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 | RXJ 0658 | 104.704 | -55.933 | 104.461428 | -55.862903 | 130.333928 | -77.302143 | 266.02429497 | -21.20357002 | 164.9362 | 54095.6181597222 | 2006-12-26 14:50:09 | 54098.4099421296 | 2006-12-29 09:50:19 | 801089010 | 101.3845 | 100 | 101.3845 | 101.3845 | 0 | 101.3845 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 84.3679 | 84.3679 | 241.1547 | 2 | PROCESSED | 57637.5971180556 | 2016-09-06 14:19:51 | 54702 | 2008-08-24 00:00:00 | 54111.5842013889 | 2007-01-11 14:01:15 | 3.0.22.44 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011448 | We propose SUZAKU X-ray observations of an intriguing cluster of galaxies, RXJ0658, to determine and characterize the nature of the hard X-ray spectral emission and other nonthermal activity. It also has many other interesting features, such as a cold front, evidence for merger, a shock, and regions of unusually high temperature, all of which are related to the hard X-ray emission and the nonthermal activity. The more accurate measure of the spectral characteristics of the hard component, when combined with the radio and other past X-ray data, can reveal the nature of the emission process and the acceleration mechanism of the relativistic electrons, provide a means of measuring the magnetic field strength, and aid in understanding the process of formation of clusters. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | VAHE PETROSIAN | USA | 1 | AO1 | HARD X-RAY EMISSION FROM CLUSTER RXJ0658 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801089010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '801089010'
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