Search Publications

Photometric and kinematic studies of open cluster NGC 1027
DOI: 10.1007/s12036-023-09955-7 Bibcode: 2023JApA...44...61T

Sharma, Saurabh; Panwar, Neelam; Kumar, Brijesh +2 more

We present photometric and kinematic analyses of an intermediate-age open cluster NGC 1027 using UBV(RI)c

2023 Journal of Astrophysics and Astronomy
Gaia 1
Spectral and timing analysis of BeXRB eRASSU J050810.4-660653 recently discovered in the Large Magellanic Cloud (LMC)
DOI: 10.1093/mnras/stac1820 Bibcode: 2023MNRAS.518..893G

Tobrej, Mohammed; Rai, Binay; Ghising, Manoj +2 more

We have studied the Be/X-ray binary (BeXRB) pulsar eRASSU J050810.4-660653 recently discovered in the Large Magellanic Cloud (LMC). Timing and spectral features of the source have been discussed in detail using NuSTAR and XMM-Newton observations. Coherent pulsation of the source was detected at ~40.578 ± 0.001 s using NuSTAR observation. We analys…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
Parameters of SU UMa and WZ Sge-Type Dwarf Novae in Quiescent State. I. FL Psc, TY Psc and V455 And
DOI: 10.1134/S1990341323010054 Bibcode: 2023AstBu..78...25D

Shimansky, V. V.; Mitrofanova, A. A.; Dudnik, A. A. +2 more

We present the results of model analysis of the optical spectra of SU UMa and WZ Sge-type dwarf novae TY Psc, FL Psc, and V455 And. Spectroscopic observations were carried out at the SAO RAS 6-m BTA telescope in 2013. The selection criterion for the systems under study is their existence in a quiescent state with an optically thin accretion disk a…

2023 Astrophysical Bulletin
Gaia 1
LAMOST J2043+3413-a Fast Disk Precession SW Sextans Candidate in Period Gap
DOI: 10.3847/1538-3881/acdd70 Bibcode: 2023AJ....166...56L

Wang, Xiaofeng; Liu, Jiren; Sun, Yongkang +5 more

We present follow-up photometric observations and time-series analysis of a nova-like, SW Sextans-type, cataclysmic variable (CV) candidate, LAMOST J204305.95+341340.6 (hereafter J2043+3413), with a Gaia G-band magnitude of 15.30 and a distance of 990 pc, which was identified from the LAMOST spectrum. The photometric data were collected with the T…

2023 The Astronomical Journal
Gaia 1
Photometric long-term variations of dwarf novae during quiescence
DOI: 10.1093/mnras/stad2464 Bibcode: 2023MNRAS.525.3682V

Vogt, N.; Vega-Manubens, I.

Using the Catalina Sky Survey and Gaia alert data bases, we have carried out a systematic search for long-term variability of the brightness of dwarf novae in quiescence. A small, but significant portion of them revealed variability on time-scales between 2 and 14 yr which can be fitted, in some of the targets, by linear slopes of 0.14 mag yr

2023 Monthly Notices of the Royal Astronomical Society
Gaia 1
The radiometric environment for Mars limb observations by the Mars Sample Return Earth Return Orbiter
DOI: 10.1016/j.asr.2023.07.019 Bibcode: 2023AdSpR..72.4048S

Montmessin, Franck; Titov, Dmitri; Wolff, Michael J. +17 more

After launching from the martian surface via the Mars Ascent Vehicle (MAV), the MAV and the Orbiting Sample (OS) capsule containing the samples collected on Mars by the Perseverance rover are to be identified by the Narrow Angle Camera (NAC) on the Earth Return Orbiter (ERO) spacecraft in order to determine the exact orbit of the capsule before re…

2023 Advances in Space Research
MEx 1
Data processing pipeline for multiple-exposure photo-plate digital archives
DOI: 10.1093/pasj/psad038 Bibcode: 2023PASJ...75..811J

Yu, Yong; Jia, Peng; Yang, Zhimin +2 more

Photo-plates are an invaluable historical legacy that have been used for over a hundred years to capture images of celestial objects. By digitizing these photo-plates and processing the images with digital image processing methods, scientists can study celestial objects that exhibit temporal variations. Multiple-exposure photo-plates are a unique …

2023 Publications of the Astronomical Society of Japan
Gaia 1
ALMA Observations of the Extraordinary Carina Pillars: A Complementary Sample
DOI: 10.3847/1538-4357/ad021b Bibcode: 2023ApJ...958..193C

Reiter, Megan; Zapata, Luis A.; Takahashi, Satoko +3 more

We present a study of six dusty and gaseous pillars (containing the Herbig-Haro (HH) objects HH 1004 and HH 1010) and globules (that contain the HH 666, HH 900, HH 1006, and HH 1066 objects) localized in the Carina Nebula using sensitive and high-angular-resolution (~0.″3) Atacama Large Millimeter/submillimeter Array observations. This is a more e…

2023 The Astrophysical Journal
eHST 1
Spectrally dispersed kernel phase interferometry with SCExAO/CHARIS: proof of concept and calibration strategies
DOI: 10.1117/1.JATIS.9.2.028004 Bibcode: 2023JATIS...9b8004C

Martinache, Frantz; Chaushev, Alexander; Sallum, Steph +7 more

Kernel phase interferometry (KPI) is a data processing technique that allows for the detection of asymmetries (such as companions or disks) in high-Strehl images, close to and within the classical diffraction limit. We show that KPI can successfully be applied to hyperspectral image cubes generated from integral field spectrographs (IFSs). We demo…

2023 Journal of Astronomical Telescopes, Instruments, and Systems
Gaia 1
Unravelling optical and X-ray properties of the disc-dominated intermediate polar IGR J15094-6649
DOI: 10.1093/mnras/stad933 Bibcode: 2023MNRAS.521.6156J

Pandey, J. C.; Scaringi, Simone; Schwope, Axel +5 more

We present analyses of an Intermediate Polar, IGR J15094-6649, based on the archival optical data obtained from the Transiting Exoplanet Survey Satellite (TESS) and X-ray data obtained from the Suzaku, NuSTAR, and Neil Gehrels Swift Observatory (Swift). Present analysis confirms and refines the previously reported spin period of IGR J15094-6649 as…

2023 Monthly Notices of the Royal Astronomical Society
Gaia Suzaku 1