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
1 SS 433 287.9527 4.99 287.334904 4.905608 290.182673 27.181461 39.69879316 -2.23786427 78.6446 53833.4611458333 2006-04-08 11:04:03 53834.4579166667 2006-04-09 10:59:24 401004010 40.1976 40 40.2216 40.1976 40.2296 40.2136 2 2 2 2 1 0 0 30.4749 30.4749 86.11 2 PROCESSED 57533.4357638889 2016-05-25 10:27:30 54400 2007-10-27 00:00:00 53906.5501736111 2006-06-20 13:12:15 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010031 SS433 is the most intensively studied jet source, however the nature of the object and the jet-formation mechanism remain unknown. We propose to examine the fundamental system parameters; the jet's mass-outflow rate and the total X-ray luminosity. The ionized or blue-shifted iron absorption edge recently discovered with XMM-Newton indicates either the absorber is photo-ionized by a hidden X-ray as luminous as 1E39 erg/s, or is moving along with the jet. SS433 may be an ultra-luminous source if seen face-on, or an unobserved cool component may coexist in the X-ray jet. The spectral continuum over 10 keV to be obtained with the HXD and the absorption edge by the XIS will reveal the nature of the absorber. GALACTIC POINT SOURCES 4 A NOBUYUKI KAWAI JAP 1 AO1 SS 433 OBSERVATIONS OF THE HARD X-RAY CONTINUUM AND THE IRON ABSORPTION EDGE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401004010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401004010'

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