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 | PKS 0745-191 | 116.8852 | -19.2901 | 116.331446 | -19.165404 | 123.663194 | -39.639458 | 236.4397894 | 3.03527791 | 293.9994 | 54231.0124884259 | 2007-05-11 00:17:59 | 54231.8216898148 | 2007-05-11 19:43:14 | 802062010 | 32.0065 | 30 | 32.0065 | 32.0305 | 0 | 32.0145 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 27.7016 | 27.7016 | 69.9099 | 0 | PROCESSED | 57538.6154976852 | 2016-05-30 14:46:19 | 54695 | 2008-08-17 00:00:00 | 54238.8868518518 | 2007-05-18 21:17:04 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021440 | PKS 0745-191 is the X-ray brightest galaxy cluster beyond a redshift of 0.1. It has a smooth surface brightness profile and appears relaxed. Using the low background of Suzaku we will measure the temperature of the intracluster medium to the virial radius of the cluster. Its high temperature means that we will be unaffected by any loss of effective area at low energies. In addition the cluster is bright enough so that the bremsstrahlung emission will be easily detected using the PIN detector. This will allow us to search for any nonthermal component as well as accurately determining the high temperature components in the cluster. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | ANDREW YOUNG | USA | 2 | AO2 | PKS 0745-191: THE BRIGHTEST CLUSTER BEYOND Z=0.1 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802062010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '802062010'
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