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開始行:
Millimeter and submillimeter images of various galaxies i...
#contents
* Nearby galaxies [#z0b5db1c]
** M 83: a nearby barred spiral galaxy hosting a nuclear ...
#ref(./M83CO32IcoVco.PNG,70%)
-- Velocity integrated intensity and intensity-weighted m...
#ref(./M83CO32-on-Ha-8um.PNG,70%)
-- Comparison of the CO(J=3-2) image with massive star fo...
- [[Muraoka, Kohno, et al., 2009, ApJ, 706, 1213>http://a...
** M 51: a grand design spiral galaxy hosting a type-2 Se...
#ref(m51-MultiLines.png)
- [[Kohno, K., Kawabe, R., Tosaki, T., and Okumura, K. S....
- [[Matsushita, S., Kohno, K., Vila-Vilaro, B., Tosaki, T...
#ref(N5194-CO-HCN-HCOp-Spectrum-updated.png)
- [[Kohno, K., et al., 2008, Ap&SS, 313, 279>http://adsab...
** NGC 1097: a low luminosity AGN accompanied with intens...
#ref(n1097all.gif)
- [[Kohno et al. 2003, PASJ, 55, L1>http://adsabs.harvard...
** NGC 5033: a low luminosity AGN with little nuclear sta...
#ref(./n5033co.png,70%)
-- CO(J=1-0) integrated intensity and intensity-weighted ...
#ref(n5033-NIRcolor-vs-CO.png)
- [[Kohno et al. 2003, PASJ, 55, 103>http://adsabs.harvar...
** NGC 6951: a Seyfert nucleus in a strongly barred spira...
#ref(n6951.png)
- [[Kohno, K., Kawabe, R., and Vila-Vilaro, B., 1999, ``D...
** NGC 5195: a barred, gas rich S0 galaxy without any sig...
#ref(n5195.png)
- [[Kohno, K. et al. 2002, "Diffuse and Gravitationally S...
** M33: one of the nearest face-on spiral galaxies [#ucba...
#ref(M33ASTE-CO32map.PNG)
- [[Miura, R., Kohno, K., Tosaki, T., et al. 2012, ApJ, 7...
-- We present a giant molecular cloud (GMC) catalog of M3...
#ref(M33AzTEC-1mm-on-Halpha.PNG)
-- 1.1 mm continuum map superposed on H alpha emission.
#ref(M33AzTEC-Tdust.PNG)
-- A map of cold dust temperature derived from the 1.1 mm...
- [[Komugi, S., Tosaki, T., Kohno, K., et al., 2011, PASJ...
-- We present wide-field 1.1 mm continuum imaging of the ...
-- Combined with far-infrared imaging at 160um, we derive...
-- Further comparison of individual regions show a strong...
* Gamma-ray bursts [#pa6d673f]
** GRB 030329: one of the brightest Gamma-ray bursts to d...
#ref(./GRB030329-fadingAfterglow.png,50%)
- [[Kohno et al., 2005, "Nobeyama Millimeter Array Observ...
- see also [[Endo, A., Kohno, K., Hatsukade, B., et al., ...
** GRB 020819B: first detection of the CO emission among ...
#ref(./naoj_alma_grb_140613_01.jpg,50%)
- Spatially resolved CO(3-2) (left) and 1.2 mm continuum ...
- [[Hatsukade et al. 2014, "Two Gamma-ray bursts from dus...
* Quasars [#x7f58976]
** BR1202-0725, a radio quiet quasar at redshift of 4.7 [...
#ref(br1202-NMA-CO54spectrum.png)
CO(J=5-4) spectrum taken with the NMA.
#ref(br1202-NMA-CO54map.png)
CO(J=5-4) velocity-integrated intensity image of BR1202-0...
- [[Ohta, K., Yamada, T., Nakanishi, K., Kohno, K., Akiya...
* (Sub)millimeter galaxies [#lab767ce]
** SSA22-AzTEC1: a proto-quasar at the center of the prot...
#ref(Tamura2010-SMAimage-on-IRAC.PNG)
- [[Tamura, Y., et al., 2010, ApJ, 724, 1270 >http://adsa...
