WISE 1405+5534

Summary of Properties

Property

Discovery Name

AllWISE Designation

CatWISE Designation

Spectral Type

F105W

Y (mag)

J (mag)

H (mag)

K (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

WISEPC J140518.40 + 553421.5

WISEA J140518.32+553421.3

CWISE J140516.62+553422.9

Y0.5pec*

21.939 (0.024)

21.41 (0.10)

21.06

21.41 (0.08)

21.61 (0.12)

18.765 (0.396)

14.097 (0.037)

12.204 (0.263)

>8.981

18.270 (0.134)

14.098 (0.014)

16.876 (0.046)

14.058 (0.019)

157.9 (3.1)

6.33 (0.12)

−2326.5 (1.7)

236.1 (1.3)

Reference

Cushing et al. (2011)

CatWISE2020

Schneider et al. (2015)

Leggett et al. (2013)

Leggett et al. (2015)

Cutri et al. (2013)

CatWISE2020

Schneider et al. (2015)

Kirkpatrick et al. (2019)

Discovery Data

Name: WISEPC J140518.40 + 553421.5
Paper: Cushing et al. (2011)
Spectral type: Y0(pec?)

Spectral Type History

Cushing et al. (2011): Y0 (pec?)
Schneider et al. (2015): Y0.5

Photometry

Spitzer

Kirkpatrick et al. (2012): [3.6]=16.88 (0.05), [4.5] = 14.06 (0.02)
Leggett et al. (2013): [3.6]=16.78 (0.01), [4.5]=14.02. (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.]
Schneider et al. (2015):[3.6]=16.876 (0.046), [4.5]=14.058 (0.019)
Martin et al. (2018): [3.6] = 16.850 (0.059), [4.5] = 14.069 (0.017)

HST

Kirkpatrick et al. (2012): F140W=21.22 (0.20)
Schneider et al. (2015): F105W=21.939 (0.024), F140W=21.271 (0.018)

Ground

Cushing et al. (2011): J(WIRC/Palomar)=20.20 (0.13), H(WIRC/Palomar)=21.45 (0.41)
Kirkpatrick et al. (2012): J(WIRC/Palomar)=20.09 (0.12), H(WIRC/Palomar)>20.5
Lodieu, Béjar, Rebolo (2013): z(OSIRIS/GTO)>23.85
Leggett et al. (2013): Y(NIRI/Gemini-MKO)=21.41 (0.10), J(NIRI/Gemini-MKO)=21.06 (0.06), H(NIRI/Gemini-MKP)=21.41 (0.08)
Leggett et al. (2015): K(NIRI/Gemini-MKO)=21.61 (0.12)

Spectroscopy

Cushing et al. (2011): WFC3/HST, 1.07-1.70 μm, R=130
Schneider et al. (2015): WFC3/HST, 0.9-1.1 μm, R=210, WFC3/HST, 1.07-1.70 μm, R=130 [re-reduction of Cushing et al. (2011)] [ASCII] [PNG]

Parallax & Proper Motion

Marsh et al. (2013): π=133 (81) mas, d>3.4 pc, μ_αcos(δ)=−2297 (96) mas yr-1, μ_δ=+212 (137) mas yr−1
Dupuy & Kraus (2013): π=129 (19) mas, d=7.8 (+1.3−1.0) pc, μ_αcos(δ)=−2263 (47) mas yr−1, μ_δ=288 (41) mas yr−1
Leggett et al. (2017): π=155 (6) mas, d=6.5 (0.2) pc, μ_αcos(δ)=−2334 (5) mas yr−1, μ_δ=+232 (5) mas yr−1
Martin et al. (2018): π=144.35 (8.60) mas, d= 6.93 (+0.44 −0.39) pc, μ_αcos(δ)=−2336.04 (6.91) mas yr−1, μ_δ=+238.02 (7.40) mas yr−1
Kirkpatrick et al. (2019): π=157.9 (3.1) mas, d= 6.33 (0.12) pc, μ_αcos(δ)=−2326.5 (1.7) mas yr−1, μ_δ=236.1 (1.3) mas yr−1

Notes

As noted by Cushing et al. (2015), Schneider et al. (2015) dropped the pec? in the spectral type by mistake.