bhardwaj, S. M. Kanbur, M. Marconi, H. P. Singh, M. Rejkuba and C-C. NgeowSymbiotic Stars in the Local Group of Galaxies: POINT-AGAPE Catalogue Revisited ………. 291K. Drozd, J. Mikołajewska, M. Darnley, K. Iłkiewicz, N. Caldwell and M. SharaDetection of Sectoral Modes in the Eclipsing Binary KIC 4851217………. 295M. Fedurco, Š. Parimucha & P. GajdošKepler-410Ab and Transit Timing Variations ………. 299P. Gajdoš, Š. Parimucha and M. FedurcoSparse Spatio-Temporal Imaging of Radio Transients ………. 303J. Girard, M. Jiang, J-L. Starck and S. CorbelTesting the SALT High-Resolution Spectrograph for Pulsation Studies of roAp Stars ………. 307D. Holdsworth and D. KurtzProbing Convective Mixing in Stellar Interiors with α Centauri A and B………. 308M. Joyce and B. ChaboyerHighly Luminous SNe Associated with GRBs………. 309D. KannSearching for Pulsating Stars Using Clustering Algorithms………. 310R. Kgoadi, I. B. Whittingham and C. A. EngelbrechtPhase-resolved Spectroscopy and Photometry of the Eclipsing Polar UZ Fornacis 314Z. N. Khangale, S. B. Potter and P. A. WoudtMeteor Sky in Time-Domain Astronomy………. 318S. V. KolomiyetsFirst Results from Project SUNBIRD: Supernovæ UNmasked By Infra-Red Detection………. 322E. C. Kool, S. D. Ryder, E. Kankare, T. Reynolds, S. Mattila, M. Pérez-Torres and R. McDermidThe X-Ray Spectrum of the X-Ray Binary 4U 1728-34, observed with Suzaku ………. 323Y. Lei, H. Zhang, H. Yuan and Y. ZhangStatistical Research into Correlation between Solar Filaments and Flare Activities………. 327G. LinA CoRoT view of the ζ Aur binary HR 6902………. 329C. Maceroni, J. Montalbán, R. Da Silva, T. Semaan, B. Mosser, M. Rainer, E. Poretti and E. GriffinSearching for Long-Period Binary Central Stars of Planetary Nebulæ with SALT HRS………. 330B. Miszalski, R. Manick, J. Mikołajewska, K. Iłkiewicz, D. Kamath and H. Van WinckelCompanion(s) of the Eclipsing Binary KIC 3832716………. 331Š. Parimucha, M. Fedurco and P. GajdošEvaluating the Fraction of Obscured Supernovæ in Luminous Infrared Galaxies with Adaptive Optics Surveys………. 335T. Reynolds, S. Mattila, E. Kool, E. Kankare, S. Ryder and M. A. Pérez-TorresDetecting AGB stars in LG Dwarf Galaxies for Understanding Galaxy Formation and Evolution………. 336E. Saremi, A. Javadi, J. van Loon, H. Khosroshahi and M. TorkiAccurate Photometry with Digitized Photographic Plates of the Moscow Collection………. 340K. V. Sokolovsky D. M. Kolesnikova, N. N. Samus, S. V. Antipin and A.A. BelinskiThe All-Sky Automated Search for Supernovæ Going Global………. 344M. Stritzinger and the ASAS-SN TeamStellar Parameterisation using KPCA and SVM………. 345H. Yuan, Y. Zhang, Y., Yiqiao Dong, Z. Bai, G. Li, W. Zhang, H. Zhang and Y. ZhaoΔa Photometric Survey of the Small Magellanic Cloud………. 349M. Zejda, E. Paunzen and Z. MikulášekDesign, Build and Test of the VOEvent Network for the SVOM Chinese Ground Segment………. 353M. Zhang, M. Huang and C. Wu

1972 ◽  
Vol 11 (03) ◽  
pp. 152-162 ◽  
Author(s):  
P. GAYNON ◽  
R. L. WONG

With the objective of providing easier access to pathology specimens, slides and kodachromes with linkage to x-ray and the remainder of the patient’s medical records, an automated natural language parsing routine, based on dictionary look-up, was written for Surgical Pathology document-pairs, each consisting of a Request for Examination (authored by clinicians) and its corresponding report (authored by pathologists). These documents were input to the system in free-text English without manual editing or coding.Two types of indices were prepared. The first was an »inverted« file, available for on-line retrieval, for display of the content of the document-pairs, frequency counts of cases or listing of cases in table format. Retrievable items are patient’s and specimen’s identification data, date of operation, name of clinician and pathologist, etc. The English content of the operative procedure, clinical findings and pathologic diagnoses can be retrieved through logical combination of key words. The second type of index was a catalog. Three catalog files — »operation«, »clinical«, and »pathology« — were prepared by alphabetization of lines formed by the rotation of phrases, headed by keywords. These keywords were automatically selected and standardized by the parsing routine and the phrases were extracted from each sentence of each input document. Over 2,500 document-pairs have been entered and are currently being utilized for purpose of medical education.


