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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner5_ra
corner5_dec
corner6_ra
corner6_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner5_ra_b1950
corner5_dec_b1950
corner6_ra_b1950
corner6_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner5_ecliptic_lon
corner5_ecliptic_lat
corner6_ecliptic_lon
corner6_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
corner5_galactic_lon
corner5_galactic_lat
corner6_galactic_lon
corner6_galactic_lat
resolve_adr_mode
resolve_thr_name
resolve_shp_date
1 201037010 ETA_CARINAE 161.26666 -59.68522 160.7801 -59.42188 202.15723 -58.92732 287.59799 -0.62976 0.00601 60892.33824 2025-08-05 08:07:04 60894.95074 2025-08-07 22:49:04 101.432 80.000 101.432 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 313430 11310 PROCESSED 2025-08-15 13:52:13 2026-08-16 00:00:00 2025-08-16 13:52:14 03.02.014.010 gen20241115_xtd20241115_rsl20241115 Hea_12Mar2025_V6.35_XRISM_28Feb2025_V002 000011206 Mass-loss is widely recognized as a key parameter to understand a stellar chemical evolution following supernova. However, a mass loss rate of Luminous Blue Variables (LBVs) are very difficult to measure due to their dense wind and understood only with digit precision of 10^-3 Mo / yr. In order to improve this accuracy, we propose to observe Eta Carinae at around the periastron passage. Eta Carinae is a long period binary of a primary LBV star and a secondary WR or O star with 5.5 yr period. During the periastron passage, the X-ray plasma heated by wind-wind collision becomes compact, the X-rays from which pierces the LBV wind with narrow beam size. Using the Fe-K absorption edge, the narrow beam enables promising us to pursue to measure the mass-loss rate of the LBV. STELLAR CORONAE, WINDS, AND YOUNG STARS 2 A YOSHITOMO MAEDA JAP 1 NOR XRISM PIERCING THE DENSE STELLAR WIND OF LUMINOUS BLUE VARIABLE IN ETA CARINAE archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201037010/ Quick Look 161.21836 -59.66078 161.21821 -59.71226 161.30293 -59.7122 161.30283 -59.7037 161.31962 -59.70376 161.3198 -59.66087 160.73203 -59.39752 160.7322 -59.449 160.81626 -59.4488 160.81611 -59.4403 160.83277 -59.44033 160.83268 -59.39745 202.09037 -58.92841 202.16313 -58.96364 202.21963 -58.9324 202.20754 -58.92662 202.21884 -58.92048 202.15836 -58.89109 287.56501 -0.61953 287.58899 -0.66509 287.62676 -0.64511 287.62275 -0.63761 287.63028 -0.63371 287.61039 -0.59572 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201037010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