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 | IRASF01475-0740 | 27.4875 | -7.3766 | 26.863598 | -7.624293 | 22.745573 | -17.452267 | 160.69718538 | -65.86110455 | 68.025 | 54661.0549652778 | 2008-07-14 01:19:09 | 54662.3023032407 | 2008-07-15 07:15:19 | 703065010 | 57.9147 | 50 | 57.9147 | 57.9183 | 0 | 57.9263 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 51.1257 | 51.1257 | 107.6988 | 0 | PROCESSED | 57543.0527546296 | 2016-06-04 01:15:58 | 55051 | 2009-08-08 00:00:00 | 54683.4056712963 | 2008-08-05 09:44:10 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 032030 | We propose 50ks observations of IRASF01475-0740 and NGC 3147, both of which are Seyfert 2s apparently unobscured in X-rays. Unsatisfied with this apparent contradiction, we seek Suzaku observations with two main aims. First, high energy observations with the HXD can reveal whether a deeply buried AGN is present above 10 keV. Second, the XIS observations will probe sensitively for short time-scale variability below 10 keV, the detection of which would establish unambiguously that the objects have genuinely unobscured nuclei and rule out the alternatives of scattered light or X-ray binaries. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | KIRPAL NANDRA | EUR | 3 | AO3 | SOLVING THE MYSTERY OF UNOBSCURED SEYFERT 2 GALAXIES | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703065010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703065010'
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