J/ApJ/914/123     Gaia DR2 and EDR3 stars with sp. follow-up     (Ibata+, 2021)

Charting the Galactic acceleration field. I. A search for stellar streams with Gaia DR2 and EDR3 with follow-up from ESPaDOnS and UVES. Ibata R., Malhan K., Martin N., Aubert D., Famaey B., Bianchini P., Monari G., Siebert A., Thomas G.F., Bellazzini M., Bonifacio P., Caffau E., Renaud F. <Astrophys. J., 914, 123 (2021)> =2021ApJ...914..123I 2021ApJ...914..123I
ADC_Keywords: Spectra, optical; Radial velocities; Associations, stellar; Proper motions; Parallaxes, trigonometric; Colors Keywords: Milky Way Galaxy ; Dark matter Abstract: We present maps of the stellar streams detected in the Gaia Data Release 2 (DR2) and Early Data Release 3 (EDR3) catalogs using the STREAMFINDER algorithm. We also report the spectroscopic follow-up of the brighter DR2 stream members obtained with the high-resolution CFHT/ESPaDOnS and VLT/UVES spectrographs as well as with the medium-resolution NTT/EFOSC2 spectrograph. Two new stellar streams that do not have a clear progenitor are detected in DR2 (named Hrid and Gunnthra), and seven are detected in EDR3 (named Gaia-6 to Gaia-12). Several candidate streams are also identified. The software also finds very long tidal tails associated with the 15 globular clusters: NGC 288, NGC 1261, NGC 1851, NGC 2298, NGC 2808, NGC 3201, M68, ωCen, NGC 5466, Palomar 5, M5, NGC 6101, M92, NGC 6397, and NGC 7089. These stellar streams will be used in subsequent contributions in this series to chart the properties of the Galactic acceleration field on ∼100pc to ∼100kpc scales. Description: To measure the radial velocities and metallicities of our Gaia DR2 sample presented in Section 2 we secured 75 hours of service-mode observation with the CFHT/ESPaDOnS instrument over five semesters between 2018 and 2020 (R=68000; wavelength range 3700-10500Å). A total of 163 stars were observed with ESPaDOnS up to the end of 2020 June. A further six nights of observation were obtained with the VLT/UVES spectrograph, in 2019 June 3 and in 2020 January 3 (R∼40000; 3730-4990Å and 5650-9460Å. We secured two six-night runs with NTT/EFOSC2 immediately before each UVES run (R∼3000; 4400-5100Å). A total of 60 stars of the stream sample have an EFOSC2 velocity measurement but no UVES velocity measurement. We complemented these velocities with measurements taken from public spectroscopic surveys. A total of 685 stars from our sample of 5960 stream candidate stars (i.e., 11.5%) end up having velocity measurements. See Section 3. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 108 5960 *The STREAMFINDER catalog of 5960 stars detected in Gaia DR2, with updated EDR3 astrometry -------------------------------------------------------------------------------- Note on table1.dat: The STREAMFINDER (Malhan & Ibata 2018MNRAS.477.4063M 2018MNRAS.477.4063M) algorithm was designed to hunt for stream-like overdensities in photometric and astrometric catalogs. See Section 2. -------------------------------------------------------------------------------- See also: III/279 : RAVE 5th data release (Kunder+, 2017) I/345 : Gaia DR2 (Gaia Collaboration, 2018) V/164 : LAMOST DR5 catalogs (Luo+, 2019) I/350 : Gaia EDR3 (Gaia Collaboration, 2020) III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020) V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020) J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009) J/ApJ/722/1373 : ω Centauri giants abundances (Johnson+, 2010) J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012) J/MNRAS/426/1137 : Radial velocities in NGC 1851 (Sollima+, 2012) J/A+A/588/A148 : NGC 6397 stars MUSE spectra (Husser+, 2016) J/ApJ/819/1 : Wide-field photometry of the GC Palomar 5 (Ibata+, 2016) J/ApJ/842/120 : Large sp. survey of Palomar 5 stellar stream (Ibata+, 2017) J/ApJ/853/86 : HST large prog. on ω Centauri. II. (Bellini+, 2018) J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018) J/MNRAS/484/2832 : Proper motions of MW globular clusters (Vasiliev, 2019) J/ApJ/901/23 : Gjoll stream stars & abund. of 4 members (Hansen+, 2020) J/A+A/645/A116 : NGC 2808, NGC 6266 & NGC 6397 GaiaDR2 sources (Kundu+, 2021) J/A+A/649/A3 : Gaia EDR3 photometric passbands (Riello+, 2021) http://www.cosmos.esa.int/gaia : Gaia home page http://www.sdss3.org/ : SDSS-III home page Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 I19 --- Gaia Gaia EDR3 star identifier 21- 31 F11.7 deg RAdeg Gaia EDR3 right ascension (J2000) 33- 43 F11.7 deg DEdeg [-81.84/84.61] Gaia EDR3 declination (J2000) 45- 50 F6.3 mas plx [-1.2/1.4] Gaia ER3 parallax 52- 58 F7.3 mas/yr pmRA [-28/24.6] Gaia EDR3 proper motion in RA, µα(*cos(δ)) 60- 66 F7.3 mas/yr pmDE [-40.5/25.2] Gaia EDR3 proper motion in DEC 68- 73 F6.3 mag Gmag0 [10.3/19.5] Gaia DR2 extinction-corrected magnitude G0 75- 79 F5.3 mag (BP-RP)0 [0.5/1.6] Gaia DR2 color (GBP-GRP)0 81- 84 F4.1 kpc dSF [1/45.6] Distance to the star estimated by STREAMFINDER 86- 93 F8.2 km/s HRV [-3838/16857]?=1000 Best heliocentric line-of-sight velocity 95- 102 F8.2 km/s e_HRV [0.02/63]?=10000 HRV uncertainty 104- 105 I2 --- r_HRV [0/13] Reference for the velocity (1) 107- 108 I2 --- Stream [1/32] A unique stream identification label; used in Figures 1-3 -------------------------------------------------------------------------------- Note (1): Heliocentric line-of-sight velocity source as follows: 0 = No measurement (5275 occurrences) 1 = APOGEE-2 (Majewski+ 2017AJ....154...94M 2017AJ....154...94M ; see III/284); 15 occurrences 2 = GALAH DR3 survey (Buder+ 2018, J/MNRAS/478/4513); 1 occurrence 3 = Gaia Radial Velocity Spectrometer (RVS) catalog; 6 occurrences 4 = LAMOST DR5 survey (Cui+ 2012RAA....12.1197C 2012RAA....12.1197C ; see V/164); 44 occurrences 5 = Radial Velocity Experiment (RAVE DR5; Kunder+ 2017, III/279); not used 6 = SDSS/Segue survey (Yanny+ 2009, J/AJ/137/4377); 135 occurrences 7 = BOSS; 86 occurrences 8 = CFHT/ESPaDOnS (this work); 155 occurrences 9 = AAT/AAOmega (from Ibata+ 2017, J/ApJ/842/120); 5 occurrences 10 = VLT/FLAMES (from Ibata+ 2017, J/ApJ/842/120); 7 occurrences 11 = VLT/UVES (from Odenkirchen+ 2009AJ....137.3378O 2009AJ....137.3378O); 6 occurrences 12 = NTT/EFOSC (this work); 44 occurrences 13 = VLT/UVES (this work); 181 occurrences -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Emmanuelle Perret [CDS] 14-Dec-2022
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