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 | ABELL 426 E2 | 50.6767 | 41.5228 | 49.847142 | 41.344864 | 59.17553 | 22.199581 | 151.03351832 | -12.94989772 | 90.0008 | 55041.7150115741 | 2009-07-29 17:09:37 | 55041.9654976852 | 2009-07-29 23:10:19 | 804057010 | 12.9048 | 10 | 12.9048 | 12.9048 | 0 | 12.9048 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 12.962 | 12.962 | 21.6399 | 1 | PROCESSED | 57547.969849537 | 2016-06-08 23:16:35 | 55419 | 2010-08-11 00:00:00 | 55050.2440277778 | 2009-08-07 05:51:24 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 041522 | Suzaku has enabled a breakthrough to be made in the study of the outer regions of galaxy clusters. For the first time, gas properties have been measured to beyond the virial radius. This is important for understanding properties such as the cluster gas and total mass, required for cosmological studies. It is also crucial for understanding how clusters link into their surrounding environments. How do large-scale filaments channel matter into clusters? Are there associated large-scale accretion shocks? This has been possible due to Suzaku's low orbit and the low background of its FI detectors, and the study of a particularly bright cluster. We propose to exploit Suzaku's unique capability to extend this result to the X-ray brightest cluster, and best target in the sky: the Perseus Cluster. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | STEVEN ALLEN | USA | 4 | AO4 | TO BEYOND THE VIRIAL RADIUS OF THE X-RAY BRIGHTEST CLUSTER IN THE SKY | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804057010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '804057010'
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