Display data from paper

Data: CH3OH_I

MAT14 - The First Very Long Baseline Interferometry Image of a 44 GHz Methanol Maser with the KVN and VERA Array (KaVA)

  Interferometry data

Short title: Matsumoto et al. (2014)
Authors: Matsumoto, Naoko Hirota, Tomoya Sugiyama, Koichiro Kim, Kee-Tae Kim, Mikyoung Byun, Do-Young Jung, Taehyun Chibueze, James O. Honma, Mareki Kameya, Osamu Kim, Jongsoo Lyo, A.-Ran Motogi, Kazuhito Oh, Chungsik Shino, Nagisa Sunada, Kazuyoshi Bae, Jaehan Chung, Hyunsoo Chung, Moon-Hee Cho, Se-Hyung Han, Myoung-Hee Han, Seog-Tae Hwang, Jung-Wook Je, Do-Heung Jike, Takaaki Jung, Dong-Kyu Jung, Jin-seung Kang, Ji-hyun Kang, Jiman Kang, Yong-Woo Kan-ya, Yukitoshi Kawaguchi, Noriyuki Kim, Bong Gyu Kim, Jaeheon Ryoung Kim, Hyo Kim, Hyun-Goo Kobayashi, Hideyuki Kono, Yusuke Kurayama, Tomoharu Lee, Changhoon Lee, Jeong Ae Lee, Jeewon Lee, Jung-Won Lee, Sang Hyun Lee, Sang-Sung Minh, Young Chol Miyazaki, Atsushi Oh, Se-Jin Oyama, Tomoaki Park, Sun-youp Roh, Duk-Gyoo Sasao, Tetsuo Sawada-Satoh, Satoko Shibata, Katsunori M. Sohn, Bong Won Song, Min-Gyu Tamura, Yoshiaki Wajima, Kiyoaki Wi, Seog-Oh Yeom, Jae-Hwan Yun, Young Joo
Journal: The Astrophysical Journal Letters, Volume 789, Issue 1, article id. L1, 6 pp. (2014).
Bibcode: 2014ApJ...789L...1M

PDF: MAT14.pdf

Detection table from Matsumoto et al. (2014)

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ID Obs. RA Obs. Dec RA offset Dec offset l b # Location Source name Image Line Vpeak Fpeak ∫F dv Telescope Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (Jy/beam) (Jy/beam*km/s)
1+18 17 50.1-12 07 4818.3202051.793897IRAS 18151-1208 Image 44 GHz (I)
29.4 .. 31.10.55 .. 16.330.55 .. 16.33KaVA2012 April 8
+18 17 50.1-12 07 48-0.1 mas-0.19 mas18.3202051.79389711IRAS 18151-120829.410.74 (12)10.74 (12)
+18 17 50.1-12 07 48-0.07 mas-0.07 mas18.3202051.79389721IRAS 18151-120829.616.33 (17)16.33 (17)
+18 17 50.1-12 07 48-0.27 mas0.03 mas18.3202051.79389731IRAS 18151-120829.814.90 (12)14.90 (12)
+18 17 50.1-12 07 480.09 mas0.12 mas18.3202051.79389741IRAS 18151-1208302.30 (9)2.30 (9)
+18 17 50.1-12 07 47.9999-3.53 mas80.52 mas18.3202051.79389752IRAS 18151-120830.45.43 (10)5.43 (10)
+18 17 50.1-12 07 47.9999-4.06 mas81.25 mas18.3202051.79389762IRAS 18151-120830.64.49 (8)4.49 (8)
+18 17 50.1-12 07 47.9999-3.06 mas80.82 mas18.3202051.79389772IRAS 18151-120830.90.74 (6)0.74 (6)
+18 17 50.1-12 07 47.9999-57.5 mas87.32 mas18.3202051.79389783IRAS 18151-120830.90.87 (6)0.87 (6)
+18 17 50.1-12 07 47.9999-58.82 mas86.62 mas18.3202051.79389793IRAS 18151-120831.10.55 (1)0.55 (1)
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  • Distribution of sources in all sky (l,b)

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  • Distribution of sources in all sky using Aladin

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  • Distribution of sources in IRAS color-color diagram

    Tip: Use "Box select" or "Lasso select" to display colour-selected sources in Aladin all-sky view

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

    Original color diagram is taken form van der Veen & Habing (1987)

    Type Description
    I Oxygen-rich non-variable stars without circumstellar shells
    II Variable stars with "young" O-rich circumstellar shells
    IIIa Variable stars with more evolved O-rich circumstellar shells
    IIIb Variable stars with thick O-rich circumstellar shells
    IV Variable stars with very thick O-rich circumstellar shells
    V Planetary nebulae and non- variable stars with very cool circumstellar shells
    VIa Variable stars with relatively cold dust at large distances; a significant part of the stars is carbon-rich
    VIb Variable stars with relatively hot dust close to the star and relatively cold dust at large distances; Some of the objects have proven to be O-rich
    VII Variable stars with more evolved C-rich circumstellar shells
    VIII Different sort of objects

  • Distribution of the detection velocities versus galactic longitude from MAT14

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

    Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

  • Distribution of sources from MAT14 in (l,b) histograms



    X
    DSS colored
    2MASS colored
    WISE colored
    SDSS color
    IRAC color I1,I2,I4
    GLIMPSE 360
    PACS color (70-160 um)
    SPIRE color (250-500 um)
    NVSS (1.4GHz)
    ATLASGAL 870 um
    ATLASGAL 870 um + Planck
    Bolocam 1.1 mm
    UKIDSS K
    2MASS K