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| Query : 2018PASJ...70...98T |
2018PASJ...70...98T - Publ. Astron. Soc. Jap., 70, 98 (2018)
Is the infrared background excess explained by the isotropic zodiacal light from the outer solar system?
TSUMURA K.
Journal keyword(s):
Simbad objects: 1
| Number of rows : 1 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | * pi.01 UMa | BY* | 08 39 11.7046112880 | +65 01 15.263122512 | 6.33 | 6.26 | 5.64 | 5.12 | 4.79 | G0.5V | 608 | 0 |
| Query : 2018PASJ...70...98T |
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Hierarchy :
number of linked objects
whatever the membership probability is (see description here ) :
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| * 3 UMa | GC 11817 |
NSV 17937
|
TD1 12726
|
| * pi.01 UMa | GCRV 5666 | PLX 2047.1 | TIC 417762326 |
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AG+65 441
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GEN# +1.00072905 | PLX 2047.10 |
TYC 4133-1971-1
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| 1AXG J083912+6500 |
GJ 311
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PPM 16705
|
UBV 8155 |
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BD+65 643
|
GSC 04133-01971
|
RBS 714 | UBV M 14477 |
| CNS5 2136 | 1H 0833+654 |
2RE J0839+650
|
uvby98 100072905
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| 1E 0834.7+6512 |
HD 72905
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2RE J083915+650149
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V* pi.01 UMa
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| 1E 0834.8+6512 |
HIC 42438
|
ROT 1354 | WEB 8162 |
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2E 2018
|
HIP 42438
|
RX J0839.1+6501 |
WISEA J083911.68+650116.0
|
| 2E 0834.7+6511 |
HR 3391
|
RX J0839.2+6501 |
WISE J083911.67+650116.5
|
| 1ES 0834+65.1 |
IRAS 08347+6511
|
1RXS J083912.0+650118
|
[ZEH2003] RX J0839.2+6501 1 |
| 2EUVE J0839+65.0 | JP11 1687 |
SAO 14609
|
Gaia DR3 1092545710514654464
|
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EUVE J0839+65.0
|
2MASS J08391162+6501151
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SKY# 16549 |
Gaia DR1 1092545706218403072
|
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EUVE J0839+64.9
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N30 2004 | SPOCS 2720 |
Gaia DR2 1092545710514654464
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References (608 between 1850 and 2026) (Total 608)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). |
Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center
Data at NED - NASA/IPAC Extragalactic Database : * pi.01 UMa
Link by name to the catalogue in VizieR :
Search by coordinates in Vizier (radius: 5 arcsec)
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