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 MARKARIAN 509 311.0451 -10.7278 310.364015 -10.909382 310.547312 7.12309 35.96880101 -29.86110163 254.2048 54066.1625810185 2006-11-27 03:54:07 54067.12875 2006-11-28 03:05:24 701093040 33.0944 32 33.0944 33.0944 0 33.0944 2 2 0 2 1 0 0 29.4544 29.4544 83.4659 1 PROCESSED 57536.2044212963 2016-05-28 04:54:22 54456 2007-12-22 00:00:00 54088.5895023148 2006-12-19 14:08:53 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 012050 We propose to perform 4 repeated Suzaku observations of 25 ks each of the Seyfert 1 galaxy MKN 509, the brightest Seyfert galaxy of the Piccinotti sample in the 2-100 keV band that is not strongly affected by neutral or ionized absorbing material. The aim of the study is to disentangle the different physical explanations for the origin of the soft excess looking at the long time--scale correlations between the variations of the emission and shape of the soft excess and the emission at high energy (E > 10 keV). EXTRAGALACTIC COMPACT SOURCES 7 A GABRIELE PONTI EUR 1 AO1 SOLVING THE NATURE OF THE SOFT EXCESS IN AGNS WITH SUZAKU XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701093040/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701093040'

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