APOGEE Survey (@apogeesurvey) 's Twitter Profile
APOGEE Survey

@apogeesurvey

Mapping Stars in the Galaxy as part of the Sloan Digital Sky Survey @sdssurveys
#ScienceForAll

ID: 2676559771

linkhttp://www.sdss.org/sdss-surveys/apogee-2/ calendar_today24-07-2014 11:16:25

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Matthias Steinmetz (@galacticrave) 's Twitter Profile Photo

Looking forward to talk this evening under the big dinosaur at @mfnberlin about Galactic Archaeology with a Billion stars ESA Gaia APOGEE Survey Wissenschaft im Sauriersaal: Galaktische Archäologie – Ausgrabungen mit einer Milliarde Sternen museumfuernaturkunde.berlin/de/museum/vera… via @mfnberlin

José G. Fernández-Trincado (@j_g_fernandez) 's Twitter Profile Photo

I've a new accepted first author paper that I titled: "Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO) I. An updated census of APOGEE Survey N-rich Giants Across the Milky Way" - We also identified two possible Hypervelocity N-rich star (HVNS) candidates with StarHorse, but ...

I've a new accepted first author paper that I titled: "Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO)
I. An updated census of <a href="/APOGEEsurvey/">APOGEE Survey</a> N-rich Giants Across the Milky Way" - We also identified two possible Hypervelocity N-rich star (HVNS) candidates with StarHorse, but ...
Jamie Tayar (@stellartayar) 's Twitter Profile Photo

In case you missed it last week ✨ellis✨ had a lovely paper out on surface rotation in stars around the Kraft Break using TESS, Kepler and APOGEE. Things you should know include: Detecting long periods (>13 days) in TESS is very hard, even if you know where to look

In case you missed it last week <a href="/ellantonia_/">✨ellis✨</a> had a lovely paper out on surface rotation in stars around the Kraft Break using TESS, Kepler and APOGEE. Things you should know include: 
Detecting long periods (&gt;13 days) in TESS is very hard, even if you know where to look
Jamie Tayar (@stellartayar) 's Twitter Profile Photo

Looking at how rotation evolves with time is hard in this regime, but you can see it if you are careful especially with the help of spectroscopy like APOGEE Survey. We actually ended up using vsini+ Rgaia => P/sini, validated against the rotation periods we could measure for this

Looking at how rotation evolves with time is hard in this regime, but you can see it if you are careful especially with the help of spectroscopy like <a href="/APOGEEsurvey/">APOGEE Survey</a>. We actually ended up using vsini+ Rgaia =&gt; P/sini, validated against the rotation periods we could measure for this
Danny Horta (@darringtonhorta) 's Twitter Profile Photo

Paper day! In this paper we examine the chemical compositions of halo substructures identified in recent years with the wealth of large-scale stellar surveys (Gaia, APOGEE, H3, LAMOST) in order to further understand their nature. A thread 1/11 Link: ui.adsabs.harvard.edu/abs/2022arXiv2…

Danny Horta (@darringtonhorta) 's Twitter Profile Photo

Check out the paper for the full deets! Many thanks to every co-author and the APOGEE Survey ESA Gaia surveys for delivering the awesome data that enabled this study!! 11/11

Khyati Malhan (@kmalhan07) 's Twitter Profile Photo

I'm excited about my first 'single-author' paper, now accepted for publication in ApJ. I study the characteristics of the "Pontus" merger of the Milky Way using #GaiaEDR3 and APOGEE Survey data. arxiv.org/abs/2204.09058 ESA Gaia Max-Planck-Institut für Astronomie Humboldt-Stiftung International Astronomical Union (IAU) The GruberFoundation

I'm excited about my first 'single-author' paper, now accepted for publication in ApJ. I study the characteristics of the "Pontus" merger of the Milky Way using #GaiaEDR3 and <a href="/APOGEEsurvey/">APOGEE Survey</a> data. 
arxiv.org/abs/2204.09058

<a href="/ESAGaia/">ESA Gaia</a> <a href="/mpi_astro/">Max-Planck-Institut für Astronomie</a> <a href="/AvHStiftung/">Humboldt-Stiftung</a> <a href="/IAU_org/">International Astronomical Union (IAU)</a> <a href="/The_Gruber_Fdtn/">The GruberFoundation</a>
Jamie Tayar (@stellartayar) 's Twitter Profile Photo

Conveniently, with optical spectroscopy from clusters and APOGEE Survey, we can now infer empirically the location of the red giant branch bump (purple), and infer where (at what logg) the lithium (green) and [C/N] (blue) drop due to extra mixing at a particular metallicity.

Conveniently, with optical spectroscopy from clusters and <a href="/APOGEEsurvey/">APOGEE Survey</a>, we can now infer empirically the location of the red giant branch bump (purple), and infer where (at what logg) the lithium (green) and [C/N] (blue) drop due to extra mixing at a particular metallicity.
Dr. Sarah Pearson (@spacewsarah) 's Twitter Profile Photo

Lucey presents and tests a novel method to dynamically estimate the Milky Way’s bar length and pattern speed directly from orbit integration of APOGEE Survey data and ESA Gaia data. She finds a dynamical bar length of ~3.5 kpc and pattern speed of 39 km/s/kpc.

Rachael (@rareflwr41) 's Twitter Profile Photo

APOGEE in Fire Mock Catalogs from 3 Latte Galaxies go live at #AAS240. 50+ Tb of simulated Milky Way goodness in a server-side platform. 🤓 Arik from IDIES will be on hand with cool 😎 notebooks to play around that show server-side awesome. Sloan Digital Sky Surveys APOGEE Survey