J/AJ/154/151 The solar neighborhood .XXXX. New young stars (Bartlett+, 2017)
The solar neighborhood.
XXXX. Parallax results from the CTIOPI 0.9 m program: new young stars near
the Sun.
Bartlett J.L., Lurie J.C., Riedel A., Ianna P.A., Jao W.-C., Henry T.J.,
Winters J.G., Finch C.T., Subasavage J.P.
<Astron. J., 154, 151-151 (2017)>
=2017AJ....154..151B 2017AJ....154..151B (SIMBAD/NED BibCode)
ADC_Keywords: Stars, nearby ; Stars, double and multiple ; Proper motions ;
Parallaxes, trigonometric ; Photometry, VRI ; Spectral types ;
Photometry, infrared ; Equivalent widths ; Stars, distances
Keywords: open clusters and associations: general - parallaxes -
proper motions - solar neighborhood - stars: fundamental parameters -
stars: late-type
Abstract:
As a step toward completing and characterizing the census of the solar
neighborhood, we present astrometric, photometric, and spectroscopic
observations of 32 systems observed with the Cerro Tololo Inter-American
Observatory 0.9 m and 1.5 m telescopes. Astrometry from the 0.9 m
indicates that among the 17 systems that had no previous published
trigonometric parallaxes, 14 are within 25 pc. In the full sample,
nine systems have proper motions larger than 0.5"/yr, including
2MASS J02511490-0352459, which exceeds 2.0"/yr. VRI photometry from
the 0.9 m and optical spectra from the 1.5 m indicate that the targets
have V=11-22 mag and spectral types M3.0V-L3.0V. For
2MASS J23062928-0502285 (TRAPPIST-1), we present updated astrometry
and photometric variability based on over 12 years of observations. Of
the nine binaries in the sample, two promise mass determinations in
the next decade: LHS 6167AB, an M4.5V system for which we present an
accurate parallax placing the binary at 9.7 pc, and
2MASS J23515048-2537367AB, an M8.5V system at 21.1 pc for which we
present the first evidence of an unseen, low-mass companion. Most
importantly, Na I and K I gravity indicators, Hα measurements,
long-term photometric variability, locations on the H-R diagram, and
kinematic assessments indicate that as many as 13 of the systems are
young, including candidate members of young moving groups, with ages
less than ∼120 Myr.
Description:
The CTIO/SMARTS 0.9 m telescope has a 2048x2048 Tektronix CCD camera
with 0.401"/pixel plate scale (Jao et al. 2003AJ....125..332J 2003AJ....125..332J). The
center quarter of the chip with a 6.8' square field of view is used
for both astrometric and photometric observations during CTIOPI. An
optimal filter is selected for each πtrig target and set of
reference stars in one of three bandpasses: "old" VJ and/or "new"
VJ, RKC or IKC (hereafter without the subscripts).
The Ritchey-Chretien spectrograph with a 2" slit and Loral 1200x800
CCD camera were used on the CTIO/SMARTS 1.5 m telescope to obtain optical
spectroscopy for the sample. Spectra covering the range 6000-9500 Å
with a resolution of 8.6 Å were obtained using grating #32 in first
order at a tilt of 15.1° and order-blocking filter OG570.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1.dat 143 32 Astrometric Results
table3.dat 114 32 Photometry and Spectral Types
table4.dat 74 30 Spectral Indices from the RECONS 1.5 m
Spectroscopy Program and Radial Velocities from
the Literature
table7.dat 82 15 Comparison of Trigonometric, Photometric,
