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
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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