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 | 2S 0921-630 | 140.6632 | -63.3 | 140.373022 | -63.085068 | 195.142403 | -68.892754 | 281.84517925 | -9.33739383 | 20.5636 | 54340.7614351852 | 2007-08-28 18:16:28 | 54341.8335532407 | 2007-08-29 20:00:19 | 402057010 | 43.2131 | 40 | 43.2131 | 43.2211 | 0 | 43.2211 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 15.8568 | 15.8568 | 92.6158 | 0 | PROCESSED | 57539.9304976852 | 2016-05-31 22:19:55 | 54721 | 2008-09-12 00:00:00 | 54353.4365625 | 2007-09-10 10:28:39 | 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/ver3.0/402057010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402057010'
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