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 | IC 342 X2 | 56.516 | 68.1498 | 55.302778 | 67.99381 | 72.573568 | 46.727351 | 138.08335694 | 10.57829767 | 91.9969 | 55415.9786689815 | 2010-08-07 23:29:17 | 55417.3765625 | 2010-08-09 09:02:15 | 705009010 | 74.379 | 80 | 74.379 | 74.379 | 0 | 74.379 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 64.1316 | 64.1316 | 120.7679 | 0 | PROCESSED | 57552.9205671296 | 2016-06-13 22:05:37 | 55794 | 2011-08-21 00:00:00 | 55428.1624537037 | 2010-08-20 03:53:56 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050041 | The nature of ultraluminous X-ray sources (ULXs) is one of the important unresolved issues in the modern astrophysics. A Suzaku HXD spectrum above 10 keV and its variation, in combination with those with XIS, provide us with an unique opportunity to determine unambiguously the physical state of ULXs, which is a key information to solve their nature. Here, two 80 ks Suzaku exposures are proposed on a bright ULX IC 342 X2, one of the most promising candidates for hard X-ray detection. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | NAOKI ISOBE | JAP | 5 | AO5 | HARD X-RAY STUDY OF ULTRALUMINOUS X-RAY SOURCES WITH SUZAKU | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705009010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '705009010'
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