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 SMC X-1 19.2661 -73.446 18.934565 -73.709172 312.334379 -66.471359 300.41753301 -43.55692043 64.0051 55740.5953819444 2011-06-28 14:17:21 55741.0960069444 2011-06-29 02:18:15 706030060 18.6682 18 18.7129 18.7049 0 18.6682 2 2 0 1 1 0 0 20.6764 20.6764 43.2479 0 PROCESSED 57602.4222800926 2016-08-02 10:08:05 56163 2012-08-24 00:00:00 55775.167974537 2011-08-02 04:01:53 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 061236 We propose a sequence of 10 18-ks observations of the wind-fed accreting X-ray pulsar SMC X-1. Distributed throughout the orbital and super-orbital period of this high-mass X-ray binary, our proposed observations will reveal the influence of wind accretion on the structure and evolution of accretion disks via three independent methods: (1) mapping the geometry of the accretion flow through soft X-ray emission line variability and ionization studies, (2) tracing the structure of the accretion disk corona with hard X-ray scattering studies, and (3) tracking the evolution of the neutron star spin period and pulse profile for comparison to changes in the warped, precessing accretion disk. EXTRAGALACTIC COMPACT SOURCES 7 A JOSEPH NEILSEN USA 6 AO6 THE WANDERING WARP OF SMC X-1 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706030060/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '706030060'

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