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 | TX COL | 85.7822 | -41.0648 | 85.383592 | -41.086265 | 82.635964 | -64.399356 | 246.79781267 | -29.77494364 | 322.4827 | 54963.6800578704 | 2009-05-12 16:19:17 | 54965.2502199074 | 2009-05-14 06:00:19 | 404031010 | 59.7818 | 40 | 59.7898 | 59.7898 | 0 | 59.7818 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 51.123 | 51.123 | 135.654 | 0 | PROCESSED | 57546.5734143518 | 2016-06-07 13:45:43 | 55345 | 2010-05-29 00:00:00 | 54978.2105439815 | 2009-05-27 05:03:11 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040113 | We propose observations of 5 Intermediate Polars, a subcategory of magnetic CVs, as the first step toward establishment of an averaged hard X-ray spectrum of IPs that exist near the Solar system.The averaged spectrum should be compared with that of the Galactic Diffese X-ray Emssion (GDXE), to investigate the claimed spectral resemblance between them in energies above 10 keV. If the averaged IP spectrum shows any discrepancy with that of the GDXE, the "point-source origin" explanation for the GDXE would face a lack of appropriate hard X-ray source populations. This in turn is expected to strengthen the competing "truly diffuse origin"explanation, which attributes the GDXE hard X-rays to non thermal emission from electrons being accelerated in the interstellar space. | GALACTIC POINT SOURCES | 4 | A | TAKAYUKI YUASA | JAP | 4 | AO4 | SURVEY OBSERVATION OF INTERMEDIATE POLARS | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404031010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404031010'
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