-- At the SMA position, we find radio-to-mid-infrared cou...
-- It is possible that SSA22-AzTEC1 is the first example ...
** Orochi (SXDF1100.1): an ultra-bright starburst galaxy ...
#ref(Orochi-overview.PNG)
- [[Ikarashi, S., Kohno, K., et al., 2011, MNRAS, 415, 30...
* Deep surveys of submillimeter galaxies [#ob8b6146]
** SSA22, a protocluster regioin traced by an overdensity...
#ref(SSA22AzTEC-fig1.PNG)
- [[Tamura, Y., Kohno, K., Nakanishi, K., Hatsukade, B., ...
- Figure 1. The positions of 1,100-mm sources and Lya emi...
SSA 22 protocluster region.
-- (a) The colour scale shows the map of signal-to-noise
ratio at 1100 um. The map shows 30 sources with signal-to...
ratios >3.5 (circles). Observations of SSA 22 (field cent...
RA 22h 17m 36s, dec. +0deg 15' 00'' (J2000)) were obtaine...
AzTEC camera, operating at 1100 um, mounted on the ASTE 1...
submillimetre telescope during the July–September 2007 ob...
The data consist of a total of 42 h of integration time o...
excellent conditions (zenith atmospheric opacity at 220 G...
tau(220GHz) > 0.01–0.10). This resulted in a root-mean-sq...
0.68–0.99 mJy per beam over 390 arcmin^2. The point sprea...
AzTEC on ASTE has a full-width at half-maximum of 2861 ar...
-- (b) The locations of the bright submillimetre galaxies...
density field of the Lya emitters is shown in the colour ...
density enhancement of the Lya emitters, which is thought...
underlying large-scale structure at z~3.1.
** AKARI Deep Field South (ADF-S) 1.1 mm view [#w9e97e40]
- [[Hatsukade, Kohno, et al. 2011, MNRAS, 411, 102>http:/...
#ref(ADFS.jpg)
-- We present results of a 1.1-mm deep survey of the AKAR...
-- We uncovered 198 sources with a significance of 3.5σ-1...
終了行:
Millimeter and submillimeter images of various galaxies i...
#contents
* Nearby galaxies [#z0b5db1c]
** M 83: a nearby barred spiral galaxy hosting a nuclear ...
#ref(./M83CO32IcoVco.PNG,70%)
-- Velocity integrated intensity and intensity-weighted m...
#ref(./M83CO32-on-Ha-8um.PNG,70%)
-- Comparison of the CO(J=3-2) image with massive star fo...
- [[Muraoka, Kohno, et al., 2009, ApJ, 706, 1213>http://a...
** M 51: a grand design spiral galaxy hosting a type-2 Se...
#ref(m51-MultiLines.png)
- [[Kohno, K., Kawabe, R., Tosaki, T., and Okumura, K. S....
- [[Matsushita, S., Kohno, K., Vila-Vilaro, B., Tosaki, T...
#ref(N5194-CO-HCN-HCOp-Spectrum-updated.png)
- [[Kohno, K., et al., 2008, Ap&SS, 313, 279>http://adsab...
** NGC 1097: a low luminosity AGN accompanied with intens...
#ref(n1097all.gif)
- [[Kohno et al. 2003, PASJ, 55, L1>http://adsabs.harvard...
** NGC 5033: a low luminosity AGN with little nuclear sta...
#ref(./n5033co.png,70%)
-- CO(J=1-0) integrated intensity and intensity-weighted ...
#ref(n5033-NIRcolor-vs-CO.png)
- [[Kohno et al. 2003, PASJ, 55, 103>http://adsabs.harvar...
** NGC 6951: a Seyfert nucleus in a strongly barred spira...
#ref(n6951.png)
- [[Kohno, K., Kawabe, R., and Vila-Vilaro, B., 1999, ``D...
** NGC 5195: a barred, gas rich S0 galaxy without any sig...
#ref(n5195.png)
- [[Kohno, K. et al. 2002, "Diffuse and Gravitationally S...
** M33: one of the nearest face-on spiral galaxies [#ucba...
#ref(M33ASTE-CO32map.PNG)
- [[Miura, R., Kohno, K., Tosaki, T., et al. 2012, ApJ, 7...