2018 ◽  
Vol 619 ◽  
pp. A138
Author(s):  
V. Perdelwitz ◽  
S. Czesla ◽  
J. Robrade ◽  
T. Pribulla ◽  
J. H. M. M. Schmitt

Context.Close binary systems provide an excellent tool for determining stellar parameters such as radii and masses with a high degree of precision. Due to the high rotational velocities, most of these systems exhibit strong signs of magnetic activity, postulated to be the underlying reason for radius inflation in many of the components. Aims.We extend the sample of low-mass binary systems with well-known X-ray properties. Methods.We analyze data from a singular XMM-Newton pointing of the close, low-mass eclipsing binary system BX Tri. The UV light curve was modeled with the eclipsing binary modeling tool PHOEBE and data acquired with the EPIC cameras was analyzed to search for hints of orbital modulation. Results.We find clear evidence of orbital modulation in the UV light curve and show that PHOEBE is fully capable of modeling data within this wavelength range. Comparison to a theoretical flux prediction based on PHOENIX models shows that the majority of UV emission is of photospheric origin. While the X-ray light curve does exhibit strong variations, the signal-to-noise ratio of the observation is insufficient for a clear detection of signs of orbital modulation. There is evidence of a Neupert-like correlation between UV and X-ray data.


2012 ◽  
Vol 746 (1) ◽  
pp. L10 ◽  
Author(s):  
Joshua C. Dolence ◽  
Charles F. Gammie ◽  
Hotaka Shiokawa ◽  
Scott C. Noble

2020 ◽  
Vol 501 (2) ◽  
pp. 2305-2315
Author(s):  
Alice Zurlo ◽  
Lucas A Cieza ◽  
Megan Ansdell ◽  
Valentin Christiaens ◽  
Sebastián Pérez ◽  
...  

ABSTRACT We present results from a near-infrared (NIR) adaptive optics (AO) survey of pre-main-sequence stars in the Lupus molecular cloud with NACO at the Very Large Telescope (VLT) to identify (sub)stellar companions down to ∼20-au separation and investigate the effects of multiplicity on circumstellar disc properties. We observe for the first time in the NIR with AO a total of 47 targets and complement our observations with archival data for another 58 objects previously observed with the same instrument. All 105 targets have millimetre Atacama Large Millimetre/sub-millimetre Array (ALMA) data available, which provide constraints on disc masses and sizes. We identify a total of 13 multiple systems, including 11 doubles and 2 triples. In agreement with previous studies, we find that the most massive (Mdust > 50 M⊕) and largest (Rdust > 70 au) discs are only seen around stars lacking visual companions (with separations of 20–4800 au) and that primaries tend to host more massive discs than secondaries. However, as recently shown in a very similar study of >200 PMS stars in the Ophiuchus molecular cloud, the distributions of disc masses and sizes are similar for single and multiple systems for Mdust < 50 M⊕ and radii Rdust < 70 au. Such discs correspond to ∼80–90 per cent of the sample. This result can be seen in the combined sample of Lupus and Ophiuchus objects, which now includes more than 300 targets with ALMA imaging and NIR AO data, and implies that stellar companions with separations >20 au mostly affect discs in the upper 10${{\ \rm per\ cent}}$ of the disc mass and size distributions.


Author(s):  
L. V. Gramajo ◽  
T. Palma ◽  
D. Minniti ◽  
R. K. Saito ◽  
J. J. Clariá ◽  
...  

Abstract We present the first results obtained from an extensive study of eclipsing binary (EB) system candidates recently detected in the VISTA Variables in the Vía Láctea (VVV) near-infrared (NIR) Survey. We analyse the VVV tile d040 in the southern part of the Galactic disc wherein the interstellar reddening is comparatively low, which makes it possible to detect hundreds of new EB candidates. We present here the light curves and the determination of the geometric and physical parameters of the best candidates found in this ‘NIR window’, including 37 contact, 50 detached, and 13 semi-detached EB systems. We infer that the studied systems have an average of the $K_s$ amplitudes of $0.8$ mag and a median period of 1.22 days where, in general, contact binaries have shorter periods. Using the ‘Physics Of Eclipsing Binaries’ (PHOEBE) interactive interface, which is based on the Wilson and Devinney code, we find that the studied systems have low eccentricities. The studied EBs present mean values of about 5 700 and 4 900 K for the $T_1$ and $T_2$ components, respectively. The mean mass ratio (q) for the contact EB stars is $\sim$ 0.44. This new galactic disk sample is a first look at the massive study of NIR EB systems.


2021 ◽  
Vol 3 (2) ◽  
Author(s):  
Ibrahim Shaik ◽  
S. K. Begum ◽  
P. V. Nagamani ◽  
Narayan Kayet

AbstractThe study demonstrates a methodology for mapping various hematite ore classes based on their reflectance and absorption spectra, using Hyperion satellite imagery. Substantial validation is carried out, using the spectral feature fitting technique, with the field spectra measured over the Bailadila hill range in Chhattisgarh State in India. The results of the study showed a good correlation between the concentration of iron oxide with the depth of the near-infrared absorption feature (R2 = 0.843) and the width of the near-infrared absorption feature (R2 = 0.812) through different empirical models, with a root-mean-square error (RMSE) between < 0.317 and < 0.409. The overall accuracy of the study is 88.2% with a Kappa coefficient value of 0.81. Geochemical analysis and X-ray fluorescence (XRF) of field ore samples are performed to ensure different classes of hematite ore minerals. Results showed a high content of Fe > 60 wt% in most of the hematite ore samples, except banded hematite quartzite (BHQ) (< 47 wt%).


