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 | SMC X-1 | 19.2675 | -73.4407 | 18.935881 | -73.70387 | 312.347206 | -66.469935 | 300.41598527 | -43.56211574 | 204.2035 | 55875.0768055556 | 2011-11-10 01:50:36 | 55875.6182291667 | 2011-11-10 14:50:15 | 706030080 | 19.8598 | 18 | 19.8881 | 19.8961 | 0 | 19.8598 | 2 | 2 | 0 | 1 | 1 | 0 | 0 | 19.2508 | 19.2508 | 46.772 | 0 | PROCESSED | 57603.7203587963 | 2016-08-03 17:17:19 | 56260 | 2012-11-29 00:00:00 | 55890.6941203704 | 2011-11-25 16:39:32 | 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/ver3.0/706030080/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706030080'
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