-- We present a giant molecular cloud (GMC) catalog of M3...
#ref(M33AzTEC-1mm-on-Halpha.PNG)
-- 1.1 mm continuum map superposed on H alpha emission.
#ref(M33AzTEC-Tdust.PNG)
-- A map of cold dust temperature derived from the 1.1 mm...
- [[Komugi, S., Tosaki, T., Kohno, K., et al., 2011, PASJ...
-- We present wide-field 1.1 mm continuum imaging of the ...
-- Combined with far-infrared imaging at 160um, we derive...
-- Further comparison of individual regions show a strong...
* Gamma-ray bursts [#pa6d673f]
** GRB 030329: one of the brightest Gamma-ray bursts to d...
#ref(./GRB030329-fadingAfterglow.png,50%)
- [[Kohno et al., 2005, "Nobeyama Millimeter Array Observ...
- see also [[Endo, A., Kohno, K., Hatsukade, B., et al., ...
** GRB 020819B: first detection of the CO emission among ...
#ref(./naoj_alma_grb_140613_01.jpg,50%)
- Spatially resolved CO(3-2) (left) and 1.2 mm continuum ...
- [[Hatsukade et al. 2014, "Two Gamma-ray bursts from dus...
* Quasars [#x7f58976]
** BR1202-0725, a radio quiet quasar at redshift of 4.7 [...
#ref(br1202-NMA-CO54spectrum.png)
CO(J=5-4) spectrum taken with the NMA.
#ref(br1202-NMA-CO54map.png)
CO(J=5-4) velocity-integrated intensity image of BR1202-0...
- [[Ohta, K., Yamada, T., Nakanishi, K., Kohno, K., Akiya...
* (Sub)millimeter galaxies [#lab767ce]
** SSA22-AzTEC1: a proto-quasar at the center of the prot...
#ref(Tamura2010-SMAimage-on-IRAC.PNG)
- [[Tamura, Y., et al., 2010, ApJ, 724, 1270 >http://adsa...
-- At the SMA position, we find radio-to-mid-infrared cou...
-- It is possible that SSA22-AzTEC1 is the first example ...
** Orochi (SXDF1100.1): an ultra-bright starburst galaxy ...
#ref(Orochi-overview.PNG)
- [[Ikarashi, S., Kohno, K., et al., 2011, MNRAS, 415, 30...
* Deep surveys of submillimeter galaxies [#ob8b6146]
** SSA22, a protocluster regioin traced by an overdensity...
#ref(SSA22AzTEC-fig1.PNG)
- [[Tamura, Y., Kohno, K., Nakanishi, K., Hatsukade, B., ...
- Figure 1. The positions of 1,100-mm sources and Lya emi...
SSA 22 protocluster region.
-- (a) The colour scale shows the map of signal-to-noise
ratio at 1100 um. The map shows 30 sources with signal-to...
ratios >3.5 (circles). Observations of SSA 22 (field cent...
RA 22h 17m 36s, dec. +0deg 15' 00'' (J2000)) were obtaine...
AzTEC camera, operating at 1100 um, mounted on the ASTE 1...
submillimetre telescope during the July–September 2007 ob...
The data consist of a total of 42 h of integration time o...
excellent conditions (zenith atmospheric opacity at 220 G...
tau(220GHz) > 0.01–0.10). This resulted in a root-mean-sq...
0.68–0.99 mJy per beam over 390 arcmin^2. The point sprea...
AzTEC on ASTE has a full-width at half-maximum of 2861 ar...
-- (b) The locations of the bright submillimetre galaxies...
density field of the Lya emitters is shown in the colour ...
density enhancement of the Lya emitters, which is thought...
underlying large-scale structure at z~3.1.
** AKARI Deep Field South (ADF-S) 1.1 mm view [#w9e97e40]
- [[Hatsukade, Kohno, et al. 2011, MNRAS, 411, 102>http:/...
#ref(ADFS.jpg)
-- We present results of a 1.1-mm deep survey of the AKAR...
-- We uncovered 198 sources with a significance of 3.5σ-1...
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