2021 ◽  
Vol 127 (4) ◽  
Author(s):  
S. Skruszewicz ◽  
S. Fuchs ◽  
J. J. Abel ◽  
J. Nathanael ◽  
J. Reinhard ◽  
...  

AbstractWe present an overview of recent results on optical coherence tomography with the use of extreme ultraviolet and soft X-ray radiation (XCT). XCT is a cross-sectional imaging method that has emerged as a derivative of optical coherence tomography (OCT). In contrast to OCT, which typically uses near-infrared light, XCT utilizes broad bandwidth extreme ultraviolet (XUV) and soft X-ray (SXR) radiation (Fuchs et al in Sci Rep 6:20658, 2016). As in OCT, XCT’s axial resolution only scales with the coherence length of the light source. Thus, an axial resolution down to the nanometer range can be achieved. This is an improvement of up to three orders of magnitude in comparison to OCT. XCT measures the reflected spectrum in a common-path interferometric setup to retrieve the axial structure of nanometer-sized samples. The technique has been demonstrated with broad bandwidth XUV/SXR radiation from synchrotron facilities and recently with compact laboratory-based laser-driven sources. Axial resolutions down to 2.2 nm have been achieved experimentally. XCT has potential applications in three-dimensional imaging of silicon-based semiconductors, lithography masks, and layered structures like XUV mirrors and solar cells.


2021 ◽  
pp. 096703352098235
Author(s):  
Tomomi Takaku ◽  
Yusuke Hattori ◽  
Tetsuo Sasaki ◽  
Tomoaki Sakamoto ◽  
Makoto Otsuka

The effect of grinding on the pharmaceutical properties of matrix tablets consisting of ground glutinous rice starch (GRS) and theophylline (TH) was predicted by near infrared (NIR) spectroscopy. Ground GRS samples were prepared by grinding GRS in a planetary ball mill for 0-120 min, measured by X-ray diffractometry (XRD) and NIR, and then evaluated for crystallinity (%XRD) based on XRD profiles. Tablets containing TH (5 w/w%), ground GRS (94 w/w%), and magnesium stearate (1 w/w%) were formed by compression. Gel-forming and drug-release processes of the tablets were measured using a dissolution instrument with X-ray computed tomography (XCT). Swelling ratio (SWE) and mean drug-release time (MDT) were evaluated based on XCT and drug-release profiles, respectively. Calibration models for predicting percent %XRD, MDT, and SWE were constructed based on the NIR of ground GRS using partial least-squares. The results indicated the possibility of controlling the pharmaceutical properties of matrix tablets by altering the pre-gelatinization of GRS based on changes in their NIR spectra during the milling process.


2021 ◽  
Vol 503 (1) ◽  
pp. 292-311
Author(s):  
Zeinab Khorrami ◽  
Maud Langlois ◽  
Paul C Clark ◽  
Farrokh Vakili ◽  
Anne S M Buckner ◽  
...  

ABSTRACT We present the sharpest and deepest near-infrared photometric analysis of the core of R136, a newly formed massive star cluster at the centre of the 30 Doradus star-forming region in the Large Magellanic Cloud. We used the extreme adaptive optics of the SPHERE focal instrument implemented on the ESO Very Large Telescope and operated in its IRDIS imaging mode for the second time with longer exposure time in the H and K filters. Our aim was to (i) increase the number of resolved sources in the core of R136, and (ii) to compare with the first epoch to classify the properties of the detected common sources between the two epochs. Within the field of view (FOV) of 10.8″ × 12.1″ ($2.7\,\text {pc}\times 3.0\, \text {pc}$), we detected 1499 sources in both H and K filters, for which 76 per cent of these sources have visual companions closer than 0.2″. The larger number of detected sources enabled us to better sample the mass function (MF). The MF slopes are estimated at ages of 1, 1.5, and 2 Myr, at different radii, and for different mass ranges. The MF slopes for the mass range of 10–300 M⊙ are about 0.3 dex steeper than the mass range of 3–300 M⊙, for the whole FOV and different radii. Comparing the JHK colours of 790 sources common in between the two epochs, 67 per cent of detected sources in the outer region (r &gt; 3″) are not consistent with evolutionary models at 1–2 Myr and with extinctions similar to the average cluster value, suggesting an origin from ongoing star formation within 30 Doradus, unrelated to R136.


2002 ◽  
Vol 16 (2) ◽  
pp. 89-98 ◽  
Author(s):  
B. J. A. Mertens ◽  
C. P. O'Donnell ◽  
D. J. O'Callaghan
Keyword(s):  

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