Search Publications

Ionization and Star Formation in the Giant H II Region SMC-N66
DOI: 10.1088/1538-3873/ac697b Bibcode: 2022PASP..134f4301G

Kniazev, A.; Hamann, W. -R.; Sabbi, E. +8 more

The NGC 346 young stellar system and associated N66 giant H II region in the Small Magellanic Cloud are the nearest example of a massive star-forming event in a low metallicity (Z ≈ 0.2Z ) galaxy. With an age of ≲3 Myr this system provides a unique opportunity to study relationships between massive stars and their associated H II regio…

2022 Publications of the Astronomical Society of the Pacific
eHST 5
Digitization, Measurement, and Analysis of a 1905 Barnard Atlas Photographic Plate
DOI: 10.1088/1538-3873/ac87cf Bibcode: 2022PASP..134i4503G

Cerny, William; Kron, Richard G.; Martinez, Michael N. +7 more

In the second paper in this series, we improve on our previous demonstration of the ability of a commercially available graphic arts scanner and cost-effective analysis tools to produce scientifically useful scans of astronomical photographic plates. We describe a method using freely available tools to extract magnitude measurements from the star …

2022 Publications of the Astronomical Society of the Pacific
Gaia 5
Role of Topocentric Parallax in Near-Earth Object Initial Orbit Determination
DOI: 10.1088/1538-3873/ac43ca Bibcode: 2022PASP..134a5005Z

Zhai, Chengxing; Shao, Michael; Saini, Navtej S. +5 more

Near-Earth Object (NEO) initial orbit determination typically uses astrometric measurements during a close approach over a time window much shorter than the orbital period of the NEO. The initial orbit is only weakly determined with dominant uncertainties in the distance of the NEO from the Earth. Topocentric astrometric measurements allow us to e…

2022 Publications of the Astronomical Society of the Pacific
Gaia 4
Interstellar Extinction and Polarization of Stars in the Open Cluster NGC 6709
DOI: 10.1088/1538-3873/ac75c6 Bibcode: 2022PASP..134h4301T

Topasna, G. A.; Kaltcheva, N. T.; Gibson, S. D.

We present BVRI polarimetric measurements of 23 stars in the direction of the open cluster NGC 6709. Fifteen stars display wavelength-dependence of polarization which is typically due to selective extinction in the interstellar medium and could be fitted to the Serkwoski equation. Based on these stars, we obtained an average maximum degree of pola…

2022 Publications of the Astronomical Society of the Pacific
Gaia 4
Photometric and Spectroscopic Studies of the Long-Period Low-Mass-Ratio Deep-Contact Binary KN Per
DOI: 10.1088/1538-3873/ac99fd Bibcode: 2022PASP..134k4202G

Wang, Xi; Guo, Ya-Ni; Li, Kai +6 more

Photometric analysis and spectroscopic study of the long-period low-mass-ratio deep-contact binary KN Per were performed. The light curves of the BV(RI) c band were from the Ningbo Bureau of Education and Xinjiang Observatory Telescope at the Xingming Observatory. Through the analysis of the Wilson-Devinney program, KN Per was found as…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3
Astrometric Precision Tests on TESS Data
DOI: 10.1088/1538-3873/ac584a Bibcode: 2022PASP..134c5004G

Lattanzi, M.; Busonero, D.; Bucciarelli, B. +5 more

Astrometry at or below the microarcsec level with an imaging telescope assumes that the uncertainty on the location of an unresolved source can be an arbitrarily small fraction of the detector pixel, given a sufficient photon budget. This paper investigates the geometric limiting precision, in terms of CCD pixel fraction, achieved by a large set o…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3
Planet Patrol: Vetting Transiting Exoplanet Candidates with Citizen Science
DOI: 10.1088/1538-3873/ac5de0 Bibcode: 2022PASP..134d4401K

Kostov, Veselin B.; Kuchner, Marc J.; Brande, Jonathan +15 more

NASA's TESS mission yields light curves for tens of millions of stars spread across the entire sky, a data set that will be a challenge to fully exploit without help from citizen scientists. To address this, we launched a new citizen science project, called "Planet Patrol", designed to analyze TESS data on exoplanet and eclipsing binary candidates…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3
A New Period Determination Method for Periodic Variable Stars
DOI: 10.1088/1538-3873/ac9e1b Bibcode: 2022PASP..134k4507X

Li, Bin; Li, Xu-Zhi; Zhu, Qing-Feng +4 more

Variable stars play a key role in understanding the Milky Way and the universe. The era of astronomical big data presents new challenges for quick identification of interesting and important variable stars. Accurately estimating the periods is the most important step to distinguish different types of variable stars. Here, we propose a new method o…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3
Relative Astrometry in an Annular Field
DOI: 10.1088/1538-3873/ac50a1 Bibcode: 2022PASP..134c5001G

Lattanzi, M. G.; Busonero, D.; Butkevich, A. G. +4 more

Background. Relative astrometry at or below the microarcsec level with a 1 m class space telescope has been repeatedly proposed as a tool for exo-planet detection and characterization, as well as for several topics at the forefront of Astrophysics and Fundamental Physics. Aim. This paper investigates the potential benefits of an instrument concept…

2022 Publications of the Astronomical Society of the Pacific
Gaia 2
Global Extinction: Gemini North and South GMOS Combined Photometry Relative to the Gaia Catalog, and Long-term Atmospheric Change
DOI: 10.1088/1538-3873/acac52 Bibcode: 2022PASP..134l5003S

Steinbring, Eric

Effects of long-term atmospheric change were looked for in photometry employing Gemini North and South twin Multi-Object Spectrograph (GMOS-N and GMOS-S) archival data. The whole GMOS imaging database, beginning from 2003, was compared against the all-sky Gaia object catalog, yielding ~106 Sloan $r^{\prime} $ -filter samples, ending in …

2022 Publications of the Astronomical Society of the Pacific
Gaia 1