DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | CYGNUS A SUB | 299.7227 | 40.8585 | 299.290982 | 40.72139 | 317.590165 | 59.487138 | 76.23979532 | 5.91406977 | 241.0006 | 56615.3145717593 | 2013-11-19 07:32:59 | 56616.3224189815 | 2013-11-20 07:44:17 | 808016010 | 42.5204 | 40 | 42.5284 | 42.5284 | 0 | 42.5204 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 38.9173 | 38.9173 | 87.0719 | 1 | PROCESSED | 57613.3640625 | 2016-08-13 08:44:15 | 56995 | 2014-12-04 00:00:00 | 56629.6679050926 | 2013-12-03 16:01:47 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 080018 | We have observed a merging cluster Cygnus A in the Suzaku GO-3 with 45ks. This observation confirmed a hot region between the main and sub components. Furthermore, we found a gas velocity shift between the main and sub by about 2500 km/s. We believe that these are colliding with each other. The current result are limited by statistics and systematic uncertainty. To improve the accurary of the measurement and complete our study, we propose two additional observations located the main and sub components at the center of the FOV. These will provide the best chance to look into a merging cluster "in motion". | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | TAKAYUKI TAMURA | JAP | 8 | AO8 | CYGNUS A CLUSTER: THE BEST MERGING SYSTEM FOR THE SUZAKU | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808016010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '808016010'
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