and Spectroscopic Distances
table8.dat 110 6 Evaluation of Wide Common Proper Motion Pairs
table9.dat 55 15 Observations of Resolved Binaries with
Separations <1"
--------------------------------------------------------------------------------
See also:
I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)
III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)
I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)
I/337 : Gaia DR1 (Gaia Collaboration, 2016)
I/345 : Gaia DR2 (Gaia Collaboration, 2018)
J/AJ/106/773 : Mass-luminosity relation (Henry+, 1993)
J/AJ/126/2421 : 2MASS-Selected sample of ultracool dwarfs (Cruz+, 2003)
J/AJ/126/3007 : Spectroscopy of faint red NLTT dwarfs (Reid+, 2003)
J/A+A/420/183 : Spectroscopic survey in solar neighborhood
(Allende Prieto+ 2004)
J/A+A/442/211 : Spectroscopic distances of 322 NLTT stars (Scholz+, 2005)
J/AJ/129/413 : New high proper motion stars (-90<DE< -47)
(Subasavage+, 2005)
J/AJ/130/1658 : New high proper motion stars (-47<δ<00)
(Subasavage+, 2005)
J/A+A/460/695 : Search for Associations Containing Young stars
(Torres+, 2006)
J/AJ/132/866 : New M dwarfs in solar neighborhood (Riaz+, 2006)
J/AJ/132/891 : Binaries among nearby L dwarfs (Reid+, 2006)
J/AJ/133/439 : Luminosity function of M7-L8 ultracool dwarfs (Cruz+, 2007)
J/AJ/133/2898 : New proper-motion stars (-90<DE< -47) (Finch+, 2007)
J/AJ/134/252 : New nearby white dwarf systems (Subasavage+, 2007)
J/AJ/136/1290 : Ultracool dwarfs from the 2MASS (Reid+, 2008)
J/ApJ/699/649 : Young M dwarfs within 25pc. I. (Shkolnik+, 2009)
J/ApJ/705/1416 : Volume-limited sample of M7-M9.5 dwarfs <20pc
(Reiners+, 2009)
J/ApJ/723/684 : NIRSPEC ultracool dwarf radial velocity survey
(Blake+, 2010)
J/MNRAS/403/1949 : UBV(RcIc)JHK photometry of HIP nearby stars (Koen+, 2010)
J/AJ/141/21 : CCD distance estimates of SCR targets (Winters+, 2011)
J/AJ/142/10 : New proper motion stars 0.40"/yr>pm≥0.18"/yr (Boyd+, 2011)
J/AJ/142/92 : New proper motion stars with pm≥0.18"/yr (Boyd+, 2011)
J/AJ/144/64 : Solar neighborhood. XXVIII. Substellar companions
(Dieterich+, 2012)
J/AJ/144/99 : Near-IR spectroscopy of 36 late M dwarfs (Deshpande+, 2012)
J/ApJ/758/56 : Young M dwarfs within 25pc. II. Kinematics (Shkolnik+, 2012)
J/AJ/147/94 : Solar neighborhood. XXXII. L and M dwarfs (Dieterich+, 2014)
J/ApJ/789/102 : Properties of late M-dwarfs (Janson+, 2014)
J/AJ/149/5 : Solar neighborhood. XXXV. Distances to M dwarfs
(Winters+, 2015)
J/AJ/150/6 : Solar neighborhood. XXXVI. VRI variability of M dwarfs
(Hosey+, 2015)
J/AJ/150/50 : Speckle interferometry at SOAR in 2014 (Tokovinin+, 2015)
J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)
J/AJ/151/160 : 1103 parallaxes and proper motions from URAT (Finch+, 2016)
J/AJ/152/24 : Trigonometric parallaxes of 134 low-mass stars
(Weinberger+, 2016)
J/AJ/152/141 : Solar neighborhood. XXXVII. RVs for M dwarfs
(Benedict+, 2016)
J/AJ/153/14 : Solar neighborhood XXXVIII. Nearby M dwarf systems
(Winters+, 2017)
J/AJ/153/95 : Catalog of Suspected Nearby Young Stars (Riedel+, 2017)
J/AJ/154/32 : Solar neighborhood. XXXIX. Nearby white dwarfs
(Subasavage+, 2017)
Byte-by-byte Description of file: table1.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 17 A17 --- Name System name
19- 20 I2 h RAh Hour of Right Ascension (J2000) (1)
