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 | LMC X-4 | 83.1804 | -66.3624 | 83.172059 | -66.39551 | 0.975905 | -87.276392 | 276.32693529 | -32.54034863 | 209.1491 | 54480.3607175926 | 2008-01-15 08:39:26 | 54480.7919560185 | 2008-01-15 19:00:25 | 702038010 | 21.6579 | 20 | 21.6726 | 21.6579 | 0 | 21.6726 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 22.8837 | 22.8837 | 37.252 | 0 | PROCESSED | 57541.3108796296 | 2016-06-02 07:27:40 | 54860 | 2009-01-29 00:00:00 | 54490.3089236111 | 2008-01-25 07:24:51 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021127 | We propose for a series of three 20ks observations of the binary X-ray pulsar LMC X-4. This source shows 13.5 s pulsations, a 1.4 d orbital period, and a long-period (~30 d) variability due to a warped, precessing accretion disk. The proposed analysis will use pulse-phase spectroscopy with XIS to explore changes in the X-ray pulses and spectra at three different phases in the disk precession. This work will give us a detailed picture of the accretion flow, particularly for the inner regions of the accretion disk that are illuminated by the X-rays from the neutron star. This project takes advantage of the strengths of the XIS, particularly its excellent spectral resolution, sufficient (1s) time resolution in Window mode, and wide PSF that limits pile-up effects. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | RYAN HICKOX | USA | 2 | AO2 | SUPERORBITAL VARIATION OF LMC X-4: EXPLORING THE ACCRETION FLOW | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702038010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702038010'
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