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ShareScore release 0.9.0
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4 results for “Pan-STARRS”
BASE-9 binarity and stellar masses from Gaia DR3, 2MASS, and Pan-STARRS data for six open clusters: NGC 2168, NGC 7789, NGC 6819, NGC 2682, NGC 188, NGC 6791
<h2>Data sets as described in "Goodbye to Chi-by-Eye: A Bayesian Analysis of Photometric Binaries in Six Open Clusters", Childs et al. 2023 <a href="https://ui.adsabs.harvard.edu/abs/2023arXiv230816282C/abstract">https://ui.adsabs.harvard.edu/abs/2023arXiv230816282C/abstract</a></h2>
Gaia data, Pan-STARRS photometry, and stream selection masks for the region around the GD-1 stream
<p>This file contains:</p> <ul> <li>relevant columns from Gaia DR2</li> <li>Pan-STARRS (PS1) photometry (grizy)</li> <li>de-reddened PS1 photometry (g0, r0, etc.)</li> <li>binary masks to apply to select out stars that pass our proper motion and color-magnitude diagram selection (pm_mask, gi_cmd_mask)</li> <li>a binary mask to apply to select out stars in the stream track defined in <a href="https://arxiv.org/abs/1805.00425">Price-Whelan & Bonaca (2018) </a>(stream_track_mask)</li> <li>GD-1 positional coordinates (phi1, phi2)</li> <li>Proper motions in the GD-1 coordinate system (pm_phi1_cosphi2, pm_phi2)</li> <li>Proper motions in the GD-1 coordinate system, corrected for solar reflex motion (pm_phi1_cosphi2_no_reflex, pm_phi2_no_reflex)</li> </ul> <p>To select out probable members of the GD-1 stream in, e.g., Python, use:</p> <pre><code class="language-python">from astropy.table import Table tbl = Table.read('gd1-with-masks.fits') tbl = tbl[tbl['pm_mask'] & tbl['gi_cmd_mask']]</code></pre> <p>To select out only stars within the stream track identified in <a href="https://arxiv.org/abs/1805.00425">Price-Whelan & Bonaca (2018)</a>, do:</p> <pre><code class="language-python">from astropy.table import Table tbl = Table.read('gd1-with-masks.fits') tbl = tbl[tbl['pm_mask'] & tbl['gi_cmd_mask'] & tbl['stream_track_mask']</code></pre> <pre> </pre>
Pan-STARRS DR1 Catalog ConeSearch
Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1). The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera (GPC1; see PS1 GPC1 camera) to image the sky in five broadband filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.The Pan-STARRS Data Release 1 Object Catalog v3 exists in the MAST holdings and is thus available through a cone search.All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
Pan-STARRS DR1 "Best" Catalog ConeSearch
Pan-STARRS is a system for wide-field astronomical imaging developed and operated by the Institute for Astronomy at the University of Hawaii. Pan-STARRS1 (PS1) is the first part of Pan-STARRS to be completed and is the basis for Data Release 1 (DR1). The PS1 survey used a 1.8 meter telescope and its 1.4 Gigapixel camera (GPC1; see PS1 GPC1 camera) to image the sky in five broadband filters (g, r, i, z, y). The PS1 Science Consortium funded the operation of the Pan-STARRS1 telescope, situated at Haleakala Observatories near the summit of Haleakala in Hawaii, for the purposes of astronomical research. The PS1 consortium is made up of astronomers and engineers from 14 institutions from six countries.The Pan-STARRS Data Release 1 Object Catalog "Best" filtered exists in the MAST holdings and is thus available through a cone search. The filtered data is a ~2billion row subset based on an object having more than 2 detections.All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
ScienceDex guides
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