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 | V1223 SGR | 283.7562 | -31.163 | 282.951401 | -31.227311 | 281.856338 | -8.287095 | 4.95737746 | -14.35200731 | 75.0006 | 56745.6297453704 | 2014-03-29 15:06:50 | 56746.5002430556 | 2014-03-30 12:00:21 | 408019010 | 29.3493 | 180 | 29.3893 | 29.3493 | 0 | 29.3967 | 1 | 1 | 0 | 2 | 1 | 0 | 0 | 26.131 | 26.131 | 75.192 | 1 | PROCESSED | 57614.1428703704 | 2016-08-14 03:25:44 | 57121 | 2015-04-09 00:00:00 | 56756.7522800926 | 2014-04-09 18:03:17 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 080086 | A 180-ks observation of the magnetic cataclysmic variable V1223 Sgr is proposed. By increasing the statistics by a factor of 4 compared to the existing 45-ks data, we investigate spin-phase dependent redshift of the iron fluorescent line, in particular its line center energy and equivalent width with smaller statistical errors than results of Hayashi et al. 2011. These parameters will provide geometrical configuration, or solid angle viewed from the post-shock region, of the pre-shock cool gas and the white dwarf reflecting surface. We use this information to make our Monte-Carlo simulator of magnetic CV more physically realistic and reliable in analyzing the high-resolution iron line profiles to be obtained with the ASTRO-H/SXS. | GALACTIC POINT SOURCES | 4 | B | TAKAYUKI YUASA | JAP | 8 | AO8 | DEEP OBSERVATION OF THE MAGNETIC CATACLYSMIC VARIABLE V1223 SGR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408019010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '408019010'
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