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 CYGNUS X-3 308.2593 40.981 307.808438 40.809488 328.80084 56.880196 79.93230299 0.62160244 252.424 54052.0902893518 2006-11-13 02:10:01 54054.3676388889 2006-11-15 08:49:24 401011010 99.7445 100 99.7462 99.7462 0 99.7445 2 2 0 2 1 0 0 95.3893 95.3893 196.745 1 PROCESSED 57536.1520717593 2016-05-28 03:38:59 54456 2007-12-22 00:00:00 54088.9545023148 2006-12-19 22:54:29 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010058 We propose an observation of the unusual X-ray binary Cygnus X-3. Cyg X-3 is a final stage of the massive binary stars consisting of a WR(N) star and a compact star. However the nature of the compact star is not well understood. We have fore scientific objective. (A)Determine the Doppler modulation of iron K lines and discuss the binary nature. (2) Determine the iron abundance in the WR wind. (3) Search for the high energy cut off about 100keV of the power law component. (4) Search for the X-ray emission from radio knots. For these four sciences, we propose 100ksec observation of Cyg X-3. GALACTIC POINT SOURCES 4 C SHUNJI KITAMOTO JAP 1 AO1 WIDE BAND OBSERVATION OF CYGNUS X-3 WITH SUZAKU SPE Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/401011010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '401011010'

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