WISE 0410+1502

Summary of Properties

Property

Discovery Name

AllWISE Designation

CatWISE Designation

Spectral Type

Y_MKO (mag)

J_MKO (mag)

H_MKO (mag)

K_MKO (mag)

AllWISE W1 (mag)

AllWISE W2 (mag)

AllWISE W3 (mag)

AllWISE W4 (mag)

CatWISE W1 (mag)

CatWISE W2 (mag)

[3.6] (mag)

[4.5] (mag)

π (mas)

d (pc)

μ_αcos(δ) (mas yr−1)

μ_δ (mas yr−1)

Value

WISEP J041022.71+150248.5

WISEA J041022.75+150247.9

CWISE J041023.09+150236.9

19.78 (0.04)

19.44 (0.03)

20.02 (0.05)

19.91 (0.07)

>18.170

14.113 (0.047)

12.314 (0.500)

>8.842

18.018 (0.171)

14.104 (0.017)

16.636 (0.042)

14.166 (0.019)

150.2 (2.4)

6.66 (0.11)

954.2 (1.1)

−2213.3 (1.1)

Reference

Cushing et al. (2011)

CatWISE2020

Cushing et al. (2011)

Leggett et al. (2013)

Cutri et al. (2013)

CatWISE2020

Schneider et al. (2015)

Kirkpatrick et al. (2019)

Discovery Data

Name: WISEP J041022.71 + 150248.5
Paper: Cushing et al. (2011)
Spectral type: Y0

Spectral Type History

Cushing et al. (2011): Y0

Photometry

Spitzer

Kirkpatrick et al. (2012): [3.6]=16.64 (0.04), [4.5]=14.18 (0.02)
Leggett et al. (2013): [3.6]=16.56 (0.01), [4.5]=14.12 (0.01) [derived from archived data for GO program 70062 and DDT program 551. A 30 mmag (3%) error should be added in quadrature to the quoted random errors for the IRAC data to account for systematics.]
Beichman et al. (2014): [3.6]=16.62 (0.05), [4.5]=14.10 (0.03)
Schneider et al. (2015): [3.6]=16.636 (0.042), [4.5]=14.166 (0.019)
Martin et al. (2018): [3.6] = 16.578 (0.047), [4.5] = 14.149 (0.018)

HST

Beichman et al. (2014): F140W=19.74 (0.03)
Schneider et al. (2015): F140W=19.634 (0.007)

Ground

Cushing et al. (2011): J(WIRC/Palomar)=19.25 (0.05), H(WIRC/Palomar)=19.05 (0.09)
Kirkpatrick et al. (2012): J(WIRC/Palomar)=19.24 (0.05) [updated from Cushing et al. (2011)]
Lodieu, Béjar, Rebolo (2013): z(OSIRIS/GTO)=22.66 (0.09)
Leggett et al. (2013): Y(NIRI/Gemini-MKO)=19.78 (0.04), J(NIRI/Gemini-MKO)=19.44 (0.03), H(NIRI/Gemini-MKO)=20.02 (0.05), K(NIRI/Gemini-MKO)=19.91 (0.07)

Spectroscopy

Cushing et al. (2011): FIRE/Magellan, 1-2.4 μm, R=250-350
Schneider et al. (2015): WFC3/HST, 1.1-1.70 μm, R=130 [ASCII] [PNG]
Leggett et al. (2017): GNIRS/Gemini, 0.95-2.5 μm, R=700

Parallax & Proper Motion

Marsh et al. (2013): π=233 (56) mas, d=4.2 (+1.2−0.6), μ_αcos(δ)=+974 (79) mas yr−1, μ_δ=−2144 (72) mas yr−1
Lodieu, Béjar, Rebolo (2013): μ_αcos(δ)=+1200 (80) mas yr−1, μ_δ=−2170 (80) mas yr−1
Dupuy & Kraus (2013): π=132 (15) mas, d=7.6 (+1.0−0.8) pc, μ_αcos(δ)=+958 (37) mas yr−1, μ_δ=−2229 (29) mas yr−1
Beichman et al. (2014): π=160 (9) mas, d=6.2 (0.4) pc, μ_αcos(δ)=+966 (13) mas yr−1, μ_δ=−2218 (13) mas yr−1
Martin et al. (2018): π=153.42(4.05) mas, d= 6.52 (+0.18 −0.17) pc, μ_αcos(δ)=−959.86 (3.57) mas yr−1, μ_δ=−2218.64 (3.46) mas yr−1
Kirkpatrick et al. (2019): π=150.2 (2.4) mas, d= 6.66 (0.11) pc, μ_αcos(δ)=954.2 (1.1) mas yr−1, μ_δ=−2213.3 (1.1) mas yr−1