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 | M33 X8 | 23.4834 | 30.5892 | 22.778431 | 30.333215 | 33.223542 | 19.296261 | 133.64723816 | -31.39681198 | 258.5185 | 55207.0743865741 | 2010-01-11 01:47:07 | 55209.5626157407 | 2010-01-13 13:30:10 | 704016010 | 106.1036 | 100 | 106.1036 | 106.1061 | 0 | 106.1061 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 6.1053 | 6.1053 | 214.9577 | 1 | PROCESSED | 57550.3046412037 | 2016-06-11 07:18:41 | 55587 | 2011-01-26 00:00:00 | 55218.6414930556 | 2010-01-22 15:23:45 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040067 | The nature of ultraluminous X-ray sources (ULXs) is one of the important unresolved issues in the modern astrophysics. In order to solve the problem, it is of crucial importance to observe X-ray spectra above 10 keV from ULXs, which enables us to determine precisely their spectral states. Therefore, Suzaku observations of two bright ULX, M33 X8 and IC 342 X2, are proposed. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | NAOKI ISOBE | JAP | 4 | AO4 | HARD X-RAY STUDY OF ULTRALUMINOUS X-RAY SOURCES | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704016010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '704016010'
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