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 2S 0921-630 140.6643 -63.2995 140.374106 -63.084565 195.141929 -68.892072 281.84516955 -9.33669084 18.1705 54342.4079166667 2007-08-30 09:47:24 54343.5134722222 2007-08-31 12:19:24 402058010 45.6937 40 45.6937 45.6937 0 45.6937 2 2 0 2 1 0 0 43.3463 43.3463 95.4998 2 PROCESSED 57539.9018981482 2016-05-31 21:38:44 54724 2008-09-15 00:00:00 54356.2760763889 2007-09-13 06:37:33 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021118 2S 0921-630 is a bright, long-period LMXB that is thought to contain an accretion disk corona. Observations with both the Chandra HETGS and XMM-Newton spectrometers revealed line emission from a photoionized plasma. The spectral features are consistent with the predictions for emission from an accretion disk corona. However, with the present data it is impossible to determine whether the emission originates in the corona or in a localized region of the disk. We propose to observer 2S 0921-630 with Suzaku at four orbital phases in order to localize and identify the emitting plasma. The simultaneous HXD coverage will also allow us to constrain the underlying continuum and allow more sensitive study of the high energy region of the spectrum. GALACTIC POINT SOURCES 4 A JEAN COTTAM USA 2 AO2 PHASE-RESOLVED SPECTROSCOPY OF 2S 0921-630 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402058010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402058010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