22- 23 I2 min RAm Minute of Right Ascension (J2000) (1)
25- 29 F5.2 s RAs Second of Right Ascension (J2000) (1)
31 A1 --- DE- Sign of the Declination (J2000) (1)
32- 33 I2 deg DEd Degree of Declination (J2000) (1)
35- 36 I2 arcmin DEm Arcminute of Declination (J2000) (1)
38- 41 F4.1 arcsec DEs Arcsecond of Declination (J2000) (1)
43 A1 --- Filt [VRI] Filter used
45- 46 I2 --- Nseas [3/10] Number of seasons observed (2)
47 A1 --- n_Nseas [cs] Note on Nseas (3)
49- 51 I3 --- Nfrm [44/167] Number of frames used in reductions
53- 59 F7.2 yr Date0 [2003.94/2005.89] Starting date of the time
interval
61- 67 F7.2 yr Date1 [2007.43/2016.73] Ending date of the time
interval
69- 73 F5.2 yr Nyr [2.24/12.15] Number of years of coverage
75- 76 I2 --- Nref [5/13] Number of reference stars
78- 83 F6.2 mas Rplx [26.96/131.14] Relative trigonometric parallax
π(rel)
85- 88 F4.2 mas e_Rplx [0.62/3.02] Uncertainty in Rplx
90- 93 F4.2 mas Cplx [0.36/3.04] Parallax correction
95- 98 F4.2 mas e_Cplx [0.04/0.76] Uncertainty in Cplx
100-105 F6.2 mas Aplx [27.77/132.07] Absolute trigonometric parallax
π(abs)
107-110 F4.2 mas e_Aplx [0.63/3.02] Uncertainty in Aplx
112-117 F6.1 mas/yr pm [129.1/2149.7] Proper motion
119-121 F3.1 mas/yr e_pm [0.3/2.5] Uncertainty in pm
123-127 F5.1 deg PA [38.9/277.5] Position angle
129-132 F4.2 deg e_PA [0.03/1] Uncertainty in PA
134-138 F5.1 km/s Vtan [10.4/112.4] Derived tangential velocity (4)
140-143 A4 --- Note Note(s) (5)
--------------------------------------------------------------------------------
Note (1): The positions are based on 2MASS positions adjusted to epoch 2000.0
using the relative µ and position angles.
Note (2): Where 3-6 months of observations count as one season for seasons in
which more than three images were taken.
Note (3): Note as follows:
c = Indicates a continuous set of observations with multiple nights of data
collected in each season;
s = Indicates scattered observations because at least one season has only one
night of observations.
Generally, "c" observations are better than "s".
Note (4): The tangential velocities in are computed from the relative µ and
absolute πtrig.
Note (5): Note as follows:
a = Parallax in Weinberger et al. (2016, J/AJ/152/24) = 113.69±0.54 mas.
b = Parallax in Finch & Zacharias (2016, J/AJ/151/160) = 90.0±9.5 mas.
c = Parallax in Weinberger et al. (2016, J/AJ/152/24) = 78.99±1.10 mas.
d = Parallaxes in Shkolnik et al. (2012, J/ApJ/758/56) = 61.4±1.5 mas and
Gaia (Cat. I/337) = 63.40±0.36 mas.
e = Parallax in Shkolnik et al. (2012, J/ApJ/758/56) = 48.2±5.0 mas.
f = Parallax in Finch & Zacharias (2016, J/AJ/151/160) = 134.9±12.1 mas.
g = Parallaxes in Weinberger et al. (2016, J/AJ/152/24) = 75.39±0.85 mas and
Finch & Zacharias (2016, J/AJ/151/160) = 96.1±15.9 mas.
h = Parallaxes in Weinberger et al. (2016, J/AJ/152/24) = 47.34±3.67 mas and
Finch & Zacharias (2016, J/AJ/151/160) = 43.3±16.9 mas.
i = Parallax in Weinberger et al. (2016, J/AJ/152/24) = 91.23±0.63 mas.
j = Parallax in Weinberger et al. (2016, J/AJ/152/24) = 53.68±0.64 mas.
k = Parallax in Weinberger et al. (2016, J/AJ/152/24) = 54.89±0.57 mas.
l = Parallax in Shkolnik et al. (2012, J/ApJ/758/56) = 53.5±1.3 mas.
m = Parallax in Shkolnik et al. (2012, J/ApJ/758/56) = 45.5±3 mas.
n = Parallax in Weinberger et al. (2016, J/AJ/152/24) = 129.57±0.31 mas.
The CTIOPI parallax listed here is identical to our value in
Mamajek et al. (2013AJ....146..154M 2013AJ....146..154M).
o = Parallaxes in Costa et al. (2006AJ....132.1234C 2006AJ....132.1234C) = 82.58±2.58 and
Weinberger et al. (2016, J/AJ/152/24) = 80.09±1.17 mas. Also known as
TRAPPIST-1.
! = System discussed in greater detail in Section 5 of the paper
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table3.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 17 A17 --- Name System name
19 A1 --- n_Name [a] Note on name (1)
21- 22 I2 h RAh Hour of Right Ascension (J2000)
24- 25 I2 min RAm Minute of Right Ascension (J2000)
27- 31 F5.2 s RAs Second of Right Ascension (J2000)
33 A1 --- DE- Sign of the Declination (J2000)
34- 35 I2 deg DEd Degree of Declination (J2000)
37- 38 I2 arcmin DEm Arcminute of Declination (J2000)
40- 43 F4.1 arcsec DEs Arcsecond of Declination (J2000)
45- 49 F5.2 mag Vmag [11.63/21.61] CTIO V band magnitude
51- 55 F5.2 mag Rmag [10.53/18.81] CTIO R band magnitude
57- 61 F5.2 mag Imag [9.12/16.55] CTIO I band magnitude
63- 67 A5 --- Nights Number of nights of VRI observations
69 I1 --- Ref [1/9] Photometry reference (2)
71 A1 --- Filt [VRI] Filter used
73- 76 F4.1 mmag Var [8.1/46.4] Variability in the filter used
78 I1 --- r_Var [2/4] Reference for Var (2)
80- 83 I4 yr Flare [2006/2013]? Year of flare detection in
the astrometric frames
85- 90 F6.3 mag Jmag [7.74/13.059] 2MASS J band magnitude
92- 97 F6.3 mag Hmag [7.146/12.254] 2MASS H band magnitude
99-104 F6.3 mag Ksmag [6.891/11.69] 2MASS KS band magnitude
106-110 A5 --- SpType MK spectral type
112 I1 --- r_SpType [3/8] Reference for SpType (2)
114 A1 --- Joint [J-] Joint? (3)
--------------------------------------------------------------------------------
Note (1): Note as follows:
a = Also known as TRAPPIST-1.
Note (2): Reference as follows:
1 = Winters et al. (2015, J/AJ/149/5);
2 = Hosey et al. (2015, J/AJ/150/6);
3 = Bartlett (2007PhDT.........2B 2007PhDT.........2B);
4 = This work;
5 = Cruz et al. (2003, J/AJ/126/2421);
6 = Reid et al. (2008, J/AJ/136/1290);
7 = Reid et al. (1995, Cat. III/198);
8 = Cruz et al. (2007, J/AJ/133/439);
9 = Mamajek et al. (2013AJ....146..154M 2013AJ....146..154M).
Note (3): A "J" indicates that joint photometry and spectroscopy data are
presented for a binary that neither of the CTIO/SMARTS telescopes
(0.9 and 1.5 m) nor 2MASS was able to resolve.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table4.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 17 A17 --- Name System name
19- 23 A5 --- SpType MK spectral type from this work (1)
25- 30 F6.2 0.1nm EW(Ha) [-24.59/0.25]? Hα equivalent width (Å)
32- 35 F4.2 --- Ind(NaI) [1.15/1.35]? Na I (8200 Å doublet) index
from this work
37- 40 F4.2 0.1nm EW(NaI) [3.74/6.16]? Na I (8200 Å doublet)
equivalent width (Å)
42- 45 F4.2 0.1nm EW(KI) [1/5.99]? K I (7699 Å) equivalent width
(Å)
47 A1 --- Joint [J-] Joint? (2)
49- 60 A12 --- Grav Spectroscopic indicator(s) suggesting that it
may be a low gravity star
62- 67 F6.2 km/s RV [-75.5/80.53]? Radial velocity
69- 72 F4.2 km/s e_RV [0.05/3]? Uncertainty in RV
74 I1 --- Ref [1/6]? Reference (3)
--------------------------------------------------------------------------------
Note (1): The uncertainty in a type is ± 0.5 subtype.
Note (2): A "J" indicates that a joint spectral type and indices are reported
for a binary that was unresolved by the CTIO/SMARTS 1.5 m.
Note (3): Reference as follows:
1 = Deshpande et al. (2012, J/AJ/144/99);
2 = Blake et al. (2010, J/ApJ/723/684);
3 = Reiners & Basri (2009, J/ApJ/705/1416);
4 = Shkolnik et al. (2012, J/ApJ/758/56);
5 = Torres et al. (J/A+A/460/695);
6 = Mamajek et al. (2013AJ....146..154M 2013AJ....146..154M).
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table7.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 17 A17 --- Name System name
19- 22 F4.1 pc Dist1 [13.5/36] Trigonometric distance
24- 26 F3.1 pc e_Dist1 [0.2/3] Uncertainty in Dist1
28- 31 F4.1 pc Dist2 [6.2/20]? Photometric distance
33- 35 F3.1 pc e_Dist2 [0.5/5]? Uncertainty in Dist2
37- 38 I2 --- Ref [1/10]? Reference (1)
40- 43 F4.1 pc Dist3 [7/20]? Spectroscopic distance
45- 47 F3.1 pc e_Dist3 [0.9/4]? Uncertainty in Dist3
49 I1 --- r_Dist3 [2/9]? Reference for Dist3 (1)
51 A1 --- Var [V] Variable? (2)
53- 82 A30 --- Note Note
--------------------------------------------------------------------------------
Note (1): Reference as follows:
1 = Siegler et al. (2005ApJ...621.1023S 2005ApJ...621.1023S);
2 = Cruz et al. (2003, J/AJ/126/2421);
3 = Reid et al. (2002, J/AJ/123/2822);
4 = Scholz et al. (2005, J/A+A/442/211);
5 = Riaz et al. (2006, J/AJ/132/866);
6 = Winters et al. (2015, J/AJ/149/5);
7 = Reid et al. (2003, J/AJ/126/3007);
8 = Montagnier et al. (2006A&A...460L..19M 2006A&A...460L..19M);
9 = Cruz et al. (2007, J/AJ/133/439);
10 = Daemgen et al. (2007ApJ...654..558D 2007ApJ...654..558D).
Note (2): Systems with "V" demonstrated a photometric variability greater than
20 mmag during astrometric observations.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table8.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 14 A14 --- Name System name
16- 17 I2 h RAh Hour of Right Ascension (J2000)
19- 20 I2 min RAm Minute of Right Ascension (J2000)
22- 26 F5.2 s RAs Second of Right Ascension (J2000)
28 A1 --- DE- Sign of the Declination (J2000)
29- 30 I2 deg DEd Degree of Declination (J2000)
32- 33 I2 arcmin DEm Arcminute of Declination (J2000)
35- 38 F4.1 arcsec DEs Arcsecond of Declination (J2000)
40- 44 F5.2 mas Aplx [15.34/73.22] Absolute trigonometric parallax
π(abs)
46- 50 F5.3 mas e_Aplx [1.69/3.61] Uncertainty in Aplx
52- 56 F5.1 mas/yr pm [185.9/296.2] Proper motion
58- 60 F3.1 mas/yr e_pm [0.8/3.5] Uncertainty in pm
62- 66 F5.1 deg PA [122.9/269.1] Position angle
68- 71 F4.2 deg e_PA [0.33/1.76] Uncertainty in PA
73 I1 --- Ref1 [1/3] Reference (1)
75- 80 F6.3 mag Vmag [10.03/14.44] CTIO V band magnitude
82 I1 --- r_Vmag [1/6] Reference for Vmag (1)
84- 88 F5.3 mag Ksmag [6.932/8.64] 2MASS KS band magnitude
90- 93 F4.2 Msun Mass [0.18/0.8] Mass (2)
95- 98 F4.2 Msun e_Mass [0.04/0.2] Uncertainty in Mass
100-104 A5 --- SpType MK spectral type
106 I1 --- Ref2 [1/7] Reference (1)
108-110 A3 --- Rel [Yes No] Physically related?
--------------------------------------------------------------------------------
Note (1): Reference as follows:
1 = This work;
2 = Lurie et al. (2014AJ....148...91L 2014AJ....148...91L);
3 = van Leeuwen (2007, Cat. I/311);
4 = Koen et al. (2010, J/MNRAS/403/1949);
5 = Shkolnik et al. (2009, J/ApJ/699/649);
6 = ESA (1997, Cat. I/239) and Hoslashg et al. (2000A&A...355L..27H 2000A&A...355L..27H);
7 = Upgren et al. (1972AJ.....77..486U 1972AJ.....77..486U);
8 = Delfosse et al. (2000A&A...364..217D 2000A&A...364..217D);
9 = Henry & McCarthy (1993, J/AJ/106/773);
10 = Elias et al. (1982AJ.....87.1029E 1982AJ.....87.1029E);
11 = Carpenter (2006, Explanatory Supplement to the 2MASS All Sky Data Release
ed R. M. Cutri et al (Pasadena, CA: IPAC)
http://www.ipac.caltech.edu/2mass/releases/allsky/doc/sec6_4b.html).
Note (2): Masses for M and K dwarfs are calculated using the mass-KCIT
relationship defined by references 8 and 9, respectively, after
transforming the 2MASS KS values to the California Institute of
Technology (CIT) system defined by reference 10 using the equations
of reference 11.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table9.dat
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 17 A17 --- Name System name
19- 23 F5.3 arcsec Sep [0.076/0.828] Separation
25- 29 F5.3 arcsec e_Sep [0.001/0.04]? Uncertainty in Sep
31- 36 F6.2 deg PA [44.1/354.7] Position angle
38- 41 F4.2 deg e_PA [0.1/1.4]? Uncertainty in PA
43- 53 A11 "date" Date Date of observation
55 I1 --- Ref [1/9] Reference (1)
--------------------------------------------------------------------------------
Note (1): Reference as follows:
1 = Siegler et al. (2005ApJ...621.1023S 2005ApJ...621.1023S);
2 = Reid et al. (2006, J/AJ/132/891);
3 = Daemgen et al. (2007ApJ...654..558D 2007ApJ...654..558D);
4 = Bergfors et al. (2010A&A...520A..54B 2010A&A...520A..54B);
5 = Shkolnik et al. (2012, J/ApJ/758/56);
6 = Montagnier et al. (2006A&A...460L..19M 2006A&A...460L..19M);
7 = Janson et al. (2014, J/ApJ/789/102);
8 = B. Mason (2015, private communication);
9 = Tokovinin et al. (2015, J/AJ/150/50).
--------------------------------------------------------------------------------
History:
From electronic version of the journal
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Jao et al. Paper XLII 2017AJ....154..191J 2017AJ....154..191J, Cat. J/AJ/154/191
Riedel et al. Paper XLIII 2018AJ....156...49R 2018AJ....156...49R, Cat. J/AJ/156/49
Henry et al. Paper XLIV 2018AJ....155..265H 2018AJ....155..265H, Cat. J/AJ/155/265
Winters et al. Paper XLV 2019AJ....157..216W 2019AJ....157..216W, Cat. J/AJ/157/216
Vrijmoet et al., Paper XLVI 2020AJ....160..215V 2020AJ....160..215V, Cat. J/AJ/160/215
Dieterich et al., Paper XLVII 2021AJ....161..172D 2021AJ....161..172D, Cat. J/AJ/161/172
Paredes et al., Paper XLVIII 2021AJ....162..176P 2021AJ....162..176P, Cat. J/AJ/162/176
Vrijmoet et al., Paper XLIX 2022AJ....163..178V 2022AJ....163..178V, Cat. J/AJ/163/178
Hubbard-James et al., Paper L 2022AJ....164..174H 2022AJ....164..174H
Kar et al., Paper LI 2024AJ....167..196K 2024AJ....167..196K, Cat. J/AJ/167/196
(End) Tiphaine Pouvreau [CDS] 12-Jul